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Article #8304Re: Neutrinos
From: Fred McGalliard
Date: Wed, 02 Apr 1997 00:00
Date: Wed, 02 Apr 1997 00:00
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Chris Wagner wrote: (a nice description of rest and relative mass. Thanks Chris.) But now I would like to take this a few steps deeper. What mass do I deal with when the object is a collection of confined photons, and possibly some neutrinos. The rest mass of a confined photon should be it's ordinary mass, or just it's energy, eh? The gravitational mass of a star then is (a bunch of stuff) + (the mass of the confined photons). When the confined photons go streaming off to infinity, they can leave as much as all of their mass/energy behind. Where is it? How is it left behind?
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X-Google-Language: ENGLISH,ASCII-7-bit X-Google-Thread: fc19f,170da24f95ceef31 X-Google-Attributes: gidfc19f,public X-Google-Thread: 10b271,d888c38d73ff4862 X-Google-Attributes: gid10b271,public X-Google-Thread: 107319,14c8003ac88779d4 X-Google-Attributes: gid107319,public From: Fred McGalliard <frederick.b.mcgalliard@boeing.com> Subject: Re: Neutrinos Date: 1997/04/02 Message-ID: <3342EBCB.6677@boeing.com> X-Deja-AN: 230258152 Sender: nntp@news.boeing.com (Boeing NNTP News Access) X-Nntp-Posting-Host: 134.52.170.219 References: <5d2m8a$ncn@Masala.CC.UH.EDU> <332BD9F9.5E4C@ucunix.san.uc.edu> Organization: Boeing D&SG Newsgroups: sci.physics,rec.arts.startrek.tech,aus.sf.star-trek