Modifying horizon thermodynamics by surface tensions
Author:
Publisher
Springer Science and Business Media LLC
Subject
Physics and Astronomy (miscellaneous)
Link
http://link.springer.com/content/pdf/10.1007/s10714-019-2617-z.pdf
Reference46 articles.
1. Padmanabhan, T.: Classical and quantum thermodynamics of horizons in spherically symmetric spacetimes. Class. Quant. Grav. 19, 5387 (2002). arXiv:gr-qc/0204019
2. Cai, R.G.: Connections between gravitational dynamics and thermodynamics. J. Phys. Conf. Ser. 484, 012003 (2014)
3. Sarkar, S., Kothawala, D.: Hawking radiation as tunneling for spherically symmetric black holes: a generalized treatment. Phys. Lett. B 659, 683 (2008). arXiv:0709.4448 [gr-qc]
4. Padmanabhan, T., Kothawala, D.: Lanczos–Lovelock models of gravity. Phys. Rep. 531, 115 (2013). arXiv:1302.2151 [gr-qc]
5. Kothawala, D., Sarkar, S., Padmanabhan, T.: Einstein’s equations as a thermodynamic identity: the cases of stationary axisymmetric horizons and evolving spherically symmetric horizons. Phys. Lett. B 652, 338 (2007). arXiv:gr-qc/0701002
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