Babichev E, Dokuchaev V, Eroshenko Yu
Institute For Nuclear Research, Russian Academy of Sciences, 60th October Anniversary Prospect 7a, 117312 Moscow, Russia.
Phys Rev Lett. 2004 Jul 9;93(2):021102. doi: 10.1103/PhysRevLett.93.021102. Epub 2004 Jul 8.
Solution for a stationary spherically symmetric accretion of the relativistic perfect fluid with an equation of state p(rho) onto the Schwarzschild black hole is presented. This solution is a generalization of Michel solution and applicable to the problem of dark energy accretion. It is shown that accretion of phantom energy is accompanied by the gradual decrease of the black hole mass. Masses of all black holes tend to zero in the phantom energy Universe approaching the Big Rip.
