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Detection of the 511 keV Galactic positron annihilation line with COSI

Detection of the 511 keV Galactic positron annihilation line with COSI

https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_journals_2321094768

Detection of the 511 keV Galactic positron annihilation line with COSI

About this item

Full title

Detection of the 511 keV Galactic positron annihilation line with COSI

Publisher

Ithaca: Cornell University Library, arXiv.org

Journal title

arXiv.org, 2020-04

Language

English

Formats

Publication information

Publisher

Ithaca: Cornell University Library, arXiv.org

More information

Scope and Contents

Contents

The signature of positron annihilation, namely the 511 keV \(\gamma\)-ray line, was first detected coming from the direction of the Galactic center in the 1970's, but the source of Galactic positrons still remains a puzzle. The measured flux of the annihilation corresponds to an intense steady source of positron production, with an annihilation rat...

Alternative Titles

Full title

Detection of the 511 keV Galactic positron annihilation line with COSI

Identifiers

Primary Identifiers

Record Identifier

TN_cdi_proquest_journals_2321094768

Permalink

https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_journals_2321094768

Other Identifiers

E-ISSN

2331-8422

DOI

10.48550/arxiv.1912.00110

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