{"total":197,"items":[{"citing_arxiv_id":"2607.01372","ref_index":93,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"AI-enabled gravitational-waves searches for binary neutron stars at optimal sensitivity","primary_cat":"astro-ph.HE","submitted_at":"2026-07-01T18:34:19+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":8.0,"formal_verification":"none","one_line_summary":"Aframe neural network achieves matched-filter sensitivity for binary neutron star GW searches at lower computational cost using heterodyning and a single GPU.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2607.01121","ref_index":4,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Smoking-gun evidence for hierarchical black-hole mergers","primary_cat":"astro-ph.HE","submitted_at":"2026-07-01T16:08:46+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"GWTC-5 population analysis finds high-spin black hole mass function traces low-spin remnant distribution with Bhattacharyya coefficient ~0.95, supporting hierarchical mergers and yielding a nuclear S-factor constraint.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2607.00845","ref_index":4,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Environmental effects vs. modified gravity in the LISA massive black hole binary population","primary_cat":"gr-qc","submitted_at":"2026-07-01T12:11:24+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":4.0,"formal_verification":"none","one_line_summary":"Population-level hierarchical analysis shows environmental effects from circumbinary disks are unlikely to bias LISA tests of general relativity for massive black hole binaries in realistic scenarios.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2607.00565","ref_index":97,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Distinct spin properties and astrophysical origin of low mass binary black holes in gravitational wave data","primary_cat":"astro-ph.HE","submitted_at":"2026-07-01T07:52:30+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"Hierarchical Bayesian analysis of GWTC-5.0 data identifies a mass transition at 15.2 solar masses separating distinct effective-spin distributions, pointing to different formation channels for low-mass binary black holes.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.31531","ref_index":6,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Probing globular clusters parameters through gravitational wave lensing with stellar-mass black hole binaries","primary_cat":"gr-qc","submitted_at":"2026-06-30T11:44:45+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":4.0,"formal_verification":"none","one_line_summary":"Simulations of wave-optics lensing of GW150914-like signals by globular clusters recover injected velocity dispersion values for favorable alignments when lens and source parameters are jointly estimated.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.31362","ref_index":18,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Running into tension: primordial black holes from ultra-slow-roll inflation, spectral running, and the Hubble tension","primary_cat":"astro-ph.CO","submitted_at":"2026-06-30T08:57:18+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"EDE models increase inferred α_s from CMB data, strengthening tension with USR PBH models that predict negative running.","context_count":1,"top_context_role":"background","top_context_polarity":"background","context_text":"Abacet al.(LIGO Scientific, VIRGO, KAGRA), (2025), arXiv:2508.18082 [gr-qc]. [16] R. Abbottet al.(LIGO Scientific, VIRGO, KAGRA), Phys. Rev. Lett.129, 061104 (2022), arXiv:2109.12197 [astro-ph.CO]. [17] R. Abbottet al.(LVK), Mon. Not. Roy. Astron. Soc. 524, 5984 (2023), [Erratum: Mon.Not.Roy.Astron.Soc. 526, 6234 (2023)], arXiv:2212.01477 [astro-ph.HE]. [18] M. Prunier, G. Morr' as, J. F. N. Siles, S. Clesse, J. Garc' ıa-Bellido, and E. Ruiz Morales, Phys. Dark Univ.46, 101582 (2024), arXiv:2311.16085 [gr-qc]. [19] G. Morraset al., Phys. Dark Univ.42, 101285 (2023), arXiv:2301.11619 [gr-qc]. [20] C. Yuan and Q.-G. Huang, JCAP09, 051 (2024), arXiv:2404.03328 [astro-ph.CO]. [21] S. Bird, I. Cholis, J. B."},{"citing_arxiv_id":"2606.31350","ref_index":15,"ref_count":2,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Compactness Inference in Gravitational-Wave Mergers with PhenomDECO: Catalog Benchmarks and Robustness Diagnostics","primary_cat":"gr-qc","submitted_at":"2026-06-30T08:47:30+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":4.0,"formal_verification":"none","one_line_summary":"PhenomDECO analysis of GWTC-3 events finds all considered signals consistent with binary black holes once low-frequency noise effects are addressed via higher starting frequencies.