For accreting Reissner-Nordstrom black holes, the momentum flux from infalling matter splits an extremal horizon into two, while energy density displaces the extremal horizon's radius.
Relativistic equations for adiabatic, spherically symmetric gravitational collapse.Phys
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Dynamical black holes and accretion-induced backreaction
For accreting Reissner-Nordstrom black holes, the momentum flux from infalling matter splits an extremal horizon into two, while energy density displaces the extremal horizon's radius.