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IceCube Search for High-energy Neutrino Emission from TeV Pulsar Wind Nebulae

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dc.contributor.authorAartsen, M. G.
dc.contributor.authorAckermann, M.
dc.contributor.authorAdams, J.
dc.contributor.authorAguilar, J. A.
dc.contributor.authorBesson, D. Z.
dc.date.accessioned2024-11-27T08:14:01Z
dc.date.available2024-11-27T08:14:01Z
dc.date.issued2020
dc.description.abstractPulsar wind nebulae (PWNe) are the main gamma-ray emitters in the Galactic plane. They are diffuse nebulae that emit nonthermal radiation. Pulsar winds, relativistic magnetized outflows from the central star, shocked in the ambient medium produce a multiwavelength emission from the radio through gamma-rays. Although the leptonic scenario is able to explain most PWNe emission, a hadronic contribution cannot be excluded. A possible hadronic contribution to the high-energy gamma-ray emission inevitably leads to the production of neutrinos. Using 9.5 yr of all-sky IceCube data, we report results from a stacking analysis to search for neutrino emission from 35 PWNe that are high-energy gamma-ray emitters. In the absence of any significant correlation, we set upper limits on the total neutrino emission from those PWNe and constraints on hadronic spectral components.
dc.identifier.citationIceCube Search for High-energy Neutrino Emission from TeV Pulsar Wind Nebulae / Aartsen, MG [et al.] // ASTROPHYSICAL JOURNAL. - 2020. - 898. - № 2. - 10.3847/1538-4357/ab9fa0
dc.identifier.doi10.3847/1538-4357/ab9fa0
dc.identifier.urihttps://www.doi.org/10.3847/1538-4357/ab9fa0
dc.identifier.urihttp://gateway.webofknowledge.com/gateway/Gateway.cgi?GWVersion=2&SrcAuth=Alerting&SrcApp=Alerting&DestApp=WOS_CPL&DestLinkType=FullRecord&UT=WOS:000570311400001
dc.identifier.urihttps://openrepository.mephi.ru/handle/123456789/22399
dc.relation.ispartofASTROPHYSICAL JOURNAL
dc.titleIceCube Search for High-energy Neutrino Emission from TeV Pulsar Wind Nebulae
dc.typeArticle
dspace.entity.typePublication
oaire.citation.issue2
oaire.citation.volume898
relation.isOrgUnitOfPublicationba0b4738-e6bd-4285-bda5-16ab2240dbd1
relation.isOrgUnitOfPublication.latestForDiscoveryba0b4738-e6bd-4285-bda5-16ab2240dbd1
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