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gr-qc2026

Solving Hamiltonian Constraint Equation with Physics-Informed Neural Networks

Yu-Chen Zhou, Hao Ma, Zhoujian Cao +6

Numerical relativity (NR), solving Einstein equation numerically, plays an important role in source modelling for gravitational wave astronomy. Traditional methods for NR including…

gr-qc2026

Constraining Dipole Radiation with Multiband Gravitational Waves from Eccentric Binary Black Holes

Han Wang, Lijing Shao

Dipole-radiation-like deviations from general relativity are most prominent during the early inspiral of compact binaries, making space-ground multiband observations a potential pr…

gr-qc2026

Detecting gravitational wave background with equivalent configurations in the network of space based optical lattice clocks

Mingzhi Lou, Hong Su, Tao Yang +1

This paper studies the use of optical lattice clock (OLC) detector networks for detecting the stochastic gravitational-wave background (SGWB). Starting from the cross-correlation f…

gr-qc2025★ 3 cited

Quasi-Normal Mode Ringing of Binary Black Hole Mergers in Scalar-Gauss-Bonnet Gravity

Zexin Hu, Daniela D. Doneva, Stoytcho S. Yazadjiev +1

Observations of gravitational waves (GWs) generated by binary black hole (BBH) mergers provide us with a powerful way to explore the strong and highly dynamical regime of gravity t…

gr-qc2025

Inferring neutron-star Love-Q relations from gravitational waves in the hierarchical Bayesian framework

Zhihao Zheng, Ziming Wang, Jinwen Deng +2

Despite the large uncertainties in the equation of state for neutron stars (NSs), a tight universal ``Love-Q'' relation exists between their dimensionless tidal deformability, ,…

gr-qc2025★ 100 cited

GW250114: testing Hawking's area law and the Kerr nature of black holes

The LIGO Scientific Collaboration, the Virgo Collaboration, the KAGRA Collaboration +1785

The gravitational-wave signal GW250114 was observed by the two LIGO detectors with a network matched-filter signal-to-noise ratio of 80. The signal was emitted by the coalescence o…

gr-qc2025

Ringdown mode amplitudes of charged binary black holes

Zexin Hu, Daniela D. Doneva, Ziming Wang +4

The ringdown phase of the binary black hole (BBH) merger provides a clean and direct probe of strong-field gravity and tests of the nature of black holes. The quasinormal mode (QNM…

gr-qc2025★ 1 cited

Anatomy of parameter-estimation biases in overlapping gravitational-wave signals: detector network

Ziming Wang, Dicong Liang, Lijing Shao

With the significantly improved sensitivity and a wider frequency band, the next-generation gravitational-wave (GW) detectors are anticipated to detect GW signals per y…

gr-qc2025★ 5 cited

GW230814: investigation of a loud gravitational-wave signal observed with a single detector

The LIGO Scientific Collaboration, The Virgo Collaboration, The Kagra Collaboration +1783

GW230814, detected by the LIGO Livingston observatory with a signal-to-noise ratio of 42.4, represents the loudest gravitational-wave signal in the GWTC-4.0 catalog. Its source is…

gr-qc2025

Lightweight posterior construction for gravitational-wave catalogs with the Kolmogorov-Arnold network

Wenshuai Liu, Yiming Dong, Ziming Wang +1

Neural density estimation has seen widespread applications in the gravitational-wave (GW) data analysis, which enables real-time parameter estimation for compact binary coalescence…

gr-qc2025★ 2 cited

Searching for continuous gravitational waves in the Parkes Pulsar Timing Array Data Release 3

Shi-Yi Zhao, Zu-Cheng Chen, Jacob Cardinal Tremblay +19

We present results from an all-sky search for continuous gravitational waves from individual supermassive binary black holes using the third data release (DR3) of the Parkes Pulsar…

gr-qc2025★ 2 cited

Scalarized neutron stars with a highly relativistic core in scalar-tensor gravity

Peixiang Ji, Lijing Shao

Compact stars in scalar-tensor (ST) gravity have been extensively investigated, but relatively few studies have focused on highly relativistic neutron stars (NSs) with an extremely…

gr-qc2025★ 1 cited

Lunar and Terrestrial Time Transformation Based on the Principle of General Relativity

