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#1904 | |
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"Mike"
Aug 2002
200408 Posts |
http://www.latimes.com/science/scien...205-story.html
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#1905 | |
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Bamboozled!
"𒉺𒌌𒇷𒆷𒀭"
May 2003
Down not across
29×3×7 Posts |
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#1906 | |
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"Kieren"
Jul 2011
In My Own Galaxy!
2·3·1,693 Posts |
https://www.theguardian.com/science/...ther-evolution
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#1907 | |
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"Mike"
Aug 2002
25·257 Posts |
http://arstechnica.com/science/2016/...to-the-jungle/
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#1908 | |
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"Kieren"
Jul 2011
In My Own Galaxy!
2·3·1,693 Posts |
http://arstechnica.com/science/2016/...go-in-jericho/
Quote:
Last fiddled with by kladner on 2016-12-12 at 21:34 |
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#1909 |
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∂2ω=0
Sep 2002
República de California
103×113 Posts |
LIGO black hole echoes hint at general-relativity breakdown | Nature
This sort of first-hint needs to taken with a huge grain of salt. Remember the ‘discovery’ in the late 1990s based on a survey of distant Type 1a “standard candle” supernovae that the universe is expanding at an accelerating rate? The one that earned the researchers a Nobel prize 5 years ago? Cf. the 10/21 phys.org piece “The universe is expanding at an accelerating rate—or is it?” Or the “exotic new particle discovered at CERN” earlier this year? The one hat led to a tsunami of ~500 papes posted to arVix within weeks? Since debunked. In the present case, the ‘evidence’ appears even more tenuous. And it’s a well-known bias that when presented with data which are not instantly explainable by known physics, physicists tend to leap at the most exotic possible explanations. New physics is ‘sexy’, basically. |
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#1910 | |
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Apr 2014
27 Posts |
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Does density of an arbitrary mass change with velocity to an observer that is travelling at the same velocity (no, I think)? A 'stationary' observer (possibly yes, I think)? Ramifications (I think these maybe ignorant questions)? |
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#1911 | |
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Bamboozled!
"𒉺𒌌𒇷𒆷𒀭"
May 2003
Down not across
29×3×7 Posts |
Quote:
Another way to see it is that non-planar gravitational waves themselves contain energy in a localised region of space-time. If they are appropriately focussed the mass-energy density of the waves is enough to cause gravitational collapse, taking with it any matter that happens to be around. Note that this can't happen for plane waves. Last fiddled with by xilman on 2016-12-13 at 07:48 |
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#1912 | |
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∂2ω=0
Sep 2002
República de California
103·113 Posts |
Quote:
Last fiddled with by ewmayer on 2016-12-13 at 09:22 |
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#1913 | |
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(loop (#_fork))
Feb 2006
Cambridge, England
72×131 Posts |
Quote:
(a strain of 100 microns per parsec at 400 megaparsecs is one kilometre per parsec at 40 parsecs, and one kilometre per parsec is five millimetres per astronomical unit) |
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#1914 |
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Apr 2012
Brady
27·3 Posts |
For anyone wishing to explore (please click the link at the bottom of the page to go to the AEI site which is one of the best in the world):
http://grtensor.phy.queensu.ca/ "Theory and experiment in gravitational physics." by Clifford Will. The software I've used for years and the book dates from the early '80's with a revised edition in the early 90's and both editions are a good introduction. Online, there is a good site at Caltech: http://www.tapir.caltech.edu/~teviet/Waves/index.html which has a few "flashy thingies" for those interested in a more dynamic presentation. Last fiddled with by jwaltos on 2016-12-13 at 16:30 Reason: addendum to site info. |
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