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Moving Supernovae Beyond the Standard model: A Study of Neutrino Flavor Mixing in Core-Collapse Supernovae

超越标准模型的超新星：核心塌陷超新星中微子味道混合的研究

基本信息

批准号：
1801844
负责人：
MacKenzie Warren
金额：
$ 10万
依托单位：
Warren MacKenzie
依托单位国家：
美国
项目类别：
Fellowship Award
财政年份：
2018
资助国家：
美国
起止时间：
2018-07-01 至 2020-12-31
项目状态：
已结题

来源：
https://www.nsf.gov/awardsearch/showAward?AWD_ID=1801844&HistoricalAwards=false
关键词：
Moving Supernovae Beyond Standard model

项目摘要

MacKenzie Warren is awarded an NSF Astronomy and Astrophysics Fellowship to carry out a program of research and education at Michigan State University. Warren will use computer simulations to study how tiny subatomic particles called neutrinos affect supernova explosions of stars. Supernovae are the engines that create and disperse most of the elements that make up the universe, and neutrinos have the strange ability to change their essence, or flavor, a behavior that physicists call "flavor mixing.' Warren's work will be the first to add neutrino flavor mixing to existing sophisticated models of supernovae arising from the collapse of the core of a dying massive star. This will help astronomers to better understand how a supernova explodes and how it creates elements. Warren will also work with an outreach program to host free astronomy nights in public spaces, with the aim of reaching communities that are not otherwise engaged by most science outreach efforts.Warren will incorporate a model of neutrino flavor mixing into the FLASH supernova code to study the effects of neutrino mixing, including matter enhancements and neutrino self-interactions on core-collapse supernovae (CCSNe). This project will use both spherically symmetric and two-dimensional simulations to study the effect of neutrino flavor transformations on the range of supernova progenitors, in particular the impact on nucleosynthesis, explodability, the observable neutrino signal, the onset of the neutrino driven winds, and the resultant neutron star and black hole mass distribution. This will lead to a more complete understanding of supernova neutrinos, which in turn will inform the interpretation of observed CCSNe neutrinos and improve our knowledge of the contribution of CCSNe to galactic chemical evolution. To provide astronomy outreach to the public, Warren will work with the Lansing chapter of the Popscope program to take telescopes to public events and public spaces and engage passersby.This award reflects NSF's statutory mission and has been deemed worthy of support through evaluation using the Foundation's intellectual merit and broader impacts review criteria.

麦肯齐·沃伦被授予美国国家科学基金会天文学和天体物理学奖学金，以在密歇根州立大学开展一项研究和教育项目。沃伦将使用计算机模拟来研究被称为中微子的微小亚原子粒子如何影响恒星的超新星爆炸。超新星是创造和分散构成宇宙的大部分元素的引擎，中微子具有改变其本质或味道的奇怪能力，物理学家将这种行为称为“味道混合”。沃伦的工作将首次将中微子混合的味道添加到现有的复杂超新星模型中，这些超新星是由一颗濒临死亡的大质量恒星的核心坍塌而产生的。这将帮助天文学家更好地了解超新星是如何爆炸的，以及它是如何产生元素的。沃伦还将与一个推广计划合作，在公共空间举办免费天文之夜，目的是接触到大多数科学推广努力没有参与的社区。沃伦将在闪电超新星代码中加入一个中微子味道混合模型，以研究中微子混合的影响，包括物质增强和中微子自身相互作用对核心塌缩超新星(CCSNe)的影响。该项目将使用球对称和二维模拟来研究中微子味道变化对超新星前驱物质范围的影响，特别是对核合成、爆炸能力、可观测到的中微子信号、中微子驱动风的开始以及由此产生的中子星和黑洞质量分布的影响。这将导致对超新星中微子的更完整的了解，这反过来将为对观测到的CCSNe中微子的解释提供信息，并提高我们对CCSNe对星系化学演化的贡献的认识。为了向公众提供天文推广，沃伦将与波普望远镜计划的兰辛分会合作，将望远镜带到公共活动和公共空间，并吸引路人参与。这一奖项反映了NSF的法定使命，并通过使用基金会的学术价值和更广泛的影响审查标准进行评估，被认为值得支持。