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.31330","ref_index":4,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Two-scalar-field $f(R)$ Thick Branes, Gravitational Resonances and Quasinormal Modes","primary_cat":"hep-th","submitted_at":"2026-06-30T08:32:30+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":4.0,"formal_verification":"none","one_line_summary":"In ghost-free two-scalar f(R) thick branes, internal structure produces no narrow real-axis tensor resonances; quasinormal modes are broad with quality factors 0.9-1.9.","context_count":1,"top_context_role":"background","top_context_polarity":"background","context_text":"X9, 031040 (2019), [arXiv:1811.12907]. [2] R. Abbott et al. (LIGO Scientific, Virgo),GWTC-2: Compact Binary Coalescences Observed by LIGO and Virgo,Phys. Rev. X11, 021053 (2021), [arXiv:2010.14527]. [3] R. Abbott et al. (KAGRA, VIRGO, LIGO Scientific),GWTC-3: Compact Binary Coalescences Observed,Phys. Rev. X13, 041039 (2023), [arXiv:2111.03606]. - 24 - [4] A. G. Abac et al. (LIGO Scientific, VIRGO, KAGRA),GWTC-4.0: Updating the Gravitational-Wave Transient Catalog, [arXiv:2508.18082]. [5] B. P. Abbott et al. (LIGO Scientific, Virgo),Tests of general relativity with GW150914, Phys. Rev. Lett.116, 221101 (2016), [arXiv:1602.03841]. [6] B. P. Abbott et al. (LIGO Scientific, Virgo),Tests of General Relativity with GW170817,"},{"citing_arxiv_id":"2606.30594","ref_index":6,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Efficient Eccentric Effective-One-Body Dynamics via Near-Identity Averaging Transformations","primary_cat":"gr-qc","submitted_at":"2026-06-29T17:35:10+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"Near-identity averaging transformations applied to osculating orbital elements reduce the computational cost of eccentric EOB inspirals by up to two orders of magnitude while maintaining accuracy for moderate to large eccentricities at NNLO.","context_count":1,"top_context_role":"background","top_context_polarity":"background","context_text":"by LIGO and Virgo During the Second Part of the Third Observing Run, arXiv preprint arXiv:2111.03606 (2021), arXiv:2111.03606 [gr-qc]. [5] R. Abbottet al.(KAGRA, VIRGO, LIGO Scientific), GWTC-3: Compact Binary Coalescences Observed by LIGO and Virgo during the Second Part of the Third Observing Run, Phys. Rev. X13, 041039 (2023), arXiv:2111.03606 [gr-qc]. [6] A. G. Abacet al.(LIGO Scientific, VIRGO, KAGRA), GWTC-4.0: Updating the Gravitational-Wave Tran- sient Catalog with Observations from the First Part of the Fourth LIGO-Virgo-KAGRA Observing Run, arXiv preprint arXiv:2508.18082 (2025), arXiv:2508.18082 [gr-qc]. [7] GWTC-5.0: Observations from the Second Part of the Fourth LIGO-Virgo-KAGRA Observing Run"},{"citing_arxiv_id":"2606.30144","ref_index":9,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Joint population and strong-lensing inference for resolved gravitational-wave events probes the black-hole merger rate beyond the peak of star formation","primary_cat":"astro-ph.HE","submitted_at":"2026-06-29T11:21:48+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"Joint strong-lensing and population inference on resolved gravitational-wave events finds no lensed events and tightens constraints on the black-hole merger rate peak redshift and high-redshift tail.","context_count":1,"top_context_role":"dataset","top_context_polarity":"use_dataset","context_text":"rence of lensing in resolved sources [32, 33]. Lensing rate predictions could be improved with knowledge of the source merger population [34], but current constraints from GWs assume no lensing occurs [35, 36]. Therefore, merger-rate constraints implied by nondetection of lens- ing have required inconsistent postprocessing of standard ∗ matthew.mould@nottingham.ac.uk population results [9] and lensing constraints for individ- ual events have assumed fixed population priors [37-41]. Here, this problem is solved by inferring the source population of BH mergers jointly with strong-lensing magnifications of each GW event. The 153 LVK detec- tions through GWTC-4 [8] identified as BH mergers with false-alarm rates (FARs)<1 yr −1 are included, assuming"},{"citing_arxiv_id":"2606.28937","ref_index":10,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Quadrupole and quadratic-in-spin effects in quasicircular, spinning, asymmetric binaries","primary_cat":"gr-qc","submitted_at":"2026-06-27T14:17:05+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":7.0,"formal_verification":"none","one_line_summary":"Calculates energy fluxes with quadratic-in-spin and quadrupole effects for small-mass-ratio spinning binaries in self-force theory, providing numerical data and sixth-order PN expansions.","context_count":1,"top_context_role":"background","top_context_polarity":"background","context_text":"quadrupole with GW241011, (2026), arXiv:2604.09828 [gr-qc]. [8] A. G. Abacet al.