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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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 |
work_keys_str_mv |
AT yoheiema earlydecayofpecceiquinnfermionandtheicecubeneutrinoevents AT takeomoroi earlydecayofpecceiquinnfermionandtheicecubeneutrinoevents |
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