June 27, 2015Lynn Cominsky1 Introduction to Particle Physics Professor Lynn Cominsky.
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Transcript of June 27, 2015Lynn Cominsky1 Introduction to Particle Physics Professor Lynn Cominsky.
April 18, 2023 Lynn Cominsky 4
Big Bang Revisited
Extrapolating back in time, we conclude that the Universe must have begun as a singularity – a place where the laws of physics and even space and time break down
However, our theories of space and time break down before the singularity at a time known as the Planck time
The Planck scale refers to the limits of mass, length, temperature and time that are what can be measured using the Uncertainty principle
April 18, 2023 Lynn Cominsky 5
Planck scale activity
The goal of this activity is to calculate the Planck mass, length, time and energy.
Remember
Uncertainty Principle x p ≥ h/2
Uncertainty Principle E t ≥ h/2
April 18, 2023 Lynn Cominsky 6
Unified Forces
The 4 forces are all unified (and therefore symmetric) at the Planck scale energy
Planck scale
The phase transition which splits off the strong nuclear force is what triggers inflation
April 18, 2023 Lynn Cominsky 7
The Vacuum Era Planck era
10-43 s after the Big Bang Temperature (kT) ~1019 GeV Beginning of time – time and space are no longer
separate entities Emergence of spacetime
Inflationary era < 10-10 s, kT ~ 100 GeV Vacuum energy dominates, driving Universe to
enormous size Fluctuations may be formed that eventually turn
into large scale structure
April 18, 2023 Lynn Cominsky 9
Radiation Era
Creation of Light>10-36 s after Big Bang - kT ~ 100 GeVVacuum energy turns into light, and equal
amounts of matter vs. anti-matterGravitational attraction beginsBackground radiation energy originatesDark matter may be formed
April 18, 2023 Lynn Cominsky 10
Radiation Era Creation of Baryonic Matter (Baryogenesis)
>10-36 s after Big Bang Temperature (kT) ~ 100 GeV A small excess of quarks and electrons is formed
(compared to anti-quarks and anti-electrons)
Electroweak (Unification) Era 10-10 s after the Big Bang, kT ~ 100 GeV Forces and matter become distinguishable forms of
energy with different behavior Masses of particles are defined May include baryogenesis
April 18, 2023 Lynn Cominsky 11
Radiation Era Strong Era
10-4 s after the Big Bang - kT~ 0.2 Gev Quark soup turns into neutrons and protons Dark matter may be formed
Electroweak Decoupling 1 s after the Big Bang - kT ~ 1 MeV Neutrons and protons no longer interchange
(leaving 7 p for each n) Cosmic neutrino background is formed Electrons and positrons annihilate, adding energy
to the cosmic background radiation, and an excess of electrons
April 18, 2023 Lynn Cominsky 12
Radiation Era Creation of light element nuclei
100 s after the Big Bang – kT ~ 0.1 MeV Nucleosynthesis begins as neutrons and protons
are cool enough to stick together to form Helium, some Deuterium, and a little bit of Lithium
Precise elemental abundances are established
Radiation Decoupling 1 month after the Big Bang – kT ~ 500 eV Interactions between matter and radiation are
fewer and farther between Blackbody background spectrum is determined
April 18, 2023 Lynn Cominsky 14
Atomic Particles
Atoms are made of protons, neutrons and electrons
99.999999999999% of the atom is empty space Electrons have locations
described by probability functions
Nuclei have protons and neutrons
nucleus
mp = 1836 me
April 18, 2023 Lynn Cominsky 15
Leptons An electron is the most common example of a lepton
– particles which appear pointlike Neutrinos are also leptons There are 3 generations of leptons, each has a
massive particle and an associated neutrino Each lepton also has an anti-lepton (for example the
electron and positron) Heavier leptons decay into lighter leptons plus
neutrinos (but lepton number must be conserved in these decays)
Lepton number: =+1 for leptons, -1 for anti-leptons, and 0 for non-leptons
April 18, 2023 Lynn Cominsky 16
Types of Leptons
Lepton Charge
Mass (GeV/c2)
Electron neutrino
0 0
Electron -1 0.000511
Muon neutrino
0 0
Muon -1 0.106
Tau neutrino
0 0
Tau -1 175
April 18, 2023 Lynn Cominsky 17
Quarks
Experiments have shown that protons and neutrons are made of smaller particles
We call them “quarks”, a phrase coined by Murray Gellman after James Joyce’s “three quarks for Muster Mark”
