EXTREMAL BLACK HOLES AND THE LIMITS OF THE THIRD LAW

DOI10.1142/S0218271801000937zbMath1155.83347arXivgr-qc/0008018OpenAlexW2089245374WikidataQ62580940 ScholiaQ62580940MaRDI QIDQ3376487

Sebastiano Sonego, Tony Rothman, Stefano Liberati

Publication date: 23 March 2006

Published in: International Journal of Modern Physics D (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/gr-qc/0008018

Mathematics Subject Classification ID

Black holes (83C57) Quantum field theory on curved space or space-time backgrounds (81T20) Methods of quantum field theory in general relativity and gravitational theory (83C47)

Related Items

TWO-DIMENSIONAL DILATONIC BLACK HOLES AND HAWKING RADIATION, ENTROPY OF SEMICLASSICAL 2D DILATON BLACK HOLES AWAY FROM THE HAWKING TEMPERATURE, Bounded energy exchange as an alternative to the third law of thermodynamics, Is the semi-classical analysis valid for extreme black holes?, ZERO SURFACE GRAVITY BLACK HOLES AND THE FAILURE OF SEMICLASSICAL ANALYSIS

Cites Work

• Particle creation by black holes
• Hamiltonian evolution and quantization for extremal black holes
• The gravitational Hamiltonian, action, entropy and surface terms