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20242026
most citedGW241011 and GW241110: Exploring Binary Formation and Fundamental Physics with Asymmetric, High-Spin Black Hole Coalescence

34 citations · 110 across the 16 of their papers we have counts for

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13 papers · 1 filter

astro-ph.HE2026

Dynamical pairing in gravitational wave populations

Fabio Antonini, Aleksandra Olejak, Isobel Romero-Shaw +1

Binary black holes formed dynamically in star clusters are often associated with nearly equal-mass pairing. We show that this expectation is incomplete. The more general prediction…

astro-ph.HE2026

Distinct spin properties and astrophysical origin of low mass binary black holes in gravitational wave data

Elizabeth Flanagan, Jakob Stegmann, Isobel Romero-Shaw +3

We analyze the effective-spin distribution of binary black hole mergers in GWTC-5.0 as a function of primary black hole mass using hierarchical Bayesian inference. We model the pop…

astro-ph.HE2026

GWTC-5.0: Population Properties of Merging Compact Binaries

The LIGO Scientific Collaboration, the Virgo Collaboration, the KAGRA Collaboration +1813

We present the population properties of merging compact binaries inferred using 267 mergers from the cumulative Gravitational-Wave Transient Catalog 5.0. As this data set contains…

astro-ph.HE2026

Transitions in the Mass-ratio and Spin Properties of Binary Black Holes in GWTC-5

Elizabeth Flanagan, Fabio Antonini, Thomas Callister +4

We analyze the mass-ratio and effective-spin () distributions of binary black hole mergers in the latest gravitational-wave catalog, GWTC-5, as a function of primary m…

astro-ph.HE2026

Second-Generation Mass Peak in the Gravitational-Wave Population as a Probe of Globular Clusters

Yonadav Barry Ginat, Fabio Antonini, Elizabeth Flanagan +1

Gravitational-wave observations have revealed an excess of binary black hole mergers with primary masses near . We show that if this feature originates from dynam…

astro-ph.HE2026

Repopulating the pair-instability mass gap without sustained growth to massive IMBHs: the case of 47\,Tuc

Debatri Chattopadhyay, Daniel Marín Pina, Mark Gieles +2

We model the formation and retention of the most massive black hole (BH) in 47~Tuc using the semi-analytical code \texttt{cBHBd}, coupling cluster evolution with binary BH dynamics…

astro-ph.HE2025★ 12 cited

Gravitational-wave Observations Suggest Most Black Hole Mergers Form in Triples

Jakob Stegmann, Fabio Antonini, Aleksandra Olejak +4

The spin-orbit tilt angles of merging stellar-mass black holes provide key insights into their astrophysical origin. Non-parametric population modelling of The LIGO, Vir…

astro-ph.HE2025★ 34 cited

GW241011 and GW241110: Exploring Binary Formation and Fundamental Physics with Asymmetric, High-Spin Black Hole Coalescence

The LIGO Scientific Collaboration, the Virgo Collaboration, the KAGRA Collaboration +1783

We report the observation of gravitational waves from two binary black hole coalescences during the fourth observing run of the LIGO--Virgo--KAGRA detector network, GW241011 and GW…

astro-ph.HE2025★ 1 cited

Gravitational-wave constraints on the pair-instability mass gap and nuclear burning in massive stars

Fabio Antonini, Isobel Romero-Shaw, Thomas Callister +5

Pair-instability should prevent the direct formation of black holes above about creating a pair-instability mass gap. Yet gravitational-wave observations have detected…

astro-ph.HE2025

Inferring the pair-instability mass gap from gravitational wave data

Fabio Antonini, Thomas Callister, Fani Dosopoulou +2

We use hierarchical Bayesian inference with non-parametric Gaussian process models to investigate the effective inspiral spin parameter, , as a function of primary bla…

astro-ph.HE2025★ 14 cited

Possible binary neutron star merger history of the primary of GW230529

Parthapratim Mahapatra, Debatri Chattopadhyay, Anuradha Gupta +4

Black holes (BHs) with masses between , produced by a binary neutron star (BNS) merger, can further pair up with a neutron star or BH and merge again within a Hu…

astro-ph.HE2024★ 5 cited

The Impact of Astrophysical Priors on Parameter Inference for GW230529

Debatri Chattopadhyay, Sama Al-Shammari, Fabio Antonini +3

We investigate the effects of prior selection on the inferred mass and spin parameters of the neutron star-black hole merger GW230529\_181500. Specifically, we explore models motiv…

astro-ph.HE2024★ 28 cited

Reconstructing the Genealogy of LIGO-Virgo Black Holes

Parthapratim Mahapatra, Debatri Chattopadhyay, Anuradha Gupta +4

We propose a Bayesian inference framework to predict the merger history of LIGO-Virgo binary black holes (BHs), whose binary components may have undergone hierarchical mergers in t…