Constraints on oscillation parameters through the MSW effect of supernova neutrinos

S. Kawagoe, T. Kajino, H. Suzuki, K. Sumiyoshi, S. Yamada

研究成果: Conference article

3 引用 (Scopus)

抜粋

We try to constrain the neutrino oscillation parameters by studying the MSW matter effect on supernova neutrinos. Using an implicit Lagrangian code for general relativistic spherical hydrodynamics (Yamada, 1997), we calculate the propagation of shock waves passing through the stellar envelopes over dozens of seconds, which is based on modeling the adiabatic collapse of iron core. We study how quantitatively the influence of the shock propagation appears in the deformation of neutrino energy spectrum. In addition, we are able to examine the θ13 dependence of time evolution of the neutrino detection rates at SK. Using our supernova model, we found that the MSW effect appears, at first, from low-energy region and moves toward high-energy region as the shock wave propagates. We find that the shock propagation has strong influence on the supernova neutrino oscillation through the evolution of density profile induced by the shock propagation.

元の言語English
記事番号052020
ジャーナルJournal of Physics: Conference Series
120
発行部数Part 5
DOI
出版物ステータスPublished - 2008 1 1
イベント10th International Conference on Topics in Astroparticle and Underground Physics, TAUP 2007 - Sendai , Japan
継続期間: 2007 9 112007 9 15

ASJC Scopus subject areas

  • Physics and Astronomy(all)

フィンガープリント Constraints on oscillation parameters through the MSW effect of supernova neutrinos' の研究トピックを掘り下げます。これらはともに一意のフィンガープリントを構成します。

  • これを引用