COSMOLOGICAL PRINCIPLE AND PRIMORDIAL SPINOR FIELDS

Authors
SORG M
Citation
M. Sorg, COSMOLOGICAL PRINCIPLE AND PRIMORDIAL SPINOR FIELDS, letters in mathematical physics, 33(2), 1995, pp. 113-125
Citations number
13
Categorie Soggetti
Mathematical Method, Physical Science","Physycs, Mathematical
Journal title
letters in mathematical physics → ACNP
ISSN journal
03779017
Volume
33
Issue
2
Year of publication
1995
Pages
113 - 125
Database
ISI
SICI code
0377-9017(1995)33:2<113:CPAPSF>2.0.ZU;2-6
Abstract
An exact solution of Dirac's equation in an open Robertson-Walker univ erse is constructed such that the corresponding energy-momentum densit y T(mu nu) obeys the cosmological principle. However, in an open unive rse, this principle must always be violated by the other physical dens ities of the cosmological solution (e.g. pseudoscalar, (axial-) curren t and polarization). If the current density j(mu) = psiBARgamma(mu)PSI is required to obey the cosmological principle, then the universe mus t be flat.