Casimir energy in a small volume multiply connected static hyperbolic preinflationary universe


Autoria(s): Muller, D.; Fagundes, H. V.; Opher, R.
Contribuinte(s)

Universidade Estadual Paulista (UNESP)

Data(s)

20/05/2014

20/05/2014

15/06/2001

Resumo

A few years ago, Cornish, Spergel and Starkman (CSS) suggested that a multiply connected small universe could allow for classical chaotic mixing as a preinflationary homogenization process. The smaller the volume, the more important the process. Also, a smaller universe has a greater probability of being spontaneously created. Previously DeWitt, Hart and Isham (DHI) calculated the Casimir energy for static multiply connected fat space-times. Because of the interest in small volume hyperbolic universes (e.g., CSS), we generalize the DHI calculation by making a numerical investigation of the Casimir energy for a conformally coupled, massive scalar field in a static universe, whose spatial sections are the Weeks manifold, the smallest universe of negative curvature known. In spite of being a numerical calculation, our result is in fact exact. It is shown that there is spontaneous vacuum excitation of low multipolar components.

Formato

5

Identificador

http://dx.doi.org/10.1103/PhysRevD.63.123508

Physical Review D. College Pk: American Physical Soc, v. 63, n. 12, 5 p., 2001.

0556-2821

http://hdl.handle.net/11449/23350

10.1103/PhysRevD.63.123508

WOS:000169288400014

WOS000169288400014.pdf

Idioma(s)

eng

Publicador

American Physical Soc

Relação

Physical Review D

Direitos

closedAccess

Tipo

info:eu-repo/semantics/article