Black hole binaries in shift-symmetric Einstein-scalar-Gauss-Bonnet gravity experience a slower merger phase
gr-qc, astro-ph.HE, hep-ph
Submitted: 2025-11-24
Updated: 2026-09-25
Terminology
Sources
- New Horizons for Fundamental Physics with LISA
- Bounding Alternative Theories of Gravity with Multi-Band GW Observations
- Black holes, gravitational waves and fundamental physics: a roadmap
- Open Data from LIGO, Virgo, and KAGRA through the First Part of the Fourth Observing Run
- Directional Search for Persistent Gravitational Waves: Results from the First Part of LIGO-Virgo-KAGRA's Fourth Observing Run
- Laser Interferometer Space Antenna
- Science Case for the Einstein Telescope
- Cosmic Explorer: The U.S. Contribution to Gravitational-Wave Astronomy beyond LIGO
- Linking Tests of Gravity On All Scales: from the Strong-Field Regime to Cosmology
- Tests of General Relativity with the Binary Black Hole Signals from the LIGO-Virgo Catalog GWTC-1
- Tests of General Relativity with Binary Black Holes from the second LIGO-Virgo Gravitational-Wave Transient Catalog
- Tests of General Relativity with GWTC-3
- Black Hole Spectroscopy and Tests of General Relativity with GW250114
- GW250114: testing Hawking's area law and the Kerr nature of black holes
- Positivity Bounds for Scalar Theories
- Causality Constraints on Gravitational Effective Field Theories
- Causal Effective Field Theories
- Positivity-causality competition: a road to ultimate EFT consistency constraints
- Effective Field Theory for Inflation
- Dilatonic Black Holes in Higher Curvature String Gravity
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