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|    sci.physics.research    |    Current physics research. (Moderated)    |    17,516 messages    |
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|    Message 16,325 of 17,516    |
|    Lawrence Crowell to Y Porat    |
|    Re: Does 'dark matter' has different den    |
|    11 Aug 18 07:59:58    |
      From: goldenfieldquaternions@gmail.com              On Friday, August 10, 2018 at 10:24:26 AM UTC-5, Y Porat wrote:       > On Tuesday, August 7, 2018 at 10:04:42 AM UTC+3, Y Porat wrote:       >> Does 'Dark matter ' has different densities       >> in different locations of space ??       >> =====       >> TIA       >> Y.Porat       >> ===============================================       >       > i would add and say (and ask )       > that according the picture/example       > that Crowell brought j ust above       > we can say that next a bigger masess       > a **wider zone** of dark matter is created       > ??       > ==       > Y.P       > ====================              We really do not know the relationship between ordinary matter and dark       matter for certain. A general rule for the relative prevalence of       ordinary and dark matter is most likely beyond our knowledge.              Clumping of matter occurred with gravitational waves in the early       universe that got stretched into long wavelengths. These gravitational       waves caused matter to oscillate and with ordinary matter there is       enough friction by the production of electromagnetic radiation to cause       them to clump. Dark matter has no friction so its gravitational       interaction is purely conservative. With ordinary matter losing energy       by radiation (friction) this probably provided enough gravitational       potential to bind dark matter as well. This friction driven set of       oscillations started by gravitational waves turned into acoustical       energy in the hot medium of the universe in its first seconds to hours       of existence. This anisotropy persisted with the expansion of the       universe and is found in galaxies, galaxy clusters with dark matter       halos. Comparisons between anisotropy of the CMB and subsequent galaxies       is an ongoing program.              A galaxy with little or dark matter tends to suggest there was little       dark matter around to gravitationally bind to the ordinary matter, and       so there was some initial anisotropy of dark matter. That leaves a big       question to ponder. It is very difficult to address this question       because we have no experimental evidence on what dark matter is. Eric       Verlinde thinks dark matter is a type of spacetime physics, and with       gravitational radiation around there might have been something odd. If       dark matter is due to supersymmetric partners of ordinary matter, then       the action of supergenerators to give local spacetime transformations       might have played some role with primordial gravitational       radiation. Maybe, and then again maybe not.              --- SoupGate-Win32 v1.05        * Origin: you cannot sedate... all the things you hate (1:229/2)    |
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