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=1984cha%26a...8..286c&link_type=abstract

Chinese Astronomy and Astrophysics, Volume 8, Issue 4, p. 286-289.

Astronomy and Astrophysics

Astrophysics

Scientific paper

The surface temperature of a rotating, charged body is found separately under the Kerr-Newman metric and the vector graviton metric. Particular reference is made to pulsars. It is found that, 1) under the Kerr-Newman metric, the surface temperature rises from the poles to the equator, when the radius R of the body is greater than a certain critical value, rn. When R= rn, the surface temperature is uniform. When R < rn, the above gradient is reversed. For pulsars, the equatorial temperature is some 3 × 104 K higher than the polar temperature. 2) Under the Vector graviton field metric, a similar temperature differential exists, but it is much smaller in size.

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