A further generalization of Vaidya's star metric

Details A further generalization of Vaidya's star metric A further generalization of Vaidya's star metric

Dec 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984acaps...4..152w&link_type=abstract

(Acta Astrophysica Sinica, vol. 4, no. 2-3, 1984, p. 152-157) Chinese Astronomy and Astrophysics (ISSN 0275-1062), vol. 8, Dec.

Statistics

Computation

Computational Astrophysics, Gravitational Fields, Reissner-Nordstrom Solution, Stellar Models, Acceleration (Physics), Field Theory (Physics), Space-Time Functions, Stellar Gravitation

Scientific paper

The gravitational field of a point/mass with arbitrary acceleration and charge is investigated analytically, generalizing the metric developed by Vaidya (1951) and expanded by Kinnersley (1969) to obtain a metric comprising five arbitrary time functions and having wide applicability. The formulation of Newman and Penrose (1962) is used for the field equations, and the metric derived is shown to reduce to a Reissner-Nordstroem metric in a particular case.

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