Are black holes springlike?

2015

Full text Open access: Green Metadata (CSL-JSON)
DOI 10.1103/physrevd.91.044031
Data confidence 70 medium
How this score is calculated

It is built from checkable properties of the record itself: whether the article has a DOI, how many independent sources confirmed its data, whether the required fields are filled in, and how recent the latest confirmation is. Disagreement between sources and a missing identifier lower it. A value of 80 or above means the record was published without further checking; 60 to 79 means it is published at reduced confidence, with a manual check advisable. A record verified by an editor by hand is never pushed below 90 by a recalculation. This scores our data about the article, not the article itself.

Abstract

A ($3+1$)-dimensional asymptotically flat Kerr black hole angular speed ${\mathrm{\ensuremath{\Omega}}}_{+}$ can be used to define an effective spring constant, $k=m{\mathrm{\ensuremath{\Omega}}}_{+}^{2}$. Its maximum value is the Schwarzschild surface gravity, $k=\ensuremath{\kappa}$, which rapidly weakens as the black hole spins down and the temperature increases. The Hawking temperature is expressed in terms of the spring constant: $2\ensuremath{\pi}T=\ensuremath{\kappa}\ensuremath{-}k$. Hooke's law, in the extremal limit, provides the force $F=1/4$, which is consistent with the conjecture of maximum force in general relativity.