Collaborative Research: Mapping the Supernova Polarization Landscape

合作研究：绘制超新星偏振景观

• 批准号: 2010001
• 负责人: Douglas Leonard
• 金额: $ 24.63万
• 依托单位: San Diego State University Foundation
• 依托单位国家: 美国
• 项目类别: Standard Grant
• 财政年份: 2020
• 资助国家: 美国
• 起止时间: 2020-08-01 至 2024-07-31
• 项目状态: 已结题
• 来源: https://www.nsf.gov/awardsearch/showAward?AWD_ID=2010001&HistoricalAwards=false
• 关键词: Collaborative; Research; Mapping; Supernova; Polarization

Supernovae, or the explosions of massive stars, are critical to understand, both because they produce and disperse many of the atomic elements that make up planets and life, and because their brightness throughout the Universe is used to measure the expansion of the Universe. Supernova (SN) explosions are not spherical, but rather geometrically complex phenomena, whose aspherical structures cause variations in observed characteristics over time as the explosion evolves. A research collaboration between the University of Denver (DU) and San Diego State University (SDSU) uses an observational technique called spectropolarimetry to provide detailed three-dimensional information about SNe, probing spatial scales that cannot be resolved through direct imaging from earth or even from space. Spectropolarimetry combines detection of the polarization of light from a supernova with measurement of the spectrum of that light. This information reveals the changing densities, temperatures, and illumination patterns in the ejecta over time; and gives clues to the explosion mechanisms and the nature of progenitor systems. The project will advance the future of discovery by training students in these types of observations and modeling. It will also contribute to the training of a future diverse STEM community. The investigators will develop a hands-on learning module demonstrating the concept of polarization, for direct integration into two activities: the DU SciTech camp, co-directed by the DU principal investigator (PI), which brings middle-school girls of color to campus for a week-long discovery-based STEM camp each year, and also the extensive outreach activities led by the SDSU PI. The scientists will use data collected from 2011 to 2018 by the Supernova Spectropolarimetry (SNSPOL) Project, the largest existing database of spectropolarimetric observations of SNe of all types, which includes 106 SNe of all types, with 50 observed at 3+ epochs. They will interpret these data with new state-of-the-art modeling techniques. Observational surveys are discovering supernovae and related transients at an ever-increasing rate. The project will broaden the scientific impact of these discoveries by greatly expanding the existing catalog of SNe examined with spectropolarimetry and quantitatively establishing the common signatures of each SN type. The multi-epoch observations in the SNSPOL database trace each SN’s evolution as the photosphere recedes, probing ever deeper into the ejecta and revealing clues to the very nature of the explosion itself. Extracting and analyzing the most salient spectropolarimetric features from these data will make the wealth of information they contain available to future researchers. The results will build a fuller understanding of the 3D nature of SNe of all types and form a key discriminant for stellar explosion models.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.

超新星，或大质量恒星的爆炸，对理解至关重要，因为它们产生和分散了许多构成行星和生命的原子元素，还因为它们在整个宇宙中的亮度被用来测量宇宙的膨胀。 超新星（SN）爆炸不是球形的，而是几何上复杂的现象，其非球形结构会随着爆炸的演变而引起观测特征的变化。丹佛大学（DU）和圣地亚哥州立大学（SDSU）之间的研究合作使用一种称为分光偏振法的观测技术来提供有关SNe的详细三维信息，探索无法通过直接成像解决的空间尺度从地球甚至太空。分光偏振测量法将超新星发出的光的偏振探测与光谱测量结合起来。 这些信息揭示了喷出物随时间变化的密度、温度和照明模式;并为爆炸机制和祖先系统的性质提供了线索。 该项目将通过培训学生进行这些类型的观察和建模来推进发现的未来。它还将有助于培养未来多元化的STEM社区。研究人员将开发一个实践学习模块，展示极化的概念，直接融入两个活动：DU SciTech阵营，由DU首席研究员（PI）共同指导，每年将有色人种的中学女生带到校园进行为期一周的基于发现的STEM阵营，以及由SDSU PI领导的广泛的外展活动。科学家们将使用超新星分光偏振测量（SNSPOL）项目从2011年到2018年收集的数据，该项目是现有最大的所有类型SNe分光偏振观测数据库，其中包括106种所有类型的SNe，其中50种在3个以上的时期观测到。 他们将用最先进的建模技术解释这些数据。观测调查发现超新星和相关的瞬变以不断增加的速度。该项目将扩大这些发现的科学影响，大大扩展现有的SNe目录，用分光偏振法进行检查，并定量建立每种SN类型的共同特征。SNSPOL数据库中的多历元观测跟踪了每个SN在光球消退时的演变，更深入地探索了喷出物，并揭示了爆炸本身的本质。从这些数据中提取和分析最显著的光谱偏振特征将使它们所包含的丰富信息可供未来的研究人员使用。该奖项反映了NSF的法定使命，并通过使用基金会的智力价值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

A High-velocity Scatterer Revealed in the Thinning Ejecta of a Type II Supernova

II 型超新星变薄喷射物中揭示的高速散射体

• DOI: 10.3847/2041-8213/ac31bf
• 发表时间: 2021
• 期刊: The Astrophysical Journal Letters
• 作者: Leonard, Douglas C.;Dessart, Luc;Hillier, D. John;Pignata, Giuliano;Williams, G. Grant;Hoffman, Jennifer L.;Milne, Peter;Smith, Nathan;Smith, Paul S.;Khandrika, Harish G.
• 通讯作者: Khandrika, Harish G.

Infrared spectropolarimetric detection of intrinsic polarization from a core-collapse supernova

• DOI: 10.1038/s41550-021-01320-4
• 发表时间: 2021-02
• 期刊: Nature Astronomy
• 影响因子: 14.1
• 作者: S. Tinyanont;M. Millar-Blanchaer;M. Kasliwal;D. Mawet;D. Leonard;M. Bulla;K. De;N. Jovanovic;M. Hankins;G. Vasisht;E. Serabyn

Polarization signatures of a high-velocity scatterer in nebular-phase spectra of Type II supernovae

II 型超新星星云相光谱中高速散射体的偏振特征

• DOI: 10.1051/0004-6361/202140409
• 发表时间: 2021
• 期刊: Astronomy & Astrophysics
• 影响因子: 6.5
• 作者: Dessart, Luc;John Hillier, D.;Leonard, Douglas C.
• 通讯作者: Leonard, Douglas C.

SN 2014ab: an aspherical Type IIn supernova with low polarization

• DOI: 10.1093/mnras/staa2617
• 发表时间: 2020-07
• 期刊: Monthly Notices of the Royal Astronomical Society
• 影响因子: 4.8
• 作者: C. Bilinski;N. Smith;G. Williams;Paul S. Smith;J. Andrews;K. Clubb;Wei Zheng;A. Filippenko;O. Fox;G. Hosseinzadeh;D. Howell;P. Kelly;P. Milne;D. Sand;J. Hoffman;D. Leonard;Samantha K. Cargill;Chadwick F. E. Casper;Goni Halevy;Haejung Kim;Sahana Kumar;Kenia Pina;H. Yuk

Multiepoch VLT–FORS spectropolarimetric observations of supernova 2012aw reveal an asymmetric explosion

• DOI: 10.1051/0004-6361/202140281
• 发表时间: 2021-01
• 期刊: Astronomy & Astrophysics
• 影响因子: 6.5
• 作者: L. Dessart;D. Leonard;D. Hillier;G. Pignata