Download - Spinor Gravity

Transcript
Page 1: Spinor Gravity

Spinor GravitySpinor Gravity

A.Hebecker,C.Wetterich

Page 2: Spinor Gravity

Unified TheoryUnified Theoryof fermions and bosonsof fermions and bosons

Fermions fundamentalFermions fundamental Bosons compositeBosons composite

Alternative to supersymmetryAlternative to supersymmetry Bosons look fundamental at large Bosons look fundamental at large

distances, distances, e.g. hydrogen atom, helium nucleuse.g. hydrogen atom, helium nucleus Graviton, photon, gluons, W-,Z-bosons , Graviton, photon, gluons, W-,Z-bosons ,

Higgs scalar : all compositeHiggs scalar : all composite

Page 3: Spinor Gravity

Geometrical degrees of Geometrical degrees of freedomfreedom

ΨΨ(x) : spinor field ( Grassmann (x) : spinor field ( Grassmann variable)variable)

vielbein : fermion bilinearvielbein : fermion bilinear

Page 4: Spinor Gravity

Gauge bosons, scalars …

from vielbein components in higher dimensions(Kaluza,Klein)

concentrate first on gravity

Page 5: Spinor Gravity

actionaction

contains 2d powers of spinors !

Page 6: Spinor Gravity

symmetriessymmetries General coordinate transformations General coordinate transformations

(diffeomorphisms)(diffeomorphisms) Spinor Spinor ψψ(x) : transforms (x) : transforms

as scalaras scalar Vielbein : transforms Vielbein : transforms

as vectoras vector Action S : invariantAction S : invariantK.Akama,Y.Chikashige,T.Matsuki,H.Terazawa (1978)

K.Akama (1978)A.Amati,G.Veneziano (1981)G.Denardo,E.Spallucci (1987)

Page 7: Spinor Gravity

Lorentz- transformationsLorentz- transformationsGlobal Lorentz transformations:Global Lorentz transformations: spinor spinor ψψ vielbein transforms as vector vielbein transforms as vector action invariantaction invariant

Local Lorentz transformations:Local Lorentz transformations: vielbein does vielbein does notnot transform as vector transform as vector inhomogeneous piece, missing covariant inhomogeneous piece, missing covariant

derivativederivative

Page 8: Spinor Gravity

Gravity with Gravity with globalglobal and and not not locallocal Lorentz Lorentz

symmetry ?symmetry ?

Compatible with Compatible with observation !observation !

Page 9: Spinor Gravity

How to get gravitational How to get gravitational field equations ?field equations ?

How to determine How to determine vielbein and metric ?vielbein and metric ?

Page 10: Spinor Gravity

Functional integral Functional integral formulation formulation

of gravityof gravity

CalculabilityCalculability ( at least in principle)( at least in principle) Quantum gravityQuantum gravity Non-perturbative formulationNon-perturbative formulation

Page 11: Spinor Gravity

Vielbein and metricVielbein and metric

Generating functional

Page 12: Spinor Gravity

IfIf regularized functional regularized functional measuremeasure

can be definedcan be defined(consistent with (consistent with

diffeomorphisms)diffeomorphisms)

Non- perturbative Non- perturbative definition of definition of quantum quantum

gravitygravity

Page 13: Spinor Gravity

Effective actionEffective action

W=ln Z

Gravitational field equation

Page 14: Spinor Gravity

Gravitational field equationGravitational field equationand energy momentum and energy momentum

tensortensor

Special case : effective action depends only on metric

Page 15: Spinor Gravity

Symmetries dictate Symmetries dictate general form of general form of

gravitational field gravitational field equationequation

diffeomorphisms !diffeomorphisms !

Page 16: Spinor Gravity

Unified theory in higher Unified theory in higher dimensionsdimensions

and energy momentum and energy momentum tensortensor

No additional fields – no genuine sourceNo additional fields – no genuine source JJμμ

m m : expectation values different from : expectation values different from vielbein, e.g. incoherent fluctuationsvielbein, e.g. incoherent fluctuations

Can account for matter or radiation in Can account for matter or radiation in effective four dimensional theory effective four dimensional theory ( including gauge fields as higher ( including gauge fields as higher dimensional vielbein-components)dimensional vielbein-components)

Page 17: Spinor Gravity

Approximative computation Approximative computation

of field equationof field equation

Page 18: Spinor Gravity

Loop- and Loop- and Schwinger-Dyson- Schwinger-Dyson-

equationsequations

Terms with two derivatives

covariant derivative

expected

new !

has no spin connection !

