Loading…
Baryogenesis and dark matter from freeze-in
We propose a simple model in which the baryon asymmetry and dark matter are created via the decays and inverse decays of QCD-triplet scalars, at least one of which must be in the TeV mass range. Singlet fermions produced in these decays constitute the dark matter. The singlets never reach equilibriu...
Saved in:
Published in: | Physical review. D 2020-06, Vol.101 (11), p.1, Article 115023 |
---|---|
Main Authors: | , |
Format: | Article |
Language: | English |
Subjects: | |
Citations: | Items that this one cites Items that cite this one |
Online Access: | Get full text |
Tags: |
Add Tag
No Tags, Be the first to tag this record!
|
cited_by | cdi_FETCH-LOGICAL-c322t-8b24699a8d35f2c5f05d3246a43da4a53394eff1e36cda9b57272034a77b868e3 |
---|---|
cites | cdi_FETCH-LOGICAL-c322t-8b24699a8d35f2c5f05d3246a43da4a53394eff1e36cda9b57272034a77b868e3 |
container_end_page | |
container_issue | 11 |
container_start_page | 1 |
container_title | Physical review. D |
container_volume | 101 |
creator | Shuve, Brian Tucker-Smith, David |
description | We propose a simple model in which the baryon asymmetry and dark matter are created via the decays and inverse decays of QCD-triplet scalars, at least one of which must be in the TeV mass range. Singlet fermions produced in these decays constitute the dark matter. The singlets never reach equilibrium, and their coherent production, propagation, and annihilation generates a baryon asymmetry. We find that the out-of-equilibrium condition and the dark matter density constraint typically require the lightest scalar to be long-lived, giving good prospects for detection or exclusion in current and upcoming colliders. In generalizing the leptogenesis mechanism of Akhmedov, Rubakov and Smirnov, our model expands the phenomenological possibilities for low-scale baryogenesis. We propose a simple model in which the baryon asymmetry and dark matter are created via the decays and inverse decays of QCD-triplet scalars, at least one of which must be in the TeV mass range. Singlet fermions produced in these decays constitute the dark matter. The singlets never reach equilibrium, and their coherent production, propagation, and annihilation generates a baryon asymmetry. We find that the out-of-equilibrium condition and the dark matter density constraint typically require the lightest scalar to be long-lived, giving good prospects for detection or exclusion in current and upcoming colliders. In generalizing the leptogenesis mechanism of Akhmedov, Rubakov and Smirnov, our model expands the phenomenological possibilities for low-scale baryogenesis. |
doi_str_mv | 10.1103/PhysRevD.101.115023 |
format | article |
fullrecord | <record><control><sourceid>proquest_cross</sourceid><recordid>TN_cdi_proquest_journals_2429072050</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><sourcerecordid>2429072050</sourcerecordid><originalsourceid>FETCH-LOGICAL-c322t-8b24699a8d35f2c5f05d3246a43da4a53394eff1e36cda9b57272034a77b868e3</originalsourceid><addsrcrecordid>eNo9kE9LxDAQxYMouKz7CbwUPErXSSZpm6Ouf2FBET2HtJloV7ddk66wfnojVS8zjx-PGd5j7JjDnHPAs4fXXXykz8s5B56IAoF7bCJkCTmA0Pv_msMhm8W4giQL0CXnE3Z6YcOuf6GOYhsz27nM2fCWre0wUMh86NdpEH1R3nZH7MDb90iz3z1lz9dXT4vbfHl_c7c4X-YNCjHkVS1kobWtHCovGuVBOUzISnRWWoWoJXnPCYvGWV2rUpQCUNqyrKuiIpyyk_HuJvQfW4qDWfXb0KWXRkihIbkVJBeOrib0MQbyZhPadUpjOJifYsxfMQlwMxaD33Z-VcI</addsrcrecordid><sourcetype>Aggregation Database</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype><pqid>2429072050</pqid></control><display><type>article</type><title>Baryogenesis and dark matter from freeze-in</title><source>American Physical Society:Jisc Collections:APS Read and Publish 2023-2025 (reading list)</source><creator>Shuve, Brian ; Tucker-Smith, David</creator><creatorcontrib>Shuve, Brian ; Tucker-Smith, David</creatorcontrib><description>We propose a simple model in which the baryon asymmetry and dark matter are created via the decays and inverse decays of QCD-triplet scalars, at least one of which must be in the TeV mass range. Singlet fermions produced in these decays constitute the dark matter. The singlets never reach equilibrium, and their coherent production, propagation, and annihilation generates a baryon asymmetry. We find that the out-of-equilibrium condition and the dark matter density constraint typically require the lightest scalar to be long-lived, giving good prospects for detection or exclusion in current and upcoming colliders. In generalizing the leptogenesis mechanism of Akhmedov, Rubakov and Smirnov, our model expands the phenomenological possibilities for low-scale