B. Panico , O. Adriani , G.C. Barbarino , G.A. Bazilevskaya , R. Bellotti , M. Boezio , E.A. Bogomolov , M. Bongi , V. Bonvicini , S. Bottai , A. Bruno , F. Cafagna , D. Campana , R. Carbone , P. Carlson , M. Casolino , G. Castellini , C. De Donato , C. De Santis , N. De Simone , V.G. Zverev
{"title":"用Pamela数据检测正电子各向异性的方法","authors":"B. Panico , O. Adriani , G.C. Barbarino , G.A. Bazilevskaya , R. Bellotti , M. Boezio , E.A. Bogomolov , M. Bongi , V. Bonvicini , S. Bottai , A. Bruno , F. Cafagna , D. Campana , R. Carbone , P. Carlson , M. Casolino , G. Castellini , C. De Donato , C. De Santis , N. De Simone , V.G. Zverev","doi":"10.1016/j.nuclphysbps.2014.10.020","DOIUrl":null,"url":null,"abstract":"<div><p>The PAMELA experiment is collecting data since 2006; its results indicate the presence of a large flux of positron with respect to electrons in the CR spectrum above 10 GeV. This excess might also be originated in objects such as pulsars and microquasars or through dark matter annihilation. Here the electrons and positrons events collected by PAMELA have been analized searching for anisotropies. The analysis is performed at different angular scales and results will be presented at the conference.</p></div>","PeriodicalId":93343,"journal":{"name":"Nuclear physics. B, Proceedings, supplements","volume":"256 ","pages":"Pages 173-178"},"PeriodicalIF":0.0000,"publicationDate":"2014-11-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://sci-hub-pdf.com/10.1016/j.nuclphysbps.2014.10.020","citationCount":"2","resultStr":"{\"title\":\"A method to detect positron anisotropies with Pamela data\",\"authors\":\"B. Panico , O. Adriani , G.C. Barbarino , G.A. Bazilevskaya , R. Bellotti , M. Boezio , E.A. Bogomolov , M. Bongi , V. Bonvicini , S. Bottai , A. Bruno , F. Cafagna , D. Campana , R. Carbone , P. Carlson , M. Casolino , G. Castellini , C. De Donato , C. De Santis , N. De Simone , V.G. Zverev\",\"doi\":\"10.1016/j.nuclphysbps.2014.10.020\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"<div><p>The PAMELA experiment is collecting data since 2006; its results indicate the presence of a large flux of positron with respect to electrons in the CR spectrum above 10 GeV. This excess might also be originated in objects such as pulsars and microquasars or through dark matter annihilation. Here the electrons and positrons events collected by PAMELA have been analized searching for anisotropies. The analysis is performed at different angular scales and results will be presented at the conference.</p></div>\",\"PeriodicalId\":93343,\"journal\":{\"name\":\"Nuclear physics. B, Proceedings, supplements\",\"volume\":\"256 \",\"pages\":\"Pages 173-178\"},\"PeriodicalIF\":0.0000,\"publicationDate\":\"2014-11-01\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"https://sci-hub-pdf.com/10.1016/j.nuclphysbps.2014.10.020\",\"citationCount\":\"2\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"Nuclear physics. B, Proceedings, supplements\",\"FirstCategoryId\":\"1085\",\"ListUrlMain\":\"https://www.sciencedirect.com/science/article/pii/S092056321400214X\",\"RegionNum\":0,\"RegionCategory\":null,\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"\",\"JCRName\":\"\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"Nuclear physics. B, Proceedings, supplements","FirstCategoryId":"1085","ListUrlMain":"https://www.sciencedirect.com/science/article/pii/S092056321400214X","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
A method to detect positron anisotropies with Pamela data
The PAMELA experiment is collecting data since 2006; its results indicate the presence of a large flux of positron with respect to electrons in the CR spectrum above 10 GeV. This excess might also be originated in objects such as pulsars and microquasars or through dark matter annihilation. Here the electrons and positrons events collected by PAMELA have been analized searching for anisotropies. The analysis is performed at different angular scales and results will be presented at the conference.
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