Page 19: Spinor Gravity

Fermion determinant in Fermion determinant in background fieldbackground field

Comparison with Einstein gravity : totally antisymmetric part of spin connection is missing !

Page 20: Spinor Gravity

Ultraviolet divergenceUltraviolet divergencenew piece from missing totally antisymmetricspin connection :

naïve momentum cutoff Λ :

Ω → K

Page 21: Spinor Gravity

Functional measure needs Functional measure needs regularization !regularization !

Page 22: Spinor Gravity

Assume diffeomorphism symmetry Assume diffeomorphism symmetry preserved :preserved :

relative coefficients become relative coefficients become calculablecalculable

B. De Witt

D=4 :

τ=3

New piece from violation of local Lorentz – symmetry !

Page 23: Spinor Gravity

Gravity with Gravity with globalglobal and and not not locallocal Lorentz Lorentz

symmetry ?symmetry ?

Compatible with Compatible with observation !observation !

Page 24: Spinor Gravity

Phenomenology, d=4Phenomenology, d=4Most general form of effective action Most general form of effective action

which is consistent with which is consistent with diffeomorphism and diffeomorphism and

global global Lorentz symmetryLorentz symmetry

Derivative expansionDerivative expansion

newnot in one loop

Page 25: Spinor Gravity

New gravitational degree of New gravitational degree of freedomfreedom

for local Lorentz-symmetry:H is gauge degree of freedom

matrix notation :

standard vielbein :

Page 26: Spinor Gravity

new invariants ( only new invariants ( only globalglobal Lorentz Lorentz symmetry ) :symmetry ) :

derivative terms for Hderivative terms for Hmnmn

Page 27: Spinor Gravity

Gravity with Gravity with global Lorentz symmetry global Lorentz symmetry

has additional fieldhas additional field

Page 28: Spinor Gravity

Local Lorentz symmetry not Local Lorentz symmetry not tested!tested!

loop and SD- approximation : loop and SD- approximation : ββ =0 =0

new invariant ~ new invariant ~ ττ is compatible with all is compatible with all present tests !present tests !

Page 29: Spinor Gravity

linear approximation ( weak linear approximation ( weak gravity )gravity )

for β = 0 : only new massless field cμν

Page 30: Spinor Gravity

Post-Newtonian gravityPost-Newtonian gravity

No change in lowest nontrivial order in Post-Newtonian-Gravity !

beyond linear gravity

Page 31: Spinor Gravity

most general bilinear most general bilinear termterm

dilatation mode σ is affected !

For β ≠ 0 : linear and Post-Newtonian gravity modified !

Page 32: Spinor Gravity

Newtonian gravityNewtonian gravity

Page 33: Spinor Gravity

Schwarzschild solutionSchwarzschild solution

no modification for β = 0 !strong experimental bound on β !

Page 34: Spinor Gravity

cosmologycosmology

only the effective Planck mass differs between cosmology and Newtonian gravity if β = 0

general isotropic and homogeneous vielbein :

Otherwise : same cosmological equations !

Page 35: Spinor Gravity

Modifications only for Modifications only for ββ ≠ ≠ 0 !0 !

Valid theory with global Valid theory with global instead of local Lorentz instead of local Lorentz invariance for invariance for ββ = 0 ! = 0 !

General form in one loop / SDE : β = 0 Can hidden symmetry be responsible?

Page 36: Spinor Gravity

geometrygeometryOne can define new curvature free connection

Torsion

Page 37: Spinor Gravity

Time space asymmetryTime space asymmetry Difference in signature from spontaneous Difference in signature from spontaneous

symmetry breakingsymmetry breaking With spinors : signature depends on With spinors : signature depends on

signature of Lorentz groupsignature of Lorentz group

Unified setting with Unified setting with complex orthogonal complex orthogonal groupgroup::

Both Both euclideaneuclidean orthogonal group and orthogonal group and minkowskianminkowskian Lorentz group are subgroups Lorentz group are subgroups

Realized signature depends on ground Realized signature depends on ground state !state !

