Results 11 to 20 of about 162,795 (306)
The impact of mass-transfer physics on the observable properties of field binary black hole populations [PDF]
We study the impact of mass-transfer physics on the observable properties of binary black hole populations that formed through isolated binary evolution. We used the POSYDON framework to combine detailed MESA binary simulations with the COSMIC population
S. Bavera +15 more
semanticscholar +1 more source
We report the X-ray timing results of the black hole candidate MAXI J1820+070 during its 2018 outburst using the Hard X-ray Modulation Telescope (Insight-HXMT) and Neutron Star Interior Composition Explorer Mission (NICER) observations.
X. Ma +15 more
doaj +1 more source
Gravitational Collider Physics via Pulsar–Black Hole Binaries [PDF]
We propose to use pulsar–black hole binaries as a probe of gravitational collider physics. Induced by the gravitation of the pulsar, the atomic transitions of the boson cloud around the black hole backreact on the orbital motion.
Qianhang Ding, Xinan Tong, Yi Wang
semanticscholar +1 more source
We present the first results from a 100-day Swift, NICER, and ground-based X-ray–UV–optical reverberation mapping campaign of the Narrow-line Seyfert 1 Mrk 335, when it was in an unprecedented low X-ray flux state.
Erin Kara +39 more
doaj +1 more source
Critical point in the phase diagram of primordial quark-gluon matter from black hole physics [PDF]
Strongly interacting matter undergoes a crossover phase transition at high temperatures $T\ensuremath{\sim}{10}^{12}\text{ }\text{ }\mathrm{K}$ and zero net-baryon density.
R. Critelli +9 more
semanticscholar +1 more source
No ensemble averaging below the black hole threshold [PDF]
In the AdS/CFT correspondence, amplitudes associated to connected bulk manifolds with disconnected boundaries have presented a longstanding mystery. A possible interpretation is that they reflect the effects of averaging over an ensemble of boundary ...
Jean-Marc Schlenker, E. Witten
semanticscholar +1 more source
We elaborate on various aspects of our top-down celestial holographic duality wherein the semiclassical bulk spacetime is a 4d asymptotically flat, self-dual Kähler geometry known as Burns space.
Kevin Costello +2 more
doaj +1 more source
Minimum Length Effects in Black Hole Physics [PDF]
We review the main consequences of the possible existence of a minimum measurable length, of the order of the Planck scale, on quantum effects occurring in black hole physics.
R. Casadio, O. Micu, P. Nicolini
semanticscholar +1 more source
Carrollian physics at the black hole horizon [PDF]
We show that the geometry of a black hole horizon can be described as a Carrollian geometry emerging from an ultra-relativistic limit where the near-horizon radial coordinate plays the role of a virtual velocity of light tending to zero.
L. Donnay, Charles Marteau
semanticscholar +1 more source
Sharp Signals of Boson Clouds in Black Hole Binary Inspirals. [PDF]
Gravitational waves (GWs) are an exciting new probe of physics beyond the standard models of gravity and particle physics. One interesting possibility is provided by the so-called "gravitational atom," wherein a superradiant instability spontaneously ...
D. Baumann +3 more
semanticscholar +1 more source

