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#51
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"galactic X-ray background" produced by hundreds of millionsof individual stars
Spaceman wrote:
"BlagooBlanaa" wrote in message ... so does this mean that non keplerian orbits can now be explained without dork matter? hope so Keplerian orbits can already be explained without dork matter. It is not needed for such at all. BlagooBlanaa was asking about non keplerian orbits! Spit****, Space****, Spaceman, or whatever you call the little troll has quite the track record and is a registered crank at crank dot net. http://www.google.com/search?q=Space...Awww.crank.net For a few laughs try the Spaceman [space****] Emulator http://www.hyperdeath.co.uk/spaceman/ |
#52
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"galactic X-ray background" produced by hundreds of millions of individual stars
"Sam Wormley" wrote in message news:XtuPf.807187$x96.432885@attbi_s72... Spaceman wrote: "BlagooBlanaa" wrote in message ... so does this mean that non keplerian orbits can now be explained without dork matter? hope so Keplerian orbits can already be explained without dork matter. It is not needed for such at all. BlagooBlanaa was asking about non keplerian orbits! Oops, my bad. Non keplarian orbits can already be explained without dork matter. and... just for other things.. it (dork matter) is not needed for anything in the universe to be explained. |
#53
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"galactic X-ray background" produced by hundreds of millionsof individual stars
Spaceman wrote:
Oops, my bad. Non keplarian orbits can already be explained without dork matter. and... just for other things.. it (dork matter) is not needed for anything in the universe to be explained. I will assume that you are referring to matter that exhibits gravitation but is not emitting (or absorbing) electromagnetic radiation as far as we can tell to date. These mysteries are what science is all about! Particle Dark Matter: Evidence, Candidates and Constraints http://arxiv.org/abs/hep-ph/0404175 In this review article, we discuss the current status of particle dark matter, including experimental evidence and theoretical motivations. We discuss a wide array of candidates for particle dark matter, but focus on neutralinos in models of supersymmetry and Kaluza-Klein dark matter in models of universal extra dimensions. We devote much of our attention to direct and indirect detection techniques, the constraints placed by these experiments and the reach of future experimental efforts. |
#54
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"galactic X-ray background" produced by hundreds of millions of individual stars
On Wed, 08 Mar 2006 16:00:26 +0000, Sam Wormley wrote:
Spaceman wrote: [quoted text muted] I will assume that you are referring to matter that exhibits gravitation but is not emitting (or absorbing) electromagnetic radiation as far as we can tell to date. These mysteries are what science is all about! Particle Dark Matter: Evidence, Candidates and Constraints http://arxiv.org/abs/hep-ph/0404175 In this review article, we discuss the current status of particle dark matter, including experimental evidence and theoretical motivations. We discuss a wide array of candidates for particle dark matter, but focus on neutralinos in models of supersymmetry and Kaluza-Klein dark matter in models of universal extra dimensions. We devote much of our attention to direct and indirect detection techniques, the constraints placed by these experiments and the reach of future experimental efforts. Personally, I think dark matter is fine; it's just the dark bits between stars, somewhat a la Oort cloud/Kuypier belt objects/comets/whatnot. They don't do much, though dodging them during interstellar travel might be an interesting exercise. (Assuming we ever develop such; the contemporary hypotheses assume multigenerational ships that would take tens of thousands of years to voyage, and even my best efforts, which rely on an impossible engine, would suggest an effective speed of about 0.10 c (i.e., voyage time of 80 years to get to Sirius, about 8 lightyears distant), if one isn't sure of fuel at the destination to refill one's tank. But at least my impossible engine doesn't require exotic fuels such as antimatter. :-) ) What puzzles me is dark energy. Of course, they're probably still working on that, too... :-) -- #191, Windows Vista. Because everyone wants a really slick-looking 8-sided wheel. |
#55
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"galactic X-ray background" produced by hundreds of millions of individual stars
On Sat, 11 Mar 2006 19:24:42 -0800, Brian Tung wrote:
The Ghost In The Machine wrote: Personally, I think dark matter is fine; it's just the dark bits between stars, somewhat a la Oort cloud/Kuypier belt objects/comets/whatnot. They don't do much, though dodging them during interstellar travel might be an interesting exercise. You don't have to dodge anything; dark matter as it is currently understood doesn't interact electromagnetically, so you'd go right through it. It therefore cannot be anything like comets or asteroids or anything like. This gets *really* weird, but if I read you correctly you're suggesting a form of matter (MACHOs or WIMPs, as I understand it) that does not interact with ordinary fermions but still causes gravitational curvature? :-) Ow, my brain. Still, let's hope we don't find out the hard way during an interstellar space cruise, unlikely as those appear to be at the moment. (Fun notion. c/(100 N/kg) = 34 days. Unless Star Trek magically invented some sort of null-gravity adaptor there's some interesting logistics problems here...) -- #191, Windows Vista. Because everyone wants a really slick-looking 8-sided wheel. |
#56
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"galactic X-ray background" produced by hundreds of millions of individual stars
The Ghost In The Machine wrote:
This gets *really* weird, but if I read you correctly you're suggesting a form of matter (MACHOs or WIMPs, as I understand it) that does not interact with ordinary fermions but still causes gravitational curvature? :-) MACHOs are ordinary matter, so they wouldn't qualify; WIMPs would. And to be precise, I'm not suggesting it at all--I don't have enough of a physics background to do so. I'm just relaying what others have suggested. -- Brian Tung The Astronomy Corner at http://astro.isi.edu/ Unofficial C5+ Home Page at http://astro.isi.edu/c5plus/ The PleiadAtlas Home Page at http://astro.isi.edu/pleiadatlas/ My Own Personal FAQ (SAA) at http://astro.isi.edu/reference/faq.html (Location of these pages soon to change. Stay tuned for updates.) |
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