Spectroscopy of low energy solar neutrinos by MOON - Mo observatory of neutrinos

被引：10
|
作者：
Hazama, R [1 ]
Doe, P
Ejiri, H
Elliott, SR
Engel, J
Finger, M
Formaggio, JA
Fushimi, K
Gehman, V
Gorin, A
Greenfield, M
Ichihara, K
Ikegami, Y
Ishii, H
Itahashi, T
Kavitov, P
Kekelidze, V
Kuroda, K
Kutsalo, V
Manouilov, I
Matsuoka, K
Nakamura, H
Nomachi, M
Para, A
Rielage, K
Rjazantsev, A
Robertson, RGH
Shichijo, Y
Shima, T
Shimada, Y
Shirkov, G
Sissakian, A
Sugaya, Y
Titov, A
Vatulin, V
Vilches, OE
Voronov, V
Wilkerson, JF
Will, DI
Yoshida, S
机构：
[1] Osaka Univ, OULNS, Toyonaka, Osaka 5600043, Japan
[2] Univ Washington, CENPA, Seattle, WA 98195 USA
[3] Osaka Univ, RCNP, Osaka 5670047, Japan
[4] LANL, Los Alamos, NM 87545 USA
[5] Univ N Carolina, Chapel Hill, NC 27599 USA
[6] Charles Univ Prague, FMP, CZ-18000 Prague 8, Czech Republic
[7] Univ Tokushima, IAS, Tokushima 7708592, Japan
[8] IHEP, Protvino 142284, Russia
[9] Int Christian Univ, Tokyo 1818585, Japan
[10] VNIIEF, Sarov, Russia
[11] Joint Inst Nucl Res, Dubna 141980, Russia
[12] CERN Prevessian, CH-1211 Geneva 23, Switzerland
[13] Fermilab Natl Accelerator Lab, Batavia, IL 60510 USA
来源：
NUCLEAR PHYSICS B-PROCEEDINGS SUPPLEMENTS | 2005年 / 138卷
关键词：
D O I：
10.1016/j.nuclphysbps.2004.11.025
中图分类号：
O412 [相对论、场论]; O572.2 [粒子物理学];
学科分类号：
摘要：
The MOON (Molybdenum Observatory Of Neutrinos) project aims at high sensitive studies of the double beta (betabeta) decays with sensitivity to Majorana v mass of the order of < m(v) >similar to0.03 eV and the charged-current (CC) neutrino spectroscopy of the major components of the pp and Be-7 solar v's. The present status of MOON for the low energy solar v experiment is briefly discussed. The inverse 3 rays from solar-v captures of Mo-100 are measured in delayed coincidence with the subsequent beta decay of Tc-100. MOON's exclusive CC value by Be-7 solar v, together with the GNO CC data, will provide the pp solar v flux with good accuracy.
引用
收藏
页码：102 / 105
页数：4
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