Results 131 to 140 of about 99,723 (258)
Wormholes in spacetime and their use for interstellar travel: A tool for teaching general relativity
M. S. Morris, K. Thorne
semanticscholar +1 more source
Scalarizations of qOS-extremal black hole and Aretakis instability
We study scalarization of quantum Oppenheimer–Snyder (qOS)-extremal black hole in the Einstein–Gauss–Bonnet-scalar theory. This black hole is described by mass ( $$M=4\sqrt{\alpha }/3\sqrt{3}$$ M = 4 α / 3 3 ) with $$\alpha $$ α quantum parameter ...
Yun Soo Myung
doaj +1 more source
Shadow radius and classical scattering analysis of two secondary hair Horndeski black holes
We perform the shadow radius analysis of a charged Horndeski black hole (CHB) and the naked singularity (NS) with secondary scalar hair obtained from the Einstein-Horndeski-Maxwell theory. For this analysis, we include the beyond Horndeski black hole (bH)
Yun Soo Myung
doaj +1 more source
On completeness and dynamics of compact Brinkmann spacetimes [PDF]
Lilia Mehidi, Abdelghani Zeghib
openalex +1 more source
We undertake a comprehensive analysis of the supersymmetric partition function of the U(N) k × U(N) −k ABJM theory on a U(1) fibration over a Riemann surface, evaluating it to all orders in the 1/N-perturbative expansion up to exponentially suppressed ...
Junho Hong
doaj +1 more source
Topological properties of curved spacetime Su-Schrieffer-Heeger model [PDF]
Priyanuj Rajbongshi, Ranjan Modak
openalex +1 more source
Optimal transport and timelike lower Ricci curvature bounds on Finsler spacetimes [PDF]
Mathias Braun, Shin‐ichi Ohta
openalex +1 more source
Differential topology and micro-structure of black hole in Einstein–Euler–Heisenberg spacetimes with exponential entropy [PDF]
Yasir Muhammad +2 more
openalex +1 more source
We obtain quantum parameter ( $$\alpha $$ α )-mass (M) induced spontaneous scalarization of quantum Oppenheimer–Snyder (qOS)-black hole in the Einstein–Gauss–Bonnet-scalar theory with the unknown qOS action.
Yun Soo Myung
doaj +1 more source
Thermodynamic analysis and shadow bound of black holes surrounded by a dark matter halo
We perform the thermodynamic analysis of a black hole (BH) immersed in a dark matter halo (DMH). It is shown that the BH could not be in thermal equilibrium with the DMH in any regions outside the event horizon.
Yun Soo Myung
doaj +1 more source

