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• W3149697229 startingPage "2150060" @default.
• W3149697229 abstract "We discuss the merger process of binary black holes with Hawking radiation taken into account. Besides the redshifted radiation to infinity, binary black holes can exchange radiation between themselves, which is first redshifted and then blueshifted when it propagates from one hole to the other. The exchange rate should be large when the temperature-divergent horizons are penetrating each other to form a single horizon with unique temperature. This will cause non-negligible mass and angular momentum transfer between the black holes during the merging process of the horizons. We further argue in the large mass ratio limit that the light hole whose local evaporation is enhanced by the competing redshift-blueshift effects will probably evaporate or decay completely before reaching the the horizon of the heavy one. We also discuss the possibility of testing Hawking radiation and even exploring the information loss puzzle in gravitational wave observations." @default.
• W3149697229 created "2021-04-13" @default.
• W3149697229 creator A5000168358 @default.
• W3149697229 creator A5051858605 @default.
• W3149697229 date "2021-04-29" @default.
• W3149697229 modified "2023-09-27" @default.
• W3149697229 title "Towards the merger of Hawking radiating black holes" @default.
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• W3149697229 doi "https://doi.org/10.1142/s0218271821500607" @default.
• W3149697229 hasPublicationYear "2021" @default.
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