Relay-Version: version B 2.10 5/3/83; site utzoo.UUCP Posting-Version: version B 2.10.1 6/24/83; site fortune.UUCP Path: utzoo!linus!decvax!harpo!ulysses!mhuxl!ihnp4!fortune!rpw3 From: rpw3@fortune.UUCP Newsgroups: net.physics Subject: Re: Re: eV Revisited - (nf) Message-ID: <2513@fortune.UUCP> Date: Sat, 11-Feb-84 11:04:02 EST Article-I.D.: fortune.2513 Posted: Sat Feb 11 11:04:02 1984 Date-Received: Wed, 15-Feb-84 04:18:54 EST Sender: notes@fortune.UUCP Organization: Fortune Systems, Redwood City, CA Lines: 65 #R:rlgvax:-168600:fortune:8600013:000:2555 fortune!rpw3 Feb 11 05:04:00 1984 Guy is right. It's just that jargon is confusing to some. Physicists have gotten so used to talking about mass in eV that they don't realize that people don't understand that they don't mean the mass of an electron IS 511KeV, they mean the mass of the electron is EQUIVALENT to 511KeV when said mass is converted to energy (via the c^2). See, in an accelerator near the speed of light it all gets blurred anyway, since nobody really CARES what the rest "mass" is when the relativistic "mass/energy" is 100-1000 times rest mass. So the language gets sloppy. People naturally contract "rest mass equivalent energy" ==> rest mass energy => rest "mass". <> Note that other units can be converted for amusement and amazement... Anybody remember Cpt. Grace Hopper's standard guest lecture, with the punch-line when she reaches into the bag and pulls out some "nanoseconds"? Little pieces of telephone wire, 11.9 inches long! Somebody once showed me the corresponding equivalence of mass and length, if I can just remember it. Let's see (this is a bit weird)... 1. F = m * a force due to acceleration 2. F = G * (m1 * m2) / r^2 force due to gravity (r = distance) 1,2=> 3. a = G * m / r^2 acceleration (of a point mass) due to gravity. 4. a = S / t^2 Def'n of acceleration (S = distance) 3,4=> 5. S / t^2 = G * m / r^2 or, m = 1/G * S * (r/t)^2 (rearranging) 6. c = c0 * (r/t) (let c0 be just the number ~2.99e8 with no units) 5,6=> 7. m = 1/(G*c0^2) * c^2 * S and voila, pulling the same trick of scaling by c^2, we get 8. m = K * S where constant K = c^2 / (G * c0^2) or, S = K' * m where K' = 1 / K Anyway, the dimensional analysis holds, if you want to play the game. The way I heard it, by the time you have all the scaling constants worked out, the mass of the Sun is ~ 1.1 kilometers, which led a wag to suggest that that's how far the Sun has ejected itself from our space-time due to its mass. Rubber-sheet geometry lives! :-) Rob Warnock UUCP: {sri-unix,amd70,hpda,harpo,ihnp4,allegra}!fortune!rpw3 DDD: (415)595-8444 USPS: Fortune Systems Corp, 101 Twin Dolphins Drive, Redwood City, CA 94065 p.s. You can also get length in terms of mass by starting with the following two equations and playing the same games (hint: expand everything out to mass, distance, and time, and start cancelling terms 'til you're left with m = S), but the constant of proportionality comes out different. Any explanations? 1. E = m * c^2 Einstein 2. E = F * S force * distance ... N. S = k" * m (what's K"?)