Chiral black hole in three-dimensional gravitational Chern-Simons

Details Chiral black hole in three-dimensional gravitational Chern-Simons Chiral black hole in three-dimensional gravitational Chern-Simons

2008-12-28

arxiv.org/abs/0812.4790v2

Mod.Phys.Lett.A24:1829-1834,2009

Physics

High Energy Physics

High Energy Physics - Theory

6 pages, a reference added, minor changes to introduction

Scientific paper

10.1142/S0217732309031181

A chiral black hole can be defined from the three-dimensional pure gravitational Chern-Simons action as an independent gravitational theory. The third order derivative of the Cotton tensor gives a dimensional constant which plays a role of the cosmological constant. The handedness of angular momentum depends on the signature of the Chern-Simons coefficient. Even in the massless black hole which corresponds to the static black hole, it has a nonvanishing angular momentum. We also study statistical entropy and thermodynamic stability.

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