baryogenesis. We propose a simple model in which the baryon asymmetry and dark matter are created via the decays and inverse decays of QCD-triplet scalars, at least one of which must be in the TeV mass range. Singlet fermions produced in these decays constitute the dark matter. The singlets never reach equilibrium, and their coherent production, propagation, and annihilation generates a baryon asymmetry. We find that the out-of-equilibrium condition and the dark matter density constraint typically require the lightest scalar to be long-lived, giving good prospects for detection or exclusion in current and upcoming colliders. In generalizing the leptogenesis mechanism of Akhmedov, Rubakov and Smirnov, our model expands the phenomenological possibilities for low-scale baryogenesis.</description><identifier>ISSN: 2470-0010</identifier><identifier>EISSN: 2470-0029</identifier><identifier>DOI: 10.1103/PhysRevD.101.115023</identifier><language>eng</language><publisher>College Park: American Physical Society</publisher><subject>Asymmetry ; Baryons ; Cosmology ; Dark matter ; Decay ; Density ; Equilibrium ; Fermions ; Propagation ; Scalars</subject><ispartof>Physical review. D, 2020-06, Vol.101 (11), p.1, Article 115023</ispartof><rights>Copyright American Physical Society Jun 1, 2020</rights><lds50>peer_reviewed</lds50><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c322t-8b24699a8d35f2c5f05d3246a43da4a53394eff1e36cda9b57272034a77b868e3</citedby><cites>FETCH-LOGICAL-c322t-8b24699a8d35f2c5f05d3246a43da4a53394eff1e36cda9b57272034a77b868e3</cites><orcidid>0000-0002-3524-2021 ; 0000-0003-3345-4108</orcidid></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>314,780,784,27924,27925</link.rule.ids></links><search><creatorcontrib>Shuve, Brian</creatorcontrib><creatorcontrib>Tucker-Smith, David</creatorcontrib><title>Baryogenesis and dark matter from freeze-in</title><title>Physical review. D</title><description>We propose a simple model in which the baryon asymmetry and dark matter are created via the decays and inverse decays of QCD-triplet scalars, at least one of which must be in the TeV mass range. Singlet fermions produced in these decays constitute the dark matter. The singlets never reach equilibrium, and their coherent production, propagation, and annihilation generates a baryon asymmetry. We find that the out-of-equilibrium condition and the dark matter density constraint typically require the lightest scalar to be long-lived, giving good prospects for detection or exclusion in current and upcoming colliders. In generalizing the leptogenesis mechanism of Akhmedov, Rubakov and Smirnov, our model expands the phenomenological possibilities for low-scale baryogenesis. We propose a simple model in which the baryon asymmetry and dark matter are created via the decays and inverse decays of QCD-triplet scalars, at least one of which must be in the TeV mass range. Singlet fermions produced in these decays constitute the dark matter. The singlets never reach equilibrium, and their coherent production, propagation, and annihilation generates a baryon asymmetry. We find that the out-of-equilibrium condition and the dark matter density constraint typically require the lightest scalar to be long-lived, giving good prospects for detection or exclusion in current and upcoming colliders. In generalizing the leptogenesis mechanism of Akhmedov, Rubakov and Smirnov, our model expands the phenomenological possibilities for low-scale baryogenesis.</description><subject>Asymmetry</subject><subject>Baryons</subject><subject>Cosmology</subject><subject>Dark matter</subject><subject>Decay</subject><subject>Density</subject><subject>Equilibrium</subject><subject>Fermions</subject><subject>Propagation</subject><subject>Scalars</subject><issn>2470-0010</issn><issn>2470-0029</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2020</creationdate><recordtype>article</recordtype><recordid>eNo9kE9LxDAQxYMouKz7CbwUPErXSSZpm6Ouf2FBET2HtJloV7ddk66wfnojVS8zjx-PGd5j7JjDnHPAs4fXXXykz8s5B56IAoF7bCJkCTmA0Pv_msMhm8W4giQL0CXnE3Z6YcOuf6GOYhsz27nM2fCWre0wUMh86NdpEH1R3nZH7MDb90iz3z1lz9dXT4vbfHl_c7c4X-YNCjHkVS1kobWtHCovGuVBOUzISnRWWoWoJXnPCYvGWV2rUpQCUNqyrKuiIpyyk_HuJvQfW4qDWfXb0KWXRkihIbkVJBeOrib0MQbyZhPadUpjOJifYsxfMQlwMxaD33Z-VcI</recordid><startdate>20200601</startdate><enddate>20200601</enddate><creator>Shuve, Brian</creator><creator>Tucker-Smith, David</creator><general>American Physical Society</general><scope>AAYXX</scope><scope>CITATION</scope><scope>7U5</scope><scope>8FD</scope><scope>H8D</scope><scope>L7M</scope><orcidid>https://orcid.org/0000-0002-3524-2021</orcidid><orcidid>https://orcid.org/0000-0003-3345-4108</orcidid></search><sort><creationdate>20200601</creationdate><title>Baryogenesis