J
John F. Beacom
Researcher at Ohio State University
Publications - 359
Citations - 28360
John F. Beacom is an academic researcher from Ohio State University. The author has contributed to research in topics: Neutrino & Supernova. The author has an hindex of 80, co-authored 338 publications receiving 24601 citations. Previous affiliations of John F. Beacom include Fermilab & University of Wisconsin-Madison.
Papers
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Measuring flavor ratios of high-energy astrophysical neutrinos
TL;DR: In this article, the authors discuss the prospects for next generation neutrino telescopes, such as IceCube, to measure the flavor ratios of high-energy astrophysical neutrinos.
Journal ArticleDOI
ASASSN-15lh: A highly super-luminous supernova
Subo Dong,Benjamin J. Shappee,J. L. Prieto,J. L. Prieto,Saurabh Jha,Krzysztof Z. Stanek,Thomas W.-S. Holoien,Christopher S. Kochanek,Todd A. Thompson,Nidia Morrell,Ian B. Thompson,U. Basu,John F. Beacom,D. Bersier,J. Brimacombe,J. S. Brown,Filomena Bufano,Ping Chen,E. Conseil,A. B. Danilet,E. E. Falco,Dirk Grupe,S. Kiyota,G. Masi,B. Nicholls,G. Pignata,G. Pignata,G. Pojmanski,G. V. Simonian,D. M. Szczygiel,Przemysław Woźniak +30 more
TL;DR: ASASSN-15lh (SN 2015L) as mentioned in this paper is the most luminous supernova yet found, reaching an absolute magnitude of Mu, AB = −23.5 ± 0.1 and bolometric luminosity Lbol = (2.2 ± 0.2) × 1045 ergs s−1.
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Stringent constraints on cosmological neutrino-antineutrino asymmetries from synchronized flavor transformation
TL;DR: In this article, the authors assess a mechanism which can transform neutrino-antineutrino asymmetries between flavors in the early universe, and confirm that such transformation is unavoidable in the near bi-maximal framework emerging for the neutrinos mixing matrix.
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The Star Formation Rate in the Reionization Era as Indicated by Gamma-ray Bursts
TL;DR: In this paper, the authors show that the implied SFR to beyond z = 8 is consistent with LBG-based measurements after accounting for unseen galaxies at the faint end of the UV luminosity function.
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Diffuse supernova neutrino background is detectable in Super-Kamiokande
TL;DR: The diffuse supernova neutrino background (DSNB) provides an immediate opportunity to study the emission of MeV thermal neutrinos from core-collapse supernovae as mentioned in this paper.