Timeline for Detection of the Electric Charge of a Black Hole: How can an electromagnetic field escape the event horizon of a Reissner-Nordström black hole?
Current License: CC BY-SA 3.0
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Jul 12, 2011 at 17:41 | vote | accept | Benjamin Horowitz | ||
Jul 12, 2011 at 14:36 | comment | added | Ted Bunn | Well, when we picture electric field lines, we picture them at a moment in time, so the answer to this question depends on a choice of a time coordinate (or at least of a particular foliation of spacetime into constant-time slices). If you use Schwarzschild coordinates for this, then yes, the field lines end on (or just barely outside of) the horizon. There's a good reason for this: in Schwarzschild coordinates, infalling matter appears to get "stuck" at the horizon, not crossing it until $t=\infty$. (I say "appears to" because this is just an artifact of a coordinate singularity.) | |
Jul 12, 2011 at 9:21 | comment | added | Georg | ""Even after the material collapses to form a black hole, the field lines are still there, a relic of the material that formed the black hole."" So, the field lines end on the event horizon? Where is the charge? Inside or on the horizon? | |
Jul 12, 2011 at 0:59 | history | edited | Ted Bunn | CC BY-SA 3.0 |
added 415 characters in body
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Jul 12, 2011 at 0:50 | history | answered | Ted Bunn | CC BY-SA 3.0 |