Origin of the highest energy cosmic rays

被引:29
作者
Biermann, PL
Ahn, EJ
Medina-Tanco, G
Stanev, T
机构
[1] Max Planck Inst Radioastron, D-5300 Bonn, Germany
[2] Seoul Natl Univ, Dept Phys, Seoul 151742, South Korea
[3] Univ Sao Paulo, Inst Astron & Geophys, Sao Paulo, Brazil
[4] Univ Delaware, Bartol Res Inst, Newark, DE 19716 USA
基金
巴西圣保罗研究基金会; 美国国家航空航天局;
关键词
D O I
10.1016/S0920-5632(00)00708-8
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
Introducing a simple Galactic wind model patterned after the solar wind we show that back-tracing the orbits of the highest energy cosmic events suggests that they may all come from the Virgo cluster, and so probably from the active radio galaxy M87. This confirms a long standing expectation. Those powerful radio galaxies that have their relativistic jets stuck in the interstellar medium of the host galaxy, such as 3C147, will then enable us to derive limits on the production of any new kind of particle, expected in some extensions of the standard model in particle physics. New data from HIRES will be crucial in testing the model proposed here.
引用
收藏
页码:417 / 419
页数:3
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