Antiprotons at solar maximum

被引:83
作者
Bieber, JW [1 ]
Burger, RA
Engel, R
Gaisser, TK
Roesler, S
Stanev, T
机构
[1] Univ Delaware, Bartol Res Inst, Newark, DE 19716 USA
[2] Potchefstroom Univ Christian Higher Educ, Sch Phys, Space Res Unit, ZA-2520 Potchefstroom, South Africa
[3] CERN, CH-1211 Geneva 23, Switzerland
基金
美国国家科学基金会;
关键词
D O I
10.1103/PhysRevLett.83.674
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
New measurements with good statistics will make it possible to observe the time variation of cosmic antiprotons at I AU through the approaching peak of solar activity. We report a new computation of the interstellar antiproton spectrum expected from collisions between cosmic protons and the interstellar gas. This spectrum is then used as input to a steady-state drift model of solar modulation, in order to provide predictions for the antiproton spectrum as well as the antiproton/proton ratio at 1 AU. Our model predicts a surprisingly large, rapid increase in the antiproton/proton ratio through the next solar maximum, followed by a large excursion in the ratio during the following decade.
引用
收藏
页码:674 / 677
页数:4
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