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Pis'ma v Zh. Èksper. Teoret. Fiz., 2015, Volume 101, Issue 1, Pages 3–8 (Mi jetpl4509)  

This article is cited in 28 scientific papers (total in 28 papers)

ASTROPHYSICS AND COSMOLOGY

Fast radio bursts and axion miniclusters

I. I. Tkachev

Institute for Nuclear Research, Russian Academy of Sciences, Moscow

Abstract: Non-linear effects in the evolution of the axion field in the early Universe may lead to the formation of gravitationally bound clumps of axions, known as “miniclusters.” Minicluster masses should be in the range $M_{mc}\sim10^{-12} M_\odot$, and in plausible early-Universe scenarios a significant fraction of the mass density of the Universe may be in the form of axion miniclusters. Here I argue that observed properties (total energy release, duration, high brightness temperature, event rate) of recently discovered Fast Radio Bursts can be matched in a model which assumes explosive decay of axion miniclusters.

DOI: https://doi.org/10.7868/S0370274X15010014

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English version:
Journal of Experimental and Theoretical Physics Letters, 2015, 101:1, 1–6

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Received: 11.11.2014
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Citation: I. I. Tkachev, “Fast radio bursts and axion miniclusters”, Pis'ma v Zh. Èksper. Teoret. Fiz., 101:1 (2015), 3–8; JETP Letters, 101:1 (2015), 1–6

Citation in format AMSBIB
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\by I.~I.~Tkachev
\paper Fast radio bursts and axion miniclusters
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\pages 3--8
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  •       Pis'ma v Zhurnal ksperimental'noi i Teoreticheskoi Fiziki
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