"been teaching literature for over 35 years"
Gerry Quinn · 09 Sep 2013, 14:42
· from 2013-September.txt.gz
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From: gerry at bindweed.com (Gerry Quinn) Date: Mon, 9 Sep 2013 15:42:28 +0100 Subject: (urth) "been teaching literature for over 35 years" In-Reply-To: <522DD836.6050803 at clueland.com> References: <52290769.660c320a.7def.fffff916 at mx.google.com><1378442246.57552.YahooMailNeo at web124504.mail.ne1.yahoo.com><1378489682.63899.YahooMailNeo at web124506.mail.ne1.yahoo.com><522A4070.4070407 at irit.fr> <5B8EEAEF-B206-4F5D-A277-349B6C60AD19 at gmail.com><1378614309.6288.YahooMailNeo at web124502.mail.ne1.yahoo.com> <522C7085.3060202 at verizon.net><D75A571ED1584BAF8820AA540F92E8CF@Rover> <522CA3B6.70903 at verizon.net><0398640b3bd4fdc0229df649e074727b.squirrel at webmail.prismnet.com><1378703957.73667.YahooMailNeo at web124505.mail.ne1.yahoo.com><BDD66FCCDD7B4949ADF7A85B5195143A@Rover><522DB883.6040101 at clueland.com><D263433829BF4B73BC8A9442F1D5BCCF@Rover><522DCADA.4080402 at clueland.com><747004DA7C8F40EBA20B8CBD4E3472BC@Rover> <522DD836.6050803 at clueland.com> Message-ID: <B1CBDD7D141E40DD8309E61100E2F20F@Rover> From: Jeffery Wilson On 9/9/2013 8:56 AM, Gerry Quinn wrote: > From: Jeffery Wilson >>> > It doesn't matter (in engineering terms) whether stuff that reaches >>> > the >>> > event horizon goes somewhere else or not (that's kind of the >>> > definition >>> > of an event horizon). But an accretion disk outside the Schwarzschild >>> > radius is just standard dynamics for any super-condensed object. > >>> What force acts on the matter to prevent it from following the usual >>> swarm of elliptical orbits instead of the disk? > >> In a word, friction. The matter would be gaseous in this case and >> particles could not swirl in independent orbits. But even if it were >> composed of solid particles, they would soon collide, which would (1) >> heat the colliding particles (2) reduce their energy, and (3) set the >> colliding particles on closer trajectories than they were before. >But all the stuff inside the sun's already colliding and touching. >How is the axis and irection of rotation of the disk picked? The Sun is already rotating, so its matter has angular momentum. Any difference in angular momentum gets magnified as an object shrinks (e.g. spinning skater pulling her arms in spins faster). And angular momentum is conserved - there's nowhere for it to go except into the black hole, and even then it's one of the three kinds of 'hair' a black hole can have - i.e. a black hole's angular momentum can still interact with its surroundings, as can its electric charge and gravitational field. A rotating object has a defined axis as well as direction. This has happened before as the solar system was formed: note how all the planets and asteroids are in a plane, rotating in the same direction (bar the odd outlier that had some heavy collisions that sent it on an unusual trajectory)? And the sun and planets also tend to rotate on their own axes in the same direction. The solar system has a specific axis of rotation, because collisions early on resulted in a single axis dominating. Another example: water draining out of a bathtub picks a direction, and sticks with it. - Gerry Quinn
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