Affleck-Dine cogenesis of baryon and dark matter

Abstract We propose a mechanism for cogenesis of baryon and dark matter (DM) in the universe via the Affleck-Dine (AD) route. An AD field which breaks the lepton number symmetry, leads to the generation of lepton asymmetry by virtue of its cosmic evolution, which then gets transferred into lepton an...

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Main Authors: Debasish Borah, Suruj Jyoti Das, Nobuchika Okada
Format: Article
Language:English
Published: SpringerOpen 2023-05-01
Series:Journal of High Energy Physics
Subjects:
Online Access:https://doi.org/10.1007/JHEP05(2023)004
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author Debasish Borah
Suruj Jyoti Das
Nobuchika Okada
author_facet Debasish Borah
Suruj Jyoti Das
Nobuchika Okada
author_sort Debasish Borah
collection DOAJ
description Abstract We propose a mechanism for cogenesis of baryon and dark matter (DM) in the universe via the Affleck-Dine (AD) route. An AD field which breaks the lepton number symmetry, leads to the generation of lepton asymmetry by virtue of its cosmic evolution, which then gets transferred into lepton and dark sectors. While the lepton asymmetry gets converted into baryon asymmetry via sphalerons, the dark sector asymmetry leads to the final DM abundance with the symmetric part being annihilated away due to resonantly enhanced annihilation, which we choose to be provided by a gauged B − L portal. Stringent constraints from DM direct detection forces DM and B − L gauge boson masses to be light, in the few GeV ballpark. While a large portion of the model parameter space is already ruled out, the remaining parameter space is within sensitivity of laboratory as well as cosmology based experiments. The AD field also plays the role of inflaton with the required dynamics by virtue of its non-minimal coupling to gravity, consistent with observations.
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spelling doaj.art-2d996a28565d41b09d989de5d28d46012023-08-27T11:06:36ZengSpringerOpenJournal of High Energy Physics1029-84792023-05-012023511710.1007/JHEP05(2023)004Affleck-Dine cogenesis of baryon and dark matterDebasish Borah0Suruj Jyoti Das1Nobuchika Okada2Department of Physics, Indian Institute of Technology GuwahatiDepartment of Physics, Indian Institute of Technology GuwahatiDepartment of Physics, University of AlabamaAbstract We propose a mechanism for cogenesis of baryon and dark matter (DM) in the universe via the Affleck-Dine (AD) route. An AD field which breaks the lepton number symmetry, leads to the generation of lepton asymmetry by virtue of its cosmic evolution, which then gets transferred into lepton and dark sectors. While the lepton asymmetry gets converted into baryon asymmetry via sphalerons, the dark sector asymmetry leads to the final DM abundance with the symmetric part being annihilated away due to resonantly enhanced annihilation, which we choose to be provided by a gauged B − L portal. Stringent constraints from DM direct detection forces DM and B − L gauge boson masses to be light, in the few GeV ballpark. While a large portion of the model parameter space is already ruled out, the remaining parameter space is within sensitivity of laboratory as well as cosmology based experiments. The AD field also plays the role of inflaton with the required dynamics by virtue of its non-minimal coupling to gravity, consistent with observations.https://doi.org/10.1007/JHEP05(2023)004Baryo-and LeptogenesisNew Gauge InteractionsParticle Nature of Dark Matter
spellingShingle Debasish Borah
Suruj Jyoti Das
Nobuchika Okada
Affleck-Dine cogenesis of baryon and dark matter
Journal of High Energy Physics
Baryo-and Leptogenesis
New Gauge Interactions
Particle Nature of Dark Matter
title Affleck-Dine cogenesis of baryon and dark matter
title_full Affleck-Dine cogenesis of baryon and dark matter
title_fullStr Affleck-Dine cogenesis of baryon and dark matter
title_full_unstemmed Affleck-Dine cogenesis of baryon and dark matter
title_short Affleck-Dine cogenesis of baryon and dark matter
title_sort affleck dine cogenesis of baryon and dark matter
topic Baryo-and Leptogenesis
New Gauge Interactions
Particle Nature of Dark Matter
url https://doi.org/10.1007/JHEP05(2023)004
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