Supernova inelastic neutrino-nucleus cross sections from high-resolution electron scattering experiments and shell-model calculations
- Autor
- LANGANKE, K1 ; MARTINEZ-PINEDO, G2 ; VON NEUMANN-COSEL, P3 ; RICHTER, A3
[1] Institute for Physics and Astronomy, University of Århus, 8000 Århus, Denmark
[2] ICREA and Institut d'Estudis Espacials de Catalunya, Edifici Nexus, Gran Capità 2, 08034 Barcelona, Spain
[3] Institut für Kernphysik, Technische Universität Darmstadt, 64289 Darmstadt, Germany - Fuente
Physical review letters. 2004, Vol 93, Num 20, pp 202501.1-202501.4 ; ref : 33 ref
- CODEN
- PRLTAO
- ISSN
- 0031-9007
- Campo Científico
- Optics; Atomic molecular physics; Condensed state physics; Physics; Plasma physics
- Editor
- American Physical Society, Ridge, NY
- País de la publicación
- United States
- Tipo de documento
- Article
- Idioma
- English
- Palabra clave (fr)
- Chrome 52 Diffusion inélastique Diffusion neutrino noyau Diffusion électron Explosion supernova Fer 54 Modèle couche électronique Section efficace Titane 50
- Palabra clave (in)
- Chromium 52 Inelastic scattering Neutrino-nucleus scattering Electron scattering Supernovae explosion Iron 54 Shell models Cross sections Titanium 50
- Palabra clave (es)
- Difusión electrón Explosión supernova
- Clasificación
- Pascal
- 001 Exact sciences and technology / 001B Physics / 001B20 Nuclear physics / 001B20A Nuclear structure / 001B20A60 Nuclear-structure models and methods / 001B20A60C Shell model
- Pascal
- 001 Exact sciences and technology / 001B Physics / 001B20 Nuclear physics / 001B20E Nuclear reactions: specific reactions / 001B20E30 Lepton-induced reactions / 001B20E30D Inelastic electron scattering to specific states
- Disciplina
- Nuclear physics
- Procedencia
- Inist-CNRS
- Base de datos
- PASCAL
- Identificador INIST
- 16309199
Sauf mention contraire ci-dessus, le contenu de cette notice bibliographique peut être utilisé dans le cadre d’une licence CC BY 4.0 Inist-CNRS / Unless otherwise stated above, the content of this bibliographic record may be used under a CC BY 4.0 licence by Inist-CNRS / A menos que se haya señalado antes, el contenido de este registro bibliográfico puede ser utilizado al amparo de una licencia CC BY 4.0 Inist-CNRS
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DOI
10.1103/PhysRevLett.93.202501 
https://dx.doi.org/10.1103/PhysRevLett.93.202501
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