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

页码：102 / 105

页数：4