Van der Waals black hole
Aruna RajagopalPerimeter Institute, 31 Caroline St. N., Waterloo, Ontario, N2L 2Y5, CanadaDavid KubizňákDepartment of Physics and Astronomy, University of Waterloo, Waterloo, Ontario, N2L 3G1, CanadaRobert B. MannDepartment of Physics and Astronomy, University of Waterloo, Waterloo, Ontario, N2L 3G1, Canada
2014nl
ABI
Annotatsiya
In the context of extended phase space, where the negative cosmological constant is treated as a thermodynamic pressure in the first law of black hole thermodynamics, we find an asymptotically AdS metric whose thermodynamics matches exactly that of the Van der Waals fluid. We show that as a solution of Einstein's equations, the corresponding stress energy tensor obeys (at least for certain range of metric parameters) all three weak, strong, and dominant energy conditions.
Hali tarjima qilinmagan
Identifikatorlar
Iqtiboslar va manbalar
5 ta iqtibos0 ta foydalanilgan manba