Microscopic Origins for Gauge and Space Time Symmetries S.Randjbar-Daemi, Greece June 2005.
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Transcript of Microscopic Origins for Gauge and Space Time Symmetries S.Randjbar-Daemi, Greece June 2005.
![Page 1: Microscopic Origins for Gauge and Space Time Symmetries S.Randjbar-Daemi, Greece June 2005.](https://reader030.fdocuments.in/reader030/viewer/2022032521/56649d595503460f94a3907c/html5/thumbnails/1.jpg)
Microscopic Origins for Gauge and Space Time
Symmetries
S.Randjbar-Daemi,
Greece June 2005
![Page 2: Microscopic Origins for Gauge and Space Time Symmetries S.Randjbar-Daemi, Greece June 2005.](https://reader030.fdocuments.in/reader030/viewer/2022032521/56649d595503460f94a3907c/html5/thumbnails/2.jpg)
References:
• S. Randjbar-Daemi and J.A. Strathdee Phys. Lett B337, ( 1994) 309 and Int. Journal of Modern Physics A 10 (1995) 4651
• S.R. D Work in Progress
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Introduction
• Local Quantum Field Theories are inevitable in low energy physics: They reconcile quantum mechanics with special relativity
• Renormalizable theories are probably the only consistent ones: They are insensitive to short distance physics.
• To each QFT there may correspond a large class of models with the same Low E sector
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On the other hand…..•
Relativistic Invariance may not be Fundamental but merely an approximate feature of the Low Energy Sector!
• General Relativity is a very successful theory of large scale gravitational phenomena, BUT
• it is not renormalizable and hence is sensitive to the short distance
effects
• There is no experimental guide to a Microscopic Theory of Gravity
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We have no guide to lead us to a microscopic theory of gravity
• Only recently corrections to sub- millimeter gravity have been examined ( Brane World Scenarios)
• Any Quantum Theory of Gravity will be SPECULATIVE
• Superstring theory is probably the best ( and the most ambitious) speculative theory of gravity and certainly the most elegant!
• But there may be others……(less ambitious!) and less elegant! The may help us to appreciate the elegance of string theory.
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Our Idea
• The microscopic d.o.f of gravity may be different from what we see at long distances, i.e. the metric tensor of space and time
• In this sense gravity is an emergent effect which manifests itself in terms of different variables at different scales
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Plan of This talk
• The Model• Generalized Effective Action• Gap Equations• Ground State and its Symmetries• Fermion Propagator• Gauge Sector• Example• Gravity
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Our Model consists of an array of sites with a Grassman variable
attached to each site
This is invariant under the permutation group provided we also transform the couplings J
The total action may contain an extra term, S(J), invariant under the permutation group
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The Model
Relation to Ising Type Models
Spin variables S(A)= 0, 1 at each site and the partition function:
ABABS
A SiSJS exp Z
The leading term as 0J
produces the 4-Fermi action
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Rewrite the Ising Z(J)
)1/2- exp()1(
)1/2- exp()exp1(dJ) (det2
)S(i2
1-exp
d)2(det Z(J)
0ABA
1ABA
A
1/2-
AA1
AB
A
2/1
S
A
BA
BAA
BA
A
Je
Ji
J
J
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Each Differentiation yields a factor of J. The leading term is:
0A )2/1exp()( BABAA
J
Takes the form of a sum over all pairings of the sites and can be expressedby an integral over Grassmann variables
BAA BA
B)J(A, dd exp
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Basic Quantity:
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12N
n
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Impose some structures:Assumptions:
• Our Lattice is composed of 4d cells
labeled by integers n.
• Within each cell there are N sites
• Notation : A=(i, n), where i=1,2,…N
and 4Zn
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The Action becomes:
Where
in the Grassmann variables!
This is a 4-Fermi model with no bilinears
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Our Aim:
• Obtain information about the structure of the ground state of this model and the spectrum of long-wavelength oscillations
• Since there are no bilinears in the Grassmann variables we should ask:
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• Are there any propagating d.o.f?
• Are there any light modes in the spectrum?
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Methodology:
• Set up a set of Generalized Gap equations for the Propagator,
• These Equations are difficult to solve, even in simplest cases. But
• We can study the property of the system about an assumed solution by making some simplifying assumptions
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Generalized Effective Action:
• Ref: C. De Dominicis J. Math. Phys. 3( 1962)983
• R. Jakiw and K. Johnson Phys.Rev. D8 (1973) 2386
• J.M. Cornwall and R.E. Norton Phys. Rev D8 (1973) 3338
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Generalized Action:
• Depends on the 2 point functions as well as the fields
• The equation for the 2 point functions is obtained as an extremal condition
• The Generalized action functional is represented by a loop expansion of 2-particle-irreducible vacuum graphs in which the lines are associated with the unknown functions.
