Fermions, Bosons and their Statistics - uni-osnabrueck.deFermions, Bosons and their Statistics Peter...

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Fermions, Bosons and their Statistics Peter Hertel Fundamental particles Spin and statistics Many particles Gibbs state Fermions Zero temperature White dwarfs and neutron stars Bosons Black body radiation Bose-Einstein condensation Fermions, Bosons and their Statistics Peter Hertel University of Osnabr¨ uck, Germany Lecture presented at APS, Nankai University, China http://www.home.uni-osnabrueck.de/phertel March/April 2011

Transcript of Fermions, Bosons and their Statistics - uni-osnabrueck.deFermions, Bosons and their Statistics Peter...

Page 1: Fermions, Bosons and their Statistics - uni-osnabrueck.deFermions, Bosons and their Statistics Peter Hertel Fundamental particles Spin and statistics Many particles Gibbs state Fermions

Fermions,Bosons and

theirStatistics

Peter Hertel

Fundamentalparticles

Spin andstatistics

Many particles

Gibbs state

Fermions

Zerotemperature

White dwarfsand neutronstars

Bosons

Black bodyradiation

Bose-Einsteincondensation

Fermions, Bosons and their Statistics

Peter Hertel

University of Osnabruck, Germany

Lecture presented at APS, Nankai University, China

http://www.home.uni-osnabrueck.de/phertel

March/April 2011

Page 2: Fermions, Bosons and their Statistics - uni-osnabrueck.deFermions, Bosons and their Statistics Peter Hertel Fundamental particles Spin and statistics Many particles Gibbs state Fermions

Fermions,Bosons and

theirStatistics

Peter Hertel

Fundamentalparticles

Spin andstatistics

Many particles

Gibbs state

Fermions

Zerotemperature

White dwarfsand neutronstars

Bosons

Black bodyradiation

Bose-Einsteincondensation

Structure fermions

charge -1 -2/3 -1/3 0 +1/3 +2/3 +1

generation 1 e− u d νe , νe d u e+

generation 2 µ− c s νµ, νµ s c µ+

generation 3 τ− t b ντ , ντ b t τ+

• all structure particles have spin 1/2

• proton p=(uud) and neutron n=(udd)

• both have spin 1/2

• excited states ∆++=(uuu)∗, ∆+=(uud)∗ etc.

• they have spin 3/2

• p is stable, n → p+e−+ν is allowed

Page 3: Fermions, Bosons and their Statistics - uni-osnabrueck.deFermions, Bosons and their Statistics Peter Hertel Fundamental particles Spin and statistics Many particles Gibbs state Fermions

Fermions,Bosons and

theirStatistics

Peter Hertel

Fundamentalparticles

Spin andstatistics

Many particles

Gibbs state

Fermions

Zerotemperature

White dwarfsand neutronstars

Bosons

Black bodyradiation

Bose-Einsteincondensation

Structure fermions

charge -1 -2/3 -1/3 0 +1/3 +2/3 +1

generation 1 e− u d νe , νe d u e+

generation 2 µ− c s νµ, νµ s c µ+

generation 3 τ− t b ντ , ντ b t τ+

• all structure particles have spin 1/2

• proton p=(uud) and neutron n=(udd)

• both have spin 1/2

• excited states ∆++=(uuu)∗, ∆+=(uud)∗ etc.

• they have spin 3/2

• p is stable, n → p+e−+ν is allowed

Page 4: Fermions, Bosons and their Statistics - uni-osnabrueck.deFermions, Bosons and their Statistics Peter Hertel Fundamental particles Spin and statistics Many particles Gibbs state Fermions

Fermions,Bosons and

theirStatistics

Peter Hertel

Fundamentalparticles

Spin andstatistics

Many particles

Gibbs state

Fermions

Zerotemperature

White dwarfsand neutronstars

Bosons

Black bodyradiation

Bose-Einsteincondensation

Structure fermions

charge -1 -2/3 -1/3 0 +1/3 +2/3 +1

generation 1 e− u d νe , νe d u e+

generation 2 µ− c s νµ, νµ s c µ+

generation 3 τ− t b ντ , ντ b t τ+

• all structure particles have spin 1/2

• proton p=(uud) and neutron n=(udd)

• both have spin 1/2

• excited states ∆++=(uuu)∗, ∆+=(uud)∗ etc.

• they have spin 3/2

• p is stable, n → p+e−+ν is allowed

Page 5: Fermions, Bosons and their Statistics - uni-osnabrueck.deFermions, Bosons and their Statistics Peter Hertel Fundamental particles Spin and statistics Many particles Gibbs state Fermions

Fermions,Bosons and

theirStatistics

Peter Hertel

Fundamentalparticles

Spin andstatistics

Many particles

Gibbs state

Fermions

Zerotemperature

White dwarfsand neutronstars

Bosons

Black bodyradiation

Bose-Einsteincondensation

Structure fermions

charge -1 -2/3 -1/3 0 +1/3 +2/3 +1

generation 1 e− u d νe , νe d u e+

generation 2 µ− c s νµ, νµ s c µ+

generation 3 τ− t b ντ , ντ b t τ+

• all structure particles have spin 1/2

• proton p=(uud) and neutron n=(udd)

• both have spin 1/2

• excited states ∆++=(uuu)∗, ∆+=(uud)∗ etc.

• they have spin 3/2

• p is stable, n → p+e−+ν is allowed

Page 6: Fermions, Bosons and their Statistics - uni-osnabrueck.deFermions, Bosons and their Statistics Peter Hertel Fundamental particles Spin and statistics Many particles Gibbs state Fermions

Fermions,Bosons and

theirStatistics

Peter Hertel

Fundamentalparticles

Spin andstatistics

Many particles

Gibbs state

Fermions

Zerotemperature

White dwarfsand neutronstars

Bosons

Black bodyradiation

Bose-Einsteincondensation

Structure fermions

charge -1 -2/3 -1/3 0 +1/3 +2/3 +1

generation 1 e− u d νe , νe d u e+

generation 2 µ− c s νµ, νµ s c µ+

generation 3 τ− t b ντ , ντ b t τ+

• all structure particles have spin 1/2

• proton p=(uud) and neutron n=(udd)

• both have spin 1/2

• excited states ∆++=(uuu)∗, ∆+=(uud)∗ etc.

• they have spin 3/2

• p is stable, n → p+e−+ν is allowed

Page 7: Fermions, Bosons and their Statistics - uni-osnabrueck.deFermions, Bosons and their Statistics Peter Hertel Fundamental particles Spin and statistics Many particles Gibbs state Fermions

Fermions,Bosons and

theirStatistics

Peter Hertel

Fundamentalparticles

Spin andstatistics

Many particles

Gibbs state

Fermions

Zerotemperature

White dwarfsand neutronstars

Bosons

Black bodyradiation

Bose-Einsteincondensation

Structure fermions

charge -1 -2/3 -1/3 0 +1/3 +2/3 +1

generation 1 e− u d νe , νe d u e+

generation 2 µ− c s νµ, νµ s c µ+

generation 3 τ− t b ντ , ντ b t τ+

• all structure particles have spin 1/2

• proton p=(uud) and neutron n=(udd)

• both have spin 1/2

• excited states ∆++=(uuu)∗, ∆+=(uud)∗ etc.

• they have spin 3/2

• p is stable, n → p+e−+ν is allowed

Page 8: Fermions, Bosons and their Statistics - uni-osnabrueck.deFermions, Bosons and their Statistics Peter Hertel Fundamental particles Spin and statistics Many particles Gibbs state Fermions

Fermions,Bosons and

theirStatistics

Peter Hertel

Fundamentalparticles

Spin andstatistics

Many particles

Gibbs state

Fermions

Zerotemperature

White dwarfsand neutronstars

Bosons

Black bodyradiation

Bose-Einsteincondensation

Exchange bosons

W− νee− νµµ

− νττ− ud cs tb

γ,Z 0 e+e− µ+µ− τ+τ− (νeνe νµνµ ντντ ) dd uu ss cc bb tt

W+ e+νe µ+νµ τ

+ντ du sc bt

• W+, γ, Z0, W− mediate electro-weak interaction

• the photon couples to charged particles only

• there are also gluons which mediate strong interactions

• e.g. n=(udd) → (uud)+W− → p+νe+e−

• is there also a graviton G ?

• is there also a Higgs boson H ?

Page 9: Fermions, Bosons and their Statistics - uni-osnabrueck.deFermions, Bosons and their Statistics Peter Hertel Fundamental particles Spin and statistics Many particles Gibbs state Fermions

Fermions,Bosons and

theirStatistics

Peter Hertel

Fundamentalparticles

Spin andstatistics

Many particles

Gibbs state

Fermions

Zerotemperature

White dwarfsand neutronstars

Bosons

Black bodyradiation

Bose-Einsteincondensation

Exchange bosons

W− νee− νµµ

− νττ− ud cs tb

γ,Z 0 e+e− µ+µ− τ+τ− (νeνe νµνµ ντντ ) dd uu ss cc bb tt

W+ e+νe µ+νµ τ

+ντ du sc bt

• W+, γ, Z0, W− mediate electro-weak interaction

• the photon couples to charged particles only

• there are also gluons which mediate strong interactions

• e.g. n=(udd) → (uud)+W− → p+νe+e−

• is there also a graviton G ?

• is there also a Higgs boson H ?

Page 10: Fermions, Bosons and their Statistics - uni-osnabrueck.deFermions, Bosons and their Statistics Peter Hertel Fundamental particles Spin and statistics Many particles Gibbs state Fermions

Fermions,Bosons and

theirStatistics

Peter Hertel

Fundamentalparticles

Spin andstatistics

Many particles

Gibbs state

Fermions

Zerotemperature

White dwarfsand neutronstars

Bosons

Black bodyradiation

Bose-Einsteincondensation

Exchange bosons

W− νee− νµµ

− νττ− ud cs tb

γ,Z 0 e+e− µ+µ− τ+τ− (νeνe νµνµ ντντ ) dd uu ss cc bb tt

W+ e+νe µ+νµ τ

+ντ du sc bt

• W+, γ, Z0, W− mediate electro-weak interaction

• the photon couples to charged particles only

• there are also gluons which mediate strong interactions

• e.g. n=(udd) → (uud)+W− → p+νe+e−

• is there also a graviton G ?

• is there also a Higgs boson H ?

Page 11: Fermions, Bosons and their Statistics - uni-osnabrueck.deFermions, Bosons and their Statistics Peter Hertel Fundamental particles Spin and statistics Many particles Gibbs state Fermions

Fermions,Bosons and

theirStatistics

Peter Hertel

Fundamentalparticles

Spin andstatistics

Many particles

Gibbs state

Fermions

Zerotemperature

White dwarfsand neutronstars

Bosons

Black bodyradiation

Bose-Einsteincondensation

Exchange bosons

W− νee− νµµ

− νττ− ud cs tb

γ,Z 0 e+e− µ+µ− τ+τ− (νeνe νµνµ ντντ ) dd uu ss cc bb tt

W+ e+νe µ+νµ τ

+ντ du sc bt

• W+, γ, Z0, W− mediate electro-weak interaction

• the photon couples to charged particles only

• there are also gluons which mediate strong interactions

• e.g. n=(udd) → (uud)+W− → p+νe+e−

• is there also a graviton G ?

• is there also a Higgs boson H ?

Page 12: Fermions, Bosons and their Statistics - uni-osnabrueck.deFermions, Bosons and their Statistics Peter Hertel Fundamental particles Spin and statistics Many particles Gibbs state Fermions

Fermions,Bosons and

theirStatistics

Peter Hertel

Fundamentalparticles

Spin andstatistics

Many particles

Gibbs state

Fermions

Zerotemperature

White dwarfsand neutronstars

Bosons

Black bodyradiation

Bose-Einsteincondensation

Exchange bosons

W− νee− νµµ

− νττ− ud cs tb

γ,Z 0 e+e− µ+µ− τ+τ− (νeνe νµνµ ντντ ) dd uu ss cc bb tt

W+ e+νe µ+νµ τ

+ντ du sc bt

• W+, γ, Z0, W− mediate electro-weak interaction

• the photon couples to charged particles only

• there are also gluons which mediate strong interactions

• e.g. n=(udd) → (uud)+W− → p+νe+e−

• is there also a graviton G ?

• is there also a Higgs boson H ?

Page 13: Fermions, Bosons and their Statistics - uni-osnabrueck.deFermions, Bosons and their Statistics Peter Hertel Fundamental particles Spin and statistics Many particles Gibbs state Fermions

Fermions,Bosons and

theirStatistics

Peter Hertel

Fundamentalparticles

Spin andstatistics

Many particles

Gibbs state

Fermions

Zerotemperature

White dwarfsand neutronstars

Bosons

Black bodyradiation

Bose-Einsteincondensation

Exchange bosons

W− νee− νµµ

− νττ− ud cs tb

γ,Z 0 e+e− µ+µ− τ+τ− (νeνe νµνµ ντντ ) dd uu ss cc bb tt

W+ e+νe µ+νµ τ

+ντ du sc bt

• W+, γ, Z0, W− mediate electro-weak interaction

• the photon couples to charged particles only

• there are also gluons which mediate strong interactions

• e.g. n=(udd) → (uud)+W− → p+νe+e−

• is there also a graviton G ?

• is there also a Higgs boson H ?

