Collaborative Research: WoU-MMA Constraining the nuclear equation of state and population of neutron star mergers through observations of transient and persistent phenomena

合作研究：WoU-MMA 通过观察瞬态和持续现象来约束中子星并合的核状态方程和布居数

• 批准号: 2206321
• 负责人: Richard O'Shaughnessy
• 金额: $ 44.69万
• 依托单位: Rochester Institute of Tech
• 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: 2022-12-01 至 2025-11-30
• 项目状态: 未结题
• 来源: https://www.nsf.gov/awardsearch/showAward?AWD_ID=2206321&HistoricalAwards=false
• 关键词: Collaborative; Research; WoU; MMA; Constraining

Neutron stars (NSs) are formed when a massive star reaches the end of its life: the outer layers of the star are ejected in a violent explosion but the core of the star collapses to form a small, dense remnant. NSs that form a binary system with another NS sometimes in-spiral and merge, producing gravitational waves and a bright transient that is thousands of times more luminous than a nova (a so-called kilonova). NS-NS mergers have been detected by the NSF-funded Laser Interferometer Gravitational wave Observatory (LIGO). A team from the Rochester Institute of Technology and the University of Tennessee Knoxville will continue their program to use advanced computational models to better understand NS-NS mergers and NS physics. They will produce realistic models of the kilonova explosion, improve estimates of the neutron mass distribution, and better understand neutron star populations. The models will be benchmarked against gravitational wave and electromagnetic detections of NS-NS mergers. The program includes training and mentoring of graduate students and postdoctoral researchers; participation in a Rochester Institute of Technology program (ROAR) that introduces high school students from underrepresented minorities to research; and development of a new undergraduate course at the University of Tennessee Knoxville focused on gravitational waves. The detailed science goals of the proposal are; extend ongoing work to produce more systematic kilonova models, calibrated to simulations and exploring relevant systematic uncertainties; incorporate rapid r-process observations systematically into joint inference about NS population properties and the equation of state (EOS), allowing for alternatives, to assess the origin of r-process elements; use the tools developed as part of this program to reconstruct the population of NS, the nuclear EOS, and the origin of r-process elements; and assess the ability of the tools to draw these inferences. The proposed research involves producing realistic models of the kilonova explosion that occurs when neutron stars collide and merge. These models will be benchmarked against gravitational wave and electromagnetic detections of NS-NS mergers, thereby improving estimates of the neutron mass distribution and better understanding neutron star populations. Thus, this project is aligned with the science mission of the Windows on the Universe: Multi-Messenger Astronomy (WoU-MMA) Big Idea.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.

中子星（NS）是在大质量星星达到其生命终点时形成的：星星的外层在剧烈的爆炸中被喷射出来，但星星的核心坍缩形成一个小而致密的残余物。与另一个NS形成一个双星系统的NS有时会螺旋并合并，产生引力波和比新星（所谓的千新星）亮数千倍的明亮瞬变。NS-NS合并已经被NSF资助的激光干涉引力波天文台（LIGO）探测到。来自罗切斯特理工学院和田纳西大学诺克斯维尔的一个研究小组将继续他们的计划，使用先进的计算模型来更好地理解NS-NS合并和NS物理。他们将制作出千诺瓦爆炸的真实模型，改进对中子质量分布的估计，并更好地了解中子星星的数量。这些模型将以NS-NS合并的引力波和电磁探测为基准。该计划包括培训和指导研究生和博士后研究人员;参与罗切斯特理工学院的一项计划（ROAR），该计划将来自代表性不足的少数民族的高中生引入研究;以及在田纳西大学诺克斯维尔开发一门新的本科课程，重点是引力波。该提案的详细科学目标是：扩大正在进行的工作，以制作更系统的kilonova模型，根据模拟进行校准，并探索相关的系统不确定性;将快速r-过程观测系统地纳入关于NS总体特性和状态方程的联合推断，考虑到替代方案，以评估r-过程元素的起源;使用开发的工具，作为该计划的一部分，以重建NS的人口，核EOS，和r-过程元素的起源，并评估这些工具的能力，以得出这些推论。拟议中的研究包括制作中子星碰撞和合并时发生的千诺瓦爆炸的真实模型。这些模型将以NS-NS合并的引力波和电磁探测为基准，从而改善对中子质量分布的估计，并更好地了解中子星星种群。因此，该项目符合"宇宙之窗：多信使天文学（WoU-MMA）大创意“的科学使命。该奖项反映了NSF的法定使命，并通过使用基金会的知识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

Cost minimization in acquisition for gravitational wave surrogate modeling

引力波替代建模采集成本最小化

• DOI: 10.1103/physrevd.106.084020
• 发表时间: 2022
• 期刊: Physical Review D
• 影响因子: 5
• 作者: Daningburg, Karl;O’Shaughnessy, Richard
• 通讯作者: O’Shaughnessy, Richard

Iteratively comparing gravitational-wave observations to the evolution of massive stellar binaries

• DOI: 10.1103/physrevd.108.043023
• 发表时间: 2023-03
• 期刊: Physical Review D
• 影响因子: 5
• 作者: V. Delfavero;R. O’Shaughnessy;K. Belczynski;Paweł Drozda;D. Wysocki

Interpolated kilonova spectra models: Examining the effects of a phenomenological, blue component in the fitting of AT2017gfo spectra

• DOI: 10.1103/physrevresearch.5.043106
• 发表时间: 2023-11
• 期刊: Physical Review Research
• 影响因子: 4.2
• 作者: M. Ristić;Richard O'Shaughnessy;V. A. Villar;R. Wollaeger;O. Korobkin;Chris L. Fryer;C. Fontes;Atul Kedia

Surrogate light curve models for kilonovae with comprehensive wind ejecta outflows and parameter estimation for AT2017gfo

• DOI: 10.1103/physrevresearch.5.013168
• 发表时间: 2022-11
• 期刊: Physical Review Research
• 影响因子: 4.2
• 作者: Atul Kedia;M. Ristić;R. O’Shaughnessy;A. Yelikar;R. Wollaeger;O. Korobkin;E. Chase;Chris L. Fryer;C. Fontes

Constraining Inputs to Realistic Kilonova Simulations through Comparison to Observed r-process Abundances

• DOI: 10.3847/1538-4357/acf3e0
• 发表时间: 2022-06
• 期刊: The Astrophysical Journal
• 作者: M. Ristić;E. Holmbeck;R. Wollaeger;O. Korobkin;E. Champion;R. O’Shaughnessy;Chris L. Fryer;C. Fontes;M. Mumpower;T. Sprouse