Dark Energy Accretion onto a Black Hole in an Expanding Universe
Abstract
By using the solution describing a black hole embedded in the FLRW universe, we obtain the evolving equation of the black hole mass expressed in terms of the cosmological parameters. The evolving equation indicates that in the phantom dark energy universe the black hole mass becomes zero before the Big Rip is reached.
 Publication:

Communications in Theoretical Physics
 Pub Date:
 September 2009
 DOI:
 10.1088/02536102/52/3/12
 arXiv:
 arXiv:0812.2996
 Bibcode:
 2009CoTPh..52..441S
 Keywords:

 High Energy Physics  Theory
 EPrint:
 7 pages, no figures, errors is corrected