Page 14: Fermions, Bosons and their Statistics - uni-osnabrueck.deFermions, Bosons and their Statistics Peter Hertel Fundamental particles Spin and statistics Many particles Gibbs state Fermions

Fermions,Bosons and

theirStatistics

Peter Hertel

Fundamentalparticles

Spin andstatistics

Many particles

Gibbs state

Fermions

Zerotemperature

White dwarfsand neutronstars

Bosons

Black bodyradiation

Bose-Einsteincondensation The Aleph detector (opened) at Cern

Page 15: Fermions, Bosons and their Statistics - uni-osnabrueck.deFermions, Bosons and their Statistics Peter Hertel Fundamental particles Spin and statistics Many particles Gibbs state Fermions

Fermions,Bosons and

theirStatistics

Peter Hertel

Fundamentalparticles

Spin andstatistics

Many particles

Gibbs state

Fermions

Zerotemperature

White dwarfsand neutronstars

Bosons

Black bodyradiation

Bose-Einsteincondensation

Spin 1/2 fermions

• massive structure fermion (quarks, electrons) have spin1/2

• or helicity 1/2 and -1/2

• massless structure fermions (neutrinos) have either helicity1/2 or -1/2

• this explains parity violation

• spin and statistics are related

Page 16: Fermions, Bosons and their Statistics - uni-osnabrueck.deFermions, Bosons and their Statistics Peter Hertel Fundamental particles Spin and statistics Many particles Gibbs state Fermions

Fermions,Bosons and

theirStatistics

Peter Hertel

Fundamentalparticles

Spin andstatistics

Many particles

Gibbs state

Fermions

Zerotemperature

White dwarfsand neutronstars

Bosons

Black bodyradiation

Bose-Einsteincondensation

Spin 1/2 fermions

• massive structure fermion (quarks, electrons) have spin1/2

• or helicity 1/2 and -1/2

• massless structure fermions (neutrinos) have either helicity1/2 or -1/2

• this explains parity violation

• spin and statistics are related

Page 17: Fermions, Bosons and their Statistics - uni-osnabrueck.deFermions, Bosons and their Statistics Peter Hertel Fundamental particles Spin and statistics Many particles Gibbs state Fermions

Fermions,Bosons and

theirStatistics

Peter Hertel

Fundamentalparticles

Spin andstatistics

Many particles

Gibbs state

Fermions

Zerotemperature

White dwarfsand neutronstars

Bosons

Black bodyradiation

Bose-Einsteincondensation

Spin 1/2 fermions

• massive structure fermion (quarks, electrons) have spin1/2

• or helicity 1/2 and -1/2

• massless structure fermions (neutrinos) have either helicity1/2 or -1/2

• this explains parity violation

• spin and statistics are related

Page 18: Fermions, Bosons and their Statistics - uni-osnabrueck.deFermions, Bosons and their Statistics Peter Hertel Fundamental particles Spin and statistics Many particles Gibbs state Fermions

Fermions,Bosons and

theirStatistics

Peter Hertel

Fundamentalparticles

Spin andstatistics

Many particles

Gibbs state

Fermions

Zerotemperature

White dwarfsand neutronstars

Bosons

Black bodyradiation

Bose-Einsteincondensation

Spin 1/2 fermions

• massive structure fermion (quarks, electrons) have spin1/2

• or helicity 1/2 and -1/2

• massless structure fermions (neutrinos) have either helicity1/2 or -1/2

• this explains parity violation

• spin and statistics are related

Page 19: Fermions, Bosons and their Statistics - uni-osnabrueck.deFermions, Bosons and their Statistics Peter Hertel Fundamental particles Spin and statistics Many particles Gibbs state Fermions

Fermions,Bosons and

theirStatistics

Peter Hertel

Fundamentalparticles

Spin andstatistics

Many particles

Gibbs state

Fermions

Zerotemperature

White dwarfsand neutronstars

Bosons

Black bodyradiation

Bose-Einsteincondensation

Spin 1/2 fermions

• massive structure fermion (quarks, electrons) have spin1/2

• or helicity 1/2 and -1/2

• massless structure fermions (neutrinos) have either helicity1/2 or -1/2

• this explains parity violation

• spin and statistics are related

Page 20: Fermions, Bosons and their Statistics - uni-osnabrueck.deFermions, Bosons and their Statistics Peter Hertel Fundamental particles Spin and statistics Many particles Gibbs state Fermions

Fermions,Bosons and

theirStatistics

Peter Hertel

Fundamentalparticles

Spin andstatistics

Many particles

Gibbs state

Fermions

Zerotemperature

White dwarfsand neutronstars

Bosons

Black bodyradiation

Bose-Einsteincondensation

Spin 1/2 fermions

• massive structure fermion (quarks, electrons) have spin1/2

• or helicity 1/2 and -1/2

• massless structure fermions (neutrinos) have either helicity1/2 or -1/2

• this explains parity violation

• spin and statistics are related

Page 21: Fermions, Bosons and their Statistics - uni-osnabrueck.deFermions, Bosons and their Statistics Peter Hertel Fundamental particles Spin and statistics Many particles Gibbs state Fermions

Fermions,Bosons and

theirStatistics

Peter Hertel

Fundamentalparticles

Spin andstatistics

Many particles

Gibbs state

Fermions

Zerotemperature

White dwarfsand neutronstars

Bosons

Black bodyradiation

Bose-Einsteincondensation

Spin and statisics

• rotation of a particle with spin s is described by

ψR = ei~α · Sψ

• a 360 rotation yields

ψ = e2πis

ψ = φRψ

• φR = +1 for integer spin (bosons), and -1 for half-integerspin (fermions)

• exchanging two identicle particles must not change |ψ|2

ψ(σ1x1, σ2x2) = φXψ(σ2x2, σ1x1)

• spin-statistics theorem says φR = φX

• for fermions: ψ(σ1x1, σ2x2) = −ψ(σ2x2, σ1x1)

• Pauli exclusion principle

Page 22: Fermions, Bosons and their Statistics - uni-osnabrueck.deFermions, Bosons and their Statistics Peter Hertel Fundamental particles Spin and statistics Many particles Gibbs state Fermions

Fermions,Bosons and

theirStatistics

Peter Hertel

Fundamentalparticles

Spin andstatistics

Many particles

Gibbs state

Fermions

Zerotemperature

White dwarfsand neutronstars

Bosons

Black bodyradiation

Bose-Einsteincondensation

Spin and statisics

• rotation of a particle with spin s is described by

ψR = ei~α · Sψ

• a 360 rotation yields

ψ = e2πis

ψ = φRψ

• φR = +1 for integer spin (bosons), and -1 for half-integerspin (fermions)

• exchanging two identicle particles must not change |ψ|2

ψ(σ1x1, σ2x2) = φXψ(σ2x2, σ1x1)

• spin-statistics theorem says φR = φX

• for fermions: ψ(σ1x1, σ2x2) = −ψ(σ2x2, σ1x1)

• Pauli exclusion principle

Page 23: Fermions, Bosons and their Statistics - uni-osnabrueck.deFermions, Bosons and their Statistics Peter Hertel Fundamental particles Spin and statistics Many particles Gibbs state Fermions

Fermions,Bosons and

theirStatistics

Peter Hertel

Fundamentalparticles

Spin andstatistics

Many particles

Gibbs state

Fermions

Zerotemperature

White dwarfsand neutronstars

Bosons

Black bodyradiation

Bose-Einsteincondensation

Spin and statisics

• rotation of a particle with spin s is described by

ψR = ei~α · Sψ

• a 360 rotation yields

ψ = e2πis

ψ = φRψ

• φR = +1 for integer spin (bosons), and -1 for half-integerspin (fermions)

• exchanging two identicle particles must not change |ψ|2

ψ(σ1x1, σ2x2) = φXψ(σ2x2, σ1x1)

• spin-statistics theorem says φR = φX

• for fermions: ψ(σ1x1, σ2x2) = −ψ(σ2x2, σ1x1)

• Pauli exclusion principle

Page 24: Fermions, Bosons and their Statistics - uni-osnabrueck.deFermions, Bosons and their Statistics Peter Hertel Fundamental particles Spin and statistics Many particles Gibbs state Fermions

Fermions,Bosons and

theirStatistics

Peter Hertel

Fundamentalparticles

Spin andstatistics

Many particles

Gibbs state

Fermions

Zerotemperature

White dwarfsand neutronstars

Bosons

Black bodyradiation

Bose-Einsteincondensation

Spin and statisics

• rotation of a particle with spin s is described by

ψR = ei~α · Sψ

• a 360 rotation yields

ψ = e2πis

ψ = φRψ

• φR = +1 for integer spin (bosons), and -1 for half-integerspin (fermions)

• exchanging two identicle particles must not change |ψ|2

ψ(σ1x1, σ2x2) = φXψ(σ2x2, σ1x1)

• spin-statistics theorem says φR = φX

• for fermions: ψ(σ1x1, σ2x2) = −ψ(σ2x2, σ1x1)

• Pauli exclusion principle

Page 25: Fermions, Bosons and their Statistics - uni-osnabrueck.deFermions, Bosons and their Statistics Peter Hertel Fundamental particles Spin and statistics Many particles Gibbs state Fermions

Fermions,Bosons and

theirStatistics

Peter Hertel

Fundamentalparticles

Spin andstatistics

Many particles

Gibbs state

Fermions

Zerotemperature

White dwarfsand neutronstars

Bosons

Black bodyradiation

Bose-Einsteincondensation

Spin and statisics

• rotation of a particle with spin s is described by

ψR = ei~α · Sψ

• a 360 rotation yields

ψ = e2πis

ψ = φRψ

• φR = +1 for integer spin (bosons), and -1 for half-integerspin (fermions)

• exchanging two identicle particles must not change |ψ|2

ψ(σ1x1, σ2x2) = φXψ(σ2x2, σ1x1)

• spin-statistics theorem says φR = φX

• for fermions: ψ(σ1x1, σ2x2) = −ψ(σ2x2, σ1x1)

• Pauli exclusion principle

Page 26: Fermions, Bosons and their Statistics - uni-osnabrueck.deFermions, Bosons and their Statistics Peter Hertel Fundamental particles Spin and statistics Many particles Gibbs state Fermions

Fermions,Bosons and

theirStatistics

Peter Hertel

Fundamentalparticles

Spin andstatistics

Many particles

Gibbs state

Fermions

Zerotemperature

White dwarfsand neutronstars

Bosons

Black bodyradiation

Bose-Einsteincondensation

Spin and statisics

• rotation of a particle with spin s is described by

ψR = ei~α · Sψ

• a 360 rotation yields

ψ = e2πis

ψ = φRψ

• φR = +1 for integer spin (bosons), and -1 for half-integerspin (fermions)

• exchanging two identicle particles must not change |ψ|2

ψ(σ1x1, σ2x2) = φXψ(σ2x2, σ1x1)

• spin-statistics theorem says φR = φX

• for fermions: ψ(σ1x1, σ2x2) = −ψ(σ2x2, σ1x1)

• Pauli exclusion principle

Page 27: Fermions, Bosons and their Statistics - uni-osnabrueck.deFermions, Bosons and their Statistics Peter Hertel Fundamental particles Spin and statistics Many particles Gibbs state Fermions

Fermions,Bosons and

theirStatistics

Peter Hertel

Fundamentalparticles

Spin andstatistics

Many particles

Gibbs state

Fermions

Zerotemperature

White dwarfsand neutronstars

Bosons

Black bodyradiation

Bose-Einsteincondensation

Spin and statisics

• rotation of a particle with spin s is described by

ψR = ei~α · Sψ

• a 360 rotation yields

ψ = e2πis

ψ = φRψ

• φR = +1 for integer spin (bosons), and -1 for half-integerspin (fermions)

• exchanging two identicle particles must not change |ψ|2

ψ(σ1x1, σ2x2) = φXψ(σ2x2, σ1x1)

• spin-statistics theorem says φR = φX

• for fermions: ψ(σ1x1, σ2x2) = −ψ(σ2x2, σ1x1)

• Pauli exclusion principle

Page 28: Fermions, Bosons and their Statistics - uni-osnabrueck.deFermions, Bosons and their Statistics Peter Hertel Fundamental particles Spin and statistics Many particles Gibbs state Fermions

Fermions,Bosons and

theirStatistics

Peter Hertel

Fundamentalparticles

Spin andstatistics

Many particles

Gibbs state

Fermions

Zerotemperature

White dwarfsand neutronstars

Bosons

Black bodyradiation

Bose-Einsteincondensation

Wolfgang Pauli, Austrian/Swiss Physicist, Nobel prize 1945

Page 29: Fermions, Bosons and their Statistics - uni-osnabrueck.deFermions, Bosons and their Statistics Peter Hertel Fundamental particles Spin and statistics Many particles Gibbs state Fermions

Fermions,Bosons and

theirStatistics

Peter Hertel

Fundamentalparticles

Spin andstatistics

Many particles

Gibbs state

Fermions

Zerotemperature

White dwarfsand neutronstars

Bosons

Black bodyradiation

Bose-Einsteincondensation

Arbitrary number of particles

• A∗ creates a particle, A = (A∗)† annihilates a particle

• (A,A) = 0, (A∗,A∗) = 0, (A,A∗) = I

• bosons: (X ,Y ) = [X ,Y ] = XY − YX , the commutator

• fermions: (X ,Y ) = X ,Y = XY + YX , theanti-commutator

• N = A∗A is number operator

• Ω is vacuum

• create n particles

ψn =1√n!

(A∗)n Ω

• Nψn = nψn

• bosons: n = 0, 1, 2, . . .

• fermions: n = 0, 1

Page 30: Fermions, Bosons and their Statistics - uni-osnabrueck.deFermions, Bosons and their Statistics Peter Hertel Fundamental particles Spin and statistics Many particles Gibbs state Fermions

Fermions,Bosons and

theirStatistics

Peter Hertel

Fundamentalparticles

Spin andstatistics

Many particles

Gibbs state

Fermions

Zerotemperature

White dwarfsand neutronstars

Bosons

Black bodyradiation

Bose-Einsteincondensation

Arbitrary number of particles

• A∗ creates a particle, A = (A∗)† annihilates a particle

• (A,A) = 0, (A∗,A∗) = 0, (A,A∗) = I

• bosons: (X ,Y ) = [X ,Y ] = XY − YX , the commutator

• fermions: (X ,Y ) = X ,Y = XY + YX , theanti-commutator

• N = A∗A is number operator

• Ω is vacuum

• create n particles

ψn =1√n!

(A∗)n Ω

• Nψn = nψn

• bosons: n = 0, 1, 2, . . .

• fermions: n = 0, 1

Page 31: Fermions, Bosons and their Statistics - uni-osnabrueck.deFermions, Bosons and their Statistics Peter Hertel Fundamental particles Spin and statistics Many particles Gibbs state Fermions

Fermions,Bosons and

theirStatistics

Peter Hertel

Fundamentalparticles

Spin andstatistics

Many particles

Gibbs state

Fermions

Zerotemperature

White dwarfsand neutronstars

Bosons

Black bodyradiation

Bose-Einsteincondensation

Arbitrary number of particles

• A∗ creates a particle, A = (A∗)† annihilates a particle

• (A,A) = 0, (A∗,A∗) = 0, (A,A∗) = I

• bosons: (X ,Y ) = [X ,Y ] = XY − YX , the commutator

• fermions: (X ,Y ) = X ,Y = XY + YX , theanti-commutator

• N = A∗A is number operator

• Ω is vacuum

• create n particles

ψn =1√n!

(A∗)n Ω

• Nψn = nψn

• bosons: n = 0, 1, 2, . . .

