MASS LIMITS FOR DARK-MATTER PARTICLES DERIVED FROM HIGH-ENERGY NEUTRINOS FROM THE SUN

被引：20

作者：

SATO, N

HIRATA, KS

KAJITA, T

KIFUNE, T

KIHARA, K

NAKAHATA, M

NAKAMURA, K

OHARA, S

SUZUKI, Y

TOTSUKA, Y

YAGINUMA, Y

MORI, M

OYAMA, Y

SUZUKI, A

TAKAHASHI, K

TAKEI, H

TANIMORI, T

KOSHIBA, M

SUDA, T

TAJIMA, T

MIYANO, K

MIYATA, H

YAMADA, M

FUKUDA, Y

KANEYUKI, K

NAGASHIMA, Y

TAKITA, M

BEIER, EW

FELDSCHER, LR

FRANK, ED

FRATI, W

KIM, SB

MANN, AK

NEWCOMER, FM

VANBERG, R

ZHANG, W

机构：

[1] UNIV TOKYO,INST COSM RAY RES,TANASHI,TOKYO 188,JAPAN

[2] NIIGATA UNIV,NIIGATA 95021,JAPAN

[3] TOKAI UNIV,SHIBUYA,TOKYO 151,JAPAN

[4] KOBE UNIV,DEPT PHYS,KOBE 657,JAPAN

[5] OSAKA UNIV,DEPT PHYS,TOYONAKA,OSAKA 560,JAPAN

[6] UNIV PENN,DEPT PHYS,PHILADELPHIA,PA 19104

来源：

PHYSICAL REVIEW D | 1991年 / 44卷 / 08期

关键词：

D O I：

10.1103/PhysRevD.44.2220

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

High-energy neutrinos could be emitted from the center of the Sun as annihilation products of heavy galactic dark-matter particles. We analyze neutrino events observed by the Kamiokande detector to search for such neutrinos. The observed upper limits on solar high-energy neutrinos from these data set limits on the mass and density of certain galactic dark matter. The particles analyzed are heavy Dirac neutrinos (nu-D), heavy Majorana neutrinos (nu-M), Higgsinos (h approximately), sneutrinos (nu approximately) with three flavors, and photinos (gamma approximately) as the lightest supersymmetric particles. Excluded mass regions are obtained for each dark-matter candidate: 3 GeV < m-nu-D < 100 GeV, 3 GeV < m-nu approximately e < 90 GeV, 3 GeV < m-nu approximately mu < 90 GeV, and 4 GeV < m-nu approximately tau < 90 GeV. No limits are obtained on the masses of nu-M, h approximately, and gamma approximately yet.

引用

页码：2220 / 2240

页数：21

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