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Constraints on the intergalactic magnetic field using Fermi-LAT and H.E.S.S. blazar observations

Constraints on the intergalactic magnetic field using Fermi-LAT and H.E.S.S. blazar observations

https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_journals_2824147253

Constraints on the intergalactic magnetic field using Fermi-LAT and H.E.S.S. blazar observations

About this item

Full title

Constraints on the intergalactic magnetic field using Fermi-LAT and H.E.S.S. blazar observations

Publisher

Ithaca: Cornell University Library, arXiv.org

Journal title

arXiv.org, 2023-06

Language

English

Formats

Publication information

Publisher

Ithaca: Cornell University Library, arXiv.org

More information

Scope and Contents

Contents

Magnetic fields in galaxies and galaxy clusters are believed to be the result of the amplification of intergalactic seed fields during the formation of large-scale structures in the universe. However, the origin, strength, and morphology of this intergalactic magnetic field (IGMF) remain unknown. Lower limits on (or indirect detection of) the IGMF...

Alternative Titles

Full title

Constraints on the intergalactic magnetic field using Fermi-LAT and H.E.S.S. blazar observations

Identifiers

Primary Identifiers

Record Identifier

TN_cdi_proquest_journals_2824147253

Permalink

https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_journals_2824147253

Other Identifiers

E-ISSN

2331-8422

DOI

10.48550/arxiv.2306.05132

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