scholarly journals Fluxes of higher-spin currents and Hawking radiation from charged black holes

2007 ◽  
Vol 76 (6) ◽  
Author(s):  
Satoshi Iso ◽  
Takeshi Morita ◽  
Hiroshi Umetsu
Keyword(s):  
Black Holes ◽  
Hawking Radiation ◽  
Charged Black Holes ◽  
Spin Currents ◽  
Higher Spin

scholarly journals Higher-spin currents and thermal flux from Hawking radiation

2007 ◽  
Vol 75 (12) ◽  
Author(s):  
Satoshi Iso ◽  
Takeshi Morita ◽  
Hiroshi Umetsu
Keyword(s):  
Hawking Radiation ◽  
Thermal Flux ◽  
Spin Currents ◽  
Higher Spin

scholarly journals GRAVITATIONAL ANOMALIES: A RECIPE FOR HAWKING RADIATION

2008 ◽  
Vol 17 (03n04) ◽  
pp. 533-539 ◽  
Author(s):  
SAURYA DAS ◽  
SEAN P. ROBINSON ◽  
ELIAS C. VAGENAS
Keyword(s):  
Black Holes ◽  
Hawking Radiation ◽  
Effective Theory ◽  
General Covariance ◽  
Quantum Level ◽  
Gravitational Anomaly ◽  
Charged Black Holes ◽  
Black Rings ◽  
Rotating Black Holes ◽  
Arbitrary Space

We explore the method of Robinson and Wilczek for deriving the Hawking temperature of a black hole. In this method, the Hawking radiation restores general covariance in an effective theory of near-horizon physics which otherwise exhibits a gravitational anomaly at the quantum level. The method has been shown to work for broad classes of black holes in arbitrary space–time dimensions. These include static black holes, accreting or evaporating black holes, charged black holes, rotating black holes, and even black rings. In the cases of charged and rotating black holes, the expected superradiant current is also reproduced.

scholarly journals Islands and stretched horizon

2021 ◽  
Vol 2021 (7) ◽  
Author(s):  
Yoshinori Matsuo
Keyword(s):  
Black Holes ◽  
Black Hole ◽  
Hawking Radiation ◽  
Entanglement Entropy ◽  
Total System ◽  
Island Rule ◽  
Asymptotically Flat ◽  
Flat Spacetime ◽  
Ads Spacetime ◽  
Hole Geometry

Abstract Recently it was proposed that the entanglement entropy of the Hawking radiation contains the information of a region including the interior of the event horizon, which is called “island.” In studies of the entanglement entropy of the Hawking radiation, the total system in the black hole geometry is separated into the Hawking radiation and black hole. In this paper, we study the entanglement entropy of the black hole in the asymptotically flat Schwarzschild spacetime. Consistency with the island rule for the Hawking radiation implies that the information of the black hole is located in a different region than the island. We found an instability of the island in the calculation of the entanglement entropy of the region outside a surface near the horizon. This implies that the region contains all the information of the total system and the information of the black hole is localized on the surface. Thus the surface would be interpreted as the stretched horizon. This structure also resembles black holes in the AdS spacetime with an auxiliary flat spacetime, where the information of the black hole is localized at the interface between the AdS spacetime and the flat spacetime.

scholarly journals CFT duals on rotating charged black holes surrounded by quintessence

2021 ◽  
Vol 31 ◽  
pp. 100778
Author(s):  
Muhammad F.A.R. Sakti ◽  
Freddy P. Zen
Keyword(s):  
Black Holes ◽  
Charged Black Holes
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