Tightening the Penrose inequality
نویسندگان
چکیده
The Penrose inequality estimates the lower bound of mass a black hole in terms area its horizon. This is relatively loose for extremal or near holes. We propose new Penrose-like static holes involving mass, event horizon and temperature. Our includes as corollary, it saturated by both Schwarzschild Reissner-Nordström In spherically symmetric case, we prove this assuming null trace energy conditions.
منابع مشابه
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ژورنال
عنوان ژورنال: Science China Physics, Mechanics & Astronomy
سال: 2022
ISSN: ['1869-1927', '1674-7348']
DOI: https://doi.org/10.1007/s11433-022-2016-3