publication . Article . Preprint . 2007

A statistical mechanical problem in Schwarzschild spacetime

David Klein;
Open Access
  • Published: 14 Mar 2007 Journal: General Relativity and Gravitation, volume 39, pages 737-755 (issn: 0001-7701, eissn: 1572-9532, Copyright policy)
  • Publisher: Springer Science and Business Media LLC
We use Fermi coordinates to calculate the canonical partition function for an ideal gas in a circular geodesic orbit in Schwarzschild spacetime. To test the validity of the results we prove theorems for limiting cases. We recover the Newtonian gas law subject only to tidal forces in the Newtonian limit. Additionally we recover the special relativistic gas law as the radius of the orbit increases to infinity. We also discuss how the method can be extended to the non ideal gas case.
arXiv: Astrophysics::Galaxy AstrophysicsAstrophysics::Earth and Planetary Astrophysics
free text keywords: Physics and Astronomy (miscellaneous), General Relativity and Quantum Cosmology
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