Every quark has an anti-quark
Modern picture of atom
April 18, 2023 Lynn Cominsky 18
Atomic sizes
Atoms are about 10-10 m Nuclei are about 10-14 m Protons are about 10-15 m The size of electrons and
quarks has not been measured, but they are at least 1000 times smaller than a proton
April 18, 2023 Lynn Cominsky 19
Types of Quarks
Flavor Charge Mass (GeV/c2)
Up 2/3 0.003
Down -1/3 0.006
Charm 2/3 1.3
Strange -1/3 0.1
Top 2/3 175
Bottom -1/3 4.3
Quarks come in three generations
All normal matter is made of the lightest 2 quarks
April 18, 2023 Lynn Cominsky 20
Quarks
Physics Chanteuse
Up, down, charm, strange, top and bottomThe world is made up of quarks and leptons…
Quark Sing-A-long
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Combining Quarks
Particles made of quarks are called hadrons
3 quarks can combine to make a baryon (examples are protons and neutrons)
A quark and an anti-quark can combine to make a meson (examples are muons, pions and kaons)
proton
meson
Fractional quark electromagnetic charges add to integers in all hadrons
Baryon numbers
Baryon numbers are only approximately conserved in particle interactions
The baryon number is defined on the basis of quarks and anti-quarks:NB = 1/3 (Q – Q)
What is the baryon number of a proton?What is the baryon number of a pi
meson?
April 18, 2023 Lynn Cominsky 22
April 18, 2023 Lynn Cominsky 23
Rules of the game activity
Analyze the observed particle events to see what the combination rules are
April 18, 2023 Lynn Cominsky 24
Color charges
Each quark has a color charge and each anti-quark has an anti-color charge
Particles made of quarks are color neutral, either R+B+G or color + anti-color
Quarks are continually changing their colors – they are not one color
April 18, 2023 Lynn Cominsky 26
Atomic Forces
Electrons are bound to nucleus by Coulomb (electromagnetic) force
Protons in nucleus are held together by residual strong nuclear force
Neutrons can beta-decay into protons by weak nuclear force, emitting an electron and an anti-neutrino
F = k q1 q2
r2
n = p + e +
April 18, 2023 Lynn Cominsky 27
Fundamental Forces
Gravity and the electromagnetic forces both have infinite range but gravity is 1036 times weaker at a given distance
The strong and weak forces are both short range forces (<10-14 m)
The weak force is 10-8 times weaker than the strong force within a nucleus
April 18, 2023 Lynn Cominsky 28
Force Carriers
Each force has a particle which carries the force
Photons carry the electromagnetic force between charged particles. Photons are not affected by the EM force.
Gluons carry the strong force between color charged quarks but they are affected by the strong force.
April 18, 2023 Lynn Cominsky 29
Force Carriers
Separating two quarks creates more quarks as energy from the color-force field increases until it is enough to form 2 new quarks
Weak force is carried by W and Z particles; heavier quarks and leptons decay into lighter ones by changing flavor
End of Part 1 Next you will hear from Helen Quinn,
Professor at SLAC Prof. Quinn got her PhD at Stanford, but is
originally from Australia She also worked at DESY (German
accelerator) and at Harvard The Peccei-Quinn theory has been proposed
to explain why strong interactions maintain CP symmetry when weak ones do not (more about CP symmetry later.)
April 18, 2023 Lynn Cominsky
Tuesday AM
Discussion – what were the hardest concepts for you to understand yesterday?
April 18, 2023 Lynn Cominsky 32
April 18, 2023 Lynn Cominsky 33
Particle DecaysNuclear decay – nucleus splits into
smaller constituents
Particle decay – fundamental particles “decay” (transform) into other (totally different) fundamental particlesHow does this happen?What are the rules?
238U
234Th
c
s
W
u
d
Any difference in masses is carried away as kinetic energy by new particles
April 18, 2023 Lynn Cominsky 34
Weak Particle Decays
Fundamental particle decays into another, less massive, fundamental particle plus a force-carrier particle This is always a W-boson for fundamental
particles In this example, the charm quark decays into a W
plus strange quark. The force-carrier particle then decays into
other fundamental particles (in this example, W decays into up and down quarks)
However, the mass of the W boson is 80.4 GeV/c2 – this is much more than a quark!
