{ "id": "1412.8361", "version": "v1", "published": "2014-12-29T15:02:20.000Z", "updated": "2014-12-29T15:02:20.000Z", "title": "Star-forming galaxies as the origin of the IceCube PeV neutrinos", "authors": [ "Xiao-Chuan Chang", "Ruo-Yu Liu", "Xiang-Yu Wang" ], "comment": "8 pages, 6 figures", "categories": [ "astro-ph.HE" ], "abstract": "Star-forming galaxies, due to their high star-formation rates and hence large number of supernova remnants therein, are huge reservoirs of cosmic rays (CRs). These CRs collide with the gas in the galaxy and produce high-energy neutrinos through $pp$ collisions. In this paper, we calculate the neutrino production efficiency in star-forming galaxies by considering realistic galaxy properties, such as the gas density and galactic wind properties in star-forming galaxies. To calculate the accumulated neutrino flux, we use the infrared luminosity functions of star-forming galaxies obtained by Herschel PEP/HerMES survey recently. The intensity of CRs producing PeV neutrinos in star-forming galaxies is normalized with the observed CR flux at EeV, assuming that supernovae remnants or hypernova remnants in star-forming galaxies can accelerate protons to EeV energies. Our calculations show that the accumulated neutrino emission produced by CRs in star-forming galaxies can account for the flux and spectrum of the sub-PeV/PeV neutrinos under reasonable assumption about the CR confinement time in these galaxies.", "revisions": [ { "version": "v1", "updated": "2014-12-29T15:02:20.000Z" } ], "analyses": { "keywords": [ "star-forming galaxies", "icecube pev neutrinos", "considering realistic galaxy properties", "cr confinement time", "produce high-energy neutrinos" ], "publication": { "doi": "10.1088/0004-637X/805/2/95", "journal": "The Astrophysical Journal", "year": 2015, "month": "Jun", "volume": 805, "number": 2, "pages": 95 }, "note": { "typesetting": "TeX", "pages": 8, "language": "en", "license": "arXiv", "status": "editable", "inspire": 1335638, "adsabs": "2015ApJ...805...95C" } } }