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Physical Review D

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Modeling matter in seobnrv5thm: Generating fast and accurate effective-one-body waveforms for spin-aligned binary neutron stars

Marcus Haberland1,*, Alessandra Buonanno1,2,†, and Jan Steinhoff1,‡

  • *Contact author: marcus.haberland@aei.mpg.de
  • †Contact author: alessandra.buonanno@aei.mpg.de
  • ‡Contact author: jan.steinhoff@aei.mpg.de

Gravitational-Wave Signatures of Nonviolent Nonlocality

Brian C. Seymour and Yanbei Chen

Phys. Rev. Lett. 136 011401 (2026)

Investigating the impact of quasiuniversal relations on neutron star constraints in third-generation detectors

Natalie Williams, Anna Puecher, Guilherme Grams, César V. Flores, and Tim Dietrich

Phys. Rev. D 114 024063 (2026)

Difference between quark stars and neutron stars in universal relations and their effect on gravitational waves

Duanyuan Gao, Hao-Jui Kuan, Yurui Zhou, Zhiqiang Miao, Ming-Zhe Han, Yong Gao, Chen Zhang, and Enping Zhou

Phys. Rev. D 114 043058 (2026)

Binary neutron star mergers with a subsolar mass star

Maxence Corman, William E. East, and Jocelyn S. Read

Phys. Rev. D 114 063040 (2026)

Quadrupole and quadratic-in-spin effects in quasicircular, spinning, asymmetric binaries

Mostafizur Rahman, Misbah Shahzadi, Adam Pound, and Josh Mathews

Phys. Rev. D 114 064034 (2026)

Relativistic mode sums for neutron-star tidal response

Abhishek Hegade K. R., K. J. Kwon, Tejaswi Venumadhav, Hang Yu, and Nicolas Yunes

Phys. Rev. D 114 064048 (2026)

Adiabatic tides in compact binaries on quasielliptic orbits: Dynamics at the second-and-a-half relative post-Newtonian order

Quentin Henry and Anna Heffernan

Phys. Rev. D 114 064061 (2026)

Adiabatic tides in compact binaries on quasielliptic orbits: Radiation at the second-and-a-half relative post-Newtonian order

Quentin Henry

Phys. Rev. D 114 064062 (2026)

Accurate waveforms for generic planar-orbit binary black holes: The multipolar effective-one-body model SEOBNRv6EHM

Aldo Gamboa, Alessandra Buonanno, Lorenzo Pompili, Raffi Enficiaud, Michael Boyle, Lawrence E. Kidder, Oliver Long, Peter James Nee, Harald P. Pfeiffer, Antoni Ramos-Buades, and Mark A. Scheel

Phys. Rev. D 114 104010 (2026)

Adding equatorial-asymmetric effects for spin-precessing binaries into the seobnrv5phm waveform model

Héctor Estellés, Alessandra Buonanno, Raffi Enficiaud, Cheng Foo, and Lorenzo Pompili

Phys. Rev. D 113 044049 (2026)

Orbital eccentricity can make neutron star g -mode resonances observable with current gravitational-wave detectors

János Takátsy, Lorenz Zwick, Pankaj Saini, and Johan Samsing

Phys. Rev. D 113 103047 (2026)

Nonlinear relativistic tidal response of neutron stars

Paolo Pani, Massimiliano Maria Riva, Luca Santoni, Nikola Savić, and Filippo Vernizzi

J. High Energ. Phys. 2026 74 (2026)

GR-Athena++ simulations of spinning binary black hole mergers

Estuti Shukla, Alireza Rashti, Rossella Gamba, David Radice, and Koustav Chandra

Class. Quantum Grav. 43 065019 (2026)

Impact on inferred neutron star equation of state due to nonlinear hydrodynamics, background spin, and relativity

Joseph Bretz and Hang Yu

Class. Quantum Grav. 43 125011 (2026)

Eccentricity Constraints Disfavor Single–Single Capture in Nuclear Star Clusters as the Origin of all LIGO–Virgo–KAGRA Binary Black Holes

Nihar Gupte, M. Coleman Miller, Rhiannon Udall, Sophie Bini, Alexandre Toubiana, Alessandra Buonanno, Jonathan Gair, Aldo Gamboa, Lorenzo Pompili, Antoni Ramos-Buades, Maximilian Dax, Stephen R. Green, Annalena Kofler, Jakob Macke, and Bernhard Schölkopf

ApJ 1009 90 (2026)

Leveraging NRTidalv3 to develop gravitational waveform models with higher-order modes for binary neutron star systems

Adrian Abac, Felip A. Ramis Vidal, Marta Colleoni, Anna Puecher, Alejandra Gonzalez, and Tim Dietrich

Phys. Rev. D 112 104026 (2025)

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