Image de couverture de livre

Phenomenological model of gravitational self-force enhanced tides in inspiralling binary neutron stars

Fuente: arXiv

Enregistré dans:

Détails bibliographiques
Auteurs principaux:	Williams, Natalie, Schmidt, Patricia, Pratten, Geraint
Format:	Preprint
Publié:	2024
Sujets:	General Relativity and Quantum Cosmology High Energy Astrophysical Phenomena
Accès en ligne:	Acceder al recurso
Tags:	Ajouter un tag Pas de tags, Soyez le premier à ajouter un tag!

Documents similaires

Improved post-Newtonian waveform model for inspiralling precessing-eccentric compact binaries
par: Morras, Gonzalo, et autres
Publié: (2025)

Impact of eccentricity on the population properties of neutron star - black hole mergers
par: Morras, Gonzalo, et autres
Publié: (2026)

Orbital eccentricity in a neutron star - black hole merger
par: Morras, Gonzalo, et autres
Publié: (2025)

Post-Newtonian inspiral waveform model for eccentric precessing binaries with higher-order modes and matter effects
par: Morras, Gonzalo, et autres
Publié: (2026)

New gravitational waveform model for precessing binary neutron stars with double-spin effects
par: Colleoni, Marta, et autres
Publié: (2023)

Fast neural network surrogate for multimodal effective-one-body gravitational waveforms from generically precessing compact binaries
par: Whittall, Christopher, et autres
Publié: (2026)

A geometric template bank for the detection of spinning low-mass compact binaries with moderate orbital eccentricity
par: Phukon, Khun Sang, et autres
Publié: (2024)

Interface modes in inspiralling neutron stars: A gravitational-wave probe of first-order phase transitions
par: Counsell, A. R., et autres
Publié: (2025)

Probing internal dissipative processes of neutron stars with gravitational waves during the inspiral of neutron star binaries
par: Ripley, Justin L., et autres
Publié: (2023)

Occurrence of gravitational collapse in the accreting neutron stars of binary-driven hypernovae
par: Becerra, L. M., et autres
Publié: (2024)

The impact of selection biases on tests of general relativity with gravitational-wave inspirals
par: Magee, Ryan, et autres
Publié: (2023)

Long-lived neutron-star remnants from asymmetric binary neutron star mergers: element formation, kilonova signals and gravitational waves
par: Bernuzzi, Sebastiano, et autres
Publié: (2024)

Leveraging NRTidalv3 to develop gravitational waveform models with higher-order modes for binary neutron star systems
par: Abac, Adrian, et autres
Publié: (2025)

Probing missing physics from inspiralling compact binaries via time-frequency tracks
par: Das, Debtroy, et autres
Publié: (2025)

Postmerger: a new and dominant contribution to the gravitational-wave background from binary neutron stars
par: Lehoucq, Léonard, et autres
Publié: (2025)

Black hole-neutron star binaries
par: Duez, Matthew D.
Publié: (2024)

Towards high-precision inspiral gravitational waveforms from binary neutron star mergers in numerical relativity
par: Kiuchi, Kenta
Publié: (2025)

Effect of spin in binary neutron star mergers
par: Karakas, Beyhan, et autres
Publié: (2024)

Stars or gas? Constraining the hardening processes of massive black-hole binaries with LISA
par: Spadaro, Alice, et autres
Publié: (2024)

Inferring binary parameters with dual-line gravitational wave detection from tight inspiraling double neutron stars
par: Feng, Wen-Fan, et autres
Publié: (2024)

Effects of orbital eccentricity on continuous gravitational waveforms from triaxially deformed precessing neutron stars in tight binaries
par: Feng, Wen-Fan, et autres
Publié: (2024)

Observing binary neutron star subpopulations with the Einstein Telescope
par: Toubiana, Alexandre, et autres
Publié: (2025)

Wide parameter-space O3 search for continuous gravitational waves from unknown neutron stars in binary systems
par: Covas, P. B., et autres
Publié: (2026)

Identifying the hosts of binary black hole and neutron star-black hole mergers with next-generation gravitational-wave detectors
par: Mo, Geoffrey, et autres
Publié: (2024)

Detectability of QCD phase transitions in binary neutron star mergers: Bayesian inference with the next generation gravitational wave detectors
par: Prakash, Aviral, et autres
Publié: (2023)

Investigating the impact of quasi-universal relations on neutron star constraints in third-generation detectors
par: Williams, Natalie, et autres
Publié: (2026)

Black hole perturbation theory and gravitational self-force
par: Pound, Adam, et autres
Publié: (2021)

A unified study of nuclear physics and dark matter constraints through gravitational-wave observations of binary neutron star mergers
par: Kunert, Nina, et autres
Publié: (2026)

General relativistic magnetohydrodynamics simulations for binary neutron star mergers
par: Kiuchi, Kenta
Publié: (2024)

Difference between quark stars and neutron stars in universal relations and their effect on gravitational waves
par: Gao, Duanyuan, et autres
Publié: (2025)

Disk mass predictions for binary neutron star mergers: limitations of proposed symbolic regression models
par: Foucart, Francois
Publié: (2025)

The anisotropy and magnetic field structure of neutron stars through gravitational wave
par: Du, Zhao-Wei, et autres
Publié: (2025)

Possible binary neutron star merger history of the primary of GW230529
par: Mahapatra, Parthapratim, et autres
Publié: (2025)

Challenging a binary neutron star merger interpretation of GW230529
par: Markin, Ivan, et autres
Publié: (2025)

Jetlike structures in low-mass binary neutron star merger remnants
par: Bamber, Jamie, et autres
Publié: (2024)

Cocoon shock breakout emission from binary neutron star mergers
par: Gutiérrez, Eduardo M., et autres
Publié: (2024)

A machine-learning classifier for the postmerger remnant of binary neutron stars
par: Puecher, Anna, et autres
Publié: (2024)

Detection possibility of continuous gravitational waves from rotating magnetized neutron stars
par: Das, Mayusree, et autres
Publié: (2023)

Tests of General Relativity with GW230529: a neutron star merging with a lower mass-gap compact object
par: Sänger, Elise M., et autres
Publié: (2024)

The error budget of binary neutron star merger simulations for configurations with high spin
par: Kuan, Hao-Jui, et autres
Publié: (2025)