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Rewrite the Fermionic Action:Introduce a scalar field
)(n
S does not have any bilinears in
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Generlized Effective Action:
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Feynmann Rules
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Lowest Order graphs:
• There is only one 2-loop graph
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• And one 3-loop graph
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The Gap Equations:
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Hartree-Fock Approximation
• Retain only the 2-loop contribution to
Where, s=n-m, G(n,m)= G(s), etc
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Ground State Symmetries1. Global symmetries:
• The Generalized Effective Action is invariant w.r.t a space group that acts on the lattice:
Where : h belongs to the point group
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The couplings are invariantJ(n’-m’)=J(n-m)
And the independent variables transform as scalars
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2. Local Symmetries: There is a local GL(N,C) Invariance w.r. to which are invariant but:
The gap equations which determine the ground state are covariant underthese global and local transformations
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• Assume that the solution of the gap equations defines a homomorphism
Such that
Where
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If such solution could be found:
1. Fermions propagate 2. They belong to a non trivial representation of the ground state symmetry group, ie. They carry
SPIN• For a reasonable Fermion Spectrum:
• Ground state symmetry group should have a factor which is a subgroup of Spin(4)
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Require that H is contained in O(4)
• Our Lattice is a 4-dimensional Crystal
• There are 227 four dimensional Crystals
• We chose the largest one. Its point group has 1152 elements and it coincides with the Weyl group of the weight lattice of the exceptional Lie Algebra
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The action of point group divides the lattice into orbits
• The number of points on each orbit can be as large as the numer of elements in H, but it can be smaller if there is a subgroup of H leaving some points fixed
• The couplings J(s) are equal for all points on the same orbit and the Green function G(s) is fully specified if it is known at one
point on each orbit
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The Lattice:
• Comprise the points with integer coefficients where the basis vectors
are expressible in the orthonormal basis by
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Some Nearby Orbits:
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Spinor Representations
Where
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Generators
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Dirac Matrices in the lattice basis
The vector representation in the lattice basis:
![Page 42: Microscopic Origins for Gauge and Space Time Symmetries S.Randjbar-Daemi, Greece June 2005.](https://reader030.fdocuments.in/reader030/viewer/2022032521/56649d595503460f94a3907c/html5/thumbnails/42.jpg)
Suppose now that the solution of the gap equations assigns fermions
to the Dirac representation, i.e
The invariance condition becomes:
Where a ranges over the entire group. For the Fourier transform
![Page 43: Microscopic Origins for Gauge and Space Time Symmetries S.Randjbar-Daemi, Greece June 2005.](https://reader030.fdocuments.in/reader030/viewer/2022032521/56649d595503460f94a3907c/html5/thumbnails/43.jpg)
Long wavelength modes
• The invaraince condition implies that near
• K=0 the fermion Green function becomes
• With Z and M numbers to be determined by solving the gap equations.
• The leading terms are O(4) invariant. Higher order terms will break it.
![Page 44: Microscopic Origins for Gauge and Space Time Symmetries S.Randjbar-Daemi, Greece June 2005.](https://reader030.fdocuments.in/reader030/viewer/2022032521/56649d595503460f94a3907c/html5/thumbnails/44.jpg)
Gauge Sector
• The Green Function G(n,m) is a dynamical variable.
• In the long wavelength regiem its dynamics should be expressible in terms of scalars, vectors, tensors, etc.
• Among the light degrees of freedom we should expect to find a Yang Mills field
• Our aim is to isolate this term
![Page 45: Microscopic Origins for Gauge and Space Time Symmetries S.Randjbar-Daemi, Greece June 2005.](https://reader030.fdocuments.in/reader030/viewer/2022032521/56649d595503460f94a3907c/html5/thumbnails/45.jpg)
• Recall the gauge transformation of G
• Adopt the Ansatz
Where The path ordered integral is along a straight line joining n and m
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Under local gauge transformations
The unbroken local symmetries must be associated with a set of Yang –Mills vectors and these must contribute a factor as indicated above, in the long wave length limit.
Of course G(n,m) must represent other d.o.f. but, for simplicity, we shall assume that they are all heavy and therefore irrelevant.
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Calculating the gauge coupling constant
• The lowest order gauge dynamics should be governed by the standard Yang-Mills action with a calculable gauge coupling.
• We must substitute our ansatz in the generalized effective action,
• Use the gap equations to eliminate
This is obviously independent of A
![Page 48: Microscopic Origins for Gauge and Space Time Symmetries S.Randjbar-Daemi, Greece June 2005.](https://reader030.fdocuments.in/reader030/viewer/2022032521/56649d595503460f94a3907c/html5/thumbnails/48.jpg)
• This depends on A !
