Cosmological Role of Weak Currents and a Quasar Model

概要

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A model of the closed universe with a spontaneously broken symmetry is considered. In this model two almost closed oppositely weakly charged CP-noninvariant worlds are joined by long range weak field lines of force flowing through narrow Reissner-Nordstrom type throat(s) connecting the two worlds to form a closed CP-invariant universe as a whole. Such a"pair-creation"model universe may arise from the Kasner type anisotropic cosmo-logical singularity possessing repulsive gravitational potential along certain spatial axis if the domain wall separating CP-noninvariant vacuum domains builds up at the saddle point of the gravitational potential in early stages of the cosmological expansion. During later stages of the cooling down of the universe below a critical temperature, initially massless primeval weak bosons in the universe undergo"superconductive"phase transitions into massive"plasmons", excepting those weak bosons contained in the throat region where the weak boson field lines are maximally contracted beyond the critical intensity. A conjecture is also made on the interpretation of quasistellar radio sources as weakly charged CP-noninvariant almost closed worlds that are joined to our world through the bottleneck structure.
理論物理学刊行会の論文
1976-08-25