Massive Dark Photons as Hot Dark Matter

IF 0.9 4区 物理与天体物理 Q3 PHYSICS, MULTIDISCIPLINARY Acta Physica Polonica B Pub Date : 2022-11-21 DOI:10.5506/aphyspolb.53.11-a2
S. Ennadifi
{"title":"Massive Dark Photons as Hot Dark Matter","authors":"S. Ennadifi","doi":"10.5506/aphyspolb.53.11-a2","DOIUrl":null,"url":null,"abstract":"Motivated by the growing interest in the existence of new massive gauge bosons, we suggest that massive dark photons A ′ can be a consequence of a broken new abelian symmetry U ( 1 ) ′ X . Such a dark symmetry U ( 1 ) ′ D is afterwards supposed to be associated with the conservation of the weak number W belonging to the Weakling Interacting Slim Particles U ( 1 ) W , being a strong candidate for Hot Dark Matter. The latters correspond then to light dark photons m ′ A . keV from a weak symmetry breaking scale & 10 keV .","PeriodicalId":7060,"journal":{"name":"Acta Physica Polonica B","volume":null,"pages":null},"PeriodicalIF":0.9000,"publicationDate":"2022-11-21","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"Acta Physica Polonica B","FirstCategoryId":"101","ListUrlMain":"https://doi.org/10.5506/aphyspolb.53.11-a2","RegionNum":4,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q3","JCRName":"PHYSICS, MULTIDISCIPLINARY","Score":null,"Total":0}
引用次数: 0

Abstract

Motivated by the growing interest in the existence of new massive gauge bosons, we suggest that massive dark photons A ′ can be a consequence of a broken new abelian symmetry U ( 1 ) ′ X . Such a dark symmetry U ( 1 ) ′ D is afterwards supposed to be associated with the conservation of the weak number W belonging to the Weakling Interacting Slim Particles U ( 1 ) W , being a strong candidate for Hot Dark Matter. The latters correspond then to light dark photons m ′ A . keV from a weak symmetry breaking scale & 10 keV .
查看原文
分享 分享
微信好友 朋友圈 QQ好友 复制链接
本刊更多论文
大质量暗光子是热暗物质
由于人们对存在新的大质量规范玻色子越来越感兴趣,我们提出大质量暗光子A '可能是新阿贝尔对称U (1) ' X被打破的结果。这样的暗对称U (1) ' D随后被认为与弱相互作用细粒子U (1) W的弱数W守恒有关,弱数W是热暗物质的有力候选者。后者对应于光暗光子m ' A。弱对称破缺尺度& 10 keV。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
求助全文
约1分钟内获得全文 去求助
来源期刊
Acta Physica Polonica B
Acta Physica Polonica B 物理-物理:综合
CiteScore
1.70
自引率
20.00%
发文量
30
审稿时长
3-8 weeks
期刊介绍: Acta Physica Polonica B covers the following areas of physics: -General and Mathematical Physics- Particle Physics and Field Theory- Nuclear Physics- Theory of Relativity and Astrophysics- Statistical Physics
期刊最新文献
Particle-theory Input for Neutron-star Physics Perturbative Computation of Thermal Characteristics of the Stoner Phase Transition Topologically Charged Rotating Wormhole The Mass Density Contrast in Perturbed Friedman–Lemaître–Robertson–Walker Cosmologies Wigner and Husimi Partonic Distributions of the Pion in a Chiral Quark Model
×
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
现在去查看 取消
×
提示
确定
0
微信
客服QQ
Book学术公众号 扫码关注我们
反馈
×
意见反馈
请填写您的意见或建议
请填写您的手机或邮箱
已复制链接
已复制链接
快去分享给好友吧!
我知道了
×
扫码分享
扫码分享
Book学术官方微信
Book学术文献互助
Book学术文献互助群
群 号:481959085
Book学术
文献互助 智能选刊 最新文献 互助须知 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 Book学术 All rights reserved.
ghs 京公网安备 11010802042870号 京ICP备2023020795号-1