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Related papers: Constraints on Dirac Neutrinos from SN 1987A

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A search has been made for neutrinos from the hep reaction in the Sun and from the diffuse supernova neutrino background (DSNB) using data collected during the first operational phase of the Sudbury Neutrino Observatory, with an exposure of…

High Energy Physics - Experiment · Physics 2012-08-27 The SNO Collaboration

The observation of the $\bar{\nu}_e$ energy spectrum from a supernova burst can provide constraints on neutrino oscillations. We derive formulas for adiabatic oscillations of supernova antineutrinos for a variety of 3- and 4-neutrino mixing…

High Energy Physics - Phenomenology · Physics 2009-11-07 Michel Sorel , Janet Conrad

Neutrino masses arising from the spontaneous violation of ungauged lepton-number are accompanied by a physical Goldstone boson, generically called Majoron. In the high-density supernova medium the effects of Majoron-emitting neutrino decays…

High Energy Physics - Phenomenology · Physics 2009-09-17 M. Kachelriess , R. Tomas , J. W. F. Valle

The splitting of neutrinos, a viable reaction for superluminal neutrinos, is shown to have phenomenologically relevant consequences if one accepts the recent OPERA results for the velocity of neutrinos. Neutrino splitting can be used to put…

High Energy Physics - Phenomenology · Physics 2011-10-04 J. M. Carmona , J. L. Cortes

We study production of sterile neutrinos in the atmosphere and their detection at Super-Kamiokande. A sterile neutrino in the mass range $1\,{\rm MeV} \lesssim M_N \lesssim 105\,{\rm MeV}$ is produced by muon or pion decay, and decays to an…

High Energy Physics - Phenomenology · Physics 2015-06-04 Takehiko Asaka , Atsushi Watanabe

The puzzling phenomenon of pulsar kicks, i.e. the observed large escape velocities of pulsars out of supernova remnants, is examined for compact stars with a strange quark matter core. The direct Urca process in quark matter is studied in…

Astrophysics · Physics 2007-05-23 I. Sagert , J. Schaffner-Bielich

The superluminal neutrinos detected by OPERA indicates Lorentz invariance violation (LIV) of the neutrino sector at the order of $10^{-5}$. We study the implications of the result in this work. We find that such a large LIV implied by OPERA…

High Energy Physics - Phenomenology · Physics 2015-03-19 Xiao-Jun Bi , Peng-Fei Yin , Zhao-Huan Yu , Qiang Yuan

It is shown that Dirac-type neutrinos display BCS superfluidity for any nonzero mass. The Cooper pairs are formed by attractive scalar Higgs boson exchange between left- and right-handed neutrinos; in the standard SU(2)xU(1) theory,…

High Energy Physics - Theory · Physics 2009-11-10 J. I. Kapusta

We report spectroscopic and imaging observations of rotational transitions of cold CO and SiO in the ejecta of SN1987A, the first such emission detected in a supernova remnant. In addition to line luminosities for the CO J=1-0, 2-1, 6-5,…

We summarize the impact of sterile neutrino dark matter on core-collapse supernova explosions. We explore various oscillations between electron neutrinos or mixed $\mu-\tau$ neutrinos and right-handed sterile neutrinos that may occur within…

High Energy Astrophysical Phenomena · Physics 2016-09-21 MacKenzie L. Warren , Grant J. Mathews , Matthew Meixner , Jun Hidaka , Toshitaka Kajino

The kink observed in the nuclear charge radius of Sn isotopes around neutron number $N = 82$ is investigated within the relativistic mean-field (RMF) framework using the NL3$^*$ parameter set. It is shown that the small components of the…

Nuclear Theory · Physics 2026-04-20 S. Marcos , N. Sandulescu , R. Niembro

If large extra dimensions exist in nature, supernova (SN) cores will emit large fluxes of Kaluza-Klein gravitons, producing a cosmic background of these particles with energies and masses up to about 100 MeV. Radiative decays then give rise…

High Energy Physics - Phenomenology · Physics 2011-05-05 Steen Hannestad , Georg Raffelt

We consider lepton-quark contact interactions in models with right-handed neutrinos, and find that observational data from SN1987A restricts the scale of such interactions to be at least $\Lambda>90$ TeV.

High Energy Physics - Phenomenology · Physics 2009-10-30 J. A. Grifols , E. Masso , R. Toldra

We describe a model for pion production off nucleons and coherent pions from nuclei induced by neutrinos in the 1 GeV energy regime. Besides the dominant Delta pole contribution, it takes into account the effect of background terms required…

Nuclear Theory · Physics 2017-08-23 M. Valverde , J. E. Amaro , E. Hernandez , J. Nieves , M. J. Vicente Vacas

We study the spin-down of a neutron star during its early stages due to the neutrino emission. The mechanism we consider is the subsequent collisions of the produced neutrinos with the outer shells of the star. We find that this mechanism…

High Energy Astrophysical Phenomena · Physics 2014-11-20 Maxim Dvornikov , Claudio O. Dib

Charged particles can be accelerated to higher than PeV energies in the electro-magnetic wind of a fast-spinning newborn pulsar to produce high-energy neutrinos, through hadronuclear interactions in the supernova remnant. Here we explore…

High Energy Astrophysical Phenomena · Physics 2015-06-05 Ke Fang

The process of Radiative Emission of Neutrino Pair (RENP) in atoms is sensitive to the absolute neutrino mass scale, the type of spectrum neutrino masses obey and the nature - Dirac or Majorana - of massive neutrinos. We analyse the…

High Energy Physics - Phenomenology · Physics 2015-06-23 D. N. Dinh , S. T. Petcov

The Zee model for Dirac neutrinos is one of the simplest models featuring one-loop Dirac neutrino masses. The interactions between the new scalars (two singly-charged fields) and neutrinos induce general neutrino interactions (GNI) which,…

High Energy Physics - Phenomenology · Physics 2021-08-04 Julián Calle , Diego Restrepo , Óscar Zapata

In this talk I review the main features of the coherent/diffractive pion production by neutrinos on nuclei. The method is based on PCAC and relates the reaction $\textbf{boson} + \textbf{nucleus} \to \textbf{pion} + \textbf{nucleus}$ to…

High Energy Physics - Phenomenology · Physics 2015-05-14 E. A. Paschos , Dario Schalla

The mass of the stellar precursor of supernova (SN) 1987A and the burst of neutrinos observed at the moment of the explosion are consistent with the core-collapse formation of a neutron star. However, no compelling evidence for the presence…

High Energy Astrophysical Phenomena · Physics 2018-04-18 P. Esposito , N. Rea , D. Lazzati , M. Matsuura , R. Perna , J. A. Pons
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