Gennaro, Sofia Di; Good, Michael R. R.; Ong, Yen Chin(PHYSICAL REVIEW RESEARCH, 2022)
We show that the notion of “Hookean law” F = kx, suitably defined in asymptotically flat singly spinning
Myers-Perry black hole space-times in dimensions d 5, is related to the Emparan-Myers fragmentation
(splitting ...
Good, Michael R. R.; Singha, Chiranjeeb; Zarikas, Vasilios(Entropy, 2022)
We examine the extreme situation of radiation from an electron that is asymptotically accelerated to the speed of light, resulting in finite emission energy. The analytic solution explicitly demonstrates the difference ...
Modeling the collapse of an extreme Reissner-Nordstr¨om (ERN) black hole by solving the corre sponding moving mirror model for the trajectory that asymptotically approaches uniform accelera tion, we obtain the non-zero ...
Zhakenuly, Abay; Good, Michael R.R.; Linder, Eric V.(arxiv, 2020)
An accelerated boundary correspondence (ABC) is solved for the de Sitter moving mirror cos mology. The beta Bogoliubov coefficients reveal the particle spectrum is a Planck distribution with
temperature inversely proportional ...
Fernandez-Silvestre, Diego; Foo, Joshua; Good, Michael R.R.(Classical and Quantum Gravity, 2022)
The Schwarzschild-de Sitter (SdS) metric is the simplest spacetime solution in general relativity with both a
black hole event horizon and a cosmological event horizon. Since the Schwarzschild metric is the most ...
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