Ultra high energy cosmic rays

被引:22
作者
Berezinsky, V [1 ]
机构
[1] Ist Nazl Fis Nucl, Lab Nazl Gran Sasso, I-67010 Assergi, AQ, Italy
[2] Russian Acad Sci, Inst Nucl Res, Moscow, Russia
关键词
D O I
10.1016/S0920-5632(98)00463-0
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
The current status of Ultra High Energy Cosmic Rays (UHECR) is reviewed, with emphasis given to theoretical interpretation of the observed events. The galactic and extragalactic origin, in case of astrophysical sources of UHE particles, have the problems either with acceleration to the observed energies or with the fluxes and spectra. Topological defects can naturally produce particles with energies as observed and much higher, but in most cases fail to produce the observed fluxes. Cosmic necklaces and monopole-antimonopole pairs are identified as most plausible sources, which can provide the observed Aux and spectrum. The relic superheavy particles are shown to be clustering in the Galactic halo, producing UHECR without Greisen-Zatsepin-Kuzmin cutoff. The Lightest Supersymmetric Particles are discussed as UHE carriers in the Universe.
引用
收藏
页码:419 / 430
页数:12
相关论文
共 84 条
[81]   THE COSMIC-RAY ENERGY-SPECTRUM ABOVE 10(17) EV [J].
WINN, MM ;
ULRICHS, J ;
PEAK, LS ;
MCCUSKER, CBA ;
HORTON, L .
JOURNAL OF PHYSICS G-NUCLEAR AND PARTICLE PHYSICS, 1986, 12 (07) :653-674
[82]   SUPERCONDUCTING STRINGS [J].
WITTEN, E .
NUCLEAR PHYSICS B, 1985, 249 (04) :557-592
[83]   THE COSMIC-RAY ENERGY-SPECTRUM ABOVE 3X10(18) EV MEASURED BY THE AKENO GIANT AIR SHOWER ARRAY [J].
YOSHIDA, S ;
HAYASHIDA, N ;
HONDA, K ;
HONDA, M ;
IMAIZUMI, S ;
INOUE, N ;
KADOTA, K ;
KAKIMOTO, F ;
KAMATA, K ;
KAWAGUCHI, S ;
KAWASUMI, N ;
MATSUBARA, Y ;
MURAKAMI, K ;
NAGANO, M ;
OHOKA, H ;
TESHIMA, M ;
TSUSHIMA, I ;
YOSHII, H .
ASTROPARTICLE PHYSICS, 1995, 3 (02) :105-123
[84]  
ZATSEPIN GT, 1966, JETP LETT-USSR, V4, P78