Page 38: Spinor Gravity

Complex orthogonal Complex orthogonal groupgroup

d=16 , ψ : 256 – component spinor , real Grassmann algebra

Page 39: Spinor Gravity

vielbeinvielbein

Complex formulation

Page 40: Spinor Gravity

Invariant actionInvariant action

For τ = 0 : local Lorentz-symmetry !!

(complex orthogonal group, diffeomorphisms )

Page 41: Spinor Gravity

Unification in d=16 or Unification in d=16 or d=18 ?d=18 ?

Start with irreducible spinorStart with irreducible spinor Dimensional reduction of gravity on suitable Dimensional reduction of gravity on suitable

internal spaceinternal space Gauge bosons from Kaluza-Klein-mechanismGauge bosons from Kaluza-Klein-mechanism 12 internal dimensions : SO(10) x SO(3) 12 internal dimensions : SO(10) x SO(3)

gauge symmetry – unification + generation gauge symmetry – unification + generation groupgroup

14 internal dimensions : more U(1) gener. 14 internal dimensions : more U(1) gener. sym.sym.

(d=18 : anomaly of local Lorentz symmetry )(d=18 : anomaly of local Lorentz symmetry )L.Alvarez-Gaume,E.Witten

Page 42: Spinor Gravity

Chiral fermion Chiral fermion generationsgenerations

Chiral fermion generations according to Chiral fermion generations according to chirality indexchirality index (C.W. , Nucl.Phys. B223,109 (1983) ; (C.W. , Nucl.Phys. B223,109 (1983) ; E. Witten , Shelter Island conference,1983 )E. Witten , Shelter Island conference,1983 ) Nonvanishing index for brane Nonvanishing index for brane (noncompact internal space )(noncompact internal space ) (C.W. , Nucl.Phys. B242,473 (1984) )(C.W. , Nucl.Phys. B242,473 (1984) ) Wharping : d=4 mod 8 possibleWharping : d=4 mod 8 possible (C.W. , Nucl.Phys. B253,366 (1985) )(C.W. , Nucl.Phys. B253,366 (1985) )

Page 43: Spinor Gravity

Rather realistic model Rather realistic model knownknown

d=18 : first step : brane compactifcation d=18 : first step : brane compactifcation

d=6, SO(12) theory :d=6, SO(12) theory : second step : monopole compactificationsecond step : monopole compactification

d=4 with three generations, d=4 with three generations, including generation symmetriesincluding generation symmetries SSB of generation sym: realistic mass and SSB of generation sym: realistic mass and

mixing hierarchies for quarks and leptonsmixing hierarchies for quarks and leptons

C.W. , Nucl.Phys. B244,359( 1984) ; 260,402 (1985) ; 261,461 (1985) ; 279,711 (1987)

Page 44: Spinor Gravity

Comparison with string Comparison with string theorytheory

Unification of bosons Unification of bosons and fermionsand fermions

Unification of all Unification of all interactions ( d >4 )interactions ( d >4 )

Non-perturbative Non-perturbative ( functional integral ) ( functional integral )

formulationformulation Manifest invariance Manifest invariance

under diffeomophismsunder diffeomophisms

SStrings SStrings Sp.Grav.Sp.Grav.

ok okok ok

ok okok ok

- - ok ok

- - ok ok

Page 45: Spinor Gravity

Comparison with string Comparison with string theorytheory

Finiteness/Finiteness/regularizationregularization

Uniqueness of ground Uniqueness of ground

state/ state/ predictivitypredictivity

No dimensionless No dimensionless parameterparameter

SStrings SStrings Sp.Grav.Sp.Grav.

ok ok - -

-- ? ?

ok ?ok ?

Page 46: Spinor Gravity

conclusionsconclusions Unified theory based only on Unified theory based only on

fermions seems possiblefermions seems possible Quantum gravity – Quantum gravity – if functional measure can be if functional measure can be

regulatedregulated Does realistic higher dimensional Does realistic higher dimensional

model exist?model exist?

Page 47: Spinor Gravity

end