(LIGO Scientific, Virgo, KAGRA), GW250114: Testing Hawking's Area Law and the Kerr Nature of Black Holes, Phys. Rev. Lett.135, 111403 (2025), arXiv:2509.08054 [gr-qc]. [9] K. G. Arunet al.(LISA), New horizons for fundamen- tal physics with LISA, Living Rev. Rel.25, 4 (2022), arXiv:2205.01597 [gr-qc]. [10] P. A. Seoaneet al.(LISA), Astrophysics with the Laser Interferometer Space Antenna, Living Rev. Rel.26, 2 (2023), arXiv:2203.06016 [gr-qc]. [11] M. Colpiet al.(LISA), LISA Definition Study Report, (2024), arXiv:2402.07571 [astro-ph.CO]. [12] A. Abacet al.(ET), The Science of the Einstein Tele- scope, JCAP03, 081, arXiv:2503.12263 [gr-qc]. [13] M. Pürrer and C."},{"citing_arxiv_id":"2606.28506","ref_index":1,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Twin Peaks: Resolving Features in the Binary Black Hole Mass Function with COSMIC-METISSE","primary_cat":"astro-ph.HE","submitted_at":"2026-06-26T18:02:39+00:00","verdict":"CONDITIONAL","verdict_confidence":"MODERATE","novelty_score":5.0,"formal_verification":"none","one_line_summary":"New MESA stellar tracks with varied winds and convective mixing produce a primary black hole mass function with twin peaks near 8 and 13 solar masses in most variations, the higher peak dominated by mass-ratio-reversal systems, with rates varying by a factor of six.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.28156","ref_index":12,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Joint inference of line-of-sight acceleration and orbital eccentricity in neutron-star--black-hole binaries","primary_cat":"gr-qc","submitted_at":"2026-06-26T14:52:41+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":7.0,"formal_verification":"none","one_line_summary":"All five NSBH events are consistent with zero line-of-sight acceleration; the joint posterior for GW200105_162426 disfavors both zero LOSA and zero eccentricity at 90% credibility.","context_count":1,"top_context_role":"background","top_context_polarity":"background","context_text":"tronomy is broadening from individual detections to the astro- physical origin of compact-binary mergers [11]. Among the source properties carried by the GW signal, orbital eccentric- ity is a particularly clean discriminator of formation channels. Binaries formed through isolated stellar evolution circularize efficiently via GW emission long before entering the sensitive band of ground-based detectors [12, 13]; by contrast, binaries assembled dynamically can retain measurable eccentricity in the frequency range to which detectors are sensitive [14-25]. Recent years have seen significant progress in modeling eccentric compact-binary signals across the full inspiral- merger-ringdown (IMR) regime. This includes the de- velopment of effective-one-body (EOB) models within the"},{"citing_arxiv_id":"2606.27643","ref_index":1,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"First Demonstration of Optical Feedback Control to Parametric Instability at Advanced LIGO","primary_cat":"gr-qc","submitted_at":"2026-06-26T01:40:14+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":8.0,"formal_verification":"none","one_line_summary":"First demonstration of optical feedback control suppressing parametric instability in a full-scale gravitational-wave detector.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.27037","ref_index":55,"ref_count":2,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Gamma-ray Bursts and Kilonovae from Gravitational Wave Events","primary_cat":"astro-ph.HE","submitted_at":"2026-06-25T13:42:28+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":2.0,"formal_verification":"none","one_line_summary":"Overview of SKAO's role in radio follow-up of GW events, GRB afterglows, and kilonovae for system characterization and population studies.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.25030","ref_index":103,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Formation of Black Hole-White Dwarf X-ray Binaries in Globular Clusters","primary_cat":"astro-ph.HE","submitted_at":"2026-06-23T18:00:04+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"Simulations identify black hole-giant collisions as the main formation channel for ultracompact black hole-white dwarf binaries in globular clusters, with mock catalogs suggesting order-one LISA-detectable sources in the Milky Way.