home *** CD-ROM | disk | FTP | other *** search
- Newsgroups: sci.physics
- Path: sparky!uunet!cs.utexas.edu!tamsun.tamu.edu!zeus.tamu.edu!dwr2560
- From: dwr2560@zeus.tamu.edu (RING, DAVID WAYNE)
- Subject: Re: Length scales in physics 4 - the Planck length
- Message-ID: <26AUG199217155442@zeus.tamu.edu>
- News-Software: VAX/VMS VNEWS 1.41
- Sender: news@tamsun.tamu.edu (Read News)
- Organization: Texas A&M University, Academic Computing Services
- References: <25AUG199211163258@zeus.tamu.edu> <1992Aug26.081107.3779@nuscc.nus.sg>
- Date: Wed, 26 Aug 1992 22:15:00 GMT
- Lines: 30
-
- matmcinn@nuscc.nus.sg (Mcinnes B T (Dr)) writes...
- >: radius' you want. A physical question would be: what if you compressed
- >: the earth from the outside? What would be the 'internal radius' as the
- >: final collapse began. The answer would be only a few times the S radius
- >: by analogy with neutron star collapse.
- >:
- >Sorry, I don't see how you know that it is only a few times. Won't it
- >depend on the degree of compression?
-
- Since the collapse starts when the external radius is a few times the S
- radius (2M) the factor 1-2M/R is not all that different from 1, so the
- internal and external radii will not differ by much.
-
- I'm sorry I can't be more quantitative, but I'm certainly not an expert at
- neutron star physics.
-
- >: String theory doesn't really replace spacetime, but treats it as a field
- >: living on the worldsheet.
- >:
- >errr....meaning what? how do you "treat spacetime as a field?"
-
- You can do the same thing with a point particle. It's path is given by
- R(t) where R is a four-vector, and t is the particle's proper time, or any
- other parameter. You can consider the particle to live in R space, or you
- can consider R to be a field living on the one dimentional t line. Then you
- can do a path integral over all paths R(t) or a functional integral over
- all fields R(t).
-
- Dave Ring
- dwr2560@zeus.tamu.edu
-