Min Liu, Jing-Song Ping, Wen-Xiao Li +8

Lunar time metrology necessitates a unified temporal framework beyond Earth, requiring an independent lunar system for timekeeping, dissemination, and calendrics. Recent American p…

gr-qc2025

Identification of Noise-Associated Glitches in KAGRA O3GK with Hveto

T. Akutsu, M. Ando, M. Aoumi +148

Transient noise ("glitches") in gravitational wave detectors can mimic or obscure true signals, significantly reducing detection sensitivity. Identifying and excluding glitch-conta…

gr-qc2025★ 1 cited

Linear analysis of I-C-Love universal relations for neutron stars

Zexin Hu, Yong Gao, Lijing Shao

Neutron stars (NSs) are excellent laboratories for testing gravity theories as they are strongly self-gravitating bodies and have rich observational phenomena. However, strong-fiel…

gr-qc2025★ 1 cited

Bumblebee cosmology: The FLRW solution and the CMB temperature anisotropy

Rui Xu, Dandan Xu, Lars Andersson +2

We put into test the idea of replacing dark energy by a vector field against the cosmic microwave background (CMB) observation using the simplest vector-tensor theory, where a mass…

gr-qc2025★ 2 cited

Rotating Einstein-Maxwell-Dilaton Black Hole as a Particle Accelerator

Muhammad Ali Raza, Sehar, M. Azam +2

Similar to particle accelerators, black holes also have the ability to accelerate particles, generating significant amounts of energy through particle collisions. In this study, we…

gr-qc2025★ 97 cited

The Science of the Einstein Telescope

Adrian Abac, Raul Abramo, Simone Albanesi +485

Einstein Telescope (ET) is the European project for a gravitational-wave (GW) observatory of third-generation. In this paper we present a comprehensive discussion of its science ob…

gr-qc2025★ 2 cited

A practical Bayesian method for gravitational-wave ringdown analysis with multiple modes

Yiming Dong, Ziming Wang, Hai-Tian Wang +2

Gravitational-wave (GW) ringdown signals from black holes (BHs) encode crucial information about the gravitational dynamics in the strong-field regime, which offers unique insights…

gr-qc2025★ 4 cited

Probing Spin-2 Ultralight Dark Matter with Space-based Gravitational Wave Detectors in the mHz Regime

Jing-Rui Zhang, Ju Chen, Heng-Sen Jiao +2

Spin-2 ultralight dark matter (ULDM) is a viable dark matter candidate and it can be constrained using gravitational wave (GW) observations. In this paper, we investigate the detec…

gr-qc2024★ 6 cited

Alternative LISA-TAIJI networks: Detectability of the Parity Violation in Stochastic Gravitational Wave Background

Ju Chen, Chang Liu, Yun-Long Zhang +1

The detection of parity violation in the isotropic stochastic gravitational wave background (SGWB) will serve a crucial probe for new physics, particularly in parity-violating theo…

gr-qc2024★ 4 cited

Constraining inflation with nonminimal derivative coupling with the Parkes Pulsar Timing Array third data release

Chang Han, Li-Yang Chen, Zu-Cheng Chen +13

We study an inflation model with nonminimal derivative coupling that features a coupling between the derivative of the inflaton field and the Einstein tensor. This model naturally…

gr-qc2024★ 7 cited

Some optical properties of rotating wormhole in Bopp-Podolsky electrodynamics

Muhammad Ali Raza, Francisco Tello-Ortiz, M. Zubair +1

In this work, we consider a static wormhole in Bopp-Podolsky electrodynamics and convert it into its rotating counterpart by reducing it into Morris-Thorne form. We further study t…

gr-qc2024★ 9 cited

Reanalyzing the ringdown signal of GW150914 using the F-statistic method

Hai-Tian Wang, Ziming Wang, Yiming Dong +2

The ringdown phase of a gravitational wave (GW) signal from a binary black hole merger provides valuable insights into the properties of the final black hole and serves as a critic…