Cosmions in the nonsymmetric gravitational theory

J. W. Moffat
Phys. Rev. D 39, 474 – Published 15 January 1989; Erratum Phys. Rev. D 40, 683 (1989)
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Abstract

A phenomenological model is presented for the conserved fermion-number current in the nonsymmetric gravitational theory (NGT) based on the numbers of stable protons, neutrons, neutrinos, and cosmions (weakly interacting massive particles). By a suitable choice of the coupling constants, it is shown that the NGT is consistent with terrestrial observations and with the data for the solar system. A fit to the data of seven nondegenerate binary systems, including the data for DI Herculis and AS Cam, is given. The overall results are in accord with a solution of the problem of the cosmological missing dark matter. Agreement is also achieved with the data for the pulsar system PSR 1913 + 16 and the close cataclysmic binary system 4U 1820-30, involving gravitational radiation.

  • Received 9 May 1988

DOI:https://doi.org/10.1103/PhysRevD.39.474

©1989 American Physical Society

Erratum

Erratum: Cosmions in the nonsymmetric gravitational theory

J. W. Moffat
Phys. Rev. D 40, 683 (1989)

Authors & Affiliations

J. W. Moffat

  • Laboratoire de Physique Théorique et Hautes Énergies, Université de Paris XI, Bâtiment 211, Orsay, France

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Issue

Vol. 39, Iss. 2 — 15 January 1989

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