PROGRESS AND PROSPECTS IN NEUTRINO ASTROPHYSICS

被引：21
|
作者：
BAHCALL, JN
LANDE, K
LANOU, RE
LEARNED, JG
ROBERTSON, RGH
WOLFENSTEIN, L
机构：
[1] UNIV PENN,DEPT PHYS,PHILADELPHIA,PA 19104
[2] BROWN UNIV,DEPT PHYS,PROVIDENCE,RI 02912
[3] UNIV HAWAII,DEPT PHYS & ASTRON,HONOLULU,HI 96822
[4] LOS ALAMOS NATL LAB,DIV PHYS,LOS ALAMOS,NM 87545
[5] UNIV WASHINGTON,DEPT PHYS,SEATTLE,WA 98195
[6] CARNEGIE MELLON UNIV,DEPT PHYS,PITTSBURGH,PA 15213
来源：
NATURE | 1995年 / 375卷 / 6526期
关键词：
D O I：
10.1038/375029a0
中图分类号：
O [数理科学和化学]; P [天文学、地球科学]; Q [生物科学]; N [自然科学总论];
学科分类号：
07 ; 0710 ; 09 ;
摘要：
Four separate experiments to detect neutrinos from the Sun have now confirmed a deficit in the flux relative to the predictions of standard theories of nuclear physics. Future experiments with new neutrino detectors promise to reveal the explanation for this shortfall. The planned detectors may also engender a new field of astronomy, based on the observation of neutrino emission from distant, energetic astrophysical sources.
引用
收藏
页码：29 / 34
页数：6
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