Generalized Quantum Theory of Recollapsing Homogeneous Cosmo(14)
时间:2025-07-12
时间:2025-07-12
A sum-over-histories generalized quantum theory is developed for homogeneous minisuperspace type A Bianchi cosmological models, focussing on the particular example of the classically recollapsing Bianchi IX universe. The decoherence functional for such uni
TheFadeev-Popovdeterminant G=detδG/δ ~detd2/dt2isinthiscaseindependentoftheintegrationvariables.Thedeltafunctionalin(3.4)thenpermitsonlytheN=constantpathstocontributetotheintegraloverN(t),leaving
1 ′′q q′′ Ch q′ =dN≥0δpδqqidt[pAq˙A NH](3.14)′expch0
afterdroppingtheconstantfactorsthatcancelinthedecoherencefunctional(3.9).Changingvariablesto
ds=Ndt,(3.15)
theGaussianfunctionalintegralsoverpmaybeperformed,leavingsimply
∞
q′′ Ch q′ =dN q′′N Ch q′0
0(3.16)
solongasweassumethecoarsegrainingdoesnotrestrictthevalueofN;otherwisetherangeoftheNintegralmustberestrictedappropriatelyaswell.Herewehavede ned
1 1q′′ q′′N Ch q′0 =δqqidt′exp
ch0 AdqGAB V,(3.17b)4ds
wherethepathintegralmeasureδqhasbeenrenormalizedintheusualmannerinducedbythemomentumintegrations.(Seetheappendixfordetails.)Thenotationonthelefthandsideof(3.17a)isinspiredbytheobservationthatthepathintegralin(3.17b)sharestheformofthatforthepropagatoroveratimeNofarelativisticparticleinapotentialV.(3.16)maybethoughtofasa“restrictedpropagator”fortheclassofpathsch,asshouldbeevidentfromtherestrictedfunctionalintegral(3.4).
Ingeneral,thecomplexityoftheminisuperspacepotentialVprecludesmuchfurtherex-plicitprogressinthenon-perturbativeevaluationof q′′ Ch q′ .Itisstillpossible,however,toshowthattheclassoperatorssatisfytheconstraint(3.5)forcoarsegrainingswhichdonotrestrictthevaluesoftheendpointsq′andq′′orthevalueofN.11Thisisdoneintheappendix.(3.8)isthusasclaimedindependentofthesurfacesonwhichwechoosetoimposetheboundaryconditionsΨandΦ.
IV.DECOHERENCEFUNCTIONALFORRECOLLAPSINGBIANCHICOS-MOLOGIES
ThegeneralformofthedecoherencefunctionalfortypeAhomogeneouscosmologiesisgivenin(3.9).Inthissectionweemploysomespeci cchoicesoftheinitialand nalconditionsapproriatetoΛ=0closed(BianchiIX)cosmologiestocastthedecoherencefunctionalintoasimplerandmorepracticallyusefulform.
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