Collaborative Research: RUI: Theoretical Studies of the Atmospheres of Highly Magnetized Neutron Stars

磁星是一颗中子星，或密度极高的恒星，它拥有非常大的磁场。磁星是宇宙中最耐人寻味的致密天体之一，已经发现了大约30颗。威廉·马什·赖斯大学、霍普学院和美国国家航空航天局戈达德太空飞行中心合作的一项研究计划将导致开发最先进的磁星大气发射理论模型。主要目标是提供一套可观测的信号预测，以加强对X射线望远镜数据的解释，从而更好地理解中子星、磁学和基础量子物理。将开发计算机模拟X射线在具有任意磁场取向的磁星大气中的传播，包括中子星表面上从磁极到赤道的所有位置。这项研究包括重要的研究生和本科生培训。莱斯大学的一名博士生将参与这项工作，其结果将导致一篇博士论文。几名本科生将致力于这项研究的独立部分，并向资深科学家和同行展示他们的发现。研究人员将向公众阐明这项工作的各个方面，以及中子星激动场的亮点。磁星为测试地球实验室目前无法获得的基础物理提供了一个独特的论坛。更好地了解磁星是将它们用作代理量子电动力学(QED)物理实验室的核心。研究人员将通过开发一项关于磁星大气发射的全面理论研究来帮助实现这一点，计算表面任何位置的偏振相关和角度相关发射率的预期。偏振信号的产生将允许区分几何源信息和强场QED物理的信号，如双折射真空偏振。这项工作将升级光球回旋吸收线物理和光子传播，为天体物理学家提供新的工具，用于其他中子星问题。该计划的结果将提高偏振望远镜在X射线波段的潜在科学产量。与磁星有关的四个悬而未决的问题将受到这项研究的重大影响。这些是(I)磁星与正常脉冲星本质上不同？，(Ii)旋转体的磁倾角是否随磁星年龄而变化，我们能否测量它以便更精确地校准恒星磁场强度？(Iii)相对于磁极，磁星表面产生准热辐射的加热位置在哪里？以及(Iv)我们能用广义相对论来确定磁星的质量半径比吗？从而探索他们的状态方程？这一裁决反映了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。

A magnetar is a neutron star, or extremely dense star, which possesses an extraordinarily large magnetic field. Magnetars, of which around 30 have been discovered, are some of the most intriguing compact objects in the Universe. A research program, which is a collaboration between William Marsh Rice University, Hope College and NASA's Goddard Space Flight Center, will lead to the development of state of the art theoretical models for the atmospheric emission of magnetars. The prime objective is to deliver a suite of observable signal predictions to enhance interpretation of data from X-ray telescopes, leading to a better understanding of neutron stars, magnetism and fundamental quantum physics. Computer simulations will be developed for the propagation of X-rays through magnetar atmospheres with arbitrary magnetic field orientations, including all locations on the neutron star surface, from magnetic pole to equator. The research includes significant graduate and undergraduate training. A PhD student at Rice University will be integral to the work, with the results leading to a doctoral thesis. Several undergraduates will work on self-contained portions of the research and present their discoveries to senior scientists and peers. The investigators will elucidate aspects of this work, and highlights of the exciting field of neutron stars, to the general public.Magnetars present a unique forum for testing fundamental physics that is not presently accessible in terrestrial laboratories. Better understanding of magnetars is central to using them as a proxy quantum electrodynamics (QED) physics laboratory. The researchers will help enable this by developing a comprehensive theoretical study of the emission from magnetar atmospheres, computing expectations for the polarization- dependent and angle-dependent emissivities at any position on the surface. The generation of polarization signatures will allow discrimination between the geometrical source information and the signatures of strong-field QED physics, like birefringent vacuum polarization. The work will feature upgrades of photospheric cyclotron absorption line physics and photon propagation, providing new tools for astrophysicists to employ in other neutron star problems. The results of this program will enhance potential science yields from polarimetric telescopes in the X-ray band. Four outstanding questions pertaining to magnetars will be significantly impacted by the research. These are (i) are magnetars inherently different from normal pulsars?, (ii) does the magnetic inclination angle of the rotator evolve with magnetar age, and can we measure it so as to more precisely calibrate the stellar field strength?, (iii) where, relative to the magnetic pole, is the site of heating in the surface that seeds quasi- thermal radiation in magnetars?, and (iv) can we use general relativity to determine the mass-to-radius ratio for magnetars, and thereby probe their equations of state?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.