Results 41 to 50 of about 1,024,610 (340)
Black holes die hard: can one spin-up a black hole past extremality?
A possible process to destroy a black hole consists on throwing point particles with sufficiently large angular momentum into the black hole. In the case of Kerr black holes, it was shown by Wald that particles with dangerously large angular momentum are
Andrea Nerozzi +4 more
core +1 more source
Stimulated by the recent researches of black hole thermodynamics for black hole with Newman–Unti–Tamburino (NUT) parameter, we investigate the thermodynamics and weak cosmic censorship conjecture for a Kerr–Newman Taub–NUT black hole.
Si-Jiang Yang +3 more
doaj +1 more source
Dilaton gravity approach to three dimensional Lifshitz black hole
The z=3 Lifshitz black hole is an exact black hole solution to the new massive gravity in three dimensions. In order to understand this black hole clearly, we perform a dimensional reduction to two dimensional dilaton gravity by utilizing the circular ...
A. Achucarro +57 more
core +1 more source
Quantum-Gravity Fluctuations and the Black-Hole Temperature [PDF]
Bekenstein has put forward the idea that, in a quantum theory of gravity, a black hole should have a discrete energy spectrum with concomitant discrete line emission.
Hod, Shahar
core +2 more sources
Black hole critical phenomena without black holes [PDF]
13 pages, 6 figures; Submission for the proceedings of ICGC 2000 in the journal ...
openaire +2 more sources
26 pages, LaTeX, 2 figures included with psfig. Several improvements in the presentation. One figure added.
Corley, Steven, Jacobson, Ted
openaire +2 more sources
The Redshift Evolution of the M •–M ⋆ Relation for JWST’s Supermassive Black Holes at z > 4
JWST has detected many overmassive galactic systems at z > 4, where the mass of the black hole, M _• , is 10–100 times larger than expected from local relations, given the host’s stellar mass, M _⋆ .
Fabio Pacucci, Abraham Loeb
doaj +1 more source
Quantum black hole–white hole entangled states
We investigate the quantum deformation of the Wheeler–DeWitt equation of a Schwarzchild black hole. Specifically, the quantum deformed black hole is a quantized model constructed from the quantum Heisenberg–Weyl Uq(h4) group.
S. Jalalzadeh
doaj +1 more source
Simulations of black hole air showers in cosmic ray detectors [PDF]
We present a comprehensive study of TeV black hole events in Earth's atmosphere originated by cosmic rays of very high energy. An advanced fortran Monte Carlo code is developed and used to simulate black hole extensive air showers from ultrahigh-energy ...
A. B. Migdal +8 more
core +3 more sources