• fermions: n = 0, 1

Page 32: Fermions, Bosons and their Statistics - uni-osnabrueck.deFermions, Bosons and their Statistics Peter Hertel Fundamental particles Spin and statistics Many particles Gibbs state Fermions

Fermions,Bosons and

theirStatistics

Peter Hertel

Fundamentalparticles

Spin andstatistics

Many particles

Gibbs state

Fermions

Zerotemperature

White dwarfsand neutronstars

Bosons

Black bodyradiation

Bose-Einsteincondensation

Arbitrary number of particles

• A∗ creates a particle, A = (A∗)† annihilates a particle

• (A,A) = 0, (A∗,A∗) = 0, (A,A∗) = I

• bosons: (X ,Y ) = [X ,Y ] = XY − YX , the commutator

• fermions: (X ,Y ) = X ,Y = XY + YX , theanti-commutator

• N = A∗A is number operator

• Ω is vacuum

• create n particles

ψn =1√n!

(A∗)n Ω

• Nψn = nψn

• bosons: n = 0, 1, 2, . . .

• fermions: n = 0, 1

Page 33: Fermions, Bosons and their Statistics - uni-osnabrueck.deFermions, Bosons and their Statistics Peter Hertel Fundamental particles Spin and statistics Many particles Gibbs state Fermions

Fermions,Bosons and

theirStatistics

Peter Hertel

Fundamentalparticles

Spin andstatistics

Many particles

Gibbs state

Fermions

Zerotemperature

White dwarfsand neutronstars

Bosons

Black bodyradiation

Bose-Einsteincondensation

Arbitrary number of particles

• A∗ creates a particle, A = (A∗)† annihilates a particle

• (A,A) = 0, (A∗,A∗) = 0, (A,A∗) = I

• bosons: (X ,Y ) = [X ,Y ] = XY − YX , the commutator

• fermions: (X ,Y ) = X ,Y = XY + YX , theanti-commutator

• N = A∗A is number operator

• Ω is vacuum

• create n particles

ψn =1√n!

(A∗)n Ω

• Nψn = nψn

• bosons: n = 0, 1, 2, . . .

• fermions: n = 0, 1

Page 34: Fermions, Bosons and their Statistics - uni-osnabrueck.deFermions, Bosons and their Statistics Peter Hertel Fundamental particles Spin and statistics Many particles Gibbs state Fermions

Fermions,Bosons and

theirStatistics

Peter Hertel

Fundamentalparticles

Spin andstatistics

Many particles

Gibbs state

Fermions

Zerotemperature

White dwarfsand neutronstars

Bosons

Black bodyradiation

Bose-Einsteincondensation

Arbitrary number of particles

• A∗ creates a particle, A = (A∗)† annihilates a particle

• (A,A) = 0, (A∗,A∗) = 0, (A,A∗) = I

• bosons: (X ,Y ) = [X ,Y ] = XY − YX , the commutator

• fermions: (X ,Y ) = X ,Y = XY + YX , theanti-commutator

• N = A∗A is number operator

• Ω is vacuum

• create n particles

ψn =1√n!

(A∗)n Ω

• Nψn = nψn

• bosons: n = 0, 1, 2, . . .

• fermions: n = 0, 1

Page 35: Fermions, Bosons and their Statistics - uni-osnabrueck.deFermions, Bosons and their Statistics Peter Hertel Fundamental particles Spin and statistics Many particles Gibbs state Fermions

Fermions,Bosons and

theirStatistics

Peter Hertel

Fundamentalparticles

Spin andstatistics

Many particles

Gibbs state

Fermions

Zerotemperature

White dwarfsand neutronstars

Bosons

Black bodyradiation

Bose-Einsteincondensation

Arbitrary number of particles

• A∗ creates a particle, A = (A∗)† annihilates a particle

• (A,A) = 0, (A∗,A∗) = 0, (A,A∗) = I

• bosons: (X ,Y ) = [X ,Y ] = XY − YX , the commutator

• fermions: (X ,Y ) = X ,Y = XY + YX , theanti-commutator

• N = A∗A is number operator

• Ω is vacuum

• create n particles

ψn =1√n!

(A∗)n Ω

• Nψn = nψn

• bosons: n = 0, 1, 2, . . .

• fermions: n = 0, 1

Page 36: Fermions, Bosons and their Statistics - uni-osnabrueck.deFermions, Bosons and their Statistics Peter Hertel Fundamental particles Spin and statistics Many particles Gibbs state Fermions

Fermions,Bosons and

theirStatistics

Peter Hertel

Fundamentalparticles

Spin andstatistics

Many particles

Gibbs state

Fermions

Zerotemperature

White dwarfsand neutronstars

Bosons

Black bodyradiation

Bose-Einsteincondensation

Arbitrary number of particles

• A∗ creates a particle, A = (A∗)† annihilates a particle

• (A,A) = 0, (A∗,A∗) = 0, (A,A∗) = I

• bosons: (X ,Y ) = [X ,Y ] = XY − YX , the commutator

• fermions: (X ,Y ) = X ,Y = XY + YX , theanti-commutator

• N = A∗A is number operator

• Ω is vacuum

• create n particles

ψn =1√n!

(A∗)n Ω

• Nψn = nψn

• bosons: n = 0, 1, 2, . . .

• fermions: n = 0, 1

Page 37: Fermions, Bosons and their Statistics - uni-osnabrueck.deFermions, Bosons and their Statistics Peter Hertel Fundamental particles Spin and statistics Many particles Gibbs state Fermions

Fermions,Bosons and

theirStatistics

Peter Hertel

Fundamentalparticles

Spin andstatistics

Many particles

Gibbs state

Fermions

Zerotemperature

White dwarfsand neutronstars

Bosons

Black bodyradiation

Bose-Einsteincondensation

Arbitrary number of particles

• A∗ creates a particle, A = (A∗)† annihilates a particle

• (A,A) = 0, (A∗,A∗) = 0, (A,A∗) = I

• bosons: (X ,Y ) = [X ,Y ] = XY − YX , the commutator

• fermions: (X ,Y ) = X ,Y = XY + YX , theanti-commutator

• N = A∗A is number operator

• Ω is vacuum

• create n particles

ψn =1√n!

(A∗)n Ω

• Nψn = nψn

• bosons: n = 0, 1, 2, . . .

• fermions: n = 0, 1

Page 38: Fermions, Bosons and their Statistics - uni-osnabrueck.deFermions, Bosons and their Statistics Peter Hertel Fundamental particles Spin and statistics Many particles Gibbs state Fermions

Fermions,Bosons and

theirStatistics

Peter Hertel

Fundamentalparticles

Spin andstatistics

Many particles

Gibbs state

Fermions

Zerotemperature

White dwarfsand neutronstars

Bosons

Black bodyradiation

Bose-Einsteincondensation

Arbitrary number of particles

• A∗ creates a particle, A = (A∗)† annihilates a particle

• (A,A) = 0, (A∗,A∗) = 0, (A,A∗) = I

• bosons: (X ,Y ) = [X ,Y ] = XY − YX , the commutator

• fermions: (X ,Y ) = X ,Y = XY + YX , theanti-commutator

• N = A∗A is number operator

• Ω is vacuum

• create n particles

ψn =1√n!

(A∗)n Ω

• Nψn = nψn

• bosons: n = 0, 1, 2, . . .

• fermions: n = 0, 1

Page 39: Fermions, Bosons and their Statistics - uni-osnabrueck.deFermions, Bosons and their Statistics Peter Hertel Fundamental particles Spin and statistics Many particles Gibbs state Fermions

Fermions,Bosons and

theirStatistics

Peter Hertel

Fundamentalparticles

Spin andstatistics

Many particles

Gibbs state

Fermions

Zerotemperature

White dwarfsand neutronstars

Bosons

Black bodyradiation

Bose-Einsteincondensation

Many states

• j labels one-particle states

• creators A∗j and annihilators Aj

• (Aj ,Ak) = (A∗j ,A∗k) = 0 and (Aj ,A

∗k) = δjk

• for fermions:

• A∗j A∗kΩ = −A∗kA∗j Ω

• Nj = A∗j Aj has eigenvalues 0 and 1, i.e.

• a state is occupied at most once

• note that [Nj ,Nk ] = 0

Page 40: Fermions, Bosons and their Statistics - uni-osnabrueck.deFermions, Bosons and their Statistics Peter Hertel Fundamental particles Spin and statistics Many particles Gibbs state Fermions

Fermions,Bosons and

theirStatistics

Peter Hertel

Fundamentalparticles

Spin andstatistics

Many particles

Gibbs state

Fermions

Zerotemperature

White dwarfsand neutronstars

Bosons

Black bodyradiation

Bose-Einsteincondensation

Many states

• j labels one-particle states

• creators A∗j and annihilators Aj

• (Aj ,Ak) = (A∗j ,A∗k) = 0 and (Aj ,A

∗k) = δjk

• for fermions:

• A∗j A∗kΩ = −A∗kA∗j Ω

• Nj = A∗j Aj has eigenvalues 0 and 1, i.e.

• a state is occupied at most once

• note that [Nj ,Nk ] = 0

Page 41: Fermions, Bosons and their Statistics - uni-osnabrueck.deFermions, Bosons and their Statistics Peter Hertel Fundamental particles Spin and statistics Many particles Gibbs state Fermions

Fermions,Bosons and

theirStatistics

Peter Hertel

Fundamentalparticles

Spin andstatistics

Many particles

Gibbs state

Fermions

Zerotemperature

White dwarfsand neutronstars

Bosons

Black bodyradiation

Bose-Einsteincondensation

Many states

• j labels one-particle states

• creators A∗j and annihilators Aj

• (Aj ,Ak) = (A∗j ,A∗k) = 0 and (Aj ,A

∗k) = δjk

• for fermions:

• A∗j A∗kΩ = −A∗kA∗j Ω

• Nj = A∗j Aj has eigenvalues 0 and 1, i.e.

• a state is occupied at most once

• note that [Nj ,Nk ] = 0

Page 42: Fermions, Bosons and their Statistics - uni-osnabrueck.deFermions, Bosons and their Statistics Peter Hertel Fundamental particles Spin and statistics Many particles Gibbs state Fermions

Fermions,Bosons and

theirStatistics

Peter Hertel

Fundamentalparticles

Spin andstatistics

Many particles

Gibbs state

Fermions

Zerotemperature

White dwarfsand neutronstars

Bosons

Black bodyradiation

Bose-Einsteincondensation

Many states

• j labels one-particle states

• creators A∗j and annihilators Aj

• (Aj ,Ak) = (A∗j ,A∗k) = 0 and (Aj ,A

∗k) = δjk

• for fermions:

• A∗j A∗kΩ = −A∗kA∗j Ω

• Nj = A∗j Aj has eigenvalues 0 and 1, i.e.

• a state is occupied at most once

• note that [Nj ,Nk ] = 0

Page 43: Fermions, Bosons and their Statistics - uni-osnabrueck.deFermions, Bosons and their Statistics Peter Hertel Fundamental particles Spin and statistics Many particles Gibbs state Fermions

Fermions,Bosons and

theirStatistics

Peter Hertel

Fundamentalparticles

Spin andstatistics

Many particles

Gibbs state

Fermions

Zerotemperature

White dwarfsand neutronstars

Bosons

Black bodyradiation

Bose-Einsteincondensation

Many states

• j labels one-particle states

• creators A∗j and annihilators Aj

• (Aj ,Ak) = (A∗j ,A∗k) = 0 and (Aj ,A

∗k) = δjk

• for fermions:

• A∗j A∗kΩ = −A∗kA∗j Ω

• Nj = A∗j Aj has eigenvalues 0 and 1, i.e.

• a state is occupied at most once

• note that [Nj ,Nk ] = 0

Page 44: Fermions, Bosons and their Statistics - uni-osnabrueck.deFermions, Bosons and their Statistics Peter Hertel Fundamental particles Spin and statistics Many particles Gibbs state Fermions

Fermions,Bosons and

theirStatistics

Peter Hertel

Fundamentalparticles

Spin andstatistics

Many particles

Gibbs state

Fermions

Zerotemperature

White dwarfsand neutronstars

Bosons

Black bodyradiation

Bose-Einsteincondensation

Many states

• j labels one-particle states

• creators A∗j and annihilators Aj

• (Aj ,Ak) = (A∗j ,A∗k) = 0 and (Aj ,A

∗k) = δjk

• for fermions:

• A∗j A∗kΩ = −A∗kA∗j Ω

• Nj = A∗j Aj has eigenvalues 0 and 1, i.e.

• a state is occupied at most once

• note that [Nj ,Nk ] = 0

Page 45: Fermions, Bosons and their Statistics - uni-osnabrueck.deFermions, Bosons and their Statistics Peter Hertel Fundamental particles Spin and statistics Many particles Gibbs state Fermions

Fermions,Bosons and

theirStatistics

Peter Hertel

Fundamentalparticles

Spin andstatistics

Many particles

Gibbs state

Fermions

Zerotemperature

White dwarfsand neutronstars

Bosons

Black bodyradiation

Bose-Einsteincondensation

Many states

• j labels one-particle states

• creators A∗j and annihilators Aj

• (Aj ,Ak) = (A∗j ,A∗k) = 0 and (Aj ,A

∗k) = δjk

• for fermions:

• A∗j A∗kΩ = −A∗kA∗j Ω

• Nj = A∗j Aj has eigenvalues 0 and 1, i.e.

• a state is occupied at most once

• note that [Nj ,Nk ] = 0

Page 46: Fermions, Bosons and their Statistics - uni-osnabrueck.deFermions, Bosons and their Statistics Peter Hertel Fundamental particles Spin and statistics Many particles Gibbs state Fermions

Fermions,Bosons and

theirStatistics

Peter Hertel

Fundamentalparticles

Spin andstatistics

Many particles

Gibbs state

Fermions

Zerotemperature

White dwarfsand neutronstars

Bosons

Black bodyradiation

Bose-Einsteincondensation

Many states

• j labels one-particle states

• creators A∗j and annihilators Aj

• (Aj ,Ak) = (A∗j ,A∗k) = 0 and (Aj ,A

∗k) = δjk

• for fermions:

• A∗j A∗kΩ = −A∗kA∗j Ω

• Nj = A∗j Aj has eigenvalues 0 and 1, i.e.

