{"title":"CR电子:走向更完整的空气-切伦科夫视图","authors":"Michele Palatiello","doi":"10.1016/j.nuclphysbps.2014.10.032","DOIUrl":null,"url":null,"abstract":"<div><p>Very high energy (VHE; <em>E</em> > 30 GeV) cosmic-ray electrons and positrons (CR<span><math><msup><mrow><mi>e</mi></mrow><mrow><mo>−</mo></mrow></msup></math></span>, <span><math><msup><mrow><mi>e</mi></mrow><mrow><mo>+</mo></mrow></msup></math></span>) reaching the Earth from beyond the solar system are important tracers of recent energetic events in our Galactic neighbourhood (1–2 kpc). Spectral measurements of this radiation may help checking standard astrophysical scenarios of CR<span><math><msup><mrow><mi>e</mi></mrow><mrow><mo>−</mo></mrow></msup></math></span>, <span><math><msup><mrow><mi>e</mi></mrow><mrow><mo>+</mo></mrow></msup></math></span> origin (e.g., pulsars, SNRs) versus exotic scenarios (e.g., DM particle annihilation). Air-Cherenkov telescopes can contribute to the measurement of the total VHE flux of CR<span><math><msup><mrow><mi>e</mi></mrow><mrow><mo>−</mo></mrow></msup></math></span>, <span><math><msup><mrow><mi>e</mi></mrow><mrow><mo>+</mo></mrow></msup></math></span>. This will allow us to consolidate relevant results by, e.g., ATIC, HESS, AMS-02, and <em>Fermi</em>-LAT.</p></div>","PeriodicalId":93343,"journal":{"name":"Nuclear physics. B, Proceedings, supplements","volume":"256 ","pages":"Pages 267-274"},"PeriodicalIF":0.0000,"publicationDate":"2014-11-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://sci-hub-pdf.com/10.1016/j.nuclphysbps.2014.10.032","citationCount":"0","resultStr":"{\"title\":\"CR electrons: towards a more complete air-Cherenkov view\",\"authors\":\"Michele Palatiello\",\"doi\":\"10.1016/j.nuclphysbps.2014.10.032\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"<div><p>Very high energy (VHE; <em>E</em> > 30 GeV) cosmic-ray electrons and positrons (CR<span><math><msup><mrow><mi>e</mi></mrow><mrow><mo>−</mo></mrow></msup></math></span>, <span><math><msup><mrow><mi>e</mi></mrow><mrow><mo>+</mo></mrow></msup></math></span>) reaching the Earth from beyond the solar system are important tracers of recent energetic events in our Galactic neighbourhood (1–2 kpc). Spectral measurements of this radiation may help checking standard astrophysical scenarios of CR<span><math><msup><mrow><mi>e</mi></mrow><mrow><mo>−</mo></mrow></msup></math></span>, <span><math><msup><mrow><mi>e</mi></mrow><mrow><mo>+</mo></mrow></msup></math></span> origin (e.g., pulsars, SNRs) versus exotic scenarios (e.g., DM particle annihilation). Air-Cherenkov telescopes can contribute to the measurement of the total VHE flux of CR<span><math><msup><mrow><mi>e</mi></mrow><mrow><mo>−</mo></mrow></msup></math></span>, <span><math><msup><mrow><mi>e</mi></mrow><mrow><mo>+</mo></mrow></msup></math></span>. This will allow us to consolidate relevant results by, e.g., ATIC, HESS, AMS-02, and <em>Fermi</em>-LAT.</p></div>\",\"PeriodicalId\":93343,\"journal\":{\"name\":\"Nuclear physics. B, Proceedings, supplements\",\"volume\":\"256 \",\"pages\":\"Pages 267-274\"},\"PeriodicalIF\":0.0000,\"publicationDate\":\"2014-11-01\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"https://sci-hub-pdf.com/10.1016/j.nuclphysbps.2014.10.032\",\"citationCount\":\"0\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"Nuclear physics. B, Proceedings, supplements\",\"FirstCategoryId\":\"1085\",\"ListUrlMain\":\"https://www.sciencedirect.com/science/article/pii/S0920563214002266\",\"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/S0920563214002266","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
CR electrons: towards a more complete air-Cherenkov view
Very high energy (VHE; E > 30 GeV) cosmic-ray electrons and positrons (CR, ) reaching the Earth from beyond the solar system are important tracers of recent energetic events in our Galactic neighbourhood (1–2 kpc). Spectral measurements of this radiation may help checking standard astrophysical scenarios of CR, origin (e.g., pulsars, SNRs) versus exotic scenarios (e.g., DM particle annihilation). Air-Cherenkov telescopes can contribute to the measurement of the total VHE flux of CR, . This will allow us to consolidate relevant results by, e.g., ATIC, HESS, AMS-02, and Fermi-LAT.