Results 141 to 150 of about 115,140,986 (222)
Charged AdS black holes in presence of string cloud and Cardy-Verlinde formula
Nuclear Physics BIn this study, charged AdS black holes with a string cloud are taken into consideration. We identify three distinct black hole solutions within a specific temperature range, which subsequently merge into a single black hole beyond this range in the case ...
Rishi Pokhrel, Tanay K. Dey
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Size and shape of rotating strings and the correspondence to black holes
Journal of High Energy PhysicsIn light of the correspondence between black holes and fundamental strings with non-zero spin, we compute the sizes of rotating strings for small, moderate, and large values of the angular momentum and compare them to the sizes of rotating black holes ...
Nejc Čeplak +3 more
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, 1997 9 pages, LaTeX, uses included style file `weird.sty', to appear in the proceedings of the 7th Canadian Conference on General Relativity and Relativistic Astrophysics, June 5-7 ...
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Rotating Einstein-Maxwell black holes in odd dimensions
Journal of High Energy PhysicsTo construct higher-dimensional counterparts of the Kerr-Newman black holes, we consider Einstein’s equations sourced by a vector field and a negative cosmological constant.
Rhucha Deshpande, Oleg Lunin
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, 2019 Black holes are the hydrogen atoms of quantum gravity. For instance solving the information loss paradox will likely require a deep understanding of how the long-sought quantum gravity theory works. In this thesis we explore how black holes are modelled and how the quantum structure emerges in the context of string theory.
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Towards Hamiltonian formalism for string field theory and nonlocality
Journal of High Energy PhysicsString field theories exhibit exponential suppression of interactions among the component fields at high energies due to infinite-derivative factors such as e ℓ 2 □ / 2 $$ {e}^{\ell^2\square /2} $$ in the vertices.
Chih-Hao Chang +3 more
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Kalb-Ramond field, black holes and black strings in (2 + 1)D
Journal of High Energy PhysicsNew rotating dilaton black hole and black string solutions in three spacetime dimensions are obtained. The solutions are asymptotically flat and, they are exact in classical string theory. The black hole solutions have only a single horizon.
Meseret Asrat
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Dichotomy of heavy and light pairs of holes in the t-J model. [PDF]
Nat Commun, 2023 Bohrdt A, Demler E, Grusdt F.
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On quivers, spectral networks and black holes. [PDF]
Lett Math PhysArnaudo P, Grassi A, Hao Q.
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