• a state is occupied at most once

• note that [Nj ,Nk ] = 0

Page 47: Fermions, Bosons and their Statistics - uni-osnabrueck.deFermions, Bosons and their Statistics Peter Hertel Fundamental particles Spin and statistics Many particles Gibbs state Fermions

Fermions,Bosons and

theirStatistics

Peter Hertel

Fundamentalparticles

Spin andstatistics

Many particles

Gibbs state

Fermions

Zerotemperature

White dwarfsand neutronstars

Bosons

Black bodyradiation

Bose-Einsteincondensation

Energy

• H =∑

j εj A∗j Aj +

∑jklm Vjklm A∗j A

∗kAlAm

• if interaction term can be neglected

• H =∑

j εj Nj

• examples are quasi-free electrons (hopping model) orphonons

• N =∑

j Nj is the particle number operator

• note that the number of particles in a system is not fixed(open system)

Page 48: Fermions, Bosons and their Statistics - uni-osnabrueck.deFermions, Bosons and their Statistics Peter Hertel Fundamental particles Spin and statistics Many particles Gibbs state Fermions

Fermions,Bosons and

theirStatistics

Peter Hertel

Fundamentalparticles

Spin andstatistics

Many particles

Gibbs state

Fermions

Zerotemperature

White dwarfsand neutronstars

Bosons

Black bodyradiation

Bose-Einsteincondensation

Energy

• H =∑

j εj A∗j Aj +

∑jklm Vjklm A∗j A

∗kAlAm

• if interaction term can be neglected

• H =∑

j εj Nj

• examples are quasi-free electrons (hopping model) orphonons

• N =∑

j Nj is the particle number operator

• note that the number of particles in a system is not fixed(open system)

Page 49: Fermions, Bosons and their Statistics - uni-osnabrueck.deFermions, Bosons and their Statistics Peter Hertel Fundamental particles Spin and statistics Many particles Gibbs state Fermions

Fermions,Bosons and

theirStatistics

Peter Hertel

Fundamentalparticles

Spin andstatistics

Many particles

Gibbs state

Fermions

Zerotemperature

White dwarfsand neutronstars

Bosons

Black bodyradiation

Bose-Einsteincondensation

Energy

• H =∑

j εj A∗j Aj +

∑jklm Vjklm A∗j A

∗kAlAm

• if interaction term can be neglected

• H =∑

j εj Nj

• examples are quasi-free electrons (hopping model) orphonons

• N =∑

j Nj is the particle number operator

• note that the number of particles in a system is not fixed(open system)

Page 50: Fermions, Bosons and their Statistics - uni-osnabrueck.deFermions, Bosons and their Statistics Peter Hertel Fundamental particles Spin and statistics Many particles Gibbs state Fermions

Fermions,Bosons and

theirStatistics

Peter Hertel

Fundamentalparticles

Spin andstatistics

Many particles

Gibbs state

Fermions

Zerotemperature

White dwarfsand neutronstars

Bosons

Black bodyradiation

Bose-Einsteincondensation

Energy

• H =∑

j εj A∗j Aj +

∑jklm Vjklm A∗j A

∗kAlAm

• if interaction term can be neglected

• H =∑

j εj Nj

• examples are quasi-free electrons (hopping model) orphonons

• N =∑

j Nj is the particle number operator

• note that the number of particles in a system is not fixed(open system)

Page 51: Fermions, Bosons and their Statistics - uni-osnabrueck.deFermions, Bosons and their Statistics Peter Hertel Fundamental particles Spin and statistics Many particles Gibbs state Fermions

Fermions,Bosons and

theirStatistics

Peter Hertel

Fundamentalparticles

Spin andstatistics

Many particles

Gibbs state

Fermions

Zerotemperature

White dwarfsand neutronstars

Bosons

Black bodyradiation

Bose-Einsteincondensation

Energy

• H =∑

j εj A∗j Aj +

∑jklm Vjklm A∗j A

∗kAlAm

• if interaction term can be neglected

• H =∑

j εj Nj

• examples are quasi-free electrons (hopping model) orphonons

• N =∑

j Nj is the particle number operator

• note that the number of particles in a system is not fixed(open system)

Page 52: Fermions, Bosons and their Statistics - uni-osnabrueck.deFermions, Bosons and their Statistics Peter Hertel Fundamental particles Spin and statistics Many particles Gibbs state Fermions

Fermions,Bosons and

theirStatistics

Peter Hertel

Fundamentalparticles

Spin andstatistics

Many particles

Gibbs state

Fermions

Zerotemperature

White dwarfsand neutronstars

Bosons

Black bodyradiation

Bose-Einsteincondensation

Energy

• H =∑

j εj A∗j Aj +

∑jklm Vjklm A∗j A

∗kAlAm

• if interaction term can be neglected

• H =∑

j εj Nj

• examples are quasi-free electrons (hopping model) orphonons

• N =∑

j Nj is the particle number operator

• note that the number of particles in a system is not fixed(open system)

Page 53: Fermions, Bosons and their Statistics - uni-osnabrueck.deFermions, Bosons and their Statistics Peter Hertel Fundamental particles Spin and statistics Many particles Gibbs state Fermions

Fermions,Bosons and

theirStatistics

Peter Hertel

Fundamentalparticles

Spin andstatistics

Many particles

Gibbs state

Fermions

Zerotemperature

White dwarfsand neutronstars

Bosons

Black bodyradiation

Bose-Einsteincondensation

Free energy

• The equilibrium (Gibbs) state of an open system is

G = e(F − H + µN)/kBT

• free energy F defined by trG = 1

• which gives

F = −kBT ln tr e(µN − H)/kBT

• temperature T defined by trGH = U = H

• chemical potential µ defined by trGN = N

• generalization to more than one species of particles isobvious

Page 54: Fermions, Bosons and their Statistics - uni-osnabrueck.deFermions, Bosons and their Statistics Peter Hertel Fundamental particles Spin and statistics Many particles Gibbs state Fermions

Fermions,Bosons and

theirStatistics

Peter Hertel

Fundamentalparticles

Spin andstatistics

Many particles

Gibbs state

Fermions

Zerotemperature

White dwarfsand neutronstars

Bosons

Black bodyradiation

Bose-Einsteincondensation

Free energy

• The equilibrium (Gibbs) state of an open system is

G = e(F − H + µN)/kBT

• free energy F defined by trG = 1

• which gives

F = −kBT ln tr e(µN − H)/kBT

• temperature T defined by trGH = U = H

• chemical potential µ defined by trGN = N

• generalization to more than one species of particles isobvious

Page 55: Fermions, Bosons and their Statistics - uni-osnabrueck.deFermions, Bosons and their Statistics Peter Hertel Fundamental particles Spin and statistics Many particles Gibbs state Fermions

Fermions,Bosons and

theirStatistics

Peter Hertel

Fundamentalparticles

Spin andstatistics

Many particles

Gibbs state

Fermions

Zerotemperature

White dwarfsand neutronstars

Bosons

Black bodyradiation

Bose-Einsteincondensation

Free energy

• The equilibrium (Gibbs) state of an open system is

G = e(F − H + µN)/kBT

• free energy F defined by trG = 1

• which gives

F = −kBT ln tr e(µN − H)/kBT

• temperature T defined by trGH = U = H

• chemical potential µ defined by trGN = N

• generalization to more than one species of particles isobvious

Page 56: Fermions, Bosons and their Statistics - uni-osnabrueck.deFermions, Bosons and their Statistics Peter Hertel Fundamental particles Spin and statistics Many particles Gibbs state Fermions

Fermions,Bosons and

theirStatistics

Peter Hertel

Fundamentalparticles

Spin andstatistics

Many particles

Gibbs state

Fermions

Zerotemperature

White dwarfsand neutronstars

Bosons

Black bodyradiation

Bose-Einsteincondensation

Free energy

• The equilibrium (Gibbs) state of an open system is

G = e(F − H + µN)/kBT

• free energy F defined by trG = 1

• which gives

F = −kBT ln tr e(µN − H)/kBT

• temperature T defined by trGH = U = H

• chemical potential µ defined by trGN = N

• generalization to more than one species of particles isobvious

Page 57: Fermions, Bosons and their Statistics - uni-osnabrueck.deFermions, Bosons and their Statistics Peter Hertel Fundamental particles Spin and statistics Many particles Gibbs state Fermions

Fermions,Bosons and

theirStatistics

Peter Hertel

Fundamentalparticles

Spin andstatistics

Many particles

Gibbs state

Fermions

Zerotemperature

White dwarfsand neutronstars

Bosons

Black bodyradiation

Bose-Einsteincondensation

Free energy

• The equilibrium (Gibbs) state of an open system is

G = e(F − H + µN)/kBT

• free energy F defined by trG = 1

• which gives

F = −kBT ln tr e(µN − H)/kBT

• temperature T defined by trGH = U = H

• chemical potential µ defined by trGN = N

• generalization to more than one species of particles isobvious

Page 58: Fermions, Bosons and their Statistics - uni-osnabrueck.deFermions, Bosons and their Statistics Peter Hertel Fundamental particles Spin and statistics Many particles Gibbs state Fermions

Fermions,Bosons and

theirStatistics

Peter Hertel

Fundamentalparticles

Spin andstatistics

Many particles

Gibbs state

Fermions

Zerotemperature

White dwarfsand neutronstars

Bosons

Black bodyradiation

Bose-Einsteincondensation

Free energy

• The equilibrium (Gibbs) state of an open system is

G = e(F − H + µN)/kBT

• free energy F defined by trG = 1

• which gives

F = −kBT ln tr e(µN − H)/kBT

• temperature T defined by trGH = U = H

• chemical potential µ defined by trGN = N

• generalization to more than one species of particles isobvious

Page 59: Fermions, Bosons and their Statistics - uni-osnabrueck.deFermions, Bosons and their Statistics Peter Hertel Fundamental particles Spin and statistics Many particles Gibbs state Fermions

Fermions,Bosons and

theirStatistics

Peter Hertel

Fundamentalparticles

Spin andstatistics

Many particles

Gibbs state

Fermions

Zerotemperature

White dwarfsand neutronstars

Bosons

Black bodyradiation

Bose-Einsteincondensation

Josiah Willard Gibbs, US American physicist, 1839-1903

Page 60: Fermions, Bosons and their Statistics - uni-osnabrueck.deFermions, Bosons and their Statistics Peter Hertel Fundamental particles Spin and statistics Many particles Gibbs state Fermions

Fermions,Bosons and

theirStatistics

Peter Hertel

Fundamentalparticles

Spin andstatistics

Many particles

Gibbs state

Fermions

Zerotemperature

White dwarfsand neutronstars

Bosons

Black bodyradiation

Bose-Einsteincondensation

Fermi-Dirac statistics

• because particle number operators commute

e(µN − H)/kBT =

∏j

e(µ− εj)Nj/kBT

• work out the trace, i. e. sum over eigenvalues n = 0, 1

tr e(µN − H)/kBT =

∏j

(1 + e

(µ− εj)/kBT)

• free energy

F = −kBT∑j

ln

(1 + e

(µ− εj)/kBT)

• in [ε, ε+ dε] there are V z(ε)dε single particle states

• one may write

F = −kBTV

∫dε z(ε) ln

(1 + e

(µ− ε)/kBT)

Page 61: Fermions, Bosons and their Statistics - uni-osnabrueck.deFermions, Bosons and their Statistics Peter Hertel Fundamental particles Spin and statistics Many particles Gibbs state Fermions

Fermions,Bosons and

theirStatistics

Peter Hertel

Fundamentalparticles

Spin andstatistics

Many particles

Gibbs state

Fermions

Zerotemperature

White dwarfsand neutronstars

Bosons

Black bodyradiation

Bose-Einsteincondensation

Fermi-Dirac statistics

• because particle number operators commute

e(µN − H)/kBT =

∏j

e(µ− εj)Nj/kBT

• work out the trace, i. e. sum over eigenvalues n = 0, 1

tr e(µN − H)/kBT =

∏j

(1 + e

(µ− εj)/kBT)

• free energy

F = −kBT∑j

ln

(1 + e

(µ− εj)/kBT)

• in [ε, ε+ dε] there are V z(ε)dε single particle states

• one may write

F = −kBTV

∫dε z(ε) ln

(1 + e

(µ− ε)/kBT)

Page 62: Fermions, Bosons and their Statistics - uni-osnabrueck.deFermions, Bosons and their Statistics Peter Hertel Fundamental particles Spin and statistics Many particles Gibbs state Fermions

Fermions,Bosons and

theirStatistics

Peter Hertel

Fundamentalparticles

Spin andstatistics

Many particles

Gibbs state

Fermions

Zerotemperature

White dwarfsand neutronstars

Bosons

Black bodyradiation

Bose-Einsteincondensation

Fermi-Dirac statistics

• because particle number operators commute

e(µN − H)/kBT =

∏j

e(µ− εj)Nj/kBT

• work out the trace, i. e. sum over eigenvalues n = 0, 1

tr e(µN − H)/kBT =

∏j

(1 + e

(µ− εj)/kBT)

• free energy

F = −kBT∑j

ln

(1 + e

(µ− εj)/kBT)

• in [ε, ε+ dε] there are V z(ε)dε single particle states

• one may write

F = −kBTV

∫dε z(ε) ln

(1 + e

(µ− ε)/kBT)

Page 63: Fermions, Bosons and their Statistics - uni-osnabrueck.deFermions, Bosons and their Statistics Peter Hertel Fundamental particles Spin and statistics Many particles Gibbs state Fermions

Fermions,Bosons and

theirStatistics

Peter Hertel

Fundamentalparticles

Spin andstatistics

Many particles

Gibbs state

Fermions

Zerotemperature

White dwarfsand neutronstars

Bosons

Black bodyradiation

Bose-Einsteincondensation

Fermi-Dirac statistics

• because particle number operators commute

e(µN − H)/kBT =

∏j

e(µ− εj)Nj/kBT

• work out the trace, i. e. sum over eigenvalues n = 0, 1

tr e(µN − H)/kBT =

∏j

(1 + e

(µ− εj)/kBT)

• free energy

F = −kBT∑j

ln

(1 + e

(µ− εj)/kBT)

• in [ε, ε+ dε] there are V z(ε) dε single particle states

• one may write

F = −kBTV

∫dε z(ε) ln

(1 + e

(µ− ε)/kBT)

Page 64: Fermions, Bosons and their Statistics - uni-osnabrueck.deFermions, Bosons and their Statistics Peter Hertel Fundamental particles Spin and statistics Many particles Gibbs state Fermions

Fermions,Bosons and

theirStatistics

Peter Hertel

Fundamentalparticles

Spin andstatistics

Many particles

Gibbs state

Fermions

Zerotemperature

White dwarfsand neutronstars

Bosons

Black bodyradiation

Bose-Einsteincondensation

Fermi-Dirac statistics

• because particle number operators commute

e(µN − H)/kBT =

∏j

e(µ− εj)Nj/kBT

• work out the trace, i. e. sum over eigenvalues n = 0, 1

tr e(µN − H)/kBT =

∏j

(1 + e

(µ− εj)/kBT)

