WebMar 30, 2024 · We show that in the mentioned class of ESTGB theories there exist new black-hole solutions that are formed by spontaneous scalarization of the Schwarzschild black holes in the extreme curvature regime. WebNov 3, 2024 · Scalarization is a mechanism that endows strongly self-gravitating bodies, such as neutron stars and black holes, with a scalar field configuration. It resembles a phase transition in that the scalar configuration only appears when a certain quantity that characterizes the compact object, e.g., its compactness or spin, is beyond a threshold. …
Critical Phenomena in Dynamical Scalarization of Charged Black Holes.
WebJul 4, 2024 · We consider a class of scalar-Gauss-Bonnet gravity theories within which no tachyonic instability can occur. Although the Schwarzschild black holes are linearly stable against scalar perturbations, we show dynamically that for certain choices of the coupling function they are unstable against nonlinear scalar perturbations. WebFeb 3, 2024 · The simplest way to answer this question would be to compare the spectra of stellar-mass and supermassive black holes before and after a state transition, to see if the spectra evolve in the same way. … black heath meadery richmond
Extreme black holes have hair that can be combed - Phys.org
WebA black hole is a region of spacetime where gravity is so strong that nothing, including light or other electromagnetic waves, has enough energy to escape its event horizon. [2] The … WebAug 17, 2024 · In Gauss-Bonnet gravity the source of the scalar field can be the curvature of the space-time. It was recently shown that for a particular type of coupling function between the scalar field and the Gauss-Bonnet invariant, … WebThe Bondi radius ( Bondi, 1952) is the radius of the sphere of gravitational influence of the black hole. A test mass inside this sphere feels the gravitational presence of the black hole. As it is derived from setting the … game xchange longview