Surface temperature of a rotating charged body

Details Surface temperature of a rotating charged body Surface temperature of a rotating charged body

Dec 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984acaps...4..158c&link_type=abstract

(Acta Astrophysica Sinica, vol. 4, no. 2-3, 1984, p. 158-165) Chinese Astronomy and Astrophysics (ISSN 0275-1062), vol. 8, Dec.

Statistics

Computation

Computational Astrophysics, Pulsars, Rotating Bodies, Surface Temperature, Gravitons, Stellar Temperature, Temperature Distribution

Scientific paper

The Kerr-Newman metric (Newman, 1965) and the vector-graviton metric (Qian, 1979) are applied separately to investigate the surface-temperature distribution of a rotating charged body. The case of a pulsar of mass 2 x 10 to the 34th g, radius 30 km, and surface temperature 10 to the 7th K is considered, and it is found that the temperature difference between the equator and polar regions is about 30,000 K for the Kerr-Newman metric and about 820 for the vector-graviton metric.

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