April 18, 2023 Lynn Cominsky 35
Virtual particles So how does a charm quark decay into
something that is heavier than itself? The answer lies in the Uncertainty principle
The W-boson only lives for a very short time (~3 x 10-25 s)
Its heavy mass limits the range of the weak force (It is equal to EM at 10-18 m.)
Since it lives for such a short time, it is known as a “virtual particle”
Initial energy and final energy (including kinetic energy of final particles) are still equal.
Flavors can change, charges can change.
April 18, 2023 Lynn Cominsky 36
Electromagnetic Decays
Example: 0 meson is made of a quark-anti-quark pair, which can annihilate, creating two photons
Photons are the force-carriers for the EM force.Photons are massless, hence the range of
the EM force is infinite
Neither colors or charge change.
April 18, 2023 Lynn Cominsky 37
Strong decays
The c particle is a charm-anticharm meson. It can undergo a strong decay into two gluons (which emerge as hadrons).
Gluons are strong-force carrier particles, and they mediate decays involving color changes.
Charge does not change, but color changes.
April 18, 2023 Lynn Cominsky 38
Annihilations
Two anti-particles annihilate, create force-carrier particles, which then decay into an entirely new pair of particles (or maybe two photons)
April 18, 2023 Lynn Cominsky 39
Unifying Forces
Weak and electromagnetic forces have been unified into the “electroweak” force They have equal strength at 10-18 m Weak force is so much weaker at larger distances
because the W and Z particles are massive and the photon is massless
Attempts to unify the strong force with the electroweak force are called “Grand Unified Theories”
There is no accepted GUT at present
April 18, 2023 Lynn Cominsky 40
Gravity
Gravity may be carried by the graviton – it has not yet been detected
Gravity is not relevant on the sub-atomic scale because it is so weak
Scientists are trying to find a “Theory of Eveything” which can connect General Relativity (the current theory of gravity) to the other 3 forces
There is no accepted Theory of Everything (TOE) at present
April 18, 2023 Lynn Cominsky 41
Spin
Spin is a purely quantum mechanical property which can be measured and which must be conserved in particle interactions
Particles with half-integer spin are “fermions” Particles with integer spin are “bosons”
* Graviton has spin 2
April 18, 2023 Lynn Cominsky 42
Quantum numbers
Electric charge (fractional for quarks, integer for everything else)
Spin (half-integer or integer) Color charge (overall neutral in particles) Flavor (type of quark) Lepton family number (electron, muon or tau) Fermions obey the Pauli exclusion principle –
no 2 fermions in the same atom can have identical quantum numbers
Bosons do not obey the Pauli principle
April 18, 2023 Lynn Cominsky 43
Standard Model
6 quarks (and 6 anti-quarks) 6 leptons (and 6 anti-leptons) 4 forces Force carriers (, W+, W-, Zo, 8 gluons, graviton)
April 18, 2023 Lynn Cominsky 44
Some questions
Do free quarks exist? Did they ever? Why do we observe matter and almost no antimatter if
we believe there is a symmetry between the two in the universe?
Why can't the Standard Model predict a particle's mass? Are quarks and leptons actually fundamental, or made
up of even more fundamental particles? Why are there exactly three generations of quarks and
leptons? How does gravity fit into all of this?
April 18, 2023 Lynn Cominsky 45
Particle Accelerators
The Standard Model of particle physics has been tested by many experiments performed in particle accelerators
Accelerators come in two types – hadron and lepton Heavier particles can be made by colliding lighter
particles that have added kinetic energy (because E=mc2)
Detectors are used to record the shower of new particles that results from the collision of the particle/anti-particle beams
Cloud Chamber Demo
We have a diffusion cloud chamber that will show us some particle tracks
April 18, 2023 Lynn Cominsky 46
High Voltage
Types of particles
Alpha particles = Helium nucleiBeta particles = either electrons or
positronsGamma “particles” = photonsCosmic rays = mostly protons, but also
nuclei of other elements.Which will we see in our Cloud
Chamber?
April 18, 2023 Lynn Cominsky 47
How it works
and particles ionize molecules of the alcohol in the cloud chamber
Vapor condenses on the ionized nuclei in the chamber
The drops of condensation appear to make tracks when lit up
X- and gamma-rays make energetic electrons, or e+/e- pairs
Can you predict which types of tracks are made by the various types of particles?
