Massive black hole binary mergers within subparsec scale gas discs

Government policy varies between nations and this guidance sets out the need for balanced decision-making about ways of working, and the ongoing safety considerations

The main aim of this work is to develop a consistent theory to determine the self-gravitational potential at an arbitrary point of each component of a detached close binary system in

By translating the cross section limits into ADD model expectations, we can exclude the production of semiclassical black holes with a minimum mass varying from 3.9 to 5.3 TeV

We have shown that within a certain range of distances to the graphene sheet, the decay rate of one emitter can be fully dominated by the graphene surface plasmons.. Due to

Here we observe the following: the ratio of far-infrared to near-infrared flux (FIR/NIR) correlates with the mm flux: flaring discs have a higher dust mass than flat discs

From the THz to the midinfrared frequency range, the Purcell factor (i.e., the decay rate near the material, normalized to the decay rate in free space) is increased by nearly 3

Abstract: We study the first-order in α 0 corrections to non-extremal 4-dimensional dy- onic Reissner-Nordstr¨ om (RN) black holes with equal electric and magnetic charges in

Given the essential role that the event horizon plays in the thermodynamic descrip- tion of a black hole and in turn of the dual thermal state, it arises the question of