Complex Kerr-Newman geometry and black-hole thermodynamics

Details Complex Kerr-Newman geometry and black-hole thermodynamics Complex Kerr-Newman geometry and black-hole thermodynamics

May 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991phrvl..66.2281b&link_type=abstract

Physical Review Letters (ISSN 0031-9007), vol. 66, May 6, 1991, p. 2281-2284.

Astronomy and Astrophysics

Astronomy

96

Black Holes (Astronomy), Space-Time Functions, Stellar Rotation, Thermodynamic Properties, Electromagnetic Fields, Formalism, Gravitational Fields

Scientific paper

It is established that in the functional-integral expression for the
grand partition function, the thermodynamic properties of a charged,
rotating black hole are derived from a complex geometry. The
corresponding real 'thermodynamical' action is constructed explicitly.

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