High energy neutrino emission from young pulsars

被引：0
|
作者：
Burgio, G. F.
Link, B.
机构：
[1] Ist Nazl Fis Nucl, Sez Catania, I-95123 Catania, Italy
[2] Montana State Univ, Dept Phys, Bozeman, MT 59717 USA
来源：
NUCLEAR INSTRUMENTS & METHODS IN PHYSICS RESEARCH SECTION A-ACCELERATORS SPECTROMETERS DETECTORS AND ASSOCIATED EQUIPMENT | 2006年 / 567卷 / 02期
关键词：
neutrinos; stars : neutron; pulsars : general; magnetic fields;
D O I：
10.1016/j.nima.2006.05.182
中图分类号：
TH7 [仪器、仪表];
学科分类号：
0804 ; 080401 ; 081102 ;
摘要：
We propose that young (t(age) <= 10(5) yr), rapidly rotating pulsars can accelerate ions to energies of similar to 1 PeV near the surface of a neutron star. Protons undergo resonant excitation with surface X-rays and produce a beam of y neutrinos with energies of several tens of TeV which could be detectable by current technology. Detection of these neutrinos would further our understanding of high-energy processes that take place in the stellar magnetosphere. (c) 2006 Elsevier B.V. All rights reserved.
引用
收藏
页码：486 / 488
页数：3
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