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JOURNALS // Pis'ma v Zhurnal Èksperimental'noi i Teoreticheskoi Fiziki // Archive

Pis'ma v Zh. Èksper. Teoret. Fiz., 2013 Volume 98, Issue 9, Pages 587–590 (Mi jetpl3558)

This article is cited 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)

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

Language: English

DOI: 10.7868/S0370274X13210017


 English version:
Journal of Experimental and Theoretical Physics Letters, 2013, 98:9, 519–522

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© Steklov Math. Inst. of RAS, 2026