Results 61 to 70 of about 707,832 (374)

Can a false vacuum bubble remove the singularity inside a black hole?

open access: yesEuropean Physical Journal C: Particles and Fields, 2020
We investigate a regular black hole model with a de Sitter-like core at its center. This type of a black hole model with a false vacuum core was introduced with the hope of singularity-resolution and is a common feature shared by many regular black holes.
Suddhasattwa Brahma, Dong-han Yeom
doaj   +1 more source

Colliding gravitational waves and singularities

open access: yesInternational Journal of Modern Physics A, 2023
We have investigated a model of colliding plain gravitational waves, proposed by Szekeres, whose structure of singularities is determined. We have evaluated a total energy of matter as a volume integral of the energy–momentum tensor (EMT), whose contributions arise only at these singularities. The total matter energy is conserved before a collision of
openaire   +2 more sources

Einstein-Klein-Gordon system by gravitational decoupling [PDF]

open access: yesEurophysics letters, 2018
We investigate how a spherically symmetric scalar field can modify the Schwarzschild vacuum solution when there is no exchange of energy-momentum between the scalar field and the central source of the Schwarzschild metric.
J. Ovalle   +6 more
semanticscholar   +1 more source

The Central Singularity in Spherical Collapse [PDF]

open access: yes, 2000
The gravitational strength of the central singularity in spherically symmetric space-times is investigated. Necessary conditions for the singularity to be gravitationally weak are derived and it is shown that these are violated in a wide variety of ...
A. Krasiński   +22 more
core   +2 more sources

Newtonian Analysis of Gravitational Waves from Naked Singularity [PDF]

open access: yes, 2000
Spherical dust collapse generally forms a shell focusing naked singularity at the symmetric center. This naked singularity is massless. Further the Newtonian gravitational potential and speed of the dust fluid elements are everywhere much smaller than ...
A. Ori   +34 more
core   +2 more sources

Instability of black hole formation under small pressure perturbations [PDF]

open access: yes, 2012
We investigate here the spectrum of gravitational collapse endstates when arbitrarily small perfect fluid pressures are introduced in the classic black hole formation scenario as described by Oppenheimer, Snyder and Datt (OSD) [1].
A Ori   +44 more
core   +3 more sources

Does a primary hair have an impact on the naked singularity formation in hairy Vaidya spacetime?

open access: yesPhysics of Complex Systems
We consider the gravitational collapse of Vaidya spacetime, which has been obtained using the gravitational decoupling method. In this paper, we are interested in whether a primary hair has any impact on the endstate of the gravitational collapse.
Виталий Дмитриевич Вертоградов
doaj   +1 more source

Matter and gravitons in the gravitational collapse

open access: yesPhysics Letters B, 2016
We consider the effects of gravitons in the collapse of baryonic matter that forms a black hole. We first note that the effective number of (soft off-shell) gravitons that account for the (negative) Newtonian potential energy generated by the baryons is ...
Roberto Casadio   +2 more
doaj   +1 more source

The spectrum of endstates of gravitational collapse with tangential stresses [PDF]

open access: yes, 2001
The final state--black hole or naked singularity--of the gravitational collapse of a marginally bound matter configuration in the presence of tangential stresses is classified, in full generality, in terms of the initial data and equation of state.
A. Ori   +21 more
core   +2 more sources

Towards conditions for black-hole singularity-resolution in asymptotically safe quantum gravity [PDF]

open access: yesClassical and quantum gravity, 2018
We explore the fate of the curvature singularity of Schwarzschild (deSitter) black holes in asymptotically safe quantum gravity. Specifically, we upgrade the classical spacetime by including the running of the Newton coupling and cosmological constant ...
Adémọ́lá Adéìfẹ́ọba   +2 more
semanticscholar   +1 more source

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