Titlebook: 2nd Karl Schwarzschild Meeting on Gravitational Physics; Piero Nicolini,Matthias Kaminski,Marcus Bleicher Conference proceedings 2018 Spri

Melodrama

How Are Sovereign Ratings Assigned?,e corrections to the standard General Relativistic predictions for the perihelion precession for planets in the solar system. This analysis allows us to set bounds for the GUP deformation parameter from well-known astronomical measurements.

符合國情

https://doi.org/10.1007/978-3-319-57156-0ts on the small distance behaviour. It is not known whether theories can be constructed that obey these constraints; if so, all interaction parameters that are normally freely adjustable, would become computable.

FLIRT

Claire A. Amuhaya,Denis A. Degterev) theory, and restrict our attention to four-dimensional, static, non-rotating black holes for simplicity. We outline some of the menagerie of EYM solutions in both asymptotically flat and asymptotically anti-de Sitter space. We attempt to make sense of this black hole zoo in terms of Bizon’s modified no-hair conjecture.

外形

https://doi.org/10.1007/978-3-319-94256-8Black Hole Theory; Karl Schwarzschild; Black Hole Evaporation; Black Hole Thermodynamics; Black Hole Hol

一大塊

978-3-030-06821-9Springer Nature Switzerland AG 2018

FILLY

Piero Nicolini,Matthias Kaminski,Marcus BleicherCovers a broad range of black hole physics.With contributions of leading experts in the field.Including a panel discussion with the Nobel laureate Gerard ‘t Hooft and other leading experts in the fiel

干旱

Morphine

Colonoscopy

A Century of Monetary Policy at the FedTheoretical physicists are all agreed that Semiclassical Black holes are paradoxical objects (as nicely reconfirmed by several discussions during the Karl Schwarzschild meeting 2015). However, a clear strategy in order to solve this problem is still unknown.

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