• After these eliminations the gauge invariant functional in the lowest order in derivative expansion must have the form
With a calculable e
The O(4) invariance is a consequence of the invariance of
w.r.t the point group. It is true only in the leading order in k!
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Some Steps in the calculation of the gauge coupling
• Basically we need to calculated the quantum induced vacuum polarization and
• Show that it satisfies the Ward identity
The basic quantity is
To be evaluated at A=0 and fixed at the extremum
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Hartree- Fock Approximation:Keep only 2-loop contributions
+ ….
The derivatives at A=0 are
Where the T’s commute with the background G
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In Fourier Space:
Where
![Page 52: Microscopic Origins for Gauge and Space Time Symmetries S.Randjbar-Daemi, Greece June 2005.](https://reader030.fdocuments.in/reader030/viewer/2022032521/56649d595503460f94a3907c/html5/thumbnails/52.jpg)
The Polarization tensor
![Page 53: Microscopic Origins for Gauge and Space Time Symmetries S.Randjbar-Daemi, Greece June 2005.](https://reader030.fdocuments.in/reader030/viewer/2022032521/56649d595503460f94a3907c/html5/thumbnails/53.jpg)
Use the Gap equation to eliminateDelta
• In the Hartree-Fock approximation
Using this we obtain
![Page 54: Microscopic Origins for Gauge and Space Time Symmetries S.Randjbar-Daemi, Greece June 2005.](https://reader030.fdocuments.in/reader030/viewer/2022032521/56649d595503460f94a3907c/html5/thumbnails/54.jpg)
Polarization
![Page 55: Microscopic Origins for Gauge and Space Time Symmetries S.Randjbar-Daemi, Greece June 2005.](https://reader030.fdocuments.in/reader030/viewer/2022032521/56649d595503460f94a3907c/html5/thumbnails/55.jpg)
using
by checked benow can 0Πkidentity Ward The μμ
)()'( identity the 11
1 kupGu
kupGkμ
.uover gintegratin and 1
)()'()2(
write0 of vicinity theIn4 kkk(k,k')Π
k' k
αβμν
![Page 56: Microscopic Origins for Gauge and Space Time Symmetries S.Randjbar-Daemi, Greece June 2005.](https://reader030.fdocuments.in/reader030/viewer/2022032521/56649d595503460f94a3907c/html5/thumbnails/56.jpg)
b.b g
basis, lattice thein defined is tensor metric thewhere
1
by given is termleading The H.grouppoint the
of tensorsinvariant bemust expansion thisin tscoefficien The
2
σρρσμννσμρμν k)kggg(g
e(k) Π
The coupling constant , 2e is thereby expressed, in the Hartree-Fock Approximation, as an integral over BZ involving )( pG
![Page 57: Microscopic Origins for Gauge and Space Time Symmetries S.Randjbar-Daemi, Greece June 2005.](https://reader030.fdocuments.in/reader030/viewer/2022032521/56649d595503460f94a3907c/html5/thumbnails/57.jpg)
Example: Replace fermionsby a single complex scalar
G. particular thegenerate equations gap thefor which couplings
ofset a find andinput an as G(s) give toisStrategy Our
matrix.N Na nrather tha
scalar a becomes G(s), function, Green The
![Page 58: Microscopic Origins for Gauge and Space Time Symmetries S.Randjbar-Daemi, Greece June 2005.](https://reader030.fdocuments.in/reader030/viewer/2022032521/56649d595503460f94a3907c/html5/thumbnails/58.jpg)
In the Hartree-Fock aproximationthe gap equations become
21211
01
11
cos2cos24~
choose and 2d in lattice square heConsider t
0
kk- M(s)eG(k)G
Δ(s)G(s)σδ(s)G
s)G(s)G((s)J(s)Δ
)G(J(s)σ
s
iks-
s,
s
![Page 59: Microscopic Origins for Gauge and Space Time Symmetries S.Randjbar-Daemi, Greece June 2005.](https://reader030.fdocuments.in/reader030/viewer/2022032521/56649d595503460f94a3907c/html5/thumbnails/59.jpg)
4cos242
cos2cos242
M,mass
of particlea of npropagatio thedescribes thissmallis MIf
21112
12
121
212
2
2
s)ω(ksik
iks
e)k - (Mπ
dk
k k M
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π
dk(G(s)
ghost! no is There
.k 0for lly monotonica increases )(k general inbut
thensmall, arek and M If
4cos242
1cos24
2
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11
22
222
Mkω(k)
k)(Mk)(M -(k)
![Page 60: Microscopic Origins for Gauge and Space Time Symmetries S.Randjbar-Daemi, Greece June 2005.](https://reader030.fdocuments.in/reader030/viewer/2022032521/56649d595503460f94a3907c/html5/thumbnails/60.jpg)
Solution of the Gap Equations
)cos(1,0)(cosk2 (0,0) )(~
)0,1(
)0,1(G-(1,0)
)0,0(
)0,0(G-(0,0)
neighborsnearest its and origin the
at except everywhere 0(s) imply that thenequations gap The
1- )1,0(G)10(G
4 M)0,0(G
neighborsnearest its
and origin at theexcept everywhere 0)(G all ofFirst
21
1-
1-
1-1-
21-
-1
kk
G
G
s
![Page 61: Microscopic Origins for Gauge and Space Time Symmetries S.Randjbar-Daemi, Greece June 2005.](https://reader030.fdocuments.in/reader030/viewer/2022032521/56649d595503460f94a3907c/html5/thumbnails/61.jpg)