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April 18, 2023 Lynn Cominsky 49
Bubble chamber Same principle as cloud
chamber, but uses super-heated gas rather than super-cooled liquid
Anti-proton enters at bottom – turns into 8 pions, one of which decays into a muon and a neutrino
April 18, 2023 Lynn Cominsky 50
How to make particle beams Electrons: Heating a metal causes electrons
to be ejected. A television, like a cathode ray tube, uses this mechanism.
Protons: They can easily be obtained by ionizing hydrogen.
Antiparticles: To get antiparticles, first have energetic particles hit a target. Then pairs of particles and antiparticles will be created via virtual photons or gluons. Magnetic fields can be used to separate them.
Particles are accelerated by changes in EM fields that push them along.
April 18, 2023 Lynn Cominsky 51
Types of accelerators Different types of collisions:
Fixed target: Shoot a particle at a fixed target. Colliding beams: Two beams of particles are
made to cross each other. (Creates more energy since two beams of particles are accelerated.)
Accelerators are shaped in one of two ways: Linacs: Linear accelerators, in which the particle
starts at one end and comes out the other. (Example: SLAC, which uses leptons.)
Synchrotrons: Accelerators built in a circle, in which the particle goes around and around and around (steered by magnetic fields). (Example: Fermilab and CERN, which use hadrons.)
April 18, 2023 Lynn Cominsky 52
FermiLab
Tevatron collides protons and anti-
protons at 2 TeV
Colliding Detector at Fermilab (CDF) D0
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FermiLab The top quark was discovered at Fermilab – and 20 years
later, Fermilab observed single top quarks (not in pairs) Main goal is search for Higgs boson, new physics (CDF) Other experiments are looking for:
matter/anti-matter asymmetry in decays of Kaons and other mesons
Neutrino oscillations – from neutrinos made at Fermilab, traveling to Soudan mine (Minnesota, 450 miles away) and other long-baseline neutrino experiments
Many scientists collaborating on CMS at LHC (CERN) Dark matter searches (CDMS) Ongoing work on future experiments, such as a muon collider,
more neutrino detectors
April 18, 2023 Lynn Cominsky 54
A tour of the CDF detector
Virtual reality movie made at Fermilab by Joe Boudreau
movie
April 18, 2023 Lynn Cominsky 55
FermiLab
Only 1 out of 1010 collisions produces a top quark
Computer analyzes detector pattern to find mesons, a positron and evidence for a neutrino
Physicists deduce that this pattern also requires a W and b quark which come from a top quark decay
April 18, 2023 Lynn Cominsky 56
Find Mass of Top Quark
Analyze the events that are seen in the D0 detector
For each jet or particle, find the x- and y- components of the momentum (using a protractor). The amplitude of the momentum for each is given on the plot
What is the missing momentum? (x- and y- components)
What is the amplitude?
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Now find the top quark mass
Since all the momenta were expressed in units of GeV/c, you can add them all up
This collision made a top and anti-top pair – so the total of all the momentum amplitudes is the momentum of 2 tops
How did your answer compare to the measured value of 173 GeV/c ?
April 18, 2023 Lynn Cominsky 60
Field Theories
1865 – James Maxwell unifies electricity and magnetism in the first field theory
Fields were proposed to explain how forces are carried between particles
Einstein’s theory of General Relativity is another example of a field theory
electromagnetic wave
April 18, 2023 Lynn Cominsky 61
Particles and Fields
Fields carry energy through spacetime Fields are present everywhere, including the
vacuum (which is the lowest energy state of all the fields)
Fields can act like both waves and particles Wave-like fields are called forces Particle-like fields are called matter or
photons Matter interacts with other matter through
forces
April 18, 2023 Lynn Cominsky 62
Quantum Electrodynamics
Quantum mechanics describes the laws of motion of sub-atomic particles
Interactions between sub-atomic particles are described by quantum field theories
QED is the quantum field theory which describes electromagnetic interactions at the sub-atomic level
Predictions from QED calculations are accurate to one part in a trillion
April 18, 2023 Lynn Cominsky 63
Quantum Electrodynamics
The 1965 Nobel prize for QED was awarded to Richard Feynman, Julian Schwinger and Sin-Itiro Tomonaga
Feynman diagrams are used to show the relation between particles and force carriers for all four forces
Feynman diagram for a
electromagnetic interaction
April 18, 2023 Lynn Cominsky 64
Electro-weak Unification
1979 Nobel Prize awarded to Steven Weinberg, Abdus Salam, and Sheldon Glashow for the development of a unified field theory of electroweak interactions
They predicted the W and Z bosons (which were discovered in 1983, Nobel in 1984 to Carlo Rubbia and Simon van der Meer)
Feynman diagram of a weak interaction
April 18, 2023 Lynn Cominsky 65
Electro-weak Unification
Q: If the electromagnetic and weak interactions are really two sides of the same coin, then why are the W and Z particles so massive (80 GeV) while the photon is massless?
