[tt] the physics arXiv blog
Eugen Leitl
<eugen at leitl.org> on
Wed Apr 16 08:04:39 UTC 2008
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From: the physics arXiv blog <howdy at arxivblog.com>
Date: Tue, 15 Apr 2008 17:33:45 -0500 (CDT)
To: eugen at leitl.org
Subject: the physics arXiv blog
Reply-To: the physics arXiv blog <howdy at arxivblog.com>
[1]the physics arXiv blog
[2]Diamonds in the sky: a miner's guide
Posted: 15 Apr 2008 12:46 AM CDT
[3]Diamonds in the sky
Astronomers have recently wondered whether carbon might form a
supercooled liquid under the huge pressures that exist in side
carbon-rich white dwarf stars and even inside medium-sized gaseous
planets such as neptune and uranus. If that's the case, then small
disturbances in the liquid could trigger the formation of diamonds the
size of automobiles.
The trouble is that nobody has been able to create these conditions on
Earth so the way in which nucleation might occur is more or less
unknown.
Now Daan Frenkel and pals from the University of Amsterdam in The
Netherlands say that computer simulations of the behaviour of several
thousand carbon atoms under these circumstances have given us the
first inkling of how nucleation occur. And the odds are that it's a
tricky process to set in motion.
Applying these results to astrophysical bodies gives two insights,
both of which are bad news for diamond hunters.
First, nucleation may be so rare that "not a single diamond could
have nucleated in a Uranus-sized body during the life of the
universe."
And second, the appropriate conditions may be common in certain white
dwarf stars.
Either way, these diamonds are outta bounds for the foreseeable
future.
Ref: [4]arxiv.org/abs/0804.1671: State-of-the-art models for the Phase
Diagram of Carbon and Diamond Nucleation
[5][arXivblog?i=sb2M7v]
[6][arXivblog?i=Sy0iZJG] [7][arXivblog?i=GxAhQGG]
[8][arXivblog?i=p855Spg] [9][arXivblog?i=fc6HoiG]
[10][arXivblog?i=LPao7dg] [11][arXivblog?i=jScc1oG]
[12][arXivblog?i=9kTWvbg] [13][arXivblog?i=Mkfd5AG]
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References
1. http://arxivblog.com/
2. http://feeds.feedburner.com/~r/arXivblog/~3/270484866/
3. http://arxivblog.com/wp-content/uploads/2008/04/diamond.JPG
4. http://arxiv.org/abs/0804.1671
5. http://feeds.feedburner.com/~a/arXivblog?a=sb2M7v
6. http://feeds.feedburner.com/~f/arXivblog?a=Sy0iZJG
7. http://feeds.feedburner.com/~f/arXivblog?a=GxAhQGG
8. http://feeds.feedburner.com/~f/arXivblog?a=p855Spg
9. http://feeds.feedburner.com/~f/arXivblog?a=fc6HoiG
10. http://feeds.feedburner.com/~f/arXivblog?a=LPao7dg
11. http://feeds.feedburner.com/~f/arXivblog?a=jScc1oG
12. http://feeds.feedburner.com/~f/arXivblog?a=9kTWvbg
13. http://feeds.feedburner.com/~f/arXivblog?a=Mkfd5AG
14. http://arxivblog.com/
15. http://www.feedburner.com/fb/a/emailunsub?id=8632699&key=kesJ612ZsV
16. http://feeds.feedburner.com/arXivblog
17. http://feeds.feedburner.com/arXivblog
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Eugen* Leitl <a href="http://leitl.org">leitl</a> http://leitl.org
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