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Pis'ma v Zhurnal Èksperimental'noi i Teoreticheskoi Fiziki, 2013, Volume 98, Issue 9, Pages 587–590
DOI: https://doi.org/10.7868/S0370274X13210017 (Mi jetpl3558) 		 
This article is cited in 11 scientific papers (total in 11 papers)

ASTROPHYSICS AND COSMOLOGY

How to see an antistar

A. D. Dolgovabcd, V. A. Novikovaebf, M. I. Vysotskygbae

a Novosibirsk State University
b Institute for Theoretical and Experimental Physics (Russian Federation State Scientific Center), Moscow
c University of Ferrara
d Istituto Nazionale di Fisica Nucleare
e Moscow Institute of Physics and Technology
f Moscow Engineering Physics Institute
g Moscow Engineering Physics Institute (State University)
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DOI: https://doi.org/10.7868/S0370274X13210017
Abstract: Polarization of photons emitted in weak decays occuring at distant star allows to determine whether this star is made from antimatter. Even more promissing is the observation of neutrinos (antineutrinos) produced at neutronization (antineutronization) reactions at the beginning of SN ($\overline{SN}$) explosion.
Received: 19.09.2013
English version:
Journal of Experimental and Theoretical Physics Letters, 2013, Volume 98, Issue 9, Pages 519–522
DOI: https://doi.org/10.1134/S0021364013220037
Bibliographic databases:
Document Type: Article
Language: English
Citation: A. D. Dolgov, V. A. Novikov, M. I. Vysotsky, “How to see an antistar”, Pis'ma v Zh. Èksper. Teoret. Fiz., 98:9 (2013), 587–590; JETP Letters, 98:9 (2013), 519–522
Citation in format AMSBIB
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\paper How to see an antistar
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\vol 98
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\pages 587--590
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    • This publication is cited in the following 11 articles:
    Citing articles in Google Scholar: Russian citations, English citations
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