How to see an antistar

被引：0
作者：
A. D. Dolgov
V. A. Novikov
M. I. Vysotsky
机构：
[1] Alikhanov Institute for Theoretical and Experimental Physics,Dipartimento di Fisica e Scienze della Terra
[2] Novosibirsk State University,Istituto Nazionale di Fisica Nucleare, Sezione di Ferrara
[3] Università degli Studi di Ferrara,undefined
[4] Polo Scientifico e Tecnologico-Edificio C,undefined
[5] Polo Scientifico e Tecnologico-Edificio C,undefined
[6] National Research Nuclear University MEPhI,undefined
[7] Moscow Institute of Physics and Technology,undefined
来源：
JETP Letters | 2014年 / 98卷
关键词：
JETP Letter; Strange Quark; Baryon Asymmetry; Stellar System; Strange Star;
D O I：
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中图分类号：
学科分类号：
摘要：
Polarization of photons emitted in weak decays occurring at distant star makes it possible to determine whether this star is made from antimatter. The observation of neutrinos (antineutrinos) produced at neutronization (antineutronization) reactions at the beginning of SN \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$\left( {\overline {SN} } \right)$$\end{document} explosion is even more promising.
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页码：519 / 522
页数：3
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