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arXiv 1601.05018astro-ph.HEastro-ph.SRhep-ph
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超新星中微子物理学的理论发展:质量修正和配对关联函数

Theoretical developments in supernova neutrino physics : mass corrections and pairing correlators

Cristina Volpe

摘要:

我们强调我们的理解的进展中微子如何改变他们的味道在天体物理环境中,特别是中微子自相互作用的影响。我们强调扩展的描述中微子在大质量恒星的传播是超越目前的平均场近似的基础上。扩展方程包括,特别是,从(反)中微子-(反)中微子配对相关性和中微子质量的修正。我们强调尚未解决的问题和挑战。

英文摘要:

We highlight the progress in our understanding of how neutrinos change their flavor in astrophysical environments, in particular effects from the neutrino self-interaction. We emphasize extended descriptions of neutrino propagation in massive stars that are beyond the current one based on the mean-field approximation. The extended equations include, in particular, corrections from (anti)neutrino-(anti)neutrino pairing correlations and from the neutrino mass. We underline open issues and challenges.

机构、总结、中文摘要均由AI分析而来,可能存在错误,请以论文正文为准。

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