• free energy

F = −kBT∑j

ln

(1 + e

(µ− εj)/kBT)

• in [ε, ε+ dε] there are V z(ε) dε single particle states

• one may write

F = −kBTV

∫dε z(ε) ln

(1 + e

(µ− ε)/kBT)

Page 65: Fermions, Bosons and their Statistics - uni-osnabrueck.deFermions, Bosons and their Statistics Peter Hertel Fundamental particles Spin and statistics Many particles Gibbs state Fermions

Fermions,Bosons and

theirStatistics

Peter Hertel

Fundamentalparticles

Spin andstatistics

Many particles

Gibbs state

Fermions

Zerotemperature

White dwarfsand neutronstars

Bosons

Black bodyradiation

Bose-Einsteincondensation

Enrico Fermi, Italian/USA physicist, 1901-1954

Page 66: Fermions, Bosons and their Statistics - uni-osnabrueck.deFermions, Bosons and their Statistics Peter Hertel Fundamental particles Spin and statistics Many particles Gibbs state Fermions

Fermions,Bosons and

theirStatistics

Peter Hertel

Fundamentalparticles

Spin andstatistics

Many particles

Gibbs state

Fermions

Zerotemperature

White dwarfsand neutronstars

Bosons

Black bodyradiation

Bose-Einsteincondensation

Paul Dirac, Britisch physicist, 1902-1984

Page 67: Fermions, Bosons and their Statistics - uni-osnabrueck.deFermions, Bosons and their Statistics Peter Hertel Fundamental particles Spin and statistics Many particles Gibbs state Fermions

Fermions,Bosons and

theirStatistics

Peter Hertel

Fundamentalparticles

Spin andstatistics

Many particles

Gibbs state

Fermions

Zerotemperature

White dwarfsand neutronstars

Bosons

Black bodyradiation

Bose-Einsteincondensation

Non-relativistic fermions

• sum over states (factor 2 for spin)∑j

= 2

∫d3x d3p

(2π~)3

• ε = p2/2m

• gives∑j

= V

∫dε z(ε)

= V1

π2

(2m

~2

)3/2 ∫dε√ε

Page 68: Fermions, Bosons and their Statistics - uni-osnabrueck.deFermions, Bosons and their Statistics Peter Hertel Fundamental particles Spin and statistics Many particles Gibbs state Fermions

Fermions,Bosons and

theirStatistics

Peter Hertel

Fundamentalparticles

Spin andstatistics

Many particles

Gibbs state

Fermions

Zerotemperature

White dwarfsand neutronstars

Bosons

Black bodyradiation

Bose-Einsteincondensation

Non-relativistic fermions

• sum over states (factor 2 for spin)∑j

= 2

∫d3x d3p

(2π~)3

• ε = p2/2m

• gives∑j

= V

∫dε z(ε)

= V1

π2

(2m

~2

)3/2 ∫dε√ε

Page 69: Fermions, Bosons and their Statistics - uni-osnabrueck.deFermions, Bosons and their Statistics Peter Hertel Fundamental particles Spin and statistics Many particles Gibbs state Fermions

Fermions,Bosons and

theirStatistics

Peter Hertel

Fundamentalparticles

Spin andstatistics

Many particles

Gibbs state

Fermions

Zerotemperature

White dwarfsand neutronstars

Bosons

Black bodyradiation

Bose-Einsteincondensation

Non-relativistic fermions

• sum over states (factor 2 for spin)∑j

= 2

∫d3x d3p

(2π~)3

• ε = p2/2m

• gives∑j

= V

∫dε z(ε)

= V1

π2

(2m

~2

)3/2 ∫dε√ε

Page 70: Fermions, Bosons and their Statistics - uni-osnabrueck.deFermions, Bosons and their Statistics Peter Hertel Fundamental particles Spin and statistics Many particles Gibbs state Fermions

Fermions,Bosons and

theirStatistics

Peter Hertel

Fundamentalparticles

Spin andstatistics

Many particles

Gibbs state

Fermions

Zerotemperature

White dwarfsand neutronstars

Bosons

Black bodyradiation

Bose-Einsteincondensation

Particle density and pressure

• recall

F = −kBTV

∫dε z(ε) ln

(1 + e

(µ− ε)/kBT)

• particle density is

n(T , µ) = − 1

V

∂F

∂µ

=

∫dε z(ε)

1

e(ε− µ)/kBT + 1

• pressure is

p = − ∂F∂V

= kBT

∫dε z(ε) ln

(1 + e

(µ− ε)/kBT)

=2

3

∫dε z(ε)

ε

e(ε− µ)/kBT + 1

Page 71: Fermions, Bosons and their Statistics - uni-osnabrueck.deFermions, Bosons and their Statistics Peter Hertel Fundamental particles Spin and statistics Many particles Gibbs state Fermions

Fermions,Bosons and

theirStatistics

Peter Hertel

Fundamentalparticles

Spin andstatistics

Many particles

Gibbs state

Fermions

Zerotemperature

White dwarfsand neutronstars

Bosons

Black bodyradiation

Bose-Einsteincondensation

Particle density and pressure

• recall

F = −kBTV

∫dε z(ε) ln

(1 + e

(µ− ε)/kBT)

• particle density is

n(T , µ) = − 1

V

∂F

∂µ

=

∫dε z(ε)

1

e(ε− µ)/kBT + 1

• pressure is

p = − ∂F∂V

= kBT

∫dε z(ε) ln

(1 + e

(µ− ε)/kBT)

=2

3

∫dε z(ε)

ε

e(ε− µ)/kBT + 1

Page 72: Fermions, Bosons and their Statistics - uni-osnabrueck.deFermions, Bosons and their Statistics Peter Hertel Fundamental particles Spin and statistics Many particles Gibbs state Fermions

Fermions,Bosons and

theirStatistics

Peter Hertel

Fundamentalparticles

Spin andstatistics

Many particles

Gibbs state

Fermions

Zerotemperature

White dwarfsand neutronstars

Bosons

Black bodyradiation

Bose-Einsteincondensation

Particle density and pressure

• recall

F = −kBTV

∫dε z(ε) ln

(1 + e

(µ− ε)/kBT)

• particle density is

n(T , µ) = − 1

V

∂F

∂µ

=

∫dε z(ε)

1

e(ε− µ)/kBT + 1

• pressure is

p = − ∂F∂V

= kBT

∫dε z(ε) ln

(1 + e

(µ− ε)/kBT)

=2

3

∫dε z(ε)

ε

e(ε− µ)/kBT + 1

Page 73: Fermions, Bosons and their Statistics - uni-osnabrueck.deFermions, Bosons and their Statistics Peter Hertel Fundamental particles Spin and statistics Many particles Gibbs state Fermions

Fermions,Bosons and

theirStatistics

Peter Hertel

Fundamentalparticles

Spin andstatistics

Many particles

Gibbs state

Fermions

Zerotemperature

White dwarfsand neutronstars

Bosons

Black bodyradiation

Bose-Einsteincondensation

Zero temperature

• if T → 01

e(ε− µ)/kBT + 1

= θ(µ− ε)

• particle density

n(0, µ) =

∫ µ

−∞dε z(ε)

• pressure

p(0, µ) =2

3

∫ µ

−∞dε z(ε) ε

• if particle density n is given, then

n = n(0, εF) =

∫ εF

−∞dε z(ε)

defines Fermi energy

Page 74: Fermions, Bosons and their Statistics - uni-osnabrueck.deFermions, Bosons and their Statistics Peter Hertel Fundamental particles Spin and statistics Many particles Gibbs state Fermions

Fermions,Bosons and

theirStatistics

Peter Hertel

Fundamentalparticles

Spin andstatistics

Many particles

Gibbs state

Fermions

Zerotemperature

White dwarfsand neutronstars

Bosons

Black bodyradiation

Bose-Einsteincondensation

Zero temperature

• if T → 01

e(ε− µ)/kBT + 1

= θ(µ− ε)

• particle density

n(0, µ) =

∫ µ

−∞dε z(ε)

• pressure

p(0, µ) =2

3

∫ µ

−∞dε z(ε) ε

• if particle density n is given, then

n = n(0, εF) =

∫ εF

−∞dε z(ε)

defines Fermi energy

Page 75: Fermions, Bosons and their Statistics - uni-osnabrueck.deFermions, Bosons and their Statistics Peter Hertel Fundamental particles Spin and statistics Many particles Gibbs state Fermions

Fermions,Bosons and

theirStatistics

Peter Hertel

Fundamentalparticles

Spin andstatistics

Many particles

Gibbs state

Fermions

Zerotemperature

White dwarfsand neutronstars

Bosons

Black bodyradiation

Bose-Einsteincondensation

Zero temperature

• if T → 01

e(ε− µ)/kBT + 1

= θ(µ− ε)

• particle density

n(0, µ) =

∫ µ

−∞dε z(ε)

• pressure

p(0, µ) =2

3

∫ µ

−∞dε z(ε) ε

• if particle density n is given, then

n = n(0, εF) =

∫ εF

−∞dε z(ε)

defines Fermi energy

Page 76: Fermions, Bosons and their Statistics - uni-osnabrueck.deFermions, Bosons and their Statistics Peter Hertel Fundamental particles Spin and statistics Many particles Gibbs state Fermions

Fermions,Bosons and

theirStatistics

Peter Hertel

Fundamentalparticles

Spin andstatistics

Many particles

Gibbs state

Fermions

Zerotemperature

White dwarfsand neutronstars

Bosons

Black bodyradiation

Bose-Einsteincondensation

Zero temperature

• if T → 01

e(ε− µ)/kBT + 1

= θ(µ− ε)

• particle density

n(0, µ) =

∫ µ

−∞dε z(ε)

• pressure

p(0, µ) =2

3

∫ µ

−∞dε z(ε) ε

• if particle density n is given, then

n = n(0, εF) =

∫ εF

−∞dε z(ε)

defines Fermi energy

Page 77: Fermions, Bosons and their Statistics - uni-osnabrueck.deFermions, Bosons and their Statistics Peter Hertel Fundamental particles Spin and statistics Many particles Gibbs state Fermions

Fermions,Bosons and

theirStatistics

Peter Hertel

Fundamentalparticles

Spin andstatistics

Many particles

Gibbs state

Fermions

Zerotemperature

White dwarfsand neutronstars

Bosons

Black bodyradiation

Bose-Einsteincondensation

Atoms and so forth

• Periodic system

• from small to huge molecules

• dielectrics, conductors, semiconductors, ferromagnets

• stability of normal matter

• stars can be stable even at T = 0

Page 78: Fermions, Bosons and their Statistics - uni-osnabrueck.deFermions, Bosons and their Statistics Peter Hertel Fundamental particles Spin and statistics Many particles Gibbs state Fermions

Fermions,Bosons and

theirStatistics

Peter Hertel

Fundamentalparticles

Spin andstatistics

Many particles

Gibbs state

Fermions

Zerotemperature

White dwarfsand neutronstars

Bosons

Black bodyradiation

Bose-Einsteincondensation

Atoms and so forth

• Periodic system

• from small to huge molecules

• dielectrics, conductors, semiconductors, ferromagnets

• stability of normal matter

• stars can be stable even at T = 0

Page 79: Fermions, Bosons and their Statistics - uni-osnabrueck.deFermions, Bosons and their Statistics Peter Hertel Fundamental particles Spin and statistics Many particles Gibbs state Fermions

Fermions,Bosons and

theirStatistics

Peter Hertel

Fundamentalparticles

Spin andstatistics

Many particles

Gibbs state

Fermions

Zerotemperature

White dwarfsand neutronstars

Bosons

Black bodyradiation

Bose-Einsteincondensation

Atoms and so forth

• Periodic system

• from small to huge molecules

• dielectrics, conductors, semiconductors, ferromagnets

• stability of normal matter

• stars can be stable even at T = 0

Page 80: Fermions, Bosons and their Statistics - uni-osnabrueck.deFermions, Bosons and their Statistics Peter Hertel Fundamental particles Spin and statistics Many particles Gibbs state Fermions

Fermions,Bosons and

theirStatistics

Peter Hertel

Fundamentalparticles

Spin andstatistics

Many particles

Gibbs state

Fermions

Zerotemperature

White dwarfsand neutronstars

Bosons

Black bodyradiation

Bose-Einsteincondensation

Atoms and so forth

• Periodic system

• from small to huge molecules

• dielectrics, conductors, semiconductors, ferromagnets

• stability of normal matter

• stars can be stable even at T = 0

Page 81: Fermions, Bosons and their Statistics - uni-osnabrueck.deFermions, Bosons and their Statistics Peter Hertel Fundamental particles Spin and statistics Many particles Gibbs state Fermions

Fermions,Bosons and

theirStatistics

Peter Hertel

Fundamentalparticles

Spin andstatistics

Many particles

Gibbs state

Fermions

Zerotemperature

White dwarfsand neutronstars

Bosons

Black bodyradiation

Bose-Einsteincondensation

Atoms and so forth

• Periodic system

• from small to huge molecules

• dielectrics, conductors, semiconductors, ferromagnets

• stability of normal matter

• stars can be stable even at T = 0

Page 82: Fermions, Bosons and their Statistics - uni-osnabrueck.deFermions, Bosons and their Statistics Peter Hertel Fundamental particles Spin and statistics Many particles Gibbs state Fermions

Fermions,Bosons and

theirStatistics

Peter Hertel

Fundamentalparticles

Spin andstatistics

Many particles

Gibbs state

Fermions

Zerotemperature

White dwarfsand neutronstars

Bosons

Black bodyradiation

Bose-Einsteincondensation

Hydrodynamic equilibrium

• The mass within a sphere of radius R is

M(r) = 4π

∫ r

0ds s2ρ(s)

• gravitational force per unit volume

f (r) = −G ρ(r)M(r)

r2

• pressure gradient and force must balance

p ′(r) = f (r)

• relate pressure with mass density

Page 83: Fermions, Bosons and their Statistics - uni-osnabrueck.deFermions, Bosons and their Statistics Peter Hertel Fundamental particles Spin and statistics Many particles Gibbs state Fermions

Fermions,Bosons and

theirStatistics

Peter Hertel

Fundamentalparticles

Spin andstatistics

Many particles

Gibbs state

Fermions

Zerotemperature

White dwarfsand neutronstars

Bosons

Black bodyradiation

Bose-Einsteincondensation

Hydrodynamic equilibrium

• The mass within a sphere of radius R is

M(r) = 4π

∫ r

0ds s2ρ(s)

