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601“…Primordial Black Holes (PBH's) can form in the early Universe from the collapse of large density fluctuations. …”
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602“…The quantum degeneracies of single-centered black holes are Fourier coefficients of this mock Jacobi form, while the Appell-Lerch sum captures the degeneracies of multi-centered black holes which decay upon wall-crossing. …”
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603por Tsang, Ka Vang“…A search for microscopic black hole production and decay in proton-proton collisions at a center-of-mass energy of 7 TeV has been conducted using Compact Muon Solenoid (CMS) detector at the CERN Large Hadron Collider. …”
Publicado 2013
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604“…We reconstruct the complete fermionic orbit of the non-extremal BTZ black hole by acting with finite supersymmetry transformations. …”
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605
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606por Gribbin, John“…Acclaimed science writer John Gribbin recounts dramatic stories that have led scientists to believe black holes and their more mysterious kin are not only real, but might actually provide a passage to other universes and travel through time.…”
Publicado 1992
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607por Prof. Günther Hasinger (Max-Planck-Institut für extraterrestrische Physik, Garching)“…--HTML-->In the last few years a change of paradigm occurred in the field of black hole research. We now believe, that stellar mass black holes are created in powerful gamma ray bursts. …”
Publicado 2004
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608“…In this article we describe new algorithms to select prompt or non-prompt jet and black hole--like objects in the silicon tracker.…”
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609“…Furthermore, we show how, using these operators, it is possible to reconcile small corrections to effective field theory correlators with the unitarity of black hole evaporation. We address and resolve all other arguments, advanced in arxiv:1304.6483 and arxiv:1307.4706, in favour of structure at the black hole horizon. …”
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610por Dvali, Georgi“…--HTML-->We review physics of black holes, both large and small, from a particle physicist's perspective, using particle physics tools for describing concepts such as entropy, temperature and quantum information processing. …”
Publicado 2014
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611por Dvali, Georgi“…--HTML-->We review physics of black holes, both large and small, from a particle physicist's perspective, using particle physics tools for describing concepts such as entropy, temperature and quantum information processing. …”
Publicado 2014
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612“…We revisit the "state-dependence" of the map that we proposed recently between bulk operators in the interior of a large AdS black hole and operators in the boundary CFT. By refining recent versions of the information paradox, we show that this feature is necessary for the CFT to successfully describe local physics behind the horizon --- not only for single-sided black holes but even in the eternal black hole. …”
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613
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614por Levin, Janna“…From the author of How the Universe Got Its Spots and A Madman Dreams of Turing Machines, the epic story of the scientific campaign to record the soundtrack of our universe. Black holes are dark. That is their essence. When black holes collide, they will do so unilluminated. …”
Publicado 2016
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615por Bambi, Cosimo“…Black holes are one of the most fascinating predictions of general relativity and are currently a very hot topic in both physics and astrophysics. …”
Publicado 2016
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616por Wald, Robert M“…In particular, the subject of black hole thermodynamics, which remains an active area of research, is treated in depth. …”
Publicado 1994
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617“…We study the effect of primordial black holes on the classical rate of nucleation of AdS regions within the standard electroweak vacuum at high temperature. …”
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618por Wandler, Frank David“…Monte Carlo simulation of quantum black hole production in the ATLAS experiment that allows for graviton radiation in the initial state is discussed and studied. …”
Publicado 2017
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619“…Arguments are also given that the enormous number of string {\it discrete (topological)} states account for the maintenance of quantum coherence during the (non-thermal) stringy evaporation process, as well as quenching the large Hawking-Bekenstein entropy associated with the black hole. Defining the latter as the measure of the loss of information for an observer at infinity, who - ignoring the higher string quantum numbers - keeps track only of the classical mass,angular momentum and charge of the black hole, one recovers the familiar a quadratic dependence on the black-hole mass by simple counting arguments on the asymptotic density of string states in a linear-dilaton background.…”
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