Article View: sci.astro
Article #3592Re: Dark matter
From: Ethan Bradford
Date: Sun, 24 Jan 1993 23:12
Date: Sun, 24 Jan 1993 23:12
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The only recent news w.r.t. dark matter that I know of was the conclusion that there was a lot more dark matter than previously thought in a small (3 galaxy) cluster. If the cluster is typical, the universe is definitely closed. The evidence for the dark matter is still indirect; in this case it is necessary to confine the hot gas in the cluster. There are active direct searches for two different promising candidates. Subatomic Weakly Interacting Massive Particles (WIMPs) are being searched for in accelerator results and in direct-detection experiments (trying to see the heat they deposit when they interact with very cold germanium). Star-sized MACHOs (MAssive Compact Halo Objects) are being probed by looking for lensing of stars in the Mageleanic Clouds. Both searches should have significant results in a few years -- either they will find something, or the possibility of that kind of dark matter will be somewhat constrained. My favorite candidate, massive neutrinos, wouldn't show up in these searches.
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Path: arc1-ca.pugleaf.net!sparky!uunet!zaphod.mps.ohio-state.edu!rpi!usenet.coe.montana.edu!news.u.washington.edu!news.u.washington.edu!ethanb From: ethanb@ptolemy.astro.washington.edu (Ethan Bradford) Newsgroups: sci.astro Subject: Re: Dark matter Date: 24 Jan 93 23:12:46 Organization: U. of Washington Lines: 17 Message-ID: <ETHANB.93Jan24231246@ptolemy.astro.washington.edu> References: <24JAN199319274130@pavo.concordia.ca> NNTP-Posting-Host: ptolemy.astro.washington.edu In-reply-to: jt_rask@pavo.concordia.ca's message of 25 Jan 93 00:27:00 GMT TO: jt_rask@pavo.concordia.ca (RASKU, JASON T.)