Titlebook: Quantum Aspects of Black Holes; Xavier Calmet Book 2015 Springer International Publishing Switzerland 2015 Black Hole Entropy.Classical an

使厌恶

Fundamental Physics with Black Holes,antum black holes enable us to probe quantum gravitational physics either directly if the Planck scale is low enough or indirectly if we integrate out quantum black holes from our low energy effective action. We discuss how quantum black holes can resolve the information paradox of black holes and e

floaters

Black Holes and Thermodynamics: The First Half Century, with the physical insights by Bekenstein about black hole entropy and the semi-classical derivation by Hawking of black hole evaporation. The black hole entropy law inspired the formulation of the holographic principle by ’t Hooft and Susskind, which is famously realized in the gauge/gravity corres

独轮车

The Firewall Phenomenon,understood as physical systems with their own thermodynamic behaviour. This same behaviour leads to paradoxical conflicts between some of the basic principles of physics whose resolution is not straightforward and that suggest a new structure—known as a firewall—may be present. This chapter provides

偏离

Monsters, Black Holes and Entropy,figurations and describe their general properties. Monsters are problematic for certain versions of the AdS/CFT duality, and possibly even for the application of statistical mechanics to quantum gravity. It is possible that they are somehow excluded from the Hilbert space of quantum gravity, althoug

lethargy

Primordial Black Holes: Sirens of the Early Universe,uding the collapse of large density perturbations, cosmic string loops and bubble collisions. The number of PBHs formed is tightly constrained by the consequences of their evaporation and their lensing and dynamical effects. Therefore PBHs are a powerful probe of the physics of the early Universe, i

带来

Self-gravitating Bose-Einstein Condensates,rophysics also. Indeed, dark matter halos could be gigantic quantum objects made of Bose-Einstein condensates. The pressure arising from the Heisenberg uncertainty principle or from the repulsive scattering of the bosons could stabilize dark matter halos against gravitational collapse and lead to sm

忘川河

majestic

观察

Black Holes at the Large Hadron Collider, has been discovered, and—yet—there are no signs of new physics beyond the standard model. The LHC set stringent limits on the existence of TeV-scale new physics phenomena, including models with low-scale quantum gravity, which predict—among other phenomena—copious production of black holes at the L

滔滔不绝的人

Minimum Length Effects in Black Hole Physics,ng in black hole physics. In particular, we focus on the ensuing minimum mass for black holes and how modified dispersion relations affect the Hawking decay, both in four space-time dimensions and in models with extra spatial dimensions. In the latter case, we briefly discuss possible phenomenologic