Path: utzoo!utgpu!jarvis.csri.toronto.edu!mailrus!iuvax!uxc!uxc.cso.uiuc.edu!m.cs.uiuc.edu!s.cs.uiuc.edu!carroll From: carroll@s.cs.uiuc.edu Newsgroups: sci.space Subject: Re: Black hole trolling Message-ID: <218100014@s.cs.uiuc.edu> Date: 13 Mar 89 15:44:00 GMT References: <605212786.amon@H.GP.CS.CMU.EDU> Lines: 27 Nf-ID: #R:<605212786.amon@H.GP.CS.CMU.EDU>:-32:s.cs.uiuc.edu:218100014:000:1490 Nf-From: s.cs.uiuc.edu!carroll Mar 13 09:44:00 1989 /* Written 4:30 pm Mar 6, 1989 by kpmancus@phoenix.Princeton.EDU in s.cs.uiuc.edu:sci.space */ Easy. The forces that hold a macroscopic object together are electromagnetic. They require the exchange of virtual photons between the particles to be held together. When the object extends across the event horizon, the photons can no longer go from the atoms inside the black hole to the atoms outside. Thus the tether is neatly sliced. /* - - */ Wouldn't that imply that anything going across the horizon would be reduced to fundamental particles? The nucleons wouldn't be able to exchange strong force particles (pions?), and the quarks wouldn't be able to exchange gluons, etc. But I've always thought that this is all moot, anyway. Given the prior existence of a black hole (without worrying about where it came from), my understanding is that due to time dilation effects, it would take an infinite amount of time for anything to fall from (mostly) flat space across the horizon*. So, nothing's fallen in yet into any black hole (assuming a finitely old universe). One might also ask how fast an infalling object is going when it crosses the horizon, assuming it fell from flat space. ------------------- * `infinite time' for an observer in flat space, finite for the object itself Alan M. Carroll "And then you say, carroll@s.cs.uiuc.edu We have the Moon, so now the Stars..." - YES CS Grad / U of Ill @ Urbana ...{ucbvax,pur-ee,convex}!s.cs.uiuc.edu!carroll