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Scale invariant extension of the SM with strongly interacting hidden sector and dark pion DM (WIMP vs. SIMP)

<!--HTML-->Scale invariant extension of the SM with QCD-like strongly interacting hidden (dark) sector is interesting, since the dimensional transmutation and chiral symmetry breaking in the hidden sector could be the origin of electroweak symmetry breaking (EWSB), and all the masses of the S...

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Autor principal: Ko, Pyungwon
Lenguaje:eng
Publicado: 2019
Materias:
Acceso en línea:http://cds.cern.ch/record/2658011
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author Ko, Pyungwon
author_facet Ko, Pyungwon
author_sort Ko, Pyungwon
collection CERN
description <!--HTML-->Scale invariant extension of the SM with QCD-like strongly interacting hidden (dark) sector is interesting, since the dimensional transmutation and chiral symmetry breaking in the hidden sector could be the origin of electroweak symmetry breaking (EWSB), and all the masses of the SM particles as well as dark pions and dark baryons that could be good cold dark matter candidates. In this talk I discuss dark pion DM as WIMP vs. SIMP. Ignoring the West-Zumio-Witten (WZW) interaction, I first discuss dark pion as a WIMP using two different approaches, the chiral perturbation theory (ChPT) and AdS/QCD. Then I include the WZW interaction and discuss dark pion within SIMP scenario. However, the analysis based on ChPT indicates that the viable parameter space for SIMP seems to be outside the validity region of ChPT. I show that this problem can be resolved if we include dark vector mesons, and the SIMP idea can be realized in the dark pion sector.
id cern-2658011
institution Organización Europea para la Investigación Nuclear
language eng
publishDate 2019
record_format invenio
spelling cern-26580112022-11-02T22:34:49Zhttp://cds.cern.ch/record/2658011engKo, PyungwonScale invariant extension of the SM with strongly interacting hidden sector and dark pion DM (WIMP vs. SIMP)Scale invariance in particle physics and cosmologyTH institutes<!--HTML-->Scale invariant extension of the SM with QCD-like strongly interacting hidden (dark) sector is interesting, since the dimensional transmutation and chiral symmetry breaking in the hidden sector could be the origin of electroweak symmetry breaking (EWSB), and all the masses of the SM particles as well as dark pions and dark baryons that could be good cold dark matter candidates. In this talk I discuss dark pion DM as WIMP vs. SIMP. Ignoring the West-Zumio-Witten (WZW) interaction, I first discuss dark pion as a WIMP using two different approaches, the chiral perturbation theory (ChPT) and AdS/QCD. Then I include the WZW interaction and discuss dark pion within SIMP scenario. However, the analysis based on ChPT indicates that the viable parameter space for SIMP seems to be outside the validity region of ChPT. I show that this problem can be resolved if we include dark vector mesons, and the SIMP idea can be realized in the dark pion sector.oai:cds.cern.ch:26580112019
spellingShingle TH institutes
Ko, Pyungwon
Scale invariant extension of the SM with strongly interacting hidden sector and dark pion DM (WIMP vs. SIMP)
title Scale invariant extension of the SM with strongly interacting hidden sector and dark pion DM (WIMP vs. SIMP)
title_full Scale invariant extension of the SM with strongly interacting hidden sector and dark pion DM (WIMP vs. SIMP)
title_fullStr Scale invariant extension of the SM with strongly interacting hidden sector and dark pion DM (WIMP vs. SIMP)
title_full_unstemmed Scale invariant extension of the SM with strongly interacting hidden sector and dark pion DM (WIMP vs. SIMP)
title_short Scale invariant extension of the SM with strongly interacting hidden sector and dark pion DM (WIMP vs. SIMP)
title_sort scale invariant extension of the sm with strongly interacting hidden sector and dark pion dm (wimp vs. simp)
topic TH institutes
url http://cds.cern.ch/record/2658011
work_keys_str_mv AT kopyungwon scaleinvariantextensionofthesmwithstronglyinteractinghiddensectoranddarkpiondmwimpvssimp
AT kopyungwon scaleinvarianceinparticlephysicsandcosmology