• gravitational force per unit volume

f (r) = −G ρ(r)M(r)

r2

• pressure gradient and force must balance

p ′(r) = f (r)

• relate pressure with mass density

Page 84: Fermions, Bosons and their Statistics - uni-osnabrueck.deFermions, Bosons and their Statistics Peter Hertel Fundamental particles Spin and statistics Many particles Gibbs state Fermions

Fermions,Bosons and

theirStatistics

Peter Hertel

Fundamentalparticles

Spin andstatistics

Many particles

Gibbs state

Fermions

Zerotemperature

White dwarfsand neutronstars

Bosons

Black bodyradiation

Bose-Einsteincondensation

Hydrodynamic equilibrium

• The mass within a sphere of radius R is

M(r) = 4π

∫ r

0ds s2ρ(s)

• gravitational force per unit volume

f (r) = −G ρ(r)M(r)

r2

• pressure gradient and force must balance

p ′(r) = f (r)

• relate pressure with mass density

Page 85: Fermions, Bosons and their Statistics - uni-osnabrueck.deFermions, Bosons and their Statistics Peter Hertel Fundamental particles Spin and statistics Many particles Gibbs state Fermions

Fermions,Bosons and

theirStatistics

Peter Hertel

Fundamentalparticles

Spin andstatistics

Many particles

Gibbs state

Fermions

Zerotemperature

White dwarfsand neutronstars

Bosons

Black bodyradiation

Bose-Einsteincondensation

Hydrodynamic equilibrium

• The mass within a sphere of radius R is

M(r) = 4π

∫ r

0ds s2ρ(s)

• gravitational force per unit volume

f (r) = −G ρ(r)M(r)

r2

• pressure gradient and force must balance

p ′(r) = f (r)

• relate pressure with mass density

Page 86: Fermions, Bosons and their Statistics - uni-osnabrueck.deFermions, Bosons and their Statistics Peter Hertel Fundamental particles Spin and statistics Many particles Gibbs state Fermions

Fermions,Bosons and

theirStatistics

Peter Hertel

Fundamentalparticles

Spin andstatistics

Many particles

Gibbs state

Fermions

Zerotemperature

White dwarfsand neutronstars

Bosons

Black bodyradiation

Bose-Einsteincondensation

Equation of state

• electron gas at T = 0

• recall

z(ε) =1

π2

2m

~2

3/2√ε

• particle density

n(0, µ) =2

3π2

2m

~2

3/2

µ3/2

• pressure

p(0, µ) =4

15π2

2m

~2

3/2

µ5/2

• eliminate chemical potential

p = a~2

mn5/3 where a = 1.2058

• since one electron is related with two nucleons

p = a~2

me

ρ

2mp

5/3

Page 87: Fermions, Bosons and their Statistics - uni-osnabrueck.deFermions, Bosons and their Statistics Peter Hertel Fundamental particles Spin and statistics Many particles Gibbs state Fermions

Fermions,Bosons and

theirStatistics

Peter Hertel

Fundamentalparticles

Spin andstatistics

Many particles

Gibbs state

Fermions

Zerotemperature

White dwarfsand neutronstars

Bosons

Black bodyradiation

Bose-Einsteincondensation

Equation of state

• electron gas at T = 0

• recall

z(ε) =1

π2

2m

~2

3/2√ε

• particle density

n(0, µ) =2

3π2

2m

~2

3/2

µ3/2

• pressure

p(0, µ) =4

15π2

2m

~2

3/2

µ5/2

• eliminate chemical potential

p = a~2

mn5/3 where a = 1.2058

• since one electron is related with two nucleons

p = a~2

me

ρ

2mp

5/3

Page 88: Fermions, Bosons and their Statistics - uni-osnabrueck.deFermions, Bosons and their Statistics Peter Hertel Fundamental particles Spin and statistics Many particles Gibbs state Fermions

Fermions,Bosons and

theirStatistics

Peter Hertel

Fundamentalparticles

Spin andstatistics

Many particles

Gibbs state

Fermions

Zerotemperature

White dwarfsand neutronstars

Bosons

Black bodyradiation

Bose-Einsteincondensation

Equation of state

• electron gas at T = 0

• recall

z(ε) =1

π2

2m

~2

3/2√ε

• particle density

n(0, µ) =2

3π2

2m

~2

3/2

µ3/2

• pressure

p(0, µ) =4

15π2

2m

~2

3/2

µ5/2

• eliminate chemical potential

p = a~2

mn5/3 where a = 1.2058

• since one electron is related with two nucleons

p = a~2

me

ρ

2mp

5/3

Page 89: Fermions, Bosons and their Statistics - uni-osnabrueck.deFermions, Bosons and their Statistics Peter Hertel Fundamental particles Spin and statistics Many particles Gibbs state Fermions

Fermions,Bosons and

theirStatistics

Peter Hertel

Fundamentalparticles

Spin andstatistics

Many particles

Gibbs state

Fermions

Zerotemperature

White dwarfsand neutronstars

Bosons

Black bodyradiation

Bose-Einsteincondensation

Equation of state

• electron gas at T = 0

• recall

z(ε) =1

π2

2m

~2

3/2√ε

• particle density

n(0, µ) =2

3π2

2m

~2

3/2

µ3/2

• pressure

p(0, µ) =4

15π2

2m

~2

3/2

µ5/2

• eliminate chemical potential

p = a~2

mn5/3 where a = 1.2058

• since one electron is related with two nucleons

p = a~2

me

ρ

2mp

5/3

Page 90: Fermions, Bosons and their Statistics - uni-osnabrueck.deFermions, Bosons and their Statistics Peter Hertel Fundamental particles Spin and statistics Many particles Gibbs state Fermions

Fermions,Bosons and

theirStatistics

Peter Hertel

Fundamentalparticles

Spin andstatistics

Many particles

Gibbs state

Fermions

Zerotemperature

White dwarfsand neutronstars

Bosons

Black bodyradiation

Bose-Einsteincondensation

Equation of state

• electron gas at T = 0

• recall

z(ε) =1

π2

2m

~2

3/2√ε

• particle density

n(0, µ) =2

3π2

2m

~2

3/2

µ3/2

• pressure

p(0, µ) =4

15π2

2m

~2

3/2

µ5/2

• eliminate chemical potential

p = a~2

mn5/3 where a = 1.2058

• since one electron is related with two nucleons

p = a~2

me

ρ

2mp

5/3

Page 91: Fermions, Bosons and their Statistics - uni-osnabrueck.deFermions, Bosons and their Statistics Peter Hertel Fundamental particles Spin and statistics Many particles Gibbs state Fermions

Fermions,Bosons and

theirStatistics

Peter Hertel

Fundamentalparticles

Spin andstatistics

Many particles

Gibbs state

Fermions

Zerotemperature

White dwarfsand neutronstars

Bosons

Black bodyradiation

Bose-Einsteincondensation

Equation of state

• electron gas at T = 0

• recall

z(ε) =1

π2

2m

~2

3/2√ε

• particle density

n(0, µ) =2

3π2

2m

~2

3/2

µ3/2

• pressure

p(0, µ) =4

15π2

2m

~2

3/2

µ5/2

• eliminate chemical potential

p = a~2

mn5/3 where a = 1.2058

• since one electron is related with two nucleons

p = a~2

me

ρ

2mp

5/3

Page 92: Fermions, Bosons and their Statistics - uni-osnabrueck.deFermions, Bosons and their Statistics Peter Hertel Fundamental particles Spin and statistics Many particles Gibbs state Fermions

Fermions,Bosons and

theirStatistics

Peter Hertel

Fundamentalparticles

Spin andstatistics

Many particles

Gibbs state

Fermions

Zerotemperature

White dwarfsand neutronstars

Bosons

Black bodyradiation

Bose-Einsteincondensation

0 0.1 0.2 0.3 0.4 0.5 0.6 0.7 0.8 0.90

0.1

0.2

0.3

0.4

0.5

0.6

0.7

0.8

0.9

1

Pressure p (decreasing) and mass M (increasing) of a white dwarf vs. distance r

from the center in natural units. We have assumed zero temperature, two

nucleons per electron which are treated non-relativistically. r = 1 corresponds to

6500 km, M = 1 to 0.85 sun masses.

Page 93: Fermions, Bosons and their Statistics - uni-osnabrueck.deFermions, Bosons and their Statistics Peter Hertel Fundamental particles Spin and statistics Many particles Gibbs state Fermions

Fermions,Bosons and

theirStatistics

Peter Hertel

Fundamentalparticles

Spin andstatistics

Many particles

Gibbs state

Fermions

Zerotemperature

White dwarfsand neutronstars

Bosons

Black bodyradiation

Bose-Einsteincondensation

Crab nebula, the cloud of debris of the 1054 supernova

Page 94: Fermions, Bosons and their Statistics - uni-osnabrueck.deFermions, Bosons and their Statistics Peter Hertel Fundamental particles Spin and statistics Many particles Gibbs state Fermions

Fermions,Bosons and

theirStatistics

Peter Hertel

Fundamentalparticles

Spin andstatistics

Many particles

Gibbs state

Fermions

Zerotemperature

White dwarfsand neutronstars

Bosons

Black bodyradiation

Bose-Einsteincondensation

There is a neutron star (pulsar) at its center.

Page 95: Fermions, Bosons and their Statistics - uni-osnabrueck.deFermions, Bosons and their Statistics Peter Hertel Fundamental particles Spin and statistics Many particles Gibbs state Fermions

Fermions,Bosons and

theirStatistics

Peter Hertel

Fundamentalparticles

Spin andstatistics

Many particles

Gibbs state

Fermions

Zerotemperature

White dwarfsand neutronstars

Bosons

Black bodyradiation

Bose-Einsteincondensation

Jagadris Chandra Bose, Indian physicist, 1858-1937

Page 96: Fermions, Bosons and their Statistics - uni-osnabrueck.deFermions, Bosons and their Statistics Peter Hertel Fundamental particles Spin and statistics Many particles Gibbs state Fermions

Fermions,Bosons and

theirStatistics

Peter Hertel

Fundamentalparticles

Spin andstatistics

Many particles

Gibbs state

Fermions

Zerotemperature

White dwarfsand neutronstars

Bosons

Black bodyradiation

Bose-Einsteincondensation

Bosons

• bosons have integer spin or integer helicity

• such as the photon

• such as (qq) states - mesons

• or (ee) - Cooper pairs

• or (ppnn), the helium nucleus or helium atom

• or phonons, the quanta of lattice vibrations

Page 97: Fermions, Bosons and their Statistics - uni-osnabrueck.deFermions, Bosons and their Statistics Peter Hertel Fundamental particles Spin and statistics Many particles Gibbs state Fermions

Fermions,Bosons and

theirStatistics

Peter Hertel

Fundamentalparticles

Spin andstatistics

Many particles

Gibbs state

Fermions

Zerotemperature

White dwarfsand neutronstars

Bosons

Black bodyradiation

Bose-Einsteincondensation

Bosons

• bosons have integer spin or integer helicity

• such as the photon

• such as (qq) states - mesons

• or (ee) - Cooper pairs

• or (ppnn), the helium nucleus or helium atom

• or phonons, the quanta of lattice vibrations

Page 98: Fermions, Bosons and their Statistics - uni-osnabrueck.deFermions, Bosons and their Statistics Peter Hertel Fundamental particles Spin and statistics Many particles Gibbs state Fermions

Fermions,Bosons and

theirStatistics

Peter Hertel

Fundamentalparticles

Spin andstatistics

Many particles

Gibbs state

Fermions

Zerotemperature

White dwarfsand neutronstars

Bosons

Black bodyradiation

Bose-Einsteincondensation

Bosons

• bosons have integer spin or integer helicity

• such as the photon

• such as (qq) states - mesons

• or (ee) - Cooper pairs

• or (ppnn), the helium nucleus or helium atom

• or phonons, the quanta of lattice vibrations

Page 99: Fermions, Bosons and their Statistics - uni-osnabrueck.deFermions, Bosons and their Statistics Peter Hertel Fundamental particles Spin and statistics Many particles Gibbs state Fermions

Fermions,Bosons and

theirStatistics

Peter Hertel

Fundamentalparticles

Spin andstatistics

Many particles

Gibbs state

Fermions

Zerotemperature

White dwarfsand neutronstars

Bosons

Black bodyradiation

Bose-Einsteincondensation

Bosons

• bosons have integer spin or integer helicity

• such as the photon

• such as (qq) states - mesons

• or (ee) - Cooper pairs

• or (ppnn), the helium nucleus or helium atom

• or phonons, the quanta of lattice vibrations

Page 100: Fermions, Bosons and their Statistics - uni-osnabrueck.deFermions, Bosons and their Statistics Peter Hertel Fundamental particles Spin and statistics Many particles Gibbs state Fermions

Fermions,Bosons and

theirStatistics

Peter Hertel

Fundamentalparticles

Spin andstatistics

Many particles

Gibbs state

Fermions

Zerotemperature

White dwarfsand neutronstars

Bosons

Black bodyradiation

Bose-Einsteincondensation

Bosons

• bosons have integer spin or integer helicity

• such as the photon

• such as (qq) states - mesons

• or (ee) - Cooper pairs

• or (ppnn), the helium nucleus or helium atom

• or phonons, the quanta of lattice vibrations

Page 101: Fermions, Bosons and their Statistics - uni-osnabrueck.deFermions, Bosons and their Statistics Peter Hertel Fundamental particles Spin and statistics Many particles Gibbs state Fermions

Fermions,Bosons and

theirStatistics

Peter Hertel

Fundamentalparticles

Spin andstatistics

Many particles

Gibbs state

Fermions

Zerotemperature

White dwarfsand neutronstars

Bosons

Black bodyradiation

Bose-Einsteincondensation

Bosons

• bosons have integer spin or integer helicity

• such as the photon

• such as (qq) states - mesons

• or (ee) - Cooper pairs

• or (ppnn), the helium nucleus or helium atom

• or phonons, the quanta of lattice vibrations

Page 102: Fermions, Bosons and their Statistics - uni-osnabrueck.deFermions, Bosons and their Statistics Peter Hertel Fundamental particles Spin and statistics Many particles Gibbs state Fermions

Fermions,Bosons and

theirStatistics

Peter Hertel

Fundamentalparticles

Spin andstatistics

Many particles

Gibbs state

Fermions

Zerotemperature

White dwarfsand neutronstars

Bosons

Black bodyradiation

Bose-Einsteincondensation

Many bosons

• recall the spin/statistics theorem

• [Aj ,Ak ] = [A∗j ,A∗k ] = 0 - commutators!

