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503por Chitishvili, Mariam, Gogberashvili, Merab, Konoplich, Rostislav, Sakharov, Alexander S.“…We conjecture that the Higgs potential can be significantly modified when it is in close proximity to the horizon of an astrophysical black hole, leading to the destabilization of the electroweak vacuum. …”
Publicado 2021
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504por Auffinger, Jérémy, Arbey, Alexandre, Sandick, Pearl, Haghi, Barmak Shams Es, Sinha, Kuver“…Light black holes could have formed in the very early universe through the collapse of large primordial density fluctuations. …”
Publicado 2022
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505
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506“…In modern theoretical ideas related to the concept of extra dimensions and multidimensional low-energy gravity, one can expect to observe the creation of the microscopic black holes at the LHC in proton-proton collisions at currently available energies.…”
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507
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508“…It has been recently pointed out that nonlinear effects are necessary to model the ringdown stage of the gravitational waveform produced by the merger of two black holes giving rise to a remnant Kerr black hole. …”
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509“…In a recent paper, Duff and Rahmfeld argued that certain massive N_R=1/2 states of the four-dimensional heterotic string correspond to extreme black hole solutions. We provide further, dynamical, evidence for this identification by comparing the scattering of these elementary string states with that of the corresponding extreme black holes, in the limit of low velocities.…”
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510“…In this paper, we extend our analysis of photon propagation in gravitational backgrounds to the Kerr spacetime describing a rotating black hole. The results support two general theorems -- a polarisation sum rule and a `horizon theorem'. …”
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511“…We give analytical arguments and demonstrate numerically the existence of black hole solutions of the 4D Effective Superstring Action in the presence of Gauss-Bonnet quadratic curvature terms. …”
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512
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513“…We compute the degeneracy for fixed charge and find it to be in accordance with U-duality (which in our formulation is manifest in six dimensions) and the statistical entropy formula of the corresponding black hole. We also briefly comment on the four-dimensional case.…”
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514“…We give analytical arguments and demonstrate numerically the existence of black hole solutions with non-trivial dilaton and Yang Mills hair for the particular case of SU(2) gauge fields. …”
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515por Behrndt, K, Lópes-Cardoso, G, de Wit, Bernard, Kallosh, Renata E, Lüst, Dieter, Mohaupt, T“…We use heterotic/type-II prepotentials to study quantum/classical black holes with half the $N=2, D=4$ supersymmetries unbroken. …”
Publicado 1996
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516
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517“…These invariants give a general definition of the ``topological'' Bekenstein-Hawking entropy formula for extremal black-holes and reduce to the square of the black-hole ADM mass for ``fixed scalars'' which extremize the black-hole ``potential'' energy. …”
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518“…We consider axion-free quantum corrected black hole solutions in the context of the heterotic S-T model with half the N=2, D=4 supersymmetries unbroken. …”
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519“…Four-dimensional supersymmetric massless black holes are the T duals in time of massive supersymmetric black holes. …”
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520por Ghosh, A.“…A one-dimensional gas model has been constructed and shown to provide correct expressions for entropies for extremal and near-extremal BTZ black holes. Recently suggested boosting of black strings is used to compute the entropy for the Schwarzschild black hole also from this gas model.…”
Publicado 1998
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