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.23788","ref_index":79,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Red vs. Blue: How metallicity shapes black hole dynamics and mergers in dense star clusters","primary_cat":"astro-ph.GA","submitted_at":"2026-06-22T18:00:02+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":4.0,"formal_verification":"none","one_line_summary":"High-metallicity star cluster simulations produce black hole mergers with masses and ratios consistent with recent LVK detections, unlike low-metallicity models.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.23305","ref_index":9,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"When the black holes align: a subpopulation of aligned massive binary black holes observed via gravitational waves","primary_cat":"astro-ph.HE","submitted_at":"2026-06-22T13:16:40+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":4.0,"formal_verification":"none","one_line_summary":"Non-parametric analysis of GWTC-5.0 data supports multiple subpopulations of binary black holes distinguished by effective spin, with one aligned subpopulation suggesting dynamical formation.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.22580","ref_index":36,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Extended parameterized spin expansion formalism for ringdown analysis with GW250114","primary_cat":"gr-qc","submitted_at":"2026-06-21T16:33:05+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"Extension of parameterized spin expansion formalism samples tilde ell and tilde p for GW250114 ringdown, showing prior-dominated tilde p posteriors and gamma-controlled weak upper bounds on tilde ell of about 83 km.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.22266","ref_index":82,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Fast targeted gravitational-wave followup search for compact binary mergers using GSTLAL pipeline","primary_cat":"astro-ph.HE","submitted_at":"2026-06-20T23:21:24+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":4.0,"formal_verification":"none","one_line_summary":"A targeted gravitational-wave search modifies the GstLAL likelihood ratio with a sky localization prior from EM triggers, showing improved detection efficiency in injection studies while controlling false alarms.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.21076","ref_index":46,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Population-level correlations in Bayesian statistics: an illustrative model for gravitational-wave astronomy","primary_cat":"gr-qc","submitted_at":"2026-06-19T03:55:04+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"An idealized Gaussian model demonstrates that single-event correlations inflate uncertainties in population correlations and that catalog-wide correlated biases can be misread as population correlations.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.19201","ref_index":12,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Impact of the Einstein Telescope's duty cycle on the estimation of binary black holes parameters","primary_cat":"gr-qc","submitted_at":"2026-06-17T15:40:01+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"ET-Δ outperforms ET-2L on luminosity distance and source-frame masses for BBH events because its redundancy produces higher multi-detector uptime under realistic duty-cycle modeling.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.18081","ref_index":179,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"The Chirp-Mass Ladder: A New Rung Emerges","primary_cat":"astro-ph.HE","submitted_at":"2026-06-16T15:45:58+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"The chirp-mass distribution of GW-detected binary black holes shows a ladder of peaks doubling in mass, with a new intermediate peak at 19 solar masses confirming a prior prediction from the hierarchical merger model.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.17765","ref_index":70,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Effective description of lensed gravitational waves diffracted by stellar fields","primary_cat":"astro-ph.HE","submitted_at":"2026-06-16T10:31:05+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":7.0,"formal_verification":"none","one_line_summary":"Authors synthesize SVD-based reduced-order models from wave-optics simulations to provide an effective stochastic description of stellar microlensing distortions on lensed gravitational waves.