Early decay of Peccei–Quinn fermion and the IceCube neutrino events

IceCube observed high-energy neutrino flux in the energy region from TeV to PeV. The decay of a massive long-lived particle in the early universe can be the origin of the IceCube neutrino events, which we call an “early decay scenario.” In this paper, we construct a particle physics model that conta...

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Main Authors: Yohei Ema, Takeo Moroi
Format: Article
Language:English
Published: Elsevier 2016-11-01
Series:Physics Letters B
Online Access:http://www.sciencedirect.com/science/article/pii/S0370269316305524
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spelling doaj-46719e7427be43a7abb067c678b87dc72020-11-25T00:31:53ZengElsevierPhysics Letters B0370-26932016-11-01762353361Early decay of Peccei–Quinn fermion and the IceCube neutrino eventsYohei Ema0Takeo Moroi1Corresponding author.; Department of Physics, Faculty of Science, The University of Tokyo, Bunkyo-ku, Tokyo 133-0033, JapanDepartment of Physics, Faculty of Science, The University of Tokyo, Bunkyo-ku, Tokyo 133-0033, JapanIceCube observed high-energy neutrino flux in the energy region from TeV to PeV. The decay of a massive long-lived particle in the early universe can be the origin of the IceCube neutrino events, which we call an “early decay scenario.” In this paper, we construct a particle physics model that contains such a massive long-lived particle based on the Peccei–Quinn model. We calculate the present neutrino flux, taking account of realistic initial energy distributions of particles produced by the decay of the massive long-lived particle. We show that the early decay scenario naturally fits into the Peccei–Quinn model, and that the neutrino flux observed by IceCube can be explained in such a framework. We also see that, based on that model, a consistent cosmological history that explains the abundance of the massive long-lived particle is realized.http://www.sciencedirect.com/science/article/pii/S0370269316305524
collection DOAJ
language English
format Article
sources DOAJ
author Yohei Ema
Takeo Moroi
spellingShingle Yohei Ema
Takeo Moroi
Early decay of Peccei–Quinn fermion and the IceCube neutrino events
Physics Letters B
author_facet Yohei Ema
Takeo Moroi
author_sort Yohei Ema
title Early decay of Peccei–Quinn fermion and the IceCube neutrino events
title_short Early decay of Peccei–Quinn fermion and the IceCube neutrino events
title_full Early decay of Peccei–Quinn fermion and the IceCube neutrino events
title_fullStr Early decay of Peccei–Quinn fermion and the IceCube neutrino events
title_full_unstemmed Early decay of Peccei–Quinn fermion and the IceCube neutrino events
title_sort early decay of peccei–quinn fermion and the icecube neutrino events
publisher Elsevier
series Physics Letters B
issn 0370-2693
publishDate 2016-11-01
description IceCube observed high-energy neutrino flux in the energy region from TeV to PeV. The decay of a massive long-lived particle in the early universe can be the origin of the IceCube neutrino events, which we call an “early decay scenario.” In this paper, we construct a particle physics model that contains such a massive long-lived particle based on the Peccei–Quinn model. We calculate the present neutrino flux, taking account of realistic initial energy distributions of particles produced by the decay of the massive long-lived particle. We show that the early decay scenario naturally fits into the Peccei–Quinn model, and that the neutrino flux observed by IceCube can be explained in such a framework. We also see that, based on that model, a consistent cosmological history that explains the abundance of the massive long-lived particle is realized.
url http://www.sciencedirect.com/science/article/pii/S0370269316305524
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