1 / 47

Spinor Gravity

Spinor Gravity. A.Hebecker,C.Wetterich. Unified Theory of fermions and bosons. Fermions fundamental Bosons composite Alternative to supersymmetry Bosons look fundamental at large distances, e.g. hydrogen atom, helium nucleus

dkerns
Download Presentation

Spinor Gravity

An Image/Link below is provided (as is) to download presentation Download Policy: Content on the Website is provided to you AS IS for your information and personal use and may not be sold / licensed / shared on other websites without getting consent from its author. Content is provided to you AS IS for your information and personal use only. Download presentation by click this link. While downloading, if for some reason you are not able to download a presentation, the publisher may have deleted the file from their server. During download, if you can't get a presentation, the file might be deleted by the publisher.

E N D

Presentation Transcript


  1. Spinor Gravity A.Hebecker,C.Wetterich

  2. Unified Theoryof fermions and bosons Fermions fundamental Bosons composite • Alternative to supersymmetry • Bosons look fundamental at large distances, e.g. hydrogen atom, helium nucleus • Graviton, photon, gluons, W-,Z-bosons , Higgs scalar : all composite

  3. Geometrical degrees of freedom • Ψ(x) : spinor field ( Grassmann variable) • vielbein : fermion bilinear

  4. Gauge bosons, scalars … from vielbein components in higher dimensions (Kaluza,Klein) concentrate first on gravity

  5. action contains 2d powers of spinors !

  6. symmetries • General coordinate transformations (diffeomorphisms) • Spinor ψ(x) : transforms as scalar • Vielbein : transforms as vector • Action S : invariant K.Akama,Y.Chikashige,T.Matsuki,H.Terazawa (1978) K.Akama (1978) A.Amati,G.Veneziano (1981) G.Denardo,E.Spallucci (1987)

  7. Lorentz- transformations Global Lorentz transformations: • spinor ψ • vielbein transforms as vector • action invariant Local Lorentz transformations: • vielbein does not transform as vector • inhomogeneous piece, missing covariant derivative

  8. Gravity with global and not local Lorentz symmetry ?Compatible with observation !

  9. How to get gravitational field equations ?How to determine vielbein and metric ?

  10. Functional integral formulation of gravity • Calculability ( at least in principle) • Quantum gravity • Non-perturbative formulation

  11. Vielbein and metric Generating functional

  12. If regularized functional measurecan be defined(consistent with diffeomorphisms)Non- perturbative definition of quantum gravity

  13. Effective action W=ln Z Gravitational field equation

  14. Gravitational field equationand energy momentum tensor Special case : effective action depends only on metric

  15. Symmetries dictate general form of gravitational field equationdiffeomorphisms !

  16. Unified theory in higher dimensionsand energy momentum tensor • No additional fields – no genuine source • Jμm : expectation values different from vielbein, e.g. incoherent fluctuations • Can account for matter or radiation in effective four dimensional theory ( including gauge fields as higher dimensional vielbein-components)

  17. Approximative computation of field equation

  18. Loop- and Schwinger-Dyson- equations Terms with two derivatives expected new ! covariant derivative has no spin connection !

  19. Fermion determinant in background field Comparison with Einstein gravity : totally antisymmetric part of spin connection is missing !

  20. Ultraviolet divergence new piece from missing totally antisymmetric spin connection : Ω→ K naïve momentum cutoff Λ :

  21. Functional measure needs regularization !

  22. Assume diffeomorphism symmetry preserved :relative coefficients become calculable B. De Witt D=4 : τ=3 New piece from violation of local Lorentz – symmetry !

  23. Gravity with global and not local Lorentz symmetry ?Compatible with observation !

  24. Phenomenology, d=4 Most general form of effective action which is consistent with diffeomorphism and global Lorentz symmetry Derivative expansion new not in one loop

  25. New gravitational degree of freedom for localLorentz-symmetry: H is gauge degree of freedom matrix notation : standard vielbein :

  26. new invariants ( only global Lorentz symmetry ) :derivative terms for Hmn

  27. Gravity with global Lorentz symmetry has additional field

  28. Local Lorentz symmetry not tested! loop and SD- approximation : β =0 new invariant ~ τ is compatible with all present tests !

  29. linear approximation ( weak gravity ) for β = 0 : only new massless field cμν

  30. Post-Newtonian gravity No change in lowest nontrivial order in Post-Newtonian-Gravity ! beyond linear gravity

  31. most general bilinear term dilatation mode σ is affected ! For β≠ 0 : linear and Post-Newtonian gravity modified !

  32. Newtonian gravity

  33. Schwarzschild solution no modification for β = 0 ! strong experimental bound on β !

  34. cosmology general isotropic and homogeneous vielbein : only the effective Planck mass differs between cosmology and Newtonian gravity if β = 0 Otherwise : same cosmological equations !

  35. Modifications only for β ≠ 0 !Valid theory with global instead of local Lorentz invariance for β = 0 ! General form in one loop / SDE : β = 0 Can hidden symmetry be responsible?

  36. geometry One can define new curvature free connection Torsion

  37. Time space asymmetry • Difference in signature from spontaneous symmetry breaking • With spinors : signature depends on signature of Lorentz group • Unified setting with complex orthogonal group: • Both euclidean orthogonal group and minkowskian Lorentz group are subgroups • Realized signature depends on ground state !

  38. Complex orthogonal group d=16 , ψ : 256 – component spinor , real Grassmann algebra

  39. vielbein Complex formulation

  40. Invariant action (complex orthogonal group, diffeomorphisms ) For τ = 0 : local Lorentz-symmetry !!

  41. Unification in d=16 or d=18 ? • Start with irreducible spinor • Dimensional reduction of gravity on suitable internal space • Gauge bosons from Kaluza-Klein-mechanism • 12 internal dimensions : SO(10) x SO(3) gauge symmetry – unification + generation group • 14 internal dimensions : more U(1) gener. sym. (d=18 : anomaly of local Lorentz symmetry ) L.Alvarez-Gaume,E.Witten

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

  43. Rather realistic model known • d=18 : first step : brane compactifcation • d=6, SO(12) theory : • second step : monopole compactification • d=4 with three generations, including generation symmetries • SSB of generation sym: realistic mass and mixing hierarchies for quarks and leptons C.W. , Nucl.Phys. B244,359( 1984) ; 260,402 (1985) ; 261,461 (1985) ; 279,711 (1987)

  44. Unification of bosons and fermions Unification of all interactions ( d >4 ) Non-perturbative ( functional integral ) formulation Manifest invariance under diffeomophisms SStrings Sp.Grav. ok ok ok ok - ok - ok Comparison with string theory

  45. Finiteness/regularization Uniqueness of ground state/ predictivity No dimensionless parameter SStrings Sp.Grav. ok - - ? ok ? Comparison with string theory

  46. conclusions • Unified theory based only on fermions seems possible • Quantum gravity – if functional measure can be regulated • Does realistic higher dimensional model exist?

  47. end

More Related