Collaborative Research: Unravelling Stripped Supernovae - Synergy between Observations and Modeling

合作研究：解开剥离超新星——观测与建模之间的协同作用

• 批准号: 2206657
• 负责人: Maryam Modjaz
• 金额: $ 23.91万
• 依托单位: University of Virginia Main Campus
• 依托单位国家: 美国
• 项目类别: Standard Grant
• 财政年份: 2022
• 资助国家: 美国
• 起止时间: 2022-09-01 至 2025-08-31
• 项目状态: 未结题
• 来源: https://www.nsf.gov/awardsearch/showAward?AWD_ID=2206657&HistoricalAwards=false
• 关键词: Collaborative; Research; Unravelling; Stripped; Supernovae

It has long been known that massive stars in the universe die in massive explosions known as supernovae (SNe). Supernovae resulting from the core collapse of massive stars are classified by astronomers in several ways. One type is normal SNe, whose massive progenitors have been stripped of their hydrogen and helium envelopes, thus known as “stripped supernovae.” Another type is classified as SNe Ic, with or without an accompanying gamma-ray burst (GRB), which emits relativistic jets of high-energy radiation. These explosions can be seen to large cosmological distances and are important for many fields of astrophysics. A research collaboration between the University of Virginia and Michigan State University will address some of the outstanding questions about SNe, such as which massive, stripped stars die in which kinds of deaths, and what is the detailed progenitor makeup for these explosions? The work will involve analyzing data from a large set of stripped SNe, as well as modeling those data and other published data via the open-source radiative transfer software called TARDIS, in combination with use of the machine-learning technology known as emulators for efficiently scanning large sets of parameters. In addition, to increase the number of members of underrepresented groups in STEM, the lead investigators will collaborate with two different programs (one, Girls Exploring the Universe, a summer program for middle school girls in Virginia, and the other at a high school in East Lansing, MI) to involve their students in different research projects that range from contributing to the TARDIS code to using the proposed widget that compares TARDIS simulations to recently observed SN spectra. Evidence suggests that school-age programs incorporating hands-on research, coding activities, and role models tend to increase self-confidence and interest of girls and minorities in STEM careers.The researchers aim to resolve two recent controversies in the SN community, with strong implications for stellar evolution, understanding the conditions needed for jet production, and for the hotly debated SN-GRB progenitor models. A clear understanding of the stellar progenitors and explosion parameters of SN and GRBs is an essential foundation for using them as indicators of star formation over cosmological distances and for assessing them as sources of re-ionizing the Universe. The proposed activities will transform the field of stripped SNe: they will quantify, for the first time, the systematic and statistical uncertainties in modeling these explosions and increase the total number of objects whose spectra have been modeled to at least 185 SNe, which constitutes the largest data set of Stripped SN in the world and allows the field to fully transition from individual objects to population studies. Moreover, the proposed framework will do so in a homogeneous and consistent manner. The proposed rapid and statistically solid theoretical interpretation framework will be made public.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.

