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121“…Dive into a mind-bending exploration of the physics of black holes Black holes, predicted by Albert Einstein's general theory of relativity more than a century ago, have long intrigued scientists and the public with their bizarre and fantastical properties. …”
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122por Loinger, Angelo“…Black holes and gravitational waves are theoretical entities of today astrophysics. …”
Publicado 2002
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123por Villhauer, Elena“…Based on the latest public results, 13 TeV data from the Large Hadron Collider at CERN has not indicated any evidence of hitherto tested models of quantum black holes, semiclassical black holes, or string balls. …”
Publicado 2018
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Enlace del recurso
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124
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125por Aretakis, Stefanos“…This Brief presents in a self-contained, non-technical and illustrative fashion the state-of-the-art results and techniques for the dynamics of extremal black holes. Extremal black holes are, roughly speaking, either maximally rotating or maximally charged. …”
Publicado 2018
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Enlace del recurso
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126“…It then presents black hole solutions, and discusses Penrose diagrams, black hole thermodynamics and entropy, the Unruh effect, Hawking radiation, the black hole information problem, black holes in supergravity and string theory, the black hole microstate counting in string theory, asymptotic symmetries in general relativity, and a particular quantum model for black holes. …”
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Enlace del recurso
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127
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128
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129
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130por Giddings, Steven B.“…A succinct summary is given of the problem of reconciling observation of black hole-like objects with quantum mechanics. If quantum black holes behave like subsystems, and also decay, their information must be transferred to their environments. …”
Publicado 2019
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Enlace del recurso
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131
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132“…We will focus on the Hawking evaporation limits extended to Kerr black holes. In particular, we will discuss the possibility to distinguish between black holes of primordial and of stellar origins based on the Thorne limit on their spin. …”
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Enlace del recurso
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133“…We argue that this result supports the idea of black hole complementarity, which states that, in the description of the black hole system appropriate to outside observers, the region behind the horizon does not establish itself as a classical region of space-time. …”
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Enlace del recurso
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134“…In this report, we provide a detailed discussion of the properties of avalanches driven by two species of charge carriers, e.g. electrons and holes in a semiconductor exposed to an electric field. …”
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135por Verlinde, Erik P.“…About twenty years ago Hawking made the remarkable suggestion that the black hole evaporation process will inevitably lead to a fundamental loss of quantum coherence. …”
Publicado 1995
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136por Wilczek, Frank“…Qualitative introduction to black holes : classical, quantum</br><br>2. Model black holes and model collapse process: The Schwarzschild and Reissner-Nordstrom metrics, The Oppenheimer-Volkov collapse scenario</br><br>3. …”
Publicado 1995
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137por Russo, J.G.“…This approach provides an explanation on why the black hole entropy is of order 1/\h and why it is independent of the number of field-theoretical degrees of freedom.…”
Publicado 1995
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Enlace del recurso
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138por Lupsasca, Alex“…--HTML--><p>What does a black hole look like? The first images of the supermassive black hole M87* display a bright ring encircling the event horizon, which appears as a dark patch in its surrounding emission. …”
Publicado 2023
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139
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140por Russo, Jorge G“…From the postulate that a black hole can be replaced by a boundary on the apparent horizon with suitable boundary conditions, an unconventional scenario for the evolution emerges. …”
Publicado 1996
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Enlace del recurso