and dark matter from freeze-in</title><author>Shuve, Brian ; Tucker-Smith, David</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c322t-8b24699a8d35f2c5f05d3246a43da4a53394eff1e36cda9b57272034a77b868e3</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2020</creationdate><topic>Asymmetry</topic><topic>Baryons</topic><topic>Cosmology</topic><topic>Dark matter</topic><topic>Decay</topic><topic>Density</topic><topic>Equilibrium</topic><topic>Fermions</topic><topic>Propagation</topic><topic>Scalars</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Shuve, Brian</creatorcontrib><creatorcontrib>Tucker-Smith, David</creatorcontrib><collection>CrossRef</collection><collection>Solid State and Superconductivity Abstracts</collection><collection>Technology Research Database</collection><collection>Aerospace Database</collection><collection>Advanced Technologies Database with Aerospace</collection><jtitle>Physical review. D</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Shuve, Brian</au><au>Tucker-Smith, David</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Baryogenesis and dark matter from freeze-in</atitle><jtitle>Physical review. D</jtitle><date>2020-06-01</date><risdate>2020</risdate><volume>101</volume><issue>11</issue><spage>1</spage><pages>1-</pages><artnum>115023</artnum><issn>2470-0010</issn><eissn>2470-0029</eissn><abstract>We propose a simple model in which the baryon asymmetry and dark matter are created via the decays and inverse decays of QCD-triplet scalars, at least one of which must be in the TeV mass range. Singlet fermions produced in these decays constitute the dark matter. The singlets never reach equilibrium, and their coherent production, propagation, and annihilation generates a baryon asymmetry. We find that the out-of-equilibrium condition and the dark matter density constraint typically require the lightest scalar to be long-lived, giving good prospects for detection or exclusion in current and upcoming colliders. In generalizing the leptogenesis mechanism of Akhmedov, Rubakov and Smirnov, our model expands the phenomenological possibilities for low-scale baryogenesis. We propose a simple model in which the baryon asymmetry and dark matter are created via the decays and inverse decays of QCD-triplet scalars, at least one of which must be in the TeV mass range. Singlet fermions produced in these decays constitute the dark matter. The singlets never reach equilibrium, and their coherent production, propagation, and annihilation generates a baryon asymmetry. We find that the out-of-equilibrium condition and the dark matter density constraint typically require the lightest scalar to be long-lived, giving good prospects for detection or exclusion in current and upcoming colliders. In generalizing the leptogenesis mechanism of Akhmedov, Rubakov and Smirnov, our model expands the phenomenological possibilities for low-scale baryogenesis.</abstract><cop>College Park</cop><pub>American Physical Society</pub><doi>10.1103/PhysRevD.101.115023</doi><orcidid>https://orcid.org/0000-0002-3524-2021</orcidid><orcidid>https://orcid.org/0000-0003-3345-4108</orcidid><oa>free_for_read</oa></addata></record> |
fulltext | fulltext |
identifier | ISSN: 2470-0010 |
ispartof | Physical review. D, 2020-06, Vol.101 (11), p.1, Article 115023 |
issn | 2470-0010 2470-0029 |
language | eng |
recordid | cdi_proquest_journals_2429072050 |
source | American Physical Society:Jisc Collections:APS Read and Publish 2023-2025 (reading list) |
subjects | Asymmetry Baryons Cosmology Dark matter Decay Density Equilibrium Fermions Propagation Scalars |
title | Baryogenesis and dark matter from freeze-in |
url | http://sfxeu10.hosted.exlibrisgroup.com/loughborough?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2024-12-28T09%3A16%3A50IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-proquest_cross&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.genre=article&rft.atitle=Baryogenesis%20and%20dark%20matter%20from%20freeze-in&rft.jtitle=Physical%20review.%20D&rft.au=Shuve,%20Brian&rft.date=2020-06-01&rft.volume=101&rft.issue=11&rft.spage=1&rft.pages=1-&rft.artnum=115023&rft.issn=2470-0010&rft.eissn=2470-0029&rft_id=info:doi/10.1103/PhysRevD.101.115023&rft_dat=%3Cproquest_cross%3E2429072050%3C/proquest_cross%3E%3Cgrp_id%3Ecdi_FETCH-LOGICAL-c322t-8b24699a8d35f2c5f05d3246a43da4a53394eff1e36cda9b57272034a77b868e3%3C/grp_id%3E%3Coa%3E%3C/oa%3E%3Curl%3E%3C/url%3E&rft_id=info:oai/&rft_pqid=2429072050&rft_id=info:pmid/&rfr_iscdi=true |