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@Drakkith and @JLowe: For all practical purposes, matter does fall in. If you let a light source fall in and calculate the expected intensity an observer far away will receive, this intensity never reaches zero - but it goes down exponentially with a short time constant. You will quickly receive the last photon you will ever get from this object. Afterwards you can calculate that it could still be 10-100 m away from the event horizon, but that doesn't make sense - it is an artifact of a poor choice of units that diverge at the event horizon. Choose different time units and the object does fall in.
Black holes can be charged, the corresponding metric has been found by Reissner and Nordström. Charge is conserved - if you shoot charged objects at a black hole, the black hole changes its charge accordingly.
Reissner, H. (1916). "Über die Eigengravitation des elektrischen Feldes nach der Einsteinschen Theorie". Annalen der Physik 50: 106–120
Nordström, G. (1918). "On the Energy of the Gravitational Field in Einstein's Theory". Verhandl. Koninkl. Ned. Akad. Wetenschap., Afdel. Natuurk., Amsterdam. 26: 1201–1208.Coming back to the original question: A black hole has a maximal charge, as discussed in post 14 already. At this maximal charge, electrostatic repulsion will be stronger than gravitational attraction for charged particles. You have to actively shoot them towards the black hole - adding so much energy that both the mass of the black hole increases enough to increase its charge as well.
The conversion factor is ##(G 4 \pi \epsilon_0)^{1/2} = 8.6 \cdot 10^{-11} C/kg = 5 \cdot 10^{-22} e/m_e = e/(2µg)## where e is the elementary charge and me is the electron mass.
We have to give the electron (or proton, or any other singly charged particle) ) the energy equivalent to 2µg of mass to get into the maximally charged black hole, assuming it has the same charge as our electron (proton/...).
It does not lose its mass, and it does not lose its charge either. Locally you don't even notice the gravitational field, one of the fundamental principles of general relativity.ivant6900 said:However we know that it can be restored in high energy fields which means that once the electron passes through the Event Horizon and heads down towards the singularity it loses its mass and essentially seizes to exist as an electron...there is no charge transfer at all...
Black holes can be charged, the corresponding metric has been found by Reissner and Nordström. Charge is conserved - if you shoot charged objects at a black hole, the black hole changes its charge accordingly.
Reissner, H. (1916). "Über die Eigengravitation des elektrischen Feldes nach der Einsteinschen Theorie". Annalen der Physik 50: 106–120
Nordström, G. (1918). "On the Energy of the Gravitational Field in Einstein's Theory". Verhandl. Koninkl. Ned. Akad. Wetenschap., Afdel. Natuurk., Amsterdam. 26: 1201–1208.Coming back to the original question: A black hole has a maximal charge, as discussed in post 14 already. At this maximal charge, electrostatic repulsion will be stronger than gravitational attraction for charged particles. You have to actively shoot them towards the black hole - adding so much energy that both the mass of the black hole increases enough to increase its charge as well.
The conversion factor is ##(G 4 \pi \epsilon_0)^{1/2} = 8.6 \cdot 10^{-11} C/kg = 5 \cdot 10^{-22} e/m_e = e/(2µg)## where e is the elementary charge and me is the electron mass.
We have to give the electron (or proton, or any other singly charged particle) ) the energy equivalent to 2µg of mass to get into the maximally charged black hole, assuming it has the same charge as our electron (proton/...).
level]You might recognize the combination of gravitational constant and 4 pi eps_0. The Planck mass and the fine-structure constants have similar combinations,, and the 2µg from above turn out to be ##\sqrt{\alpha}## times the Planck mass with the fine-structure constant ##\alpha##.