Results 91 to 100 of about 74,471 (120)
A Core-collapse Supernova Neutrino Parameterization with Enhanced Physical Interpretability
The Astrophysical Journal Supplement SeriesWe introduce a novel parameterization of supernova neutrino energy spectra with a clear physical motivation. Its central parameter, τ ( t ), quantifies the characteristic thermal-diffusion area during the explosion.
Haihao Shi +4 more
doaj +1 more source
Neutrinos from a core collapse supernova
, 2008 The neutrino burst from a galactic supernova can help determine the neutrino mass hierarchy and θ13, and provide crucial information about supernova astrophysics.
Osamu Yasuda +4 more
core +1 more source
86th Annual Meeting of the Meteoritical Society (2024)
Meteoritics &Planetary Science, Volume 59, Issue S1, Page A1-A468, August 2024.
wiley +1 more source
Decay phenomenology of supernova neutrinos
, 2019 Orientador: Orlando Luis Goulart PeresDissertação (mestrado) - Universidade Estadual de Campinas, Instituto de Física Gleb WataghinResumo: Apresentamos neste trabalho um estudo da fenomenologias dos neutrinos, que inicia com um modelo além do Modelo ...
Tapia Herrera, Luis Carlos 1982-
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A Theory for Neutron Star and Black Hole Kicks and Induced Spins
The Astrophysical JournalUsing 20 long-term 3D core-collapse supernova simulations, we find that lower compactness progenitors that explode quasi-spherically due to the short delay to explosion experience smaller neutron star recoil kicks in the ∼100−200 km s ^−1 range, while ...
Adam Burrows +3 more
doaj +1 more source
Nachweis von Supernova-Neutrinos im Flüssigszintillator-Experiment LENA
, 2014 The next-generation liquid-scintillator detector LENA is able to observe neutrinos from a galactic core-collapse supernova with high statistics. In addition, neutrinos from the last fusion stages can be observed.
Winter, Jürgen Michael Albrecht
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Collective Flavor Transformation of Supernova Neutrinos
, 2009 Duan, Huaiyu. (2009). Collective Flavor Transformation of Supernova Neutrinos.
Duan, Huaiyu
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A search for supernova neutrinos with the Sudbury Neutrino Observatory
, 2002 The Sudbury Neutrino Observatory (SNO) is an underground Cerenkov detector designed to detect neutrinos from astrophysical sources. The fiducial mass of the detector consists of 1000 tonnes of D₂0 , which provides sensitivity to all neutrino flavours ...
Heise, Jaret
core +1 more source
Cosmological search for sterile neutrinos after DESI 2024
European Physical Journal C: Particles and FieldsThe question of whether massive sterile neutrinos exist remains a crucial unresolved issue in both particle physics and cosmology. We explore the cosmological constraints on massive sterile neutrinos using the latest observational data, including the ...
Guo-Hong Du +6 more
doaj +1 more source
Simulating supernova feedback in galaxy disks [PDF]
, 2012 In this thesis I examine supernova feedback in hydrodynamical simulations of galaxy disks. Understanding this process entails the numerical evaluation of cooling in radiative shocks, and we present a set of simulations using two widely used numerical ...
CREASEY, PETER,EDWARD +1 more
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