CAREER: Research in Strong-Field Gravity and Astrophysics

职业：强场重力和天体物理学研究

• 批准号: 2145421
• 负责人: Vasileios Paschalidis
• 金额: $ 45万
• 依托单位: University of Arizona
• 依托单位国家: 美国
• 项目类别: Continuing Grant
• 财政年份: 2022
• 资助国家: 美国
• 起止时间: 2022-06-01 至 2027-05-31
• 项目状态: 未结题
• 来源: https://www.nsf.gov/awardsearch/showAward?AWD_ID=2145421&HistoricalAwards=false
• 关键词: CAREER; Research; Strong; Field; Gravity

This award is funded in part under the American Rescue Plan Act of 2021 (Public Law 117-2). The project serves the national interest, as stated by NSF's mission, by promoting the progress of science, and laying foundations that will help advance the national prosperity and welfare; In particular, the award will enable research on compact binary systems in general relativity and modified gravity by combining theory and multi-messenger observations with gravitational waves. The work will advance our understanding of nuclear physics at densities and temperatures that arise in the deep interiors of colliding neutron stars, which cannot be probed by experiments on Earth. New tools will be developed for understanding gravity through a synergy of gravitational wave observations by LIGO, and the anticipated electromagnetic signals that will be detected by ground and space-based telescopes observing from the radio to the hard gamma-ray bands. The group will develop new codes for modeling binary neutron stars and binary black hole-neutron stars with the aid of supercomputers. Such theoretical work is crucial for the successful interpretation of and the extraction of fundamental physics from existing and future observations of compact binary systems. The award will support the training, education and further career development of students in STEM fields, including minorities and women. The award will enable the development of the Computation and Mathematics Program for incoming Arizona Science Students (COMPASS) initiative, which will bridge and smooth the high school-to-college transition for students, and facilitate the success and retention of underrepresented minorities in Physics, Astronomy and other scientific fields. The specific projects have a two-fold goal: a) advance our understanding of strong field, relativistic gravity, nuclear physics and theoretical astrophysics; b) facilitate the detection and physical interpretation of gravitational waves and their possible electromagnetic counterparts. A substantial part of the effort will focus on the investigation of the inspiral and merger of compact binaries (binary neutron stars, binary black hole-neutron stars) and their gravitational wave and electromagnetic signatures. Methods will be developed for utilizing these observable signatures to extract information about fundamental physics, in particular about the nature of gravity and nuclear physics above the nuclear saturation density. More specifically, codes that run on supercomputers will be developed to solve the equations of a scalar-tensor theory of gravity with future application to binary black hole-neutron stars in order to develop techniques that test whether there are any scalar-field induced deviations from Einstein gravity that can be triggered by either charge (dark, electric or magnetic) or by magnetic fields, and to test the equivalence principle in this regime for the first time. Using existing codes, methods will be developed for probing the unknown thermal part of the equation of state at nuclear densities by using the gravitational wave and electromagnetic signatures from binary neutron star mergers. The proposed studies are extremely timely in light of the recent detection of gravitational waves by the LIGO and Virgo collaborations not only as generated by binary black holes, but also as generated by compact binaries with at least one neutron star. The project will benefit the interpretation and detection of gravitational waves and their electromagnetic counterparts not only by current and upcoming gravitational wave detectors and telescopes, but also by future ones. The proposed research will be accomplished via large-scale supercomputer simulations accompanied by analytic modeling.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.

