Bereiche | Tage | Auswahl | Suche | Aktualisierungen | Downloads | Hilfe

GR: Fachverband Gravitation und Relativitätstheorie

GR 1: Schwarze Löcher 1

GR 1.5: Vortrag

Montag, 13. März 2017, 10:10–10:30, SFG 0140

Rotating non-singular black holes — •Roman Smit and Piero Nicolini — Frankfurt Institute for Advanced Studies (FIAS), Frankfurt am Main, Germany

A variety of non-singular spherically symmetric black hole solutions have been found in the past. Their energy momentum tensor is usually an anisotropic perfect fluid with a dark-energy-like equation of state (p=-ρ) for the radial pressure.

Historically, the Kerr-Newman solution was found by applying a complexification algorithm -- the Newman-Janis algorithm -- to the Reissner-Nordstroem solution.

I will show how to modify and apply this algorithm to the known spherical non-singular black holes to obtain rotating non-singular black holes.