Strongly self-interacting vector dark matter via freeze-in

Abstract We study a vector dark matter (VDM) model in which the dark sector couples to the Standard Model sector via a Higgs portal. If the portal coupling is small enough the VDM can be produced via the freeze-in mechanism. It turns out that the electroweak phase transition have a substantial impac...

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Main Authors: Mateusz Duch, Bohdan Grzadkowski, Da Huang
Format: Article
Language:English
Published: SpringerOpen 2018-01-01
Series:Journal of High Energy Physics
Subjects:
Online Access:http://link.springer.com/article/10.1007/JHEP01(2018)020
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spelling doaj-dac18b5c36ec4f9a8574f9a43f2f15cd2020-11-24T22:03:05ZengSpringerOpenJournal of High Energy Physics1029-84792018-01-012018112510.1007/JHEP01(2018)020Strongly self-interacting vector dark matter via freeze-inMateusz Duch0Bohdan Grzadkowski1Da Huang2Faculty of Physics, University of WarsawFaculty of Physics, University of WarsawFaculty of Physics, University of WarsawAbstract We study a vector dark matter (VDM) model in which the dark sector couples to the Standard Model sector via a Higgs portal. If the portal coupling is small enough the VDM can be produced via the freeze-in mechanism. It turns out that the electroweak phase transition have a substantial impact on the prediction of the VDM relic density. We further assume that the dark Higgs boson which gives the VDM mass is so light that it can induce strong VDM self-interactions and solve the small-scale structure problems of the Universe. As illustrated by the latest LUX data, the extreme smallness of the Higgs portal coupling required by the freeze-in mechanism implies that the dark matter direct detection bounds are easily satisfied. However, the model is well constrained by the indirect detections of VDM from BBN, CMB, AMS-02, and diffuse γ/X-rays. Consequently, only when the dark Higgs boson mass is at most of O $$ \mathcal{O} $$(keV) does there exist a parameter region which leads to a right amount of VDM relic abundance and an appropriate VDM self-scattering while satisfying all other constraints simultaneously.http://link.springer.com/article/10.1007/JHEP01(2018)020Beyond Standard ModelCosmology of Theories beyond the SM
collection DOAJ
language English
format Article
sources DOAJ
author Mateusz Duch
Bohdan Grzadkowski
Da Huang
spellingShingle Mateusz Duch
Bohdan Grzadkowski
Da Huang
Strongly self-interacting vector dark matter via freeze-in
Journal of High Energy Physics
Beyond Standard Model
Cosmology of Theories beyond the SM
author_facet Mateusz Duch
Bohdan Grzadkowski
Da Huang
author_sort Mateusz Duch
title Strongly self-interacting vector dark matter via freeze-in
title_short Strongly self-interacting vector dark matter via freeze-in
title_full Strongly self-interacting vector dark matter via freeze-in
title_fullStr Strongly self-interacting vector dark matter via freeze-in
title_full_unstemmed Strongly self-interacting vector dark matter via freeze-in
title_sort strongly self-interacting vector dark matter via freeze-in
publisher SpringerOpen
series Journal of High Energy Physics
issn 1029-8479
publishDate 2018-01-01
description Abstract We study a vector dark matter (VDM) model in which the dark sector couples to the Standard Model sector via a Higgs portal. If the portal coupling is small enough the VDM can be produced via the freeze-in mechanism. It turns out that the electroweak phase transition have a substantial impact on the prediction of the VDM relic density. We further assume that the dark Higgs boson which gives the VDM mass is so light that it can induce strong VDM self-interactions and solve the small-scale structure problems of the Universe. As illustrated by the latest LUX data, the extreme smallness of the Higgs portal coupling required by the freeze-in mechanism implies that the dark matter direct detection bounds are easily satisfied. However, the model is well constrained by the indirect detections of VDM from BBN, CMB, AMS-02, and diffuse γ/X-rays. Consequently, only when the dark Higgs boson mass is at most of O $$ \mathcal{O} $$(keV) does there exist a parameter region which leads to a right amount of VDM relic abundance and an appropriate VDM self-scattering while satisfying all other constraints simultaneously.
topic Beyond Standard Model
Cosmology of Theories beyond the SM
url http://link.springer.com/article/10.1007/JHEP01(2018)020
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AT bohdangrzadkowski stronglyselfinteractingvectordarkmatterviafreezein
AT dahuang stronglyselfinteractingvectordarkmatterviafreezein
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