Ultralight Bosons Explain the Mass-Spin Correlations in the Merging Binary Black Hole Population
gr-qc, astro-ph.CO, hep-ph
Submitted: 2026-09-02
Updated: 2026-09-02
Terminology
Sources
- Prospects for Observing and Localizing Gravitational-Wave Transients with Advanced LIGO, Advanced Virgo and KAGRA
- GWTC-1: A Gravitational-Wave Transient Catalog of Compact Binary Mergers Observed by LIGO and Virgo during the First and Second Observing Runs
- GWTC-2: Compact Binary Coalescences Observed by LIGO and Virgo During the First Half of the Third Observing Run
- GWTC-2.1: Deep Extended Catalog of Compact Binary Coalescences Observed by LIGO and Virgo During the First Half of the Third Observing Run
- GWTC-3: Compact Binary Coalescences Observed by LIGO and Virgo During the Second Part of the Third Observing Run
- GWTC-5.0: Observations from the Second Part of the Fourth LIGO-Virgo-KAGRA Observing Run and Updates to the Gravitational-Wave Transient Catalog
- Population Properties of Compact Objects from the Second LIGO-Virgo Gravitational-Wave Transient Catalog
- The population of merging compact binaries inferred using gravitational waves through GWTC-3
- Evidence for hierarchical black hole mergers in the second LIGO--Virgo gravitational-wave catalog
- One Channel to Rule Them All? Constraining the Origins of Binary Black Holes using Multiple Formation Pathways
- The properties of merging black holes and neutron stars across cosmic time
- Gravitational-wave detection rates for compact binaries formed in isolation: LIGO/Virgo O3 and beyond
- Impact of Massive Binary Star and Cosmic Evolution on Gravitational Wave Observations II: Double Compact Object Rates and Properties
- The redshift evolution of the binary black hole merger rate: a weighty matter
- GWTC-4.0: Population Properties of Merging Compact Binaries
- GWTC-5.0: Population Properties of Merging Compact Binaries
- Inferring black hole formation channels in GWTC-4.0 via parametric mass-spin correlations derived from first principles
- A subpopulation of low-mass, spinning black holes: signatures of dynamical assembly
- Potential Subpopulations and Assembling Tendency of the Merging Black Holes
- The spin magnitude of stellar-mass binary black holes evolves with the mass: evidence from gravitational wave data
Related papers
- Tests of General Relativity with Einstein Telescope
- Unitary quantum matter-bounce in a universe with a positive cosmological constant
- Quasi-pole quintessential inflation in metric-affine gravity
- Dynamical tidal response of neutron stars: From effective field theory to gravitational waveforms
- Limits of the Rastall--Einstein Equivalence: Matter-Action Compatibility, FLRW Dynamics, and Exceptional Sectors
- Boson star-black hole binaries: initial data and head-on collisions