PROSPECTS FOR DETECTION OF A COSMOLOGICALLY SIGNIFICANT NEUTRINO MASS FROM A GALACTIC SUPERNOVA NEUTRINO BURST USING A NEUTRAL-CURRENT-BASED DETECTOR

被引：47

作者：

CLINE, DB

FULLER, GM

HONG, WP

MEYER, B

WILSON, J

机构：

[1] UNIV CALIF SAN DIEGO,DEPT PHYS,LA JOLLA,CA 92093

[2] LAWRENCE LIVERMORE NATL LAB,LIVERMORE,CA 94550

[3] CLEMSON UNIV,DEPT PHYS & ASTRON,CLEMSON,SC 29634

来源：

PHYSICAL REVIEW D | 1994年 / 50卷 / 02期

关键词：

D O I：

10.1103/PhysRevD.50.720

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We discuss how proposed supernova neutrino detectors could measure masses for nu(mu) or nu(tau) neutrinos in the range of 15 to 50 eV. The range for measurable masses might be extended down to 5 eV, depending on our confidence in some of the predicted features of the supernova-neutrino-burst signal. We discuss the expected characteristics of supernova neutrino signals in proposed neutral-current-based detectors.

引用

页码：720 / 729

页数：10

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