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Experimental study of terrestrial el...

Stanford University.

Experimental study of terrestrial electron anti-neutrinos with kamLAND.

紀錄類型:	書目-電子資源 : Monograph/item
正題名/作者:	Experimental study of terrestrial electron anti-neutrinos with kamLAND.
作者:	Tolich, Nikolai R.
面頁冊數:	109 p.
附註:	Adviser: Giorgio Gratta.
附註:	Source: Dissertation Abstracts International, Volume: 66-01, Section: B, page: 0336.
Contained By:	Dissertation Abstracts International66-01B.
標題:	Physics, Elementary Particles and High Energy.
電子資源:	http://pqdd.sinica.edu.tw/twdaoapp/servlet/advanced?query=3162346
ISBN:	9780496962334

Experimental study of terrestrial electron anti-neutrinos with kamLAND.
Tolich, Nikolai R.

Experimental study of terrestrial electron anti-neutrinos with kamLAND. - 109 p.

Adviser: Giorgio Gratta.

Thesis (Ph.D.)--Stanford University, 2005.

Based on a total of (2.63 +/- 0.19) x 1031 target proton-years (0.506 kton-years), the 90% confidence interval for the total number of terrestrial 238U and 212Th ne&d1;' s detected is 4 to 40. This is consistent with the best models of terrestrial 238U and 232Th content.

ISBN: 9780496962334Subjects--Topical Terms:

227490
Physics, Elementary Particles and High Energy.

Experimental study of terrestrial electron anti-neutrinos with kamLAND.
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245 1 0 $a Experimental study of terrestrial electron anti-neutrinos with kamLAND.
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502 $a Thesis (Ph.D.)--Stanford University, 2005.
520 # $a Based on a total of (2.63 +/- 0.19) x 1031 target proton-years (0.506 kton-years), the 90% confidence interval for the total number of terrestrial 238U and 212Th ne&d1;' s detected is 4 to 40. This is consistent with the best models of terrestrial 238U and 232Th content.
520 # $a The analysis presented here uses Kamioka Liquid scintillator Anti-Neutrino Detector (KamLAND) to measure the rate of electron anti-neutrinos, ne&d1;' s , produced from terrestrial 238U and 212Th. 238U and 212Th are thought to be the main heat source driving mantle convection in the Earth, which in turn is responsible for plate tectonics. The total terrestrial 238U and 212Th content has been estimated from Earth models and rock samples from a very small fraction of the Earth. Until now there have been no direct measurements. Since ne&d1;' s have an exceedingly small cross section, they propagate undisturbed in the Earth interior, and their measurement near the Earth surface can be used to gain information on their sources.
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