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Article #4203Re: Question on Hawking radiation
From: RING, DAVID WAYNE
Date: Sat, 07 Nov 1992 01:05
Date: Sat, 07 Nov 1992 01:05
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brahm@cco.caltech.edu (David E. Brahm) writes... >Can anyone explain why extreme Reissner-Nordstrom black holes (Q=M) [or >charged Kerr solutions, L^2 + Q^2 = M^2] have a vanishing Hawking >temperature (T=0)? The virtual-particle picture would make me erroneously >believe that positively-charged particles would spew out from the vicinity >of a positively-charged black hole. My guess is that it has something to >do with the inner horizon (r-) going to zero. >[* This question is originally due to Dr. Stephen Hsu at Harvard *] A stationary observer just outside the horizon does not accelerate (as measured from outside, i.e. if she is lowered from infinity on a string the string has no tension). Thus, what looks like a particle pair from outside, looks like a particle pair in a local inertial frame. And pair production from nothing is forbidden in inertial frames. But this suggests another harder question: how can the surface gravity be zero??? BTW If you talk to Steve, say hi for me. :-) Dave Ring dwr2560@zeus.tamu.edu
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Newsgroups: sci.physics Path: arc1-ca.pugleaf.net!sparky!uunet!snorkelwacker.mit.edu!tamsun.tamu.edu!zeus.tamu.edu!dwr2560 From: dwr2560@zeus.tamu.edu (RING, DAVID WAYNE) Subject: Re: Question on Hawking radiation Message-ID: <6NOV199219052860@zeus.tamu.edu> Summary: Why don't extremal black holes radiate? News-Software: VAX/VMS VNEWS 1.41 Sender: news@tamsun.tamu.edu (Read News) Organization: Texas A&M University, Academic Computing Services References: <31OCT199223312123@zeus.tamu.edu> <Nov.3.17.39.38.1992.15269@ruhets.rutgers.edu> <1d7ag2INNi5q@agate.berkeley.edu> <1d9fh1INNln@gap.caltech.edu> Date: Sat, 7 Nov 1992 01:05:00 GMT Lines: 22