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241“…An optical black-hole cavity based on transformation optics enables Q-factor enhancement and strong field confinement, by eliminating the intrinsic radiation loss of the conventional whispering-gallery modes, holding potential for applications in energy harvesting and optoelectronics.…”
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242“…The spectrum of known black-hole solutions to the stationary Einstein equations has been steadily increasing, sometimes in unexpected ways. …”
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243por Heusler, Markus“…The spectrum of known black hole solutions to the stationary Einstein equations has increased in an unexpected way during the last decade. …”
Publicado 1998
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244por Camporota, Luigi, Chiumello, Davide, Busana, Mattia, Romitti, Federica, Gattinoni, LucianoEnlace del recurso
Publicado 2020
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245por Barrow, John D.“…We investigate the consequences for the black hole area of introducing fractal structure for the horizon geometry. …”
Publicado 2020
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246“…Black hole (BH) collisions produce gravitational radiation which is generally thought, in a quantum limit, to be gravitons. …”
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247por Katayama, Haruna“…A black hole laser in analogues of gravity amplifies Hawking radiation, which is unlikely to be measured in real black holes, and makes it observable. …”
Publicado 2021
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248“…This volume brings together contributions from many of the world's leading authorities on black hole accretion. The papers within represent part of a new movement to make use of the relative advantages of studying stellar mass and supermassive black holes and to bring together the knowledge gained from the two approaches. …”
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249Publicado 2008“…Black holes, topological strings and extremal black holes and AdS2/CFT1 correspondence…”
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250“…According to the horizon fluff proposal microstates of a generic black hole belong to a certain subset of near horizon soft hairs that cannot be extended beyond the near horizon region. …”
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251“…We report on recent advances in the study of critical points of the ``black hole effective potential'' V_{BH} (usually named \textit{attractors}) of N=2, d=4 supergravity coupled to n_{V} Abelian vector multiplets, in an asymptotically flat extremal black hole background described by 2n_{V}+2 dyonic charges and (complex) scalar fields which are coordinates of an n_{V}-dimensional Special Kahler manifold.…”
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252por Hajdukovic, D“…In the next few years, theories predicting possibility to create mini black holes will be tested at CERN. Either experimental verification or rejection of these theories is of great scientific importance. …”
Publicado 2007
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253
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254“…We study five-dimensional black holes obtained by compactifying M theory on Calabi-Yau threefolds. …”
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255por Vergano, Dan“…An upcoming study adds to the long history, suggesting blakc holes, now almost taken for granted, never actually comme fully into existence, and that the solution to a decades-old black hole paradox may be simpler than supposed. (1 page)…”
Publicado 2007
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256“…Gravitational greybody factors are analytically computed for static, spherically symmetric black holes in d-dimensions, including black holes with charge and in the presence of a cosmological constant (where a proper definition of greybody factors for both asymptotically dS and AdS spacetimes is provided). …”
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257
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258“…We construct extremal, spherically symmetric black hole solutions to 4D supergravity with charge assignments that preclude BPS-saturation. …”
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259“…These lectures provide a pedagogical, introductory review of the so-called Attractor Mechanism (AM) at work in two different 4-dimensional frameworks: extremal black holes in N=2 supergravity and N=1 flux compactifications. …”
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260“…Black hole formation may occur if the spectrum of the curvature perturbation \zeta increases strongly as the scale decreases. …”
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