• [Aj ,A∗k ] = δjk I

• Nj = A∗j ,Aj - number of particles in state j

• eigenvalues are n = 0, 1, 2, . . .

• work out the trace, i. e. sum over eigenvaluesn = 0, 1, 2, . . .

• N =∑

j Nj - total number of indistinguishable particles

Page 103: Fermions, Bosons and their Statistics - uni-osnabrueck.deFermions, Bosons and their Statistics Peter Hertel Fundamental particles Spin and statistics Many particles Gibbs state Fermions

Fermions,Bosons and

theirStatistics

Peter Hertel

Fundamentalparticles

Spin andstatistics

Many particles

Gibbs state

Fermions

Zerotemperature

White dwarfsand neutronstars

Bosons

Black bodyradiation

Bose-Einsteincondensation

Many bosons

• recall the spin/statistics theorem

• [Aj ,Ak ] = [A∗j ,A∗k ] = 0 - commutators!

• [Aj ,A∗k ] = δjk I

• Nj = A∗j ,Aj - number of particles in state j

• eigenvalues are n = 0, 1, 2, . . .

• work out the trace, i. e. sum over eigenvaluesn = 0, 1, 2, . . .

• N =∑

j Nj - total number of indistinguishable particles

Page 104: Fermions, Bosons and their Statistics - uni-osnabrueck.deFermions, Bosons and their Statistics Peter Hertel Fundamental particles Spin and statistics Many particles Gibbs state Fermions

Fermions,Bosons and

theirStatistics

Peter Hertel

Fundamentalparticles

Spin andstatistics

Many particles

Gibbs state

Fermions

Zerotemperature

White dwarfsand neutronstars

Bosons

Black bodyradiation

Bose-Einsteincondensation

Many bosons

• recall the spin/statistics theorem

• [Aj ,Ak ] = [A∗j ,A∗k ] = 0 - commutators!

• [Aj ,A∗k ] = δjk I

• Nj = A∗j ,Aj - number of particles in state j

• eigenvalues are n = 0, 1, 2, . . .

• work out the trace, i. e. sum over eigenvaluesn = 0, 1, 2, . . .

• N =∑

j Nj - total number of indistinguishable particles

Page 105: Fermions, Bosons and their Statistics - uni-osnabrueck.deFermions, Bosons and their Statistics Peter Hertel Fundamental particles Spin and statistics Many particles Gibbs state Fermions

Fermions,Bosons and

theirStatistics

Peter Hertel

Fundamentalparticles

Spin andstatistics

Many particles

Gibbs state

Fermions

Zerotemperature

White dwarfsand neutronstars

Bosons

Black bodyradiation

Bose-Einsteincondensation

Many bosons

• recall the spin/statistics theorem

• [Aj ,Ak ] = [A∗j ,A∗k ] = 0 - commutators!

• [Aj ,A∗k ] = δjk I

• Nj = A∗j ,Aj - number of particles in state j

• eigenvalues are n = 0, 1, 2, . . .

• work out the trace, i. e. sum over eigenvaluesn = 0, 1, 2, . . .

• N =∑

j Nj - total number of indistinguishable particles

Page 106: Fermions, Bosons and their Statistics - uni-osnabrueck.deFermions, Bosons and their Statistics Peter Hertel Fundamental particles Spin and statistics Many particles Gibbs state Fermions

Fermions,Bosons and

theirStatistics

Peter Hertel

Fundamentalparticles

Spin andstatistics

Many particles

Gibbs state

Fermions

Zerotemperature

White dwarfsand neutronstars

Bosons

Black bodyradiation

Bose-Einsteincondensation

Many bosons

• recall the spin/statistics theorem

• [Aj ,Ak ] = [A∗j ,A∗k ] = 0 - commutators!

• [Aj ,A∗k ] = δjk I

• Nj = A∗j ,Aj - number of particles in state j

• eigenvalues are n = 0, 1, 2, . . .

• work out the trace, i. e. sum over eigenvaluesn = 0, 1, 2, . . .

• N =∑

j Nj - total number of indistinguishable particles

Page 107: Fermions, Bosons and their Statistics - uni-osnabrueck.deFermions, Bosons and their Statistics Peter Hertel Fundamental particles Spin and statistics Many particles Gibbs state Fermions

Fermions,Bosons and

theirStatistics

Peter Hertel

Fundamentalparticles

Spin andstatistics

Many particles

Gibbs state

Fermions

Zerotemperature

White dwarfsand neutronstars

Bosons

Black bodyradiation

Bose-Einsteincondensation

Many bosons

• recall the spin/statistics theorem

• [Aj ,Ak ] = [A∗j ,A∗k ] = 0 - commutators!

• [Aj ,A∗k ] = δjk I

• Nj = A∗j ,Aj - number of particles in state j

• eigenvalues are n = 0, 1, 2, . . .

• work out the trace, i. e. sum over eigenvaluesn = 0, 1, 2, . . .

• N =∑

j Nj - total number of indistinguishable particles

Page 108: Fermions, Bosons and their Statistics - uni-osnabrueck.deFermions, Bosons and their Statistics Peter Hertel Fundamental particles Spin and statistics Many particles Gibbs state Fermions

Fermions,Bosons and

theirStatistics

Peter Hertel

Fundamentalparticles

Spin andstatistics

Many particles

Gibbs state

Fermions

Zerotemperature

White dwarfsand neutronstars

Bosons

Black bodyradiation

Bose-Einsteincondensation

Many bosons

• recall the spin/statistics theorem

• [Aj ,Ak ] = [A∗j ,A∗k ] = 0 - commutators!

• [Aj ,A∗k ] = δjk I

• Nj = A∗j ,Aj - number of particles in state j

• eigenvalues are n = 0, 1, 2, . . .

• work out the trace, i. e. sum over eigenvaluesn = 0, 1, 2, . . .

• N =∑

j Nj - total number of indistinguishable particles

Page 109: Fermions, Bosons and their Statistics - uni-osnabrueck.deFermions, Bosons and their Statistics Peter Hertel Fundamental particles Spin and statistics Many particles Gibbs state Fermions

Fermions,Bosons and

theirStatistics

Peter Hertel

Fundamentalparticles

Spin andstatistics

Many particles

Gibbs state

Fermions

Zerotemperature

White dwarfsand neutronstars

Bosons

Black bodyradiation

Bose-Einsteincondensation

Free energy

• energy is H =∑

j εj A∗j Aj + . . .

• free energy is

F = −kBT ln tr e(µN − H)/kBT

• Nj commute, therefore

e(µN − H)/kBT =

∏j

e(µ− εj)Nj/kBT

• work out the trace, i. e. sum over eigenvaluesn = 0, 1, 2, . . .

tr e(µ− εj)Nj/kBT =

∞∑n=0

e

(µ− εj)/kBTn

=1

1− e(µ− εj)/kBT

Page 110: Fermions, Bosons and their Statistics - uni-osnabrueck.deFermions, Bosons and their Statistics Peter Hertel Fundamental particles Spin and statistics Many particles Gibbs state Fermions

Fermions,Bosons and

theirStatistics

Peter Hertel

Fundamentalparticles

Spin andstatistics

Many particles

Gibbs state

Fermions

Zerotemperature

White dwarfsand neutronstars

Bosons

Black bodyradiation

Bose-Einsteincondensation

Free energy

• energy is H =∑

j εj A∗j Aj + . . .

• free energy is

F = −kBT ln tr e(µN − H)/kBT

• Nj commute, therefore

e(µN − H)/kBT =

∏j

e(µ− εj)Nj/kBT

• work out the trace, i. e. sum over eigenvaluesn = 0, 1, 2, . . .

tr e(µ− εj)Nj/kBT =

∞∑n=0

e

(µ− εj)/kBTn

=1

1− e(µ− εj)/kBT

Page 111: Fermions, Bosons and their Statistics - uni-osnabrueck.deFermions, Bosons and their Statistics Peter Hertel Fundamental particles Spin and statistics Many particles Gibbs state Fermions

Fermions,Bosons and

theirStatistics

Peter Hertel

Fundamentalparticles

Spin andstatistics

Many particles

Gibbs state

Fermions

Zerotemperature

White dwarfsand neutronstars

Bosons

Black bodyradiation

Bose-Einsteincondensation

Free energy

• energy is H =∑

j εj A∗j Aj + . . .

• free energy is

F = −kBT ln tr e(µN − H)/kBT

• Nj commute, therefore

e(µN − H)/kBT =

∏j

e(µ− εj)Nj/kBT

• work out the trace, i. e. sum over eigenvaluesn = 0, 1, 2, . . .

tr e(µ− εj)Nj/kBT =

∞∑n=0

e

(µ− εj)/kBTn

=1

1− e(µ− εj)/kBT

Page 112: Fermions, Bosons and their Statistics - uni-osnabrueck.deFermions, Bosons and their Statistics Peter Hertel Fundamental particles Spin and statistics Many particles Gibbs state Fermions

Fermions,Bosons and

theirStatistics

Peter Hertel

Fundamentalparticles

Spin andstatistics

Many particles

Gibbs state

Fermions

Zerotemperature

White dwarfsand neutronstars

Bosons

Black bodyradiation

Bose-Einsteincondensation

Free energy

• energy is H =∑

j εj A∗j Aj + . . .

• free energy is

F = −kBT ln tr e(µN − H)/kBT

• Nj commute, therefore

e(µN − H)/kBT =

∏j

e(µ− εj)Nj/kBT

• work out the trace, i. e. sum over eigenvaluesn = 0, 1, 2, . . .

tr e(µ− εj)Nj/kBT =

∞∑n=0

e

(µ− εj)/kBTn

=1

1− e(µ− εj)/kBT

Page 113: Fermions, Bosons and their Statistics - uni-osnabrueck.deFermions, Bosons and their Statistics Peter Hertel Fundamental particles Spin and statistics Many particles Gibbs state Fermions

Fermions,Bosons and

theirStatistics

Peter Hertel

Fundamentalparticles

Spin andstatistics

Many particles

Gibbs state

Fermions

Zerotemperature

White dwarfsand neutronstars

Bosons

Black bodyradiation

Bose-Einsteincondensation

Free energy ctd.

• the free energy of a boson gas is

F = kBT∑j

ln

(1− e

(µ− εj)/kBT)

= kBT V

∫dε z(ε) ln

(1− e

(µ− ε)/kBT)

• compare with the free energy of a fermi gas

F = −kBT V

∫dε z(ε) ln

(1 + e

(µ− ε)/kBT)

• recall spin/statistics theorem: again the +/− difference

Page 114: Fermions, Bosons and their Statistics - uni-osnabrueck.deFermions, Bosons and their Statistics Peter Hertel Fundamental particles Spin and statistics Many particles Gibbs state Fermions

Fermions,Bosons and

theirStatistics

Peter Hertel

Fundamentalparticles

Spin andstatistics

Many particles

Gibbs state

Fermions

Zerotemperature

White dwarfsand neutronstars

Bosons

Black bodyradiation

Bose-Einsteincondensation

Free energy ctd.

• the free energy of a boson gas is

F = kBT∑j

ln

(1− e

(µ− εj)/kBT)

= kBT V

∫dε z(ε) ln

(1− e

(µ− ε)/kBT)

• compare with the free energy of a fermi gas

F = −kBT V

∫dε z(ε) ln

(1 + e

(µ− ε)/kBT)

• recall spin/statistics theorem: again the +/− difference

Page 115: Fermions, Bosons and their Statistics - uni-osnabrueck.deFermions, Bosons and their Statistics Peter Hertel Fundamental particles Spin and statistics Many particles Gibbs state Fermions

Fermions,Bosons and

theirStatistics

Peter Hertel

Fundamentalparticles

Spin andstatistics

Many particles

Gibbs state

Fermions

Zerotemperature

White dwarfsand neutronstars

Bosons

Black bodyradiation

Bose-Einsteincondensation

Free energy ctd.

• the free energy of a boson gas is

F = kBT∑j

ln

(1− e

(µ− εj)/kBT)

= kBT V

∫dε z(ε) ln

(1− e

(µ− ε)/kBT)

• compare with the free energy of a fermi gas

F = −kBT V

∫dε z(ε) ln

(1 + e

(µ− ε)/kBT)

• recall spin/statistics theorem: again the +/− difference

Page 116: Fermions, Bosons and their Statistics - uni-osnabrueck.deFermions, Bosons and their Statistics Peter Hertel Fundamental particles Spin and statistics Many particles Gibbs state Fermions

Fermions,Bosons and

theirStatistics

Peter Hertel

Fundamentalparticles

Spin andstatistics

Many particles

Gibbs state

Fermions

Zerotemperature

White dwarfsand neutronstars

Bosons

Black bodyradiation

Bose-Einsteincondensation

Black body radiation

• photon energy is ~ω = pc

• density of states can be read off from

2

∫d3x d3p

(2π~)3= V

∫dω ω2

π2c3

• µ = 0

• black body free energy is

F = kBT V

∫ ∞0

dω ω2

π2c3ln

(1− e

−~ω/kBT)

• internal energy U

• U = F + TS = F − T∂F/∂T

• Planck’s formula

U = V

∫ ∞0

dω ω2

π2c3~ω

e~ω/kBT − 1

Page 117: Fermions, Bosons and their Statistics - uni-osnabrueck.deFermions, Bosons and their Statistics Peter Hertel Fundamental particles Spin and statistics Many particles Gibbs state Fermions

Fermions,Bosons and

theirStatistics

Peter Hertel

Fundamentalparticles

Spin andstatistics

Many particles

Gibbs state

Fermions

Zerotemperature

White dwarfsand neutronstars

Bosons

Black bodyradiation

Bose-Einsteincondensation

Black body radiation

• photon energy is ~ω = pc

• density of states can be read off from

2

∫d3x d3p

(2π~)3= V

∫dω ω2

π2c3

• µ = 0

• black body free energy is

F = kBT V

∫ ∞0

dω ω2

π2c3ln

(1− e

−~ω/kBT)

• internal energy U

• U = F + TS = F − T∂F/∂T

• Planck’s formula

U = V

∫ ∞0

dω ω2

π2c3~ω

e~ω/kBT − 1

Page 118: Fermions, Bosons and their Statistics - uni-osnabrueck.deFermions, Bosons and their Statistics Peter Hertel Fundamental particles Spin and statistics Many particles Gibbs state Fermions

