Recovering information of tunneling spectrum from Weakly Isolated Horizon
arXiv:1406.0330 · doi:10.1140/epjc/s10052-015-3272-5
Abstract
In this paper we investigate the properties of tunneling spectrum from weakly isolated horizon(WIH). We find that there are correlations among Hawking radiations from weakly isolated horizon, the information can be carried out in terms of correlations between sequential emissions, and the radiation is an entropy conservation process. We generalize Refs.[11-13]' results to a more general spacetime. Through revisiting the calculation of tunneling spectrum of weakly isolated horizon, we find that Ref.[12]'s requirement that radiating particles have the same angular momenta of unit mass as that of black hole is not needed, and the energy and angular momenta of emitting particles are very arbitrary which should be restricted only by keeping the cosmic censorship of black hole.
References in corpus (16)
- Hawking Radiation as Tunneling
- The information paradox: A pedagogical introduction
- Isolated and dynamical horizons and their applications
- D-brane Approach to Black Hole Quantum Mechanics
- Information Loss in Black Holes
- A Secret Tunnel Through The Horizon
- Mechanics of Rotating Isolated Horizons
- Hawking Radiation as Tunneling through the Quantum Horizon
- Charged particles' tunnelling from the Kerr-Newman black hole
- Geometry of Generic Isolated Horizons
- Mechanics of Isolated Horizons
- Hidden Messenger Revealed in Hawking Radiation: a Resolution to the Paradox of Black Hole Information Loss
- Entropy is Conserved in Hawking Radiation as Tunneling: a Revisit of the Black Hole Information Loss Paradox
- Information conservation is fundamental: recovering the lost information in Hawking radiation
- Tunneling Effect Near Weakly Isolated Horizon
- The spacetime in the neighborhood of a general isolated black hole