Search for Supernova Relic Neutrinos

寻找超新星遗迹中微子

• 批准号: 2264700
• 金额: --
• 依托单位: University of Sheffield
• 依托单位国家: 英国
• 项目类别: Studentship
• 财政年份: 2019
• 资助国家: 英国
• 起止时间: 2019 至 无数据
• 项目状态: 已结题
• 来源: https://gtr.ukri.org/projects?ref=studentship-2264700
• 关键词: Search; Supernova; Relic; Neutrinos

Core-collapse supernovae are amongst the most energetic events in the Universe. A single supernova will outshine an entire galaxy, yet the light is less than 1% of the energy that is released. The vast majority of energy released in a supernova (99%) is emitted in the form of neutrinos, a 'ghostly' particle that almost never interacts with matter. Over thirty years ago, 24 neutrinos were detected from Supernova 1987A; these have provided most of what we currently know about supernovae.Neutrinos from the next galactic supernova are currently on their way to Earth. When they arrive, we will study them to greatly advance our knowledge of how massive stars die. However, it is impossible to predict how many years (or decades) it will be before this happens.While we wait it is also possible to search for the signal from extra-galactic supernovae in an attempt to do neutrino cosmology. Core-collapose supernovae are believed to have started in the universe shortly after star formation began. Thus, there should exist a diffuse background of neutrinos throughout all of space, originating from all of the supernovae that have previously exploded. These particles are called 'supernova relic neutrinos', and we can use them to learn about the history of supernova explosions in the universe and related cosmological quantities, such as the star formation rate and cosmic chemical evolution.Previous searches for supernova relic neutrinos have been performed, but the signal has been masked by terrestrial backgrounds. The Super-Kamiokande (SK) detector will soon be upgraded with gadolinium and re-christened as SK-Gd. With the aid of gadolinium tagging, SK-Gd will be able to identify the supernova relic neutrinos and minimise the terrestrial backgrounds, making it very likely that the supernova relic neutrinos will finally be detected in the next few years.This PhD will involve travel to Japan for participation in the SK-Gd experiment, including calibration of the detector following gadolinium loading. It will also involve data reduction, simulation, and analysis, ultimately aimed at producing the first successful observation of the supernova relic neutrinos.

核心坍缩超新星是宇宙中最具能量的事件之一。一颗超新星的亮度将超过整个星系，但其光还不到释放能量的1%。超新星释放的绝大多数能量（99%）是以中微子的形式释放的，中微子是一种几乎从不与物质相互作用的“幽灵”粒子。30多年前，从超新星1987 A中探测到了24个中微子，这些中微子提供了我们目前对超新星的大部分了解。来自下一个银河系超新星的中微子目前正在前往地球的途中。当它们到达时，我们将研究它们，以极大地推进我们对大质量恒星如何死亡的认识。然而，我们不可能预测这会发生多少年（或几十年），在等待的同时，我们也有可能寻找来自河外超新星的信号，试图进行中微子宇宙学。核心坍缩超新星被认为是宇宙中星星形成后不久就开始出现的。因此，在整个空间中应该存在一个中微子的扩散背景，起源于所有以前爆炸过的超新星。这些粒子被称为“超新星遗迹中微子”，我们可以利用它们来了解宇宙中超新星爆炸的历史以及相关的宇宙学量，如星星形成速率和宇宙化学演化。以前对超新星遗迹中微子的搜索已经进行过，但信号一直被地球背景所掩盖。Super-Kamiokande（SK）探测器将很快升级为钆，并重新命名为SK-Gd。在钆标记的帮助下，SK-Gd将能够识别超新星遗迹中微子，并最大限度地减少地球背景，使得超新星遗迹中微子很可能在未来几年内最终被探测到。这个博士学位将涉及前往日本参加SK-Gd实验，包括在钆加载后校准探测器。它还将涉及数据简化，模拟和分析，最终旨在首次成功观测超新星遗迹中微子。