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.17752","ref_index":2,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Intrinsic handedness in O1-O4a black-hole mergers: probing orbital precession, remnant retention in dense environments and cosmological mirror asymmetry","primary_cat":"gr-qc","submitted_at":"2026-06-16T10:12:59+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"92% of 91 LIGO black hole mergers favor non-zero V_GW, constraining bound remnants to at most 8% and finding no cosmological handedness preference with average near zero.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.17137","ref_index":5,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Improving low-latency multi-messenger follow-up of neutron star-black hole mergers with mode-by-mode filtering","primary_cat":"gr-qc","submitted_at":"2026-06-15T18:00:01+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"Mode-by-mode filtering of higher-order modes enables low-latency marginalization over mode information in NSBH gravitational-wave signals, tightening constraints on distance, inclination, and secondary mass.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.12931","ref_index":14,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Tests of general relativity at the fourth post-Newtonian order with GW230627 and GW250114","primary_cat":"gr-qc","submitted_at":"2026-06-11T05:51:22+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":7.0,"formal_verification":"none","one_line_summary":"Bayesian analysis of GW230627 and GW250114 finds no deviation from GR at 4PN and 4.5PN orders, setting the first empirical baseline with 90% intervals of order O(1)-O(10).","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.12792","ref_index":20,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Identification of Lensed Gravitational-Wave Beat Patterns by LISA","primary_cat":"astro-ph.CO","submitted_at":"2026-06-11T01:23:17+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"Strong lensing of MBHBs produces identifiable beat patterns in about 7% of detectable two-image LISA events, with Bayesian inference recovering time delay and magnification parameters.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.12784","ref_index":1,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Constraining Kerr supermassive black hole properties using gravitational waves from inspiraling stellar-mass binary black holes","primary_cat":"gr-qc","submitted_at":"2026-06-11T00:57:08+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"LISA observations of inspiraling stellar-mass BBHs around SMBHs can achieve relative uncertainties of 10^{-5} for SMBH mass and a few percent for spin in high-SNR cases.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.11705","ref_index":12,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Horizon absorption in eccentric precessing binary black hole inspirals and its importance for gravitational wave data analysis","primary_cat":"gr-qc","submitted_at":"2026-06-10T06:29:17+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":7.0,"formal_verification":"none","one_line_summary":"First leading-PN derivation of horizon absorption in eccentric precessing BBH inspirals, incorporated into pyEFPEHM, with estimates showing parameter biases in eccentric systems at moderate SNR.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.11380","ref_index":11,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Quasinormal modes and tidal responses of black holes in generic anisotropic matter environments","primary_cat":"gr-qc","submitted_at":"2026-06-09T19:04:09+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"A perturbative framework for black holes in anisotropic matter shows quasinormal modes dominated by gravitational redshift while tidal Love numbers exhibit order-unity deviations including vanishing and negative values.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.11294","ref_index":28,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Intermediate States in Chaotic Triple Evolution and Applications to Black Hole Merger Statistics","primary_cat":"astro-ph.HE","submitted_at":"2026-06-09T18:00:01+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"Reduces elliptic triple outcome model to one free parameter, matches N-body simulations except at low angular momentum, and finds observably eccentric merger fractions of 2.6-4.4% in 10^5-10^7 solar mass clusters.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.10823","ref_index":261,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"AGN-driven BBH mergers: Black hole populations and hierarchical 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