{"total":13,"items":[{"citing_arxiv_id":"2607.01372","ref_index":15,"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":"2607.00565","ref_index":102,"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":"2607.00539","ref_index":13,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Reference Frames and Gravitational-Wave Polarizations: Symmetry Classification and Preferred-Frame Phenomenology","primary_cat":"gr-qc","submitted_at":"2026-07-01T07:30:19+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"Derives boost transformations for GW polarizations, proposes symmetry classification without preferred frames, and analyzes preferred-frame effects in Bumblebee gravity including novel polarization conversion.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.31531","ref_index":7,"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":"2606.31364","ref_index":14,"ref_count":2,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Establishing Compactness as a Population Observable in Gravitational-Wave Astronomy","primary_cat":"gr-qc","submitted_at":"2026-06-30T08:58:24+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":4.0,"formal_verification":"none","one_line_summary":"Hierarchical analysis of GWTC-3 yields C_eff = 0.5^{+0.3}_{-0.1} consistent with black holes and limits low-compactness exotic binary merger rate to <0.7 Gpc^{-3} yr^{-1}.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.31350","ref_index":16,"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":"2606.28937","ref_index":11,"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":"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.-J. Haster, Gravitational waveform ac- curacy requirements for future ground-based detectors, Phys. Rev. Res.2, 023151 (2020), arXiv:1912."},{"citing_arxiv_id":"2606.23415","ref_index":9,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"High-Stability Deformable Mirrors for Correcting Non-Axisymmetric Residual Aberrations in Thermal Compensation of Future Gravitational Wave Interferometers","primary_cat":"gr-qc","submitted_at":"2026-06-22T14:39:44+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"Deformable mirrors combined with a modified Gerchberg-Saxton algorithm enable reproducible asymmetric intensity patterns for thermal compensation in high-power gravitational wave interferometers, shown via simulations and experiments.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.22580","ref_index":38,"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":"2606.21439","ref_index":18,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Relativistic effects in extreme-mass-ratio inspirals within scalar clouds: Eccentric and inclined orbits","primary_cat":"gr-qc","submitted_at":"2026-06-19T13:59:27+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"Extends relativistic EMRI calculations in scalar clouds from circular-equatorial to eccentric and inclined orbits around Schwarzschild black holes, revealing apsidal-precession resonances and inclination-dependent net energy transfer.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.12792","ref_index":21,"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":"2606.12205","ref_index":1,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Evidence for additional structure in the effective spin distribution hints at multiple formation pathways in GWTC-5.0","primary_cat":"astro-ph.HE","submitted_at":"2026-06-10T15:21:46+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":4.0,"formal_verification":"none","one_line_summary":"GWTC-5.0 analysis finds evidence for structure beyond a non-skewed Gaussian bulk in χ_eff, with suggestive mass-dependent excess of positive over negative spins outside the bulk at 13:1 odds in one mass bin.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.06209","ref_index":9,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"The first decade of gravitational-wave measurements of black hole spins","primary_cat":"gr-qc","submitted_at":"2026-06-04T14:14:46+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":0.0,"formal_verification":"none","one_line_summary":"A review summarizing formation-channel predictions, waveform effects, and population-level constraints on stellar-mass black hole spins from the first decade of gravitational-wave observations.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null}],"limit":50,"offset":0}