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001     580606
005     20230618013403.0
024 7 _ |a IceCube:2023esf
|2 INSPIRETeX
024 7 _ |a inspire:2638862
|2 inspire
024 7 _ |a arXiv:2303.03316
|2 arXiv
024 7 _ |a 10.3204/PUBDB-2023-01341
|2 datacite_doi
037 _ _ |a PUBDB-2023-01341
041 _ _ |a English
088 _ _ |a arXiv:2303.03316
|2 arXiv
100 1 _ |a Abbasi, R.
|b 0
245 _ _ |a Constraining High-Energy Neutrino Emission from Supernovae with IceCube
260 _ _ |c 2023
336 7 _ |a Preprint
|b preprint
|m preprint
|0 PUB:(DE-HGF)25
|s 1679903137_17171
|2 PUB:(DE-HGF)
336 7 _ |a WORKING_PAPER
|2 ORCID
336 7 _ |a Electronic Article
|0 28
|2 EndNote
336 7 _ |a preprint
|2 DRIVER
336 7 _ |a ARTICLE
|2 BibTeX
336 7 _ |a Output Types/Working Paper
|2 DataCite
500 _ _ |a Submitted to ApJ Letters
520 _ _ |a Core-collapse supernovae are a promising potential high-energy neutrino source class. We test for correlation between seven years of IceCube neutrino data and a catalog containing more than 1000 core-collapse supernovae of types IIn and IIP and a sample of stripped-envelope supernovae. We search both for neutrino emission from individual supernovae, and for combined emission from the whole supernova sample through a stacking analysis. No significant spatial or temporal correlation of neutrinos with the cataloged supernovae was found. The overall deviation of all tested scenarios from the background expectation yields a p-value of 93% which is fully compatible with background. The derived upper limits on the total energy emitted in neutrinos are $1.7\times 10^{48}$ erg for stripped-envelope supernovae, $2.8\times 10^{48}$ erg for type IIP, and $1.3\times 10^{49}$ erg for type IIn SNe, the latter disfavouring models with optimistic assumptions for neutrino production in interacting supernovae. We conclude that strippe-envelope supernovae and supernovae of type IIn do not contribute more than $14.6\%$ and $33.9\%$ respectively to the diffuse neutrino flux in the energy range of about $10^3-10^5$ GeV, assuming that the neutrino energy spectrum follows a power-law with an index of $-2.5$. Under the same assumption, we can only constrain the contribution of type IIP SNe to no more than $59.9\%$. Thus core-collapse supernovae of types IIn and stripped-envelope supernovae can both be ruled out as the dominant source of the diffuse neutrino flux under the given assumptions.
536 _ _ |a 613 - Matter and Radiation from the Universe (POF4-613)
|0 G:(DE-HGF)POF4-613
|c POF4-613
|f POF IV
|x 0
588 _ _ |a Dataset connected to INSPIRE
650 _ 7 |a neutrino: flux
|2 INSPIRE
650 _ 7 |a neutrino: particle source
|2 INSPIRE
650 _ 7 |a neutrino: energy spectrum
|2 INSPIRE
650 _ 7 |a energy: emission
|2 INSPIRE
650 _ 7 |a neutrino: production
|2 INSPIRE
650 _ 7 |a supernova
|2 INSPIRE
650 _ 7 |a background
|2 INSPIRE
650 _ 7 |a correlation
|2 INSPIRE
650 _ 7 |a collapse
|2 INSPIRE
650 _ 7 |a IceCube
|2 INSPIRE
650 _ 7 |a GeV
|2 INSPIRE
650 _ 7 |a stacking
|2 INSPIRE
650 _ 7 |a neutrino: VHE
|2 INSPIRE
650 _ 7 |a neutrino: UHE
|2 INSPIRE
650 _ 7 |a neutrino: luminosity
|2 INSPIRE
650 _ 7 |a neutrino: energy
|2 INSPIRE
693 _ _ |0 EXP:(DE-H253)IceCube-20150101
|5 EXP:(DE-H253)IceCube-20150101
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