Fermions,Bosons and

theirStatistics

Peter Hertel

Fundamentalparticles

Spin andstatistics

Many particles

Gibbs state

Fermions

Zerotemperature

White dwarfsand neutronstars

Bosons

Black bodyradiation

Bose-Einsteincondensation

Black body radiation

• photon energy is ~ω = pc

• density of states can be read off from

2

∫d3x d3p

(2π~)3= V

∫dω ω2

π2c3

• µ = 0

• black body free energy is

F = kBT V

∫ ∞0

dω ω2

π2c3ln

(1− e

−~ω/kBT)

• internal energy U

• U = F + TS = F − T∂F/∂T

• Planck’s formula

U = V

∫ ∞0

dω ω2

π2c3~ω

e~ω/kBT − 1

Page 119: Fermions, Bosons and their Statistics - uni-osnabrueck.deFermions, Bosons and their Statistics Peter Hertel Fundamental particles Spin and statistics Many particles Gibbs state Fermions

Fermions,Bosons and

theirStatistics

Peter Hertel

Fundamentalparticles

Spin andstatistics

Many particles

Gibbs state

Fermions

Zerotemperature

White dwarfsand neutronstars

Bosons

Black bodyradiation

Bose-Einsteincondensation

Black body radiation

• photon energy is ~ω = pc

• density of states can be read off from

2

∫d3x d3p

(2π~)3= V

∫dω ω2

π2c3

• µ = 0

• black body free energy is

F = kBT V

∫ ∞0

dω ω2

π2c3ln

(1− e

−~ω/kBT)

• internal energy U

• U = F + TS = F − T∂F/∂T

• Planck’s formula

U = V

∫ ∞0

dω ω2

π2c3~ω

e~ω/kBT − 1

Page 120: Fermions, Bosons and their Statistics - uni-osnabrueck.deFermions, Bosons and their Statistics Peter Hertel Fundamental particles Spin and statistics Many particles Gibbs state Fermions

Fermions,Bosons and

theirStatistics

Peter Hertel

Fundamentalparticles

Spin andstatistics

Many particles

Gibbs state

Fermions

Zerotemperature

White dwarfsand neutronstars

Bosons

Black bodyradiation

Bose-Einsteincondensation

Black body radiation

• photon energy is ~ω = pc

• density of states can be read off from

2

∫d3x d3p

(2π~)3= V

∫dω ω2

π2c3

• µ = 0

• black body free energy is

F = kBT V

∫ ∞0

dω ω2

π2c3ln

(1− e

−~ω/kBT)

• internal energy U

• U = F + TS = F − T∂F/∂T

• Planck’s formula

U = V

∫ ∞0

dω ω2

π2c3~ω

e~ω/kBT − 1

Page 121: Fermions, Bosons and their Statistics - uni-osnabrueck.deFermions, Bosons and their Statistics Peter Hertel Fundamental particles Spin and statistics Many particles Gibbs state Fermions

Fermions,Bosons and

theirStatistics

Peter Hertel

Fundamentalparticles

Spin andstatistics

Many particles

Gibbs state

Fermions

Zerotemperature

White dwarfsand neutronstars

Bosons

Black bodyradiation

Bose-Einsteincondensation

Black body radiation

• photon energy is ~ω = pc

• density of states can be read off from

2

∫d3x d3p

(2π~)3= V

∫dω ω2

π2c3

• µ = 0

• black body free energy is

F = kBT V

∫ ∞0

dω ω2

π2c3ln

(1− e

−~ω/kBT)

• internal energy U

• U = F + TS = F − T∂F/∂T

• Planck’s formula

U = V

∫ ∞0

dω ω2

π2c3~ω

e~ω/kBT − 1

Page 122: Fermions, Bosons and their Statistics - uni-osnabrueck.deFermions, Bosons and their Statistics Peter Hertel Fundamental particles Spin and statistics Many particles Gibbs state Fermions

Fermions,Bosons and

theirStatistics

Peter Hertel

Fundamentalparticles

Spin andstatistics

Many particles

Gibbs state

Fermions

Zerotemperature

White dwarfsand neutronstars

Bosons

Black bodyradiation

Bose-Einsteincondensation

Max Planck, German physicist, 1858-1947

Page 123: Fermions, Bosons and their Statistics - uni-osnabrueck.deFermions, Bosons and their Statistics Peter Hertel Fundamental particles Spin and statistics Many particles Gibbs state Fermions

Fermions,Bosons and

theirStatistics

Peter Hertel

Fundamentalparticles

Spin andstatistics

Many particles

Gibbs state

Fermions

Zerotemperature

White dwarfsand neutronstars

Bosons

Black bodyradiation

Bose-Einsteincondensation

Particle density

• recall∞∑n=0

en(µ− εj)/kBT =

1

1− e(µ− εj)/kBT

• valid only if µ < min εj = 0

• −∂F/∂µ = N is average particle number

• the average particle density n is therefore

n(T , µ) =

∫ ∞0

dε z(ε)1

e(ε− µ)/kBT − 1

• n(T , 0) is maximal density:

nmax(T ) =

∫ ∞0

dε z(ε)1

eε/kBT − 1

Page 124: Fermions, Bosons and their Statistics - uni-osnabrueck.deFermions, Bosons and their Statistics Peter Hertel Fundamental particles Spin and statistics Many particles Gibbs state Fermions

Fermions,Bosons and

theirStatistics

Peter Hertel

Fundamentalparticles

Spin andstatistics

Many particles

Gibbs state

Fermions

Zerotemperature

White dwarfsand neutronstars

Bosons

Black bodyradiation

Bose-Einsteincondensation

Particle density

• recall∞∑n=0

en(µ− εj)/kBT =

1

1− e(µ− εj)/kBT

• valid only if µ < min εj = 0

• −∂F/∂µ = N is average particle number

• the average particle density n is therefore

n(T , µ) =

∫ ∞0

dε z(ε)1

e(ε− µ)/kBT − 1

• n(T , 0) is maximal density:

nmax(T ) =

∫ ∞0

dε z(ε)1

eε/kBT − 1

Page 125: Fermions, Bosons and their Statistics - uni-osnabrueck.deFermions, Bosons and their Statistics Peter Hertel Fundamental particles Spin and statistics Many particles Gibbs state Fermions

Fermions,Bosons and

theirStatistics

Peter Hertel

Fundamentalparticles

Spin andstatistics

Many particles

Gibbs state

Fermions

Zerotemperature

White dwarfsand neutronstars

Bosons

Black bodyradiation

Bose-Einsteincondensation

Particle density

• recall∞∑n=0

en(µ− εj)/kBT =

1

1− e(µ− εj)/kBT

• valid only if µ < min εj = 0

• −∂F/∂µ = N is average particle number

• the average particle density n is therefore

n(T , µ) =

∫ ∞0

dε z(ε)1

e(ε− µ)/kBT − 1

• n(T , 0) is maximal density:

nmax(T ) =

∫ ∞0

dε z(ε)1

eε/kBT − 1

Page 126: Fermions, Bosons and their Statistics - uni-osnabrueck.deFermions, Bosons and their Statistics Peter Hertel Fundamental particles Spin and statistics Many particles Gibbs state Fermions

Fermions,Bosons and

theirStatistics

Peter Hertel

Fundamentalparticles

Spin andstatistics

Many particles

Gibbs state

Fermions

Zerotemperature

White dwarfsand neutronstars

Bosons

Black bodyradiation

Bose-Einsteincondensation

Particle density

• recall∞∑n=0

en(µ− εj)/kBT =

1

1− e(µ− εj)/kBT

• valid only if µ < min εj = 0

• −∂F/∂µ = N is average particle number

• the average particle density n is therefore

n(T , µ) =

∫ ∞0

dε z(ε)1

e(ε− µ)/kBT − 1

• n(T , 0) is maximal density:

nmax(T ) =

∫ ∞0

dε z(ε)1

eε/kBT − 1

Page 127: Fermions, Bosons and their Statistics - uni-osnabrueck.deFermions, Bosons and their Statistics Peter Hertel Fundamental particles Spin and statistics Many particles Gibbs state Fermions

Fermions,Bosons and

theirStatistics

Peter Hertel

Fundamentalparticles

Spin andstatistics

Many particles

Gibbs state

Fermions

Zerotemperature

White dwarfsand neutronstars

Bosons

Black bodyradiation

Bose-Einsteincondensation

Particle density

• recall∞∑n=0

en(µ− εj)/kBT =

1

1− e(µ− εj)/kBT

• valid only if µ < min εj = 0

• −∂F/∂µ = N is average particle number

• the average particle density n is therefore

n(T , µ) =

∫ ∞0

dε z(ε)1

e(ε− µ)/kBT − 1

• n(T , 0) is maximal density:

nmax(T ) =

∫ ∞0

dε z(ε)1

eε/kBT − 1

Page 128: Fermions, Bosons and their Statistics - uni-osnabrueck.deFermions, Bosons and their Statistics Peter Hertel Fundamental particles Spin and statistics Many particles Gibbs state Fermions

Fermions,Bosons and

theirStatistics

Peter Hertel

Fundamentalparticles

Spin andstatistics

Many particles

Gibbs state

Fermions

Zerotemperature

White dwarfsand neutronstars

Bosons

Black bodyradiation

Bose-Einsteincondensation

Bose-Einstein condensation

• If T decreases, so does nmax(T )

• if n is given, there is a temperature Tc such that

nmax(Tc) = n

• for even lower temperature, only a fraction of the particlesare in thermal equilibrium

• the rest is in the multiply occupied ground state

• supra-fluidity

• superconductivity

• light

Page 129: Fermions, Bosons and their Statistics - uni-osnabrueck.deFermions, Bosons and their Statistics Peter Hertel Fundamental particles Spin and statistics Many particles Gibbs state Fermions

Fermions,Bosons and

theirStatistics

Peter Hertel

Fundamentalparticles

Spin andstatistics

Many particles

Gibbs state

Fermions

Zerotemperature

White dwarfsand neutronstars

Bosons

Black bodyradiation

Bose-Einsteincondensation

Bose-Einstein condensation

• If T decreases, so does nmax(T )

• if n is given, there is a temperature Tc such that

nmax(Tc) = n

• for even lower temperature, only a fraction of the particlesare in thermal equilibrium

• the rest is in the multiply occupied ground state

• supra-fluidity

• superconductivity

• light

Page 130: Fermions, Bosons and their Statistics - uni-osnabrueck.deFermions, Bosons and their Statistics Peter Hertel Fundamental particles Spin and statistics Many particles Gibbs state Fermions

Fermions,Bosons and

theirStatistics

Peter Hertel

Fundamentalparticles

Spin andstatistics

Many particles

Gibbs state

Fermions

Zerotemperature

White dwarfsand neutronstars

Bosons

Black bodyradiation

Bose-Einsteincondensation

Bose-Einstein condensation

• If T decreases, so does nmax(T )

• if n is given, there is a temperature Tc such that

nmax(Tc) = n

• for even lower temperature, only a fraction of the particlesare in thermal equilibrium

• the rest is in the multiply occupied ground state

• supra-fluidity

• superconductivity

• light

Page 131: Fermions, Bosons and their Statistics - uni-osnabrueck.deFermions, Bosons and their Statistics Peter Hertel Fundamental particles Spin and statistics Many particles Gibbs state Fermions

Fermions,Bosons and

theirStatistics

Peter Hertel

Fundamentalparticles

Spin andstatistics

Many particles

Gibbs state

Fermions

Zerotemperature

White dwarfsand neutronstars

Bosons

Black bodyradiation

Bose-Einsteincondensation

Bose-Einstein condensation

• If T decreases, so does nmax(T )

• if n is given, there is a temperature Tc such that

nmax(Tc) = n

• for even lower temperature, only a fraction of the particlesare in thermal equilibrium

• the rest is in the multiply occupied ground state

• supra-fluidity

• superconductivity

• light

Page 132: Fermions, Bosons and their Statistics - uni-osnabrueck.deFermions, Bosons and their Statistics Peter Hertel Fundamental particles Spin and statistics Many particles Gibbs state Fermions

Fermions,Bosons and

theirStatistics

Peter Hertel

Fundamentalparticles

Spin andstatistics

Many particles

Gibbs state

Fermions

Zerotemperature

White dwarfsand neutronstars

Bosons

Black bodyradiation

Bose-Einsteincondensation

Bose-Einstein condensation

• If T decreases, so does nmax(T )

• if n is given, there is a temperature Tc such that

nmax(Tc) = n

• for even lower temperature, only a fraction of the particlesare in thermal equilibrium

• the rest is in the multiply occupied ground state

• supra-fluidity

• superconductivity

• light

Page 133: Fermions, Bosons and their Statistics - uni-osnabrueck.deFermions, Bosons and their Statistics Peter Hertel Fundamental particles Spin and statistics Many particles Gibbs state Fermions

Fermions,Bosons and

theirStatistics

Peter Hertel

Fundamentalparticles

Spin andstatistics

Many particles

Gibbs state

Fermions

Zerotemperature

White dwarfsand neutronstars

Bosons

Black bodyradiation

Bose-Einsteincondensation

Bose-Einstein condensation

• If T decreases, so does nmax(T )

• if n is given, there is a temperature Tc such that

nmax(Tc) = n

• for even lower temperature, only a fraction of the particlesare in thermal equilibrium

• the rest is in the multiply occupied ground state

• supra-fluidity

• superconductivity

• light

Page 134: Fermions, Bosons and their Statistics - uni-osnabrueck.deFermions, Bosons and their Statistics Peter Hertel Fundamental particles Spin and statistics Many particles Gibbs state Fermions

Fermions,Bosons and

theirStatistics

Peter Hertel

Fundamentalparticles

Spin andstatistics

Many particles

Gibbs state

Fermions

Zerotemperature

White dwarfsand neutronstars

Bosons

Black bodyradiation

Bose-Einsteincondensation

Bose-Einstein condensation

• If T decreases, so does nmax(T )

• if n is given, there is a temperature Tc such that

nmax(Tc) = n

• for even lower temperature, only a fraction of the particlesare in thermal equilibrium

• the rest is in the multiply occupied ground state

• supra-fluidity

• superconductivity

• light

Page 135: Fermions, Bosons and their Statistics - uni-osnabrueck.deFermions, Bosons and their Statistics Peter Hertel Fundamental particles Spin and statistics Many particles Gibbs state Fermions

Fermions,Bosons and

theirStatistics

Peter Hertel

Fundamentalparticles

Spin andstatistics

Many particles

Gibbs state

Fermions

Zerotemperature

White dwarfsand neutronstars

Bosons

Black bodyradiation

Bose-Einsteincondensation

Albert Einstein, German physicist, 1879-1955