{"total":10,"items":[{"citing_arxiv_id":"2607.00845","ref_index":15,"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":"2606.29039","ref_index":13,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Neural posterior estimation of Galactic Binary signals for the LISA mission","primary_cat":"astro-ph.IM","submitted_at":"2026-06-27T18:20:00+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"Conditional normalizing flows perform likelihood-free parameter estimation for single and overlapping LISA galactic binaries, generating thousands of posterior samples per second after training on simulations.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2605.28658","ref_index":57,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Measuring the Hubble constant with strongly lensed gravitational waves from space-based detector networks","primary_cat":"astro-ph.CO","submitted_at":"2026-05-27T15:57:34+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":4.0,"formal_verification":"none","one_line_summary":"Simulations indicate joint Taiji+LISA analysis of five SLGW events yields H0 95% credible interval uncertainties of 0.11 (source redshift unknown) or 0.042 (source redshift known).","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2605.15265","ref_index":72,"ref_count":2,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Eccentric Stellar-mass Binary Black Holes: Population, Detectability, and Waveform Analysis in the LISA and LIGO Era","primary_cat":"astro-ph.HE","submitted_at":"2026-05-14T18:00:00+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"Simulations of dynamical channels predict ~36 eccentric stellar-mass BBHs detectable by LISA in the Milky Way at SNR>1 over 10 years, a local merger rate of ~9 Gpc^{-3} yr^{-1}, and hundreds of faint extragalactic mHz sources.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2605.14078","ref_index":27,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Properties of natural polynomials for Schwarzschild and Kerr black holes","primary_cat":"gr-qc","submitted_at":"2026-05-13T20:01:38+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":7.0,"formal_verification":"none","one_line_summary":"Natural polynomials for Schwarzschild and Kerr quasinormal modes are Pollaczek-Jacobi polynomials with complex parameters, with recurrence peaking at the physical overtone index for Schwarzschild.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2604.13867","ref_index":38,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Robust parameter inference for Taiji via time-frequency contrastive learning and normalizing flows","primary_cat":"gr-qc","submitted_at":"2026-04-15T13:30:09+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"A glitch-robust amortized inference framework combining normalizing flows, time-frequency multimodal fusion, and contrastive learning outperforms MCMC for Taiji massive black hole binary parameter estimation under noise contamination.","context_count":1,"top_context_role":"background","top_context_polarity":"background","context_text":"[34] Y.-N. Du, J.-Y. Song, Y. Li, S.-J. Jin, L.-F. Wang, J.-F. Zhang, and X. Zhang, (2025), arXiv:2510.21521 [astro- ph.CO]. [35] P. Amaro-Seoaneet al.(LISA), (2017), arXiv:1702.00786 [astro-ph.IM]. [36] J. Luoet al.(TianQin), Class. Quant. Grav.33, 035010 (2016), arXiv:1512.02076 [astro-ph.IM]. [37] W.-R. Hu and Y.-L. Wu, Natl. Sci. Rev.4, 685 (2017). [38] A. Kleinet al., Phys. Rev. D93, 024003 (2016), arXiv:1511.05581 [gr-qc]. [39] L.-F. Wang, Z.-W. Zhao, J.-F. Zhang, and X. Zhang, JCAP11, 012 (2020), arXiv:1907.01838 [astro-ph.CO]. [40] Z.-W. Zhao, L.-F. Wang, J.-F. Zhang, and X. Zhang, Sci. Bull.65, 1340 (2020), arXiv:1912.11629 [astro- ph.CO]. [41] L.-F. Wang, S.-J. Jin, J.-F. Zhang, and X. Zhang,"},{"citing_arxiv_id":"2603.23634","ref_index":109,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Testing Dark Energy with Black Hole Ringdown","primary_cat":"gr-qc","submitted_at":"2026-03-24T18:20:49+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":7.0,"formal_verification":"none","one_line_summary":"Dynamical dark energy imprints O(1) shifts on black hole quasi-normal modes via cosmological hair, enabling constraints at 10^{-2} (LVK) to 10^{-4} (LISA) precision using the cubic Galileon as example.","context_count":1,"top_context_role":"background","top_context_polarity":"background","context_text":"[107] C. Shi, Q. Zhang, and J. Mei, \"Detectability and resolvability of quasinormal modes with space-based gravitational wave detectors,\"Phys. Rev. D110(2024) no. 12, 124007, arXiv:2407.13110 [gr-qc]. [108] S. A. Hughes and K. Menou, \"Golden binaries for LISA: Robust probes of strong-field gravity,\"Astrophys. J.623 (2005) 689-699,arXiv:astro-ph/0410148. [109] A. Ghoshet al., \"Testing general relativity using golden black-hole binaries,\"Phys. Rev. D94(2016) no. 2, 021101, arXiv:1602.02453 [gr-qc]. [110] A. Ghosh, N. K. Johnson-Mcdaniel, A. Ghosh, C. K. Mishra, P. Ajith, W. Del Pozzo, C. P. L. Berry, A. B. Nielsen, and L. London, \"Testing general relativity using gravitational wave signals from the inspiral, merger and ringdown of"},{"citing_arxiv_id":"2507.04471","ref_index":8,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"A multi-parameter expansion for the evolution of asymmetric binaries in astrophysical environments","primary_cat":"gr-qc","submitted_at":"2025-07-06T17:20:14+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"A multi-parameter formalism is developed to describe asymmetric binaries in general matter distributions by perturbing around Schwarzschild and reducing metric and fluid perturbations to wave equations similar to the vacuum case.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2311.01300","ref_index":32,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Waveform Modelling for the Laser Interferometer Space Antenna","primary_cat":"gr-qc","submitted_at":"2023-11-02T15:15:33+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":2.0,"formal_verification":"none","one_line_summary":"A review of existing waveform models for LISA sources and the challenges that must still be overcome.","context_count":1,"top_context_role":"background","top_context_polarity":"background","context_text":"• Eccentricity may be very significant and evolving in the LISA window ( e > 0.9 upon entrance into the LISA band and up to 0.1 at plunge) if triple/quadruple MBH interactions are more efficient than gas and stellar interactions to drive the binary's evolution at ∼pc scales [48]. • Event rates and SNRs can vary significantly according to the underpinning astrophysical model [32, 33, 53]: in light seed scenarios rates may be as low as a few per year, especially if feedback from supernova explosions is included [33], which results in most events having small total masses and thus low SNRs (below 100). More generally, the number of light seed detections may be threshold limited [33, 48]. This is again especially true if supernova feedback is included,"},{"citing_arxiv_id":"1907.02283","ref_index":12,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Eccentricity Without Measuring Eccentricity: Discriminating Among Stellar Mass Black Hole Binary Formation Channels","primary_cat":"astro-ph.HE","submitted_at":"2019-07-04T09:00:51+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"Eccentricity influences LISA binary counts via peak frequency, required density for LIGO rate match, and SNR reduction, enabling formation channel discrimination through frequency-dependent number counts without direct eccentricity measurement.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null}],"limit":50,"offset":0}