A: In the early Universe, when the characteristic energy kT > 80 GeV, the electromagnetic and weak forces were united. As the Universe cooled out of the electroweak era, spontaneous symmetry breaking occurred which split out the W and Z
April 18, 2023 Lynn Cominsky 66
Symmetry Breaking
Here is an example: it is unclear which glass goes with which place setting until the first one is chosen
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Spontaneous Symmetry Breaking
Balance a pencil on its tip – it has an equal chance to fall over in each direction. But when it falls over, it chooses a specific direction, and breaks the initial symmetry
Hydrogen and oxygen are symmetric molecules, yet when they combine to make water, the molecule has a characteristic angle of 105 degrees between the Hydrogen atoms.
April 18, 2023 Lynn Cominsky 68
Symmetries
Physical laws display mathematical symmetry Rotate a square through space by 90o - it will
look exactly the same Rotate a circle by any angle – it will also appear
the same Because a circle has more choices of rotation
angle, it is said to have a larger symmetry Physical laws can be invariant with respect
to changes in location, time or other types of transformations (rotation, velocity, etc.)
April 18, 2023 Lynn Cominsky 69
Symmetries
Patterns in the properties of particles can be described by mathematical symmetries which act on internal spaces – properties of the particles themselves, rather than its spacetime environment
Protons and neutrons are regarded as two different directions in an abstract internal space – although their charges are different, they have identical strong interactions (“nucleons”)
This is another example of a broken symmetry which is thought to be unified at higher energies
April 18, 2023 Lynn Cominsky 70
Transformation Laws
Laws of physics are the same at any location in space – this means that the universe is invariant under a “spatial” transformation
What if you reflect points in space through a mirror – “parity” transformation? (P) – No!
What if you turn every particle into its anti-particle – “charge conjugation” (C)? No!
But invariance is regained (almost) if you combine C and P – CP violation occurs at about 0.2% level (First proved with Kaons.)
April 18, 2023 Lynn Cominsky 71
CP Violation
CP means “charge-parity”, aka time-reversal symmetry – the symmetry that results from interchanging a particle with its anti-particle and sending it through a 3D mirror
CP violations were first observed in decays of K-mesons vs. anti-K-mesons – the decays happened at different rates (1980 Nobel, James Cronin and Val Fitch)
Studies of flavor changing interactions with K and B mesons should tell us more about CP physics
April 18, 2023 Lynn Cominsky 72
CP Violation Kaons oscillate between
two types– short-lived (green) which decay into 2 pions and long-lived (red), which decay into 3 pions
Both indirect and direct CP violation have now been observed
The weak force is responsible for these violations
April 18, 2023 Lynn Cominsky 73
CP Violation song
Written by Logan Whitehurst (formerly of the Jr. Science club, then in the Velvet Teen, now deceased) for my Cosmology class many years ago
http://www.juniorscienceclub.com/loganarchive/earthisbig/21%20sid_sheinberg_sings__cp_vi.mp3
Sid Sheinberg sings! CP Violation Song
April 18, 2023 Lynn Cominsky 74
Particle Accelerators-SLAC
2 mile long accelerator which can make up to 50 GeV electrons and positrons
Discovered the charm quark (also discovered at Brookhaven) and tau lepton; ran an accelerator producing huge numbers of B mesons.
