The QCD axion from aligned axions and diphoton excess

We argue that the QCD axion can arise from many aligned axions with decay constants much smaller than the conventional axion window. If the typical decay constant is of O(100) GeV to 1 TeV, one or more of the axions or saxions may account for the recently found diphoton excess at ∼750 GeV. Our scena...

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Main Authors: Tetsutaro Higaki, Kwang Sik Jeong, Naoya Kitajima, Fuminobu Takahashi
Format: Article
Language:English
Published: Elsevier 2016-04-01
Series:Physics Letters B
Online Access:http://www.sciencedirect.com/science/article/pii/S0370269316000745
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spelling doaj-452aab19c61348eb87618a11caa4b7b32020-11-24T21:34:16ZengElsevierPhysics Letters B0370-26932016-04-017551316The QCD axion from aligned axions and diphoton excessTetsutaro Higaki0Kwang Sik Jeong1Naoya Kitajima2Fuminobu Takahashi3Department of Physics, Keio University, Kanagawa 223-8522, JapanDepartment of Physics, Pusan National University, Busan, 609-735, Republic of Korea; Corresponding author.Asia Pacific Center for Theoretical Physics, Pohang 790-784, Republic of KoreaDepartment of Physics, Tohoku University, Sendai, Miyagi 980-8578, Japan; Kavli IPMU (WPI), UTIAS, The University of Tokyo, Kashiwa, Chiba 277-8583, JapanWe argue that the QCD axion can arise from many aligned axions with decay constants much smaller than the conventional axion window. If the typical decay constant is of O(100) GeV to 1 TeV, one or more of the axions or saxions may account for the recently found diphoton excess at ∼750 GeV. Our scenario predicts many axions and saxions coupled to gluons with decay constants of order the weak scale, and therefore many collider signatures by heavy axions and saxions will show up at different energy scales. In particular, if the inferred broad decay width is due to multiple axions or saxions, a non-trivial peak structure may become evident when more data is collected. We also discuss cosmological implications of the aligned QCD axion scenario. In the Appendix we give a possible UV completion and argue that the high quality of the Peccei–Quinn symmetry is naturally explained in our scenario.http://www.sciencedirect.com/science/article/pii/S0370269316000745
collection DOAJ
language English
format Article
sources DOAJ
author Tetsutaro Higaki
Kwang Sik Jeong
Naoya Kitajima
Fuminobu Takahashi
spellingShingle Tetsutaro Higaki
Kwang Sik Jeong
Naoya Kitajima
Fuminobu Takahashi
The QCD axion from aligned axions and diphoton excess
Physics Letters B
author_facet Tetsutaro Higaki
Kwang Sik Jeong
Naoya Kitajima
Fuminobu Takahashi
author_sort Tetsutaro Higaki
title The QCD axion from aligned axions and diphoton excess
title_short The QCD axion from aligned axions and diphoton excess
title_full The QCD axion from aligned axions and diphoton excess
title_fullStr The QCD axion from aligned axions and diphoton excess
title_full_unstemmed The QCD axion from aligned axions and diphoton excess
title_sort qcd axion from aligned axions and diphoton excess
publisher Elsevier
series Physics Letters B
issn 0370-2693
publishDate 2016-04-01
description We argue that the QCD axion can arise from many aligned axions with decay constants much smaller than the conventional axion window. If the typical decay constant is of O(100) GeV to 1 TeV, one or more of the axions or saxions may account for the recently found diphoton excess at ∼750 GeV. Our scenario predicts many axions and saxions coupled to gluons with decay constants of order the weak scale, and therefore many collider signatures by heavy axions and saxions will show up at different energy scales. In particular, if the inferred broad decay width is due to multiple axions or saxions, a non-trivial peak structure may become evident when more data is collected. We also discuss cosmological implications of the aligned QCD axion scenario. In the Appendix we give a possible UV completion and argue that the high quality of the Peccei–Quinn symmetry is naturally explained in our scenario.
url http://www.sciencedirect.com/science/article/pii/S0370269316000745
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