Extreme-mass-ratio inspirals (EMRIs) will be an important type of astrophysical source for future space-based gravitational-wave detectors. There is a trade-off between accuracy and computational speed for the EMRI waveform templates required in the analysis of data from these detectors. We discuss how the systematic error incurred by using faster templates may be reduced with improved models such as augmented kludge waveforms, and marginalised over with statistical techniques such as Gaussian process regression.
Assessing EMRI Detectability of the Rotating Quantum Oppenheimer-Snyder Black Hole
Center for Gravitation and Cosmology, College of Physical Science and Technology, Yangzhou University（扬州大学物理科学与技术学院引力与宇宙学中心）；Department of Physics, Shanghai University（上海大学物理系）
Observability of gravitational waves excited by binary stars orbiting around a supermassive black hole by space-based gravitational wave observatory
School of Physics and Electronic Information, Weifang University（潍坊学院物理与电子信息学院）；School of Physics and Technology, University of Jinan（济南大学物理科学与技术学院）；School of Physics and Technology, Wuhan University（武汉大学物理科学与技术学院）
Boson Stars in Teleparallel Gravity with a Nonminimally Coupled Field: The Violation of Energy Conditions and Gravitational Waveforms from EMRIs
Lanzhou Center for Theoretical Physics, Key Laboratory of Theoretical Physics of Gansu Province, School of Physical Science and Technology, Lanzhou University（兰州大学物理科学与技术学院）；School of Physical Science and Technology, Southwest University（西南大学物理科学与技术学院）
Extreme Love in the SPA: constraining the tidal deformability of supermassive objects with extreme mass ratio inspirals and semi-analytical, frequency-domain waveforms
Probing the gravity of a Schwarzschild black hole in the presence of a cloud of strings with EMRIs
Harbin Institute of Technology（哈尔滨工业大学）；University of Tashkent for Applied Sciences（塔什干应用科学大学）；Tashkent State Technical University（塔什干国立技术大学）；New Uzbekistan University（新乌兹别克斯坦大学）；National University of Uzbekistan（乌兹别克斯坦国立大学）
Ab uno disce omnes: Single-harmonic search for extreme mass-ratio inspirals
European Space Agency (ESA), European Space Research and Technology Centre (ESTEC)（欧洲空间局（ESA），欧洲空间研究与技术中心（ESTEC））；Universitá degli Studi di Milano-Bicocca（米兰比可卡大学）；INFN, Sezione di Milano-Bicocca（意大利国家核物理研究所，米兰比可卡分校）；University of Birmingham（伯明翰大学）
Waveforms and Fluxes of Generic Extreme-Mass-Ratio Inspirals with a Spinning Secondary
State Key Laboratory of Radio Astronomy and Technology, Shanghai Astronomical Observatory, Chinese Academy of Sciences（中国科学院上海天文台射电天文与技术重点实验室）；School of Astronomy and Space Science, University of Chinese Academy of Sciences（中国科学院大学天文与空间科学学院）；School of Fundamental Physics and Mathematical Sciences, Hangzhou Institute for Advanced Study, UCAS（中国科学院大学杭州高等研究院基础物理与数学学院）；Shanghai Astronomical Observatory, Chinese Academy of Sciences（中国科学院上海天文台）
本文研究了自旋次级物体在 Kerr 背景下的 EMRI 波形与辐射，通过线性自旋近似推导了轨道平均的运动常数方程，为生成包含次级自旋的波形提供了可行路径。
Constraining Lorentz symmetry breaking in bumblebee gravity with extreme mass-ratio inspirals
Hangzhou Institute for Advanced Study, University of Chinese Academy of Sciences（中国科学院大学杭州高等研究院）；Hunan Normal University（湖南师范大学）；Beijing Normal University（北京师范大学）；Yangzhou University（扬州大学）
Chaotic migration of LISA Extreme Mass Ratio Inspirals in a turbulent accretion disk: effect on waveform de-phasing
Center for Cosmology and Particle Physics, Physics Department, New York University（纽约大学物理系宇宙学与粒子物理中心）；Department of Astrophysics, University of Zurich（苏黎世大学天体物理学系）；Shanghai Astronomical Observatory, Chinese Academy of Sciences（中国科学院上海天文台）；National Astronomical Observatory of Japan（日本国立天文台）；Department of Astronomy & Astrophysics, University of California, Santa Cruz（加州大学圣克鲁兹分校天文与天体物理学系）；Institute for Advanced Studies, Tsinghua University（清华大学高等研究院）
Constraint on environments with eccentric extreme-mass-ratio inspirals: Bayesian inference and Fisher-matrix for dark-matter spikes
College of Computer and Big data, Putian University（莆田学院计算机与大数据学院）；Nanchang University（南昌大学）；Center for Relativistic Astrophysics and High Energy Physics, Nanchang University（南昌大学相对论天体物理与高能物理中心）
EMRI Dephasing from a Torsion-Inspired Near-Zone Kerr Deformation: Motivated by Spin-Polarized Dark Matter
Faculty of Physics, Lomonosov Moscow State University（莫斯科国立大学物理系）；International School, I.M. Sechenov First Moscow State Medical University（伊万·谢切诺夫第一莫斯科国立医科大学国际学院）；Steklov Mathematical Institute, Russian Academy of Sciences（俄罗斯科学院斯捷克洛夫数学研究所）
Coherent End-to-End Search for Generic Extreme-Mass-Ratio Inspirals
Hangzhou Institute for Advanced Study, UCAS（杭州高等研究院，中国科学院大学）；Shanghai Astronomical Observatory, Chinese Academy of Sciences（中国科学院上海天文台）；School of Astronomy and Space Science, University of Chinese Academy of Sciences（中国科学院大学天文与空间科学学院）；Department of Physics and Astronomy, The University of Texas Rio Grande Valley（德克萨斯大学里奥格兰德河谷分校物理与天文学系）
Effective-one-body waveforms for extreme-mass-ratio binaries: Consistency with second-order gravitational self-force quasicircular results and extension to nonprecessing spins and eccentricity
Not All Resonances Are Created Equal: Prioritizing Tidal Resonances in EMRIs
Institute for Mathematics, Astrophysics and Particle Physics, Radboud University（拉德堡德大学数学、天体物理与粒子物理研究所）；Faculty of Electrical Engineering, Mathematics and Computer Science, Delft University of Technology（代尔夫特理工大学电气、数学与计算机科学学院）