Now doing photon science – Linac Coherent Light Source
LCLS is using x-ray laser beams to probe inside of atoms, removing one electron at a time
April 18, 2023 Lynn Cominsky 75
SLAC B-factory
Goal is to understand the imbalance between matter and anti-matter in the Universe
1 out of every billion matter particles must have survived annihilation
Decay rates of Bs and anti-Bs should be different
Explanation goes beyond the standard model
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BaBar Experiment SLAC accelerator was used (until 2008) as an asymmetric
B-meson factory, making B-mesons and anti-B-mesons out of 9 GeV electrons and 3.1 GeV positrons. CP violation is observed in some of these decays.
Half of the 2008 Nobel Prize in Physics was awarded to Makoto Kobayashi and Toshihide Maskawa for their theory which simultaneously explained the source of matter/antimatter asymmetries in particle interactions and predicted the existence of the third generation of fundamental particles. The BABAR experiment at the SLAC National Accelerator Laboratory in the U.S., together with the Belle experiment at KEK in Japan, recently provided experimental confirmation of the theory, some thirty years after it was published, through precision measurements of matter/antimatter asymmetries. The other half of the Nobel prize went to Yoichiro Nambu for his theory of spontaneous symmetry breaking.
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Quantum Chromodynamics
QCD is the quantum field theory which describes the interactions between quarks and gluons
It is difficult to use QCD to make predictions because the gluons carry a color charge and interact with each other
QCD is a non-linear theory which can only be calculated approximately - 10% accuracy for mass of proton – calculations take months of supercomputer time
April 18, 2023 Lynn Cominsky 78
Quantum Chromodynamics
1969 Nobel to Murray Gell-Mann for quark classification scheme
Internal symmetry in the pattern of quarks predicted the - particle and its mass
ddd ddu duu uuu
dds dus uus
dss uss
sss
= charge
grea
ter m
ass
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Gauge Theories
Gauge theories are quantum field theories that have local symmetries physical laws remain the same when particle properties are exchanged at different locations in spacetime
Local internal symmetries actually require force carrier particles whose interactions create the forces
QED is an Abelian gauge theory Electro-weak Unification is a non-Abelian
gauge theory (1999 Nobel to t’Hooft and Veltman)
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Abelian Transformations
Put a pen on the table.
Rotate it by 90o then by
180o
Now start over but this time
rotate it by 180o then by 90o
2D rotations are the same in either order
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Non-Abelian Transformation
Put a pen on the table. Rotate it by 90o so the tip points to the floor then by 180o so the tip points up
Now start over but this time rotate it first by 180o then by 90o – you get a very different result!
3D rotations are not the same in either order
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Beyond the Standard Model
Standard model describes every particle and interaction that has ever been observed in a laboratory
It has 18 arbitrary constants that are put in “by hand” – where do these come from?
The masses of the W and Z particles are not easily predictable from the Standard Model
The Standard Model also does not predict the pattern of masses and the generational structure – is a new symmetry needed?
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18 Free Parameters
Fundamental electroweak mass scale (1)Strengths of the 3 forces (3)Masses of e-, and (3)Masses of u, c and t quarks (3)Masses of d, s and b quarks (3)Strength of flavor changing weak force (1)Magnitude of CP symmetry breaking (3)Higgs boson mass (1)
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Grand Unification of Forces
Strengths of three forces depend on the energy at which the observations are made
Supersymmetric theories can unify the forces at higher energies than we can observe
strong
weak
electromagnetic 1016 GeV
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Supersymmetry
Supersymmetry is a larger symmetry that treats the 3 forces as broken pieces of a larger whole, and can predict all the properties and interactions of the particles
Predicts a combination of coupling constants that agrees with what is measured in the electroweak unification regime
Predicts supersymmetric particle partners for each existing particle (the lightest “sparticle” is also known as a WIMP)
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Supersymmetry
Sparticles have not yet been seen, but require experiments which can get to energies near 1 TeV (LHC? Fermi?)