人们早就知道，宇宙中的大质量恒星在被称为超新星(SNE)的大质量爆炸中死亡。天文学家用几种方法对大质量恒星核心塌缩产生的超新星进行分类。其中一种类型是正常的SNE，其巨大的前体已经被剥离了氢气和氦的包层，因此被称为“剥离的超新星”。另一种类型被归类为SNE IC，无论有没有伴随的伽马射线暴(GRB)，它都会发射高能辐射的相对论喷流。这些爆炸可以在很远的宇宙学距离内看到，对天体物理学的许多领域都很重要。弗吉尼亚大学和密歇根州立大学之间的一项研究合作将解决关于SNE的一些悬而未决的问题，例如哪些大质量的、剥离的恒星在哪些类型的死亡中死亡，以及这些爆炸的详细祖先构成是什么？这项工作将涉及分析来自大量剥离的SNE的数据，以及通过名为TARDIS的开源辐射传输软件对这些数据和其他发布的数据进行建模，并结合使用称为仿真器的机器学习技术，以有效地扫描大型参数集。此外，为了增加STEM中代表性不足群体的成员数量，首席调查员将与两个不同的项目(一个是针对弗吉尼亚州中学女生的暑期项目，一个是针对弗吉尼亚州中学生的暑期项目，另一个是在密歇根州东兰辛的高中)合作，让他们的学生参与不同的研究项目，范围从对TARDIS代码的贡献到使用建议的小部件，将TARDIS模拟与最近观察到的SN谱进行比较。有证据表明，结合动手研究、编码活动和榜样的学龄项目往往会增加女孩和少数族裔在STEM职业生涯中的自信和兴趣。研究人员的目标是解决SN社区最近的两个争议，这两个争议对恒星演化具有强烈的影响，理解产生喷流所需的条件，以及热议的SN-GRB前体模型。清楚地了解SN和伽玛暴的恒星前体和爆炸参数是将它们用作宇宙距离上恒星形成的指示器和评估它们作为宇宙再电离来源的重要基础。拟议的活动将改变剥离SNE领域：它们将首次量化模拟这些爆炸的系统和统计不确定性，并将其光谱被模拟的天体总数增加到至少185个SNE，这构成了世界上最大的剥离SNE数据集，并使该领域能够完全从单个天体过渡到总体研究。此外，拟议的框架将以统一和一致的方式这样做。建议的快速和可靠的理论解释框架将公之于众。这一奖项反映了NSF的法定使命，并通过使用基金会的智力优势和更广泛的影响审查标准进行评估，被认为值得支持。

项目成果

Peculiar Spectral Evolution of the Type I Supernova 2019eix: A Possible Double Detonation from a Helium Shell on a Sub-Chandrasekhar-mass White Dwarf

• DOI: 10.3847/1538-4357/acdd6a
• 发表时间: 2023-05
• 期刊: The Astrophysical Journal
• 作者: E. P. Gonzalez;D. Howell;J. Burke;Yize Dong;D. Hiramatsu;C.McCully;C.Pellegrino;W. E. Kerzendorf;M. Modjaz;G. Terreran;M. Williamson

SN 2020bio: A Double-peaked, H-poor Type IIb Supernova with Evidence of Circumstellar Interaction

• DOI: 10.3847/1538-4357/ace595
• 发表时间: 2023-01
• 期刊: The Astrophysical Journal
• 作者: C. Pellegrino;D. Hiramatsu;I. Arcavi;D. Howell;K. Bostroem;P. J. Brown;J. Burke;N. Elias-Rosa;K. Itagaki;H. Kaneda;C. McCully;M. Modjaz;E. P. Gonzalez;T. Pritchard;N. Yesmin

SN 2019ewu: A Peculiar Supernova with Early Strong Carbon and Weak Oxygen Features from a New Sample of Young SN Ic Spectra

• DOI: 10.3847/2041-8213/acb549
• 发表时间: 2022-11
• 期刊: The Astrophysical Journal Letters
• 作者: M. Williamson;Christian Vogl;M. Modjaz;W. E. Kerzendorf;Jaladh Singhal;Teresa Boland;J. Burke

Shock Cooling and Possible Precursor Emission in the Early Light Curve of the Type II SN 2023ixf

• DOI: 10.3847/2041-8213/ace4c4
• 发表时间: 2023-06
• 期刊: The Astrophysical Journal Letters
• 作者: G. Hosseinzadeh;J. Farah;M. Shrestha;D. Sand;Y. Dong 董;P. Brown;K. Bostroem;S. Valenti;S. Jha;J. Andrews;I. Arcavi;J. Haislip;D. Hiramatsu;E. Hoang;D. Howell;D. Janzen;J. Jencson;V. Kouprianov;M. Lundquist;C. McCully;Nicolas E. Meza Retamal;M. Modjaz;M. Newsome;E. P. Gonzalez;J. Pearson;C. Pellegrino;A. Ravi;D. Reichart;N. Smith;G. Terreran;J. Vink'o

The Diverse Properties of Type Icn Supernovae Point to Multiple Progenitor Channels

• DOI: 10.3847/1538-4357/ac8ff6
• 发表时间: 2022-05
• 期刊: The Astrophysical Journal
• 作者: C. Pellegrino;D. Howell;G. Terreran;I. Arcavi;K. Bostroem;P. Brown;J. Burke;Y. Dong;A. Gil