2022AIP conference proceedingsRequires access

Some aspects of modified Hawking mass for two-spheres in Schwarzschild and Reissner-Nordström spacetime

Flinn C. Radjabaycolle

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Abstract

In this paper, we study several aspects of modified Hawking mass (MHM) for two-spheres in Schwarzschild and Reissner-Nordström spacetime. Our purpose is to find the MHM value and its critical points and monotonicity in Schwarzschild and Reissner-Nordström spacetime using conventional calculation methods. The calculations show that MHM is equal to M in Schwarzschild spacetime and is not greater than M in Reissner-Nordström spacetime. In addition, we also find that in Schwarzschild spacetime, MHM has a critical point and is monotone increasing. In contrast, in Reissner-Nordström spacetime, MHM has no critical point and is strictly increasing. These results are in line with our expectations.

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What this paper is about

In this paper, we study several aspects of modified Hawking mass (MHM) for two-spheres in Schwarzschild and Reissner-Nordström spacetime. Our purpose is to find the MHM value and its critical points and monotonicity in Schwarzschild and Reissner-Nordström spacetime using conventional calculation methods. The calculations show that MHM is equal to M in Schwarzschild spacetime and is not greater than M in Reissner-Nordström spacetime. In addition, we also find that in Schwarzschild spacetime, MHM has a critical point and is monotone increasing. In contrast, in Reissner-Nordström spacetime, MHM has no critical point and is strictly increasing. These results are in line with our expectations.

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Available abstract

In this paper, we study several aspects of modified Hawking mass (MHM) for two-spheres in Schwarzschild and Reissner-Nordström spacetime. Our purpose is to find the MHM value and its critical points and monotonicity in Schwarzschild and Reissner-Nordström spacetime using conventional calculation methods. The calculations show that MHM is equal to M in Schwarzschild spacetime and is not greater than M in Reissner-Nordström spacetime. In addition, we also find that in Schwarzschild spacetime, MHM has a critical point and is monotone increasing. In contrast, in Reissner-Nordström spacetime, MHM has no critical point and is strictly increasing. These results are in line with our expectations.

Key concepts: Schwarzschild radius, Spacetime, Physics, Mathematical physics, Photon sphere, Spherically symmetric spacetime, Schwarzschild metric, Quantum field theory in curved spacetime

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