Acceleration of colliding shells around a black hole: Validity of the test particle approximation in the Banados-Silk-West process

Recently, Banados, Silk and West (BSW) showed that the total energy of two colliding test particles has no upper limit in their center of mass frame in the neighborhood of an extreme Kerr black hole, even if these particles were at rest at infinity in the infinite past. We call this mechanism the BSW mechanism or BSW process. The large energy of such particles would generate strong gravity, although this has not been taken into account in the BSW analysis. A similar mechanism is seen in the collision of two spherical test shells in the neighborhood of an extreme Reissner-Nordström black hole. In this paper, in order to draw some implications concerning the effects of gravity generated by colliding particles in the BSW process, we study a collision of two spherical dust shells, since their gravity can be exactly treated. We show that the energy of two colliding shells in the center of mass frame observable from infinity has an upper limit due to their own gravity. Our result suggests that an upper limit also exists for the total energy of colliding particles in the center of mass frame in the observable domain in the BSW process due the gravity of the particles.

Figure 1

Schematic spacetime diagram of a spherical timelike shell. The shell divides spacetime into two regions $V_1$ and $V_2$.

Figure 2

Schematic spacetime diagram of two spherical timelike shells. The two shells divide the spacetime into three regions $V_1$, $V_2$ and $V_3$.