Cosmic-ray antiprotons in the AMS-02 era: A sensitive probe of dark matter.
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| Title: | Cosmic-ray antiprotons in the AMS-02 era: A sensitive probe of dark matter. |
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| Authors: | Heisig, Jan1 (AUTHOR) jan.heisig@uclouvain.be |
| Source: | Modern Physics Letters A. 2/20/2021, Vol. 36 Issue 5, pN.PAG-N.PAG. 22p. |
| Subjects: | Dark matter, Antiprotons, Annihilation reactions, Cosmic rays, Particle interactions |
| Abstract: | Cosmic-ray antiprotons are a powerful tool for astroparticle physics. While the bulk of measured antiprotons is consistent with a secondary origin, the precise data of the AMS-02 experiment provides us with encouraging prospects to search for a subdominant primary component, e.g. from dark matter. In this brief review, we discuss recent limits on heavy dark matter as well as a tentative signal from annihilation of dark matter with a mass ≲ 100 GeV. We emphasize the special role of systematic errors that can affect the signal. In particular, we discuss recent progress in the modeling of secondary production cross-sections and correlated errors in the AMS-02 data, the dominant ones originating from uncertainties in the cross-sections for cosmic-ray absorption in the detector. [ABSTRACT FROM AUTHOR] |
| Copyright of Modern Physics Letters A is the property of World Scientific Publishing Company and its content may not be copied or emailed to multiple sites without the copyright holder's express written permission. Additionally, content may not be used with any artificial intelligence tools or machine learning technologies. However, users may print, download, or email articles for individual use. This abstract may be abridged. No warranty is given about the accuracy of the copy. Users should refer to the original published version of the material for the full abstract. (Copyright applies to all Abstracts.) | |
| Database: | Engineering Source |
| FullText | Text: Availability: 0 |
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| Header | DbId: egs DbLabel: Engineering Source An: 148890645 AccessLevel: 6 PubType: Academic Journal PubTypeId: academicJournal PreciseRelevancyScore: 0 |
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| Items | – Name: Title Label: Title Group: Ti Data: Cosmic-ray antiprotons in the AMS-02 era: A sensitive probe of dark matter. – Name: Author Label: Authors Group: Au Data: <searchLink fieldCode="AR" term="%22Heisig%2C+Jan%22">Heisig, Jan</searchLink><relatesTo>1</relatesTo> (AUTHOR)<i> jan.heisig@uclouvain.be</i> – Name: TitleSource Label: Source Group: Src Data: <searchLink fieldCode="JN" term="%22Modern+Physics+Letters+A%22">Modern Physics Letters A</searchLink>. 2/20/2021, Vol. 36 Issue 5, pN.PAG-N.PAG. 22p. – Name: Subject Label: Subjects Group: Su Data: <searchLink fieldCode="DE" term="%22Dark+matter%22">Dark matter</searchLink><br /><searchLink fieldCode="DE" term="%22Antiprotons%22">Antiprotons</searchLink><br /><searchLink fieldCode="DE" term="%22Annihilation+reactions%22">Annihilation reactions</searchLink><br /><searchLink fieldCode="DE" term="%22Cosmic+rays%22">Cosmic rays</searchLink><br /><searchLink fieldCode="DE" term="%22Particle+interactions%22">Particle interactions</searchLink> – Name: Abstract Label: Abstract Group: Ab Data: Cosmic-ray antiprotons are a powerful tool for astroparticle physics. While the bulk of measured antiprotons is consistent with a secondary origin, the precise data of the AMS-02 experiment provides us with encouraging prospects to search for a subdominant primary component, e.g. from dark matter. In this brief review, we discuss recent limits on heavy dark matter as well as a tentative signal from annihilation of dark matter with a mass ≲ 100 GeV. We emphasize the special role of systematic errors that can affect the signal. In particular, we discuss recent progress in the modeling of secondary production cross-sections and correlated errors in the AMS-02 data, the dominant ones originating from uncertainties in the cross-sections for cosmic-ray absorption in the detector. [ABSTRACT FROM AUTHOR] – Name: AbstractSuppliedCopyright Label: Group: Ab Data: <i>Copyright of Modern Physics Letters A is the property of World Scientific Publishing Company and its content may not be copied or emailed to multiple sites without the copyright holder's express written permission. Additionally, content may not be used with any artificial intelligence tools or machine learning technologies. However, users may print, download, or email articles for individual use. This abstract may be abridged. No warranty is given about the accuracy of the copy. Users should refer to the original published version of the material for the full abstract.</i> (Copyright applies to all Abstracts.) |
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| RecordInfo | BibRecord: BibEntity: Identifiers: – Type: doi Value: 10.1142/S0217732321300032 Languages: – Code: eng Text: English PhysicalDescription: Pagination: PageCount: 22 StartPage: N.PAG Subjects: – SubjectFull: Dark matter Type: general – SubjectFull: Antiprotons Type: general – SubjectFull: Annihilation reactions Type: general – SubjectFull: Cosmic rays Type: general – SubjectFull: Particle interactions Type: general Titles: – TitleFull: Cosmic-ray antiprotons in the AMS-02 era: A sensitive probe of dark matter. Type: main BibRelationships: HasContributorRelationships: – PersonEntity: Name: NameFull: Heisig, Jan IsPartOfRelationships: – BibEntity: Dates: – D: 20 M: 02 Text: 2/20/2021 Type: published Y: 2021 Identifiers: – Type: issn-print Value: 02177323 Numbering: – Type: volume Value: 36 – Type: issue Value: 5 Titles: – TitleFull: Modern Physics Letters A Type: main |
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