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1201“…Work, which does not involve explicit time-evolutions, is discussed, going from rapidly-rotating strange stars to the computation of black-hole-binary initial data. Finally, the evolution of various systems of astrophysical interest are presented, from supernovae core collapse to black-hole-binary mergers.…”
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1202“…The central engines of active galactic nuclei (AGNs) are powered by accreting supermassive black holes, and while AGNs are known to play an important role in galaxy evolution, the key physical processes occur on scales that are too small to be resolved spatially (aside from a few exceptional cases). …”
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1203“…On contrary to the general expectations no energy extraction from black hole was found even though the incident wave packets was fine tuned to be maximally superradiant. …”
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1204“…The symmetric space sine-Gordon models arise by conformal reduction of ordinary 2-dim \sigma-models, and they are integrable exhibiting a black-hole type metric in target space. We provide a Lagrangian formulation of these systems by considering a triplet of Lie groups F \supset G \supset H. …”
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1205por Rudra, Prabir“…The focus is to probe the nature of singularity (black hole or naked singularity) formed out of the collapsing procedure. …”
Publicado 2020
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1206“…We show that a recently proposed solution to the Hierarchy Problem simultaneously solves the Strong CP Problem, without requiring an axion or any further new physics. Consistency of black hole physics implies a non-trivial relation between the number of particle species and particle masses, so that with ~10^{32} copies of the standard model, the TeV scale is naturally explained. …”
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1207por Datta, Shouvik“…This sector is related to the near-horizon region of the near-extremal BTZ black hole in the holographic dual. In this work we generalize this picture to CFTs with higher spin conserved currents. …”
Publicado 2021
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1208por Bakas, Ioannis“…Several gravitational string backgrounds can be interpreted as 2-dim soliton solutions of reduced axion-dilaton gravity. They include black-hole and worm-hole solutions as well as cosmological models with an exact conformal field theory description. …”
Publicado 1996
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1209por Batakis, Nikolaos A.“…The sector of GR solutions which survive is fully classified and it is found to include the Schwarzschild black hole. Two other solutions presented here have no GR counterpart and they describe expanding Friedmann universes with torsion which vanishes only asymptotically. …”
Publicado 1997
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1210“…Parker considering an expanding universe, followed in S. Hawking’s work on black hole radiation. Since their experimental observation is challenging, analogue systems have gained attention in the verification of this concept. …”
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1211“…We discuss our findings in the context of the information paradox assigned to evaporating black holes. A black hole can evaporate entirely, but the smoothness structure of spacetime will be altered and, in this way, the missing information about the initial states of matter forming the black hole will be encoded. …”
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1212por Kaufmann, William J“…The foundations of gravitational theory ; the birth of relativity theory ; the foundations of general relativity ; experimental tests of relativity ; the meaning of the redshift ; the black hole ; wormholes and white holes ; galaxies and quasars ; gravitational waves ; the shape of the Universe ; the creation of the Universe.…”
Publicado 1973
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1213por Fulling, Stephen A“…The theory of quantum fields on curved spacetimes has attracted great attention since the discovery, by Stephen Hawking, of black-hole evaporation. It remains an important subject for the understanding of such contemporary topics as inflationary cosmology…”
Publicado 1989
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1214“…The bound stems from black hole physics. It is similar to the bound appearing in theories with N particle species, though a priori, a large discrete symmetry does not imply a large number of species. …”
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1215“…We evaluate the Wald Noether charge entropy for a black hole in generalized theories of gravity. Expanding the Lagrangian to second order in gravitational perturbations, we show that contributions to the entropy density originate only from the coefficients of two-derivative terms. …”
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1216“…We demonstrate the method by computing the required integrals for black-hole scattering to the second post-Minkowskian order in Einstein gravity coupled to scalars. …”
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1217por Teresi, Daniele“…This semiclassical argument is the analogue, for dS space, of the Black-Hole information paradox. We use techniques developed to address the latter, namely the island formula, to calculate semiclassically the fine-grained entropy as seen by a Minkowskian observer after inflation and find that this follows a Page-like curve, never exceeding the thermodynamic dS entropy. …”
Publicado 2021
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1218“…We also estimate the black hole production rate. We study energy loss from graviton mediated interactions and conclude that they can not explain the cosmic ray events above the GZK energy limit. …”
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1219por Li, Caijuan, Lin, Yingqi, Chen, Yizhi, Song, Xichen, Zheng, Xiao, Li, Jiawei, He, Jun, Chen, Xiusheng, Huang, Chunhui, Wang, Wei, Wu, Jianhao, Wu, Jiaxi, Gao, Jiale, Tu, Zhuchi, Li, Xiao‐Jiang, Yan, Sen, Li, Shihua“…The Huntington protein is transported to the black hole in space via the rocket, symbolizing the interconnectedness of life and the universe. …”
Publicado 2023
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1220“…We connect the attractor equations of a certain class of N=2, d=5 supergravities with their (1,0), d=6 counterparts, by relating the moduli space of non-BPS d=5 black hole/black string attractors to the moduli space of extremal dyonic black string d=6 non-BPS attractors. …”
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