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

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
批准号:
1801844
负责人:
MacKenzie Warren
金额:
$10.0万
依托单位:
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
项目状态:
已结题
起止时间:
2018-07-01 至 2020-12-31

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英文摘要
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.
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DOI: 10.3847/1538-4357/ab609e
发表时间: 2019-02
期刊: The Astrophysical Journal
影响因子: --
作者: [S. Couch;M. Warren;E. O’Connor]
通讯作者: S. Couch;M. Warren;E. O’Connor
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