Einstein@home :: Remember, remember, the velvet November


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created:	14.05.2009 - 14:42:04
updated:	13.08.2010 - 17:56:02

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Einstein@home sa podiela na spracovani dat z vyskumnych pracovisk interferometrov LIGO (USA), GEO 600 (Nemecko,Britania) a dat z observatoria Arecibo (Portoriko,USA). Cielom vyskumu je priama detekcia gravitacnych vln, ktorych existencia vyplyva z teorie relativity (ich existencia bola zatial potvrdena iba nepriamo). Zdrojmi detekovatelnych gravitacnych vln by mali byt pulzary, binarne systemy, supernovy... Projekt ma aj graficky vystup (video).

oficialna stranka projektu
wikipedia/Einstein_at_home
server status

o projekte Einstein@home v cestine

ceske a slovenske forum k projektu
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(full verzia 20min, RealPlayer)
+ine video
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dalsie linky:
gravitacne vlny
gravitacne vlny podrobne
LISA
Teoria relativity

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A new preprint reports the second Einstein@Home discovery, of a radio pulsar orbiting a white dwarf star once every 9.4 hours. The pulsar, called J1952+2630, is spinning on its axis 48 times per second. It was discovered in data collected at Arecibo Observatory in 2005 by the PALFA Collaboration. The white-dwarf companion star is unusually massive, and weighs at least 95% as much as our sun. This means that J1952+2630 probably belongs to a rare class of intermediate-mass binary pulsars (five were previously known).

Congratulations to the two Einstein@Home participants whose computers found J1952+2630 with the highest significance: Dr. Vitaliy V. Shiryaev (Moscow, Russia) and Stacey Eastham (Darwen, UK)! And a big "thank you" to all Einstein@Home volunteers, whose continuing support makes these exciting discoveries possible.

Bruce Allen
Director, Einstein@Home
http://einstein.phys.uwm.edu/forum_thread.php?id=8788

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Home computers discover rare star (nature.com)

"Three citizen scientists - a German and an American couple - have discovered a new radio pulsar hidden in data gathered by the Arecibo Observatory. The newly discovered radio pulsar, given the designation PSR J2007+2722, is a fast-spinning neutron star which can be formed in certain types of supernovae, or stellar explosions. It is the first deep space discovery made by the project."

info na stranke projektu
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o projekte Einstein@home

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vyborna praca - ak sa kamyl nenahneva mohli by sme jeho prispevok ponat ako template pre ostatne - a ostatne tiez podobne vyrobit. Ked bude cas a chut pochopitelne.

- popis s odkazmi a grafickym vystupom
- naky pekny obrazok nech to je aj ilustrovane :)
- ceske a slovenske fora - odkazy
- video

tamto video je fantasticke, uplne vysvetluje o co ide. hned ma clovek jasnu predstavu