Astronomers Uncover Statistical Evidence for Recoiling Supermassive Black Holes
Galactic collisions are events of breathtaking proportions. The Supermassive Black Holes (SMBHs) at their centers plunge into a chaotic orbital dance that event...
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Galactic collisions are events of breathtaking proportions. The Supermassive Black Holes (SMBHs) at their centers plunge into a chaotic orbital dance that event...
A new theoretical study suggests that black holes may never completely disappear, potentially offering a way to resolve the long-standing black hole information...
Abstract page for arXiv paper 2605.31077: Super-Eddington accretion of black holes in early nuclear bursts gives birth to Little Red Dots
Abstract page for arXiv paper 2605.30449: Impact of Primordial Black Holes Induced Neutrinos on the Cosmic 21-cm Brightness Temperature
Abstract page for arXiv paper 2605.30411: Axions Create Singularities on Extremal Horizons
Abstract page for arXiv paper 2605.30417: Logarithm of charge ratio in black hole entropy
Abstract page for arXiv paper 2605.30540: Entanglement entropy of an acoustic black hole
Abstract page for arXiv paper 2605.31331: Higher-Derivative Corrections to Reissner--Nordström Black Holes from Worldline QFT
Abstract page for arXiv paper 2511.16012: Graybody factors and absorption cross-sections of non-exchange black holes in Instein-coupled scalar fields
Abstract page for arXiv paper 2605.28917: Greybody Factors, Absorption Cross Sections and Hawking Radiation of Holonomy-Corrected Schwarzschild Black Holes
Abstract page for arXiv paper 2605.28951: When the Ringing Stops: Purely Imaginary Modes in the Ringdown Spectrum of Dynamical Black Holes
Abstract page for arXiv paper 2605.28953: Signatures of loop quantum gravity in primordial black hole cosmologies
Abstract page for arXiv paper 2605.29049: Shadows of naked singularities and superspinars related to the revisited Kerr-de Sitter spacetimes
Astrophysicists may have to flip the script on how the universe's
Of all the objects in the Universe, few are as perplexing as black holes.
Abstract page for arXiv paper 2605.28676: Magnetic Configuration Imprints on Quasi-Periodic Variability in GRMHD Simulations of Thin Accretion Disks
Abstract page for arXiv paper 2605.28777: The formation of supermassive black holes from Population III.1 seeds. IV. Self-regulated seeding from supermassive st...
Abstract page for arXiv paper 2605.28715: Accurate waveforms for generic planar-orbit binary black holes: The multipolar effective-one-body model SEOBNRv6EHM
Abstract page for arXiv paper 2605.27641: Robin holography in AdS and BTZ: double-trace RG flow and exceptional points
Abstract page for arXiv paper 2605.27615: Lorentz-Violating (Regular) Black Holes in Einstein Gravity
Abstract page for arXiv paper 2605.27953: Probing Effective Field Theory Corrections with Quasinormal Modes and Gravitational Lensing in Reissner-Nordström Bla...
Abstract page for arXiv paper 2605.28580: Perturbative dynamics and relativistic effects of a dyonic Kalb-Ramond black hole
Physicists have thought for decades that microscopic black holes can theoretically emerge not from exploding stars but from delicate
A new statistical model reveals more details about the ringdown period of merging black holes.
Right on the brink of black hole formation, spacetime can get downright peculiar.
A survey of about 8,000 supermassive black holes has tracked their growth across roughly the last 10 billion years and found that accretion rates have been decl...