The Couplings:
solution. given theproduces whichJ(s) of choicesdistinct two
there Hence.for solution real twohas equation This
)(~
)(~
)2
()0,1(/)0,0(4)4(
)4()0,0(
for eq. an
yields0kfor above equation the with thisCompare
)0,0(
(0)J~
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obtain weequations gap theFrom
determine toisleft isWhat
)(~
)(~
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~1
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~1
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pGpGdp
GGM
MG
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pGpkGdp
k
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Gravity
Let us go back to the 4-fermion action
J. of dynamics thegovern to termaction an add toneed thusWe
model.our in objectsother like fielda it to promote toneed We
couplings. ofset givena as m)J(n, regarded have far we So
m)J(n, )m',(n'J'm)J(n,
particular In scalars. like transformS enetring objects theall
provided,S f wheref(n), nunder invariant is action This
)()(),()()( S
mmmnJnn
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J-Dynamics
We have not studied the action for the Pure J-field
We shall assume that our background J- values are in turn determined by
minimizing the enlarged action. The J’s are thus effectively considered as given
background fields, somewhat similar to a background metric.
![Page 64: Microscopic Origins for Gauge and Space Time Symmetries S.Randjbar-Daemi, Greece June 2005.](https://reader030.fdocuments.in/reader030/viewer/2022032521/56649d595503460f94a3907c/html5/thumbnails/64.jpg)
• Because of the general coordinate invariance, gravity should be contained among the light degrees of freedom!
• Our aim is to calculate the Einstein action
and the Newton constant in terms of the
given couplings.
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Rewrite S: Introduce a field
mn mnJ
nmmntrmmnnS
, ),(
),(),()(),()(
NN ),( mnji
Solving the field equations and substituting the result in S
reproduces the original 4-fermi action
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Integrate over
Det
mnJ
nmmntrS
mneff ln
),(
),(),(
,
This is an approximation to the Generalized effective action which we Constructed before.
The Gap Equations:
),(),(),( 1 mnmnJmn
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Let C(n-m) be a translationalInvariant solution of the Gap eq
• Ansatz for the Yang-Mills field
)(exp)(),( n
mAiTmnCmn
The integral is along a straight path from m to n
A is in the subalgebra commuting with C
Substitution in the effective action generates the Y-M Action for A
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How do we obtain gravity?
• We need to introduced more structures.• The lattice states should be embedded in a
continuum .• A projection E commuting with should be
introduced• should be regarded as a functional of a set of
vierbeins as well independent connection coefficients
n
)(ne a
x
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Then:
xE
nn
lnx
lnlnDet
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Anzatz for the light d.o.f
1/2
1
0
a1141/2
e(y) )duTexp(i
)Ke,y(x,iξexp (K)G)2π
dK(e(x)xΓ,....)χ(e,x
A
a
Where : is the geodesic between x and y ( assuming there is only one) and e(x) is the determinant of the vierbein
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The plausibility of the Anzatz
• Its structure is dictated by the symmetries of the effective action,
• It produces the correct Yan-Mills action in the absence of gravity,
• It produces the correct (leading order) minimal coupling of the fermions to the gauge fields,
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• If we replace fermions by scalar bosons it reproduces the correct( leading order) kinetic terms for the scalars,
• It reproduces the correct cosmological constant
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But……
• Although the anzatz satifies the correct Ward identities for the local gauge and general coordinate transformations it does not satisfy those for the local Lorentz transformations, unless we adjust the couplings to kill the non invariant terms!
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Conclusion:
The gravity problem still not fully
understood…….
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Outstanding Problems• Find a solution of gap equations with spin
• Study the dynamics of the J-fields
( RG equations, an action for J, etc)
• Obtain Gravity ( A better ansatz for
or G) so that the Ward identities for the local Lorentz transformations are satisfied.
• Calculate Newton’s constant….