Blackbody Distribution for Wormholes

Details Blackbody Distribution for Wormholes Blackbody Distribution for Wormholes

1993-09-13

arxiv.org/abs/gr-qc/9309009v1

Class.Quant.Grav.10:2505-2510,1993

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

8p, IMAFF-RC-06-93#

Scientific paper

10.1088/0264-9381/10/12/009

By assuming that only (i) bilocal vertex operators which are diagonal with respect to the basis for local field operators, and (ii) the convergent elements with nonzero positive energy of the density matrix representing the quantum state of multiply-connected wormholes, contribute the path integral that describes the effects of wormholes on ordinary matter fields at low energy, it is obtained that the probability measure for multiply connected wormholes with nondegenerate energy spectrum is given in terms of a Planckian probability distribution for the momenta of a quantum field $\frac{1}{2}\alpha^ {2}$, where the $\alpha$'s are the Coleman parameters, rather than a classical gaussian distribution law, and that an observable classical universe can exist if, and only if, such multiply connected wormholes are allowed to occur.

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