GUTs allow the conversion of quarks to leptons through the exchange of a very massive particle
Since protons are made of quarks, this interaction would cause protons to decay
Non-supersymmetric GUTs predict short lifetimes for protons, and have been ruled out
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Proton Decay
Supersymmetric predicted proton decay rate is a few per year per 50,000 metric tons (SuperK volume)
SuperKamiokande finds a proton lifetime > 1033 years (no events are seen in over three years study of a huge volume of protons) – can eventually reach 1034 years Super K detector
April 18, 2023 Lynn Cominsky 88
Neutrino Oscillations
A pion decays in the upper atmosphere to a muon and a muon neutrino
Neutrinos oscillate flavors between muon and tau
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Neutrino Oscillations
High energy neutrinos that travel a short distance do not change their flavor
Low energy neutrinos that travel a long distance have a 50% chance of changing flavors
(m2c4) = 0.005 eV2
April 18, 2023 Lynn Cominsky 90
Neutrino Oscillations K2K (KEK to SuperK) was an experiment testing neutrino
oscillation results Neutrinos produced at KEK were measured at near detector
and then shot 250 km across Japan to SuperK detectors Final results from runs during 1999-2004: 158+/- 9 expected,
112 detected oscillations! Seeing oscillations means that neutrinos are not massless, as
assumed in the Standard Model
April 18, 2023 Lynn Cominsky 92
Origin of Mass
Electroweak unification predicts the existence of yet another particle, the Higgs boson
The Higgs boson is a neutral particle with zero spin which is the force carrier for the Higgs field
The Higgs boson breaks the electro-weak symmetry which gives the W and Z much heavier masses than the photon
Interactions with the Higgs field are theorized to give mass to all the other particles
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Higgs Boson Standard model physics predicts the mass of
the Higgs to be less than 150 GeV/c2. However if there is physics beyond the
standard model, then the Higgs mass could be as high as 1.4 TeV/c2
The data gathered at CERN (before LHC) set lower limit of 114.4 GeV/c2
As of January 2010, combined data from two experiments at Fermilab ruled out masses between 162 - 166 GeV/c2
LHC runs began again on March 30, 2010….
April 18, 2023 Lynn Cominsky 94
CERN
European Center for Particle Physics
Near Geneva, on France-Swiss border
CERN now has the Large Hadron Collider (LHC)
LHC is now the world’s highest energy accelerator – now colliding two beams of protons at 3.4 TeV, with a design limit of 7 TeV. (Also uses lead nuclei at up to 574 GeV.)
April 18, 2023 Lynn Cominsky 95
CERN
LHC detectors (designed to study 14 TeV energy scale, same as 10-12 s after Big Bang) ATLAS (looking for the Higgs boson et al.) CMS (Higgs, electro-weak symmetry breaking) ALICE (quark-gluon plasma studies) LHCb (matter/anti-matter asymmetry using B mesons)
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How to find a Higgs
Two quarks each emit a W or Z boson which combine to make a neutral Higgs.
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LHC rap
http://www.youtube.com/watch?v=j50ZssEojtM
Now approaching 6 million views…
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Theory of Everything
Mathematical unification of gravity with the other 3 forces (which are governed by quantum mechanics)
Einstein was the first to try (and fail) to develop a ToE – unifying general relativity with quantum mechanics
Supersymmetry + quantum gravity and string theory are two attempts to develop a ToE
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Anthropic Principle
Anthropic principle - physical forces and constants are precisely balanced to allow life
Is this balance an accident or part of a grand design by a grand designer?
If the laws of physics completely explain the creation of the Universe, then what role would there be for a Creator? (Hawking)
If there really is a ToE, then the beauty and order of the physical laws indicate that a Creator must have originated the laws (Davies)
Summary
Particle physics does a good job explaining observed particles and forces
Newest experiments are finding “physics beyond the standard model”
The search for the Higgs is the most important experiment going on today
Or maybe the search for supersymmetric particles which could be dark matter…..
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Web Resources
The Particle Adventure http://particleadventure.org/
Georgia State University Hyperphysics http://hyperphysics.phy-astr.gsu.edu/hbase/hframe.html National Research Council study of Elementary Particle Physics http://www.nap.edu/readingroom/books/particle/#contents
Boston University HEP site http://hep.bu.edu
Nobel Prizes http://www.nobel.se
Brookhaven National Laboratory (RHIC) http://www.rhic.bnl.gov
April 18, 2023 Lynn Cominsky 103
Relativistic Heavy Ion Collider
Brookhaven National Laboratory
Collides gold ions to form quark-gluon plasma to simulate Big Bang conditions
QGP has never been made on Earth but should exist inside neutron stars
April 18, 2023 Lynn Cominsky 106
Relativistic Heavy Ion Collider
Brookhaven National Laboratory
Collides gold ions to form quark-gluon plasma to simulate Big Bang conditions
QGP has never been made on Earth but should exist inside neutron stars