Implication of preheating on gravity assisted baryogenesis in R2 -Higgs inflation

IF 5 2区 物理与天体物理 Q1 Physics and Astronomy
Yann Cado, Christoph Englert, Tanmoy Modak, Mariano Quirós
{"title":"Implication of preheating on gravity assisted baryogenesis in R2 -Higgs inflation","authors":"Yann Cado, Christoph Englert, Tanmoy Modak, Mariano Quirós","doi":"10.1103/physrevd.111.023042","DOIUrl":null,"url":null,"abstract":"We investigate the impact of preheating on baryogenesis in R</a:mi>2</a:mn></a:msup></a:math>-Higgs inflation. In this scenario, the inclusion of a dimension-six operator <c:math xmlns:c=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"><c:mrow><c:mo stretchy=\"false\">(</c:mo><c:mi>R</c:mi><c:mo>/</c:mo><c:msup><c:mi mathvariant=\"normal\">Λ</c:mi><c:mn>2</c:mn></c:msup><c:mo stretchy=\"false\">)</c:mo></c:mrow><c:msub><c:mi>B</c:mi><c:mrow><c:mi>μ</c:mi><c:mi>ν</c:mi></c:mrow></c:msub><c:msup><c:mover accent=\"true\"><c:mi>B</c:mi><c:mo stretchy=\"false\">˜</c:mo></c:mover><c:mrow><c:mi>μ</c:mi><c:mi>ν</c:mi></c:mrow></c:msup></c:math> abundantly generates helical hypermagnetic fields during inflation, leading to a baryon asymmetric Universe at the electroweak crossover. Focusing on the <j:math xmlns:j=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"><j:msup><j:mi>R</j:mi><j:mn>2</j:mn></j:msup></j:math>-like regime, we first derive the relevant dynamics of preheating using a doubly covariant formalism. We find that preheating can happen for the Higgs, transverse gauge, and Goldstone bosons, however, it is dependent on the value of the nonminimal coupling <l:math xmlns:l=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"><l:msub><l:mi>ξ</l:mi><l:mi>H</l:mi></l:msub></l:math> between the Standard Model Higgs field and the Ricci scalar. We identify the preheating temperature to determine the appropriate scale <n:math xmlns:n=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"><n:mi mathvariant=\"normal\">Λ</n:mi></n:math> for driving baryogenesis, which is around <q:math xmlns:q=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"><q:mrow><q:mi mathvariant=\"normal\">Λ</q:mi><q:mo>∼</q:mo><q:mn>2.2</q:mn><q:mo stretchy=\"false\">(</q:mo><q:mn>2.6</q:mn><q:mo stretchy=\"false\">)</q:mo><q:mo>×</q:mo><q:msup><q:mrow><q:mn>10</q:mn></q:mrow><q:mrow><q:mo>−</q:mo><q:mn>5</q:mn></q:mrow></q:msup><q:msub><q:mrow><q:mi>M</q:mi></q:mrow><q:mrow><q:mi mathvariant=\"normal\">P</q:mi></q:mrow></q:msub></q:mrow></q:math> for <w:math xmlns:w=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"><w:msub><w:mi>ξ</w:mi><w:mi>H</w:mi></w:msub><w:mo>∼</w:mo><w:mn>1</w:mn><w:mo stretchy=\"false\">(</w:mo><w:mn>10</w:mn><w:mo stretchy=\"false\">)</w:mo></w:math>. Our results represent the most accurate estimation of the scale of gravity induced baryogenesis in R</ab:mi>2</ab:mn></ab:msup></ab:math>-Higgs inflation to date. Areas for further improvement are identified. <jats:supplementary-material> <jats:copyright-statement>Published by the American Physical Society</jats:copyright-statement> <jats:copyright-year>2025</jats:copyright-year> </jats:permissions> </jats:supplementary-material>","PeriodicalId":20167,"journal":{"name":"Physical Review D","volume":"52 1","pages":""},"PeriodicalIF":5.0000,"publicationDate":"2025-01-24","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"Physical Review D","FirstCategoryId":"101","ListUrlMain":"https://doi.org/10.1103/physrevd.111.023042","RegionNum":2,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q1","JCRName":"Physics and Astronomy","Score":null,"Total":0}
引用次数: 0

Abstract

We investigate the impact of preheating on baryogenesis in R2-Higgs inflation. In this scenario, the inclusion of a dimension-six operator (R/Λ2)BμνB˜μν abundantly generates helical hypermagnetic fields during inflation, leading to a baryon asymmetric Universe at the electroweak crossover. Focusing on the R2-like regime, we first derive the relevant dynamics of preheating using a doubly covariant formalism. We find that preheating can happen for the Higgs, transverse gauge, and Goldstone bosons, however, it is dependent on the value of the nonminimal coupling ξH between the Standard Model Higgs field and the Ricci scalar. We identify the preheating temperature to determine the appropriate scale Λ for driving baryogenesis, which is around Λ2.2(2.6)×105MP for ξH1(10). Our results represent the most accurate estimation of the scale of gravity induced baryogenesis in R2-Higgs inflation to date. Areas for further improvement are identified. Published by the American Physical Society 2025
求助全文
约1分钟内获得全文 求助全文
来源期刊
Physical Review D
Physical Review D 物理-天文与天体物理
CiteScore
9.20
自引率
36.00%
发文量
0
审稿时长
2 months
期刊介绍: Physical Review D (PRD) is a leading journal in elementary particle physics, field theory, gravitation, and cosmology and is one of the top-cited journals in high-energy physics. PRD covers experimental and theoretical results in all aspects of particle physics, field theory, gravitation and cosmology, including: Particle physics experiments, Electroweak interactions, Strong interactions, Lattice field theories, lattice QCD, Beyond the standard model physics, Phenomenological aspects of field theory, general methods, Gravity, cosmology, cosmic rays, Astrophysics and astroparticle physics, General relativity, Formal aspects of field theory, field theory in curved space, String theory, quantum gravity, gauge/gravity duality.
×
引用
GB/T 7714-2015
复制
MLA
复制
APA
复制
导出至
BibTeX EndNote RefMan NoteFirst NoteExpress
×
提示
您的信息不完整,为了账户安全,请先补充。
现在去补充
×
提示
您因"违规操作"
具体请查看互助需知
我知道了
×
提示
确定
请完成安全验证×
copy
已复制链接
快去分享给好友吧!
我知道了
右上角分享
点击右上角分享
0
联系我们:info@booksci.cn Book学术提供免费学术资源搜索服务,方便国内外学者检索中英文文献。致力于提供最便捷和优质的服务体验。 Copyright © 2023 布克学术 All rights reserved.
京ICP备2023020795号-1
ghs 京公网安备 11010802042870号
Book学术文献互助
Book学术文献互助群
群 号:481959085
Book学术官方微信