Neutrinos as astrophysical probes

F. Cavanna, M. Costantini, O. Palamara, F. Vissani
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引用次数: 20

Abstract

The aim of these notes is to provide a brief review of the topic of neutrino astronomy and in particular of neutrinos from core collapse supernovae. They are addressed to a curious reader, beginning to work in a multidisciplinary area that involves experimental neutrino physics, astrophysics, nuclear physics and particle physics phenomenology. After an introduction to the methods and goals of neutrinos astronomy, we focus on core collapse supernovae, as (one of) the most promising astrophysical source of neutrinos. The first part is organized almost as a tale, the last part is a bit more technical. We discuss the impact of flavor oscillations on the supernova neutrino signal (=the change of perspective due to recent achievements) and consider one specific example of signal in detail. This shows that effects of oscillations are important, but astrophysical uncertainties should be thought as an essential systematics for a correct interpretation of future experimental data. Three appendices corroborate the t...
中微子作为天体物理探测器
这些笔记的目的是简要回顾中微子天文学的主题,特别是来自核心坍缩超新星的中微子。他们是给一个好奇的读者,开始在涉及实验中微子物理学,天体物理学,核物理学和粒子物理现象学的多学科领域工作。在介绍了中微子天文学的方法和目标之后,我们将重点放在核心坍缩超新星上,这是最有希望的中微子天体物理来源之一。第一部分几乎是一个故事,最后一部分有点技术性。我们讨论了风味振荡对超新星中微子信号的影响(=由于最近的成就而改变的视角),并详细考虑了信号的一个具体例子。这表明振荡的影响是重要的,但天体物理的不确定性应该被认为是正确解释未来实验数据的基本系统。三个附录证实了……
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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