Supernova Inelastic Neutrino-Nucleus Cross Sections from High-Resolution Electron Scattering Experiments and Shell-Model Calculations

K. Langanke, G. Martínez-Pinedo, P. von Neumann-Cosel, and A. Richter
Phys. Rev. Lett. 93, 202501 – Published 11 November 2004

Abstract

Highly precise data on the magnetic dipole strength distributions from the Darmstadt electron linear accelerator for the nuclei Ti50, Cr52, and Fe54 are dominated by isovector Gamow-Teller-like contributions and can therefore be translated into inelastic total and differential neutral-current neutrino-nucleus cross sections at supernova neutrino energies. The results agree well with large-scale shell-model calculations, validating this model.

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  • Received 2 February 2004

DOI:https://doi.org/10.1103/PhysRevLett.93.202501

©2004 American Physical Society

Authors & Affiliations

K. Langanke1, G. Martínez-Pinedo2, P. von Neumann-Cosel3, and A. Richter3

  • 1Institute for Physics and Astronomy, University of Århus, DK-8000 Århus C, Denmark
  • 2ICREA and Institut d’Estudis Espacials de Catalunya, Edifici Nexus, Gran Capità 2, E-08034 Barcelona, Spain
  • 3Institut für Kernphysik, Technische Universität Darmstadt, 64289 Darmstadt, Germany

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Issue

Vol. 93, Iss. 20 — 12 November 2004

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