{"title":"Limits to gauge coupling in the dark sector of super-heavy dark matter particles from the Pierre Auger Observatory data","authors":"Olivier Deligny","doi":"10.21468/scipostphysproc.13.013","DOIUrl":null,"url":null,"abstract":"Assuming that the energy density of super-heavy particles matches that of dark matter observed today, tight constraints on the couplings governing the decay process are presented as a function of the particle mass. These constraints are obtained from the lack of signatures that would be suggestive of decaying super-heavy X <mml:math xmlns:mml=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"><mml:mi>X</mml:mi></mml:math> particles in the data of the Pierre Auger Observatory. In particular, instanton-induced decay processes allow us to derive a bound on the reduced coupling constant of gauge interactions in the dark sector: \\alpha_X \\lesssim 0.09 <mml:math xmlns:mml=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"><mml:mrow><mml:msub><mml:mi>α</mml:mi><mml:mi>X</mml:mi></mml:msub><mml:mo>≲</mml:mo><mml:mn>0.09</mml:mn></mml:mrow></mml:math> , for 10^{9} \\lesssim M_X/\\mathrm{GeV} &lt; 10^{19} <mml:math xmlns:mml=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"><mml:mrow><mml:msup><mml:mn>10</mml:mn><mml:mn>9</mml:mn></mml:msup><mml:mo>≲</mml:mo><mml:msub><mml:mi>M</mml:mi><mml:mi>X</mml:mi></mml:msub><mml:mi>/</mml:mi><mml:mstyle mathvariant=\"normal\"><mml:mi>G</mml:mi><mml:mi>e</mml:mi><mml:mi>V</mml:mi></mml:mstyle><mml:mo><</mml:mo><mml:msup><mml:mn>10</mml:mn><mml:mn>19</mml:mn></mml:msup></mml:mrow></mml:math> . Cosmological aspects for super-heavy dark matter production during the reheating epoch are discussed.","PeriodicalId":355998,"journal":{"name":"SciPost Physics Proceedings","volume":"64 1","pages":"0"},"PeriodicalIF":0.0000,"publicationDate":"2023-09-28","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"1","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"SciPost Physics Proceedings","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/10.21468/scipostphysproc.13.013","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
引用次数: 1
Abstract
Assuming that the energy density of super-heavy particles matches that of dark matter observed today, tight constraints on the couplings governing the decay process are presented as a function of the particle mass. These constraints are obtained from the lack of signatures that would be suggestive of decaying super-heavy X X particles in the data of the Pierre Auger Observatory. In particular, instanton-induced decay processes allow us to derive a bound on the reduced coupling constant of gauge interactions in the dark sector: \alpha_X \lesssim 0.09 αX≲0.09 , for 10^{9} \lesssim M_X/\mathrm{GeV} < 10^{19} 109≲MX/GeV<1019 . Cosmological aspects for super-heavy dark matter production during the reheating epoch are discussed.