该奖项的部分资金来自2021年美国救援计划法案（公法117-2）。该项目服务于国家利益，正如NSF的使命所述，通过促进科学进步，奠定有助于促进国家繁荣和福利的基础;特别是，该奖项将通过将理论和多信使观测与引力波相结合，使广义相对论和修正引力中的紧凑双星系统研究成为可能。这项工作将推进我们对碰撞中子星内部深处产生的密度和温度的核物理学的理解，这些中子星无法通过地球上的实验进行探测。将开发新的工具，通过LIGO的引力波观测以及地面和空间望远镜从无线电到硬伽马射线波段观测到的预期电磁信号的协同作用来理解引力。该小组将在超级计算机的帮助下开发新的代码来模拟双中子星和双黑洞中子星。这样的理论工作是至关重要的成功解释和提取的基本物理从现有的和未来的观测紧凑的二元系统。该奖项将支持STEM领域学生的培训，教育和进一步的职业发展，包括少数民族和妇女。该奖项将使计算和数学计划的发展，为即将到来的亚利桑那州科学学生（COMPASS）倡议，这将桥梁和顺利的高中到大学的过渡，为学生，并促进成功和保留代表性不足的少数民族在物理，天文学和其他科学领域。具体项目有两个目标：a）推进我们对强场、相对论引力、核物理和理论天体物理学的理解; B）促进引力波及其可能的电磁波的检测和物理解释。这项工作的很大一部分将集中在研究致密双星（中子双星、黑洞-中子双星）的螺旋和合并及其引力波和电磁特征。将制定方法，利用这些可观察到的签名提取有关基础物理学的信息，特别是关于重力和核饱和密度以上的核物理学的性质。更具体地说，将开发在超级计算机上运行的代码，以求解标量-张量引力理论的方程，未来将应用于黑洞-中子双星，以开发测试是否存在标量场引起的偏离爱因斯坦引力的技术，（黑暗，电或磁）或磁场，并测试在这一制度的等效原理的第一次。利用现有的代码，将开发的方法来探测未知的热部分的状态方程在核密度通过使用引力波和电磁签名从双中子星星合并。鉴于LIGO和Virgo合作最近探测到的引力波不仅是由双黑洞产生的，而且也是由至少有一颗中子星星的紧凑双星产生的，因此拟议的研究非常及时。该项目将有利于解释和探测引力波及其电磁对应物，不仅是当前和即将到来的引力波探测器和望远镜，而且是未来的。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

Self-gravitating disks around rapidly spinning, tilted black holes: General-relativistic simulations

• DOI: 10.1103/physrevd.106.104010
• 发表时间: 2022-09
• 期刊: Physical Review D
• 影响因子: 5
• 作者: A. Tsokaros;M. Ruiz;S. Shapiro;V. Paschalidis

Improving the convergence order of binary neutron star merger simulations in the Baumgarte- Shapiro-Shibata-Nakamura formulation

改进 Baumgarte-Shapiro-Shibata-Nakamura 公式中双中子星并合模拟的收敛阶

• DOI: 10.1103/physrevd.106.023015
• 发表时间: 2022
• 期刊: Physical Review D
• 影响因子: 5
• 作者: Raithel, Carolyn A.;Paschalidis, Vasileios
• 通讯作者: Paschalidis, Vasileios

Astrophysics with the Laser Interferometer Space Antenna

• DOI: 10.1007/s41114-022-00041-y
• 发表时间: 2022-03
• 期刊: Living Reviews in Relativity
• 影响因子: 40.6
• 作者: P. A. Seoane;J. Andrews;M. A. Sedda;A. Askar;Quentin Baghi;R. Balasov;I. Bartos;S. Bavera

Finite-temperature effects in dynamical spacetime binary neutron star merger simulations: validation of the parametric approach

动态时空双中子星合并模拟中的有限温度效应：参数方法的验证

• DOI: 10.1093/mnras/stac2450
• 发表时间: 2022
• 期刊: Monthly Notices of the Royal Astronomical Society
• 影响因子: 4.8
• 作者: Raithel, Carolyn A.;Espino, Pedro;Paschalidis, Vasileios
• 通讯作者: Paschalidis, Vasileios

Minidisc influence on flow variability in accreting spinning black hole binaries: simulations in full general relativity

微型盘对吸积旋转黑洞双星中流动变化的影响：完全广义相对论中的模拟

• DOI: 10.1093/mnras/stad091
• 发表时间: 2023
• 期刊: Monthly Notices of the Royal Astronomical Society
• 影响因子: 4.8
• 作者: Bright, Jane C;Paschalidis, Vasileios
• 通讯作者: Paschalidis, Vasileios