{"total":17,"items":[{"citing_arxiv_id":"2606.27429","ref_index":48,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Massive scalar fields in eccentric regime: Detectability and constraints from LISA observations of extreme mass-ratio inspirals","primary_cat":"gr-qc","submitted_at":"2026-06-25T18:00:07+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"Computes scalar and tensor fluxes for eccentric EMRIs with massive scalars, quantifies dephasing, and shows via Fisher matrix that LISA can constrain scalar charge and mass.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.23021","ref_index":29,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Periodic Timelike Motion and Gravitational Wave Signatures around a Magnetically Charged Black Hole Surrounded by Quintessence","primary_cat":"gr-qc","submitted_at":"2026-06-22T08:34:40+00:00","verdict":"CONDITIONAL","verdict_confidence":"MODERATE","novelty_score":4.0,"formal_verification":"none","one_line_summary":"Quintessence parameter cq systematically shifts zoom-whirl periodic orbits and their numerical-kludge EMRI waveforms around a magnetically charged nonlinear-electrodynamics black hole into the LISA millihertz band.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.21439","ref_index":30,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"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":"2606.11728","ref_index":85,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Periodic orbits as probes of charged loop quantum gravity black holes through gravitational waves","primary_cat":"gr-qc","submitted_at":"2026-06-10T07:06:19+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"Periodic orbits in charged LQG black holes produce zoom-whirl gravitational waveforms detectable by future space-based observatories, with features depending on the fixed polymerization parameter.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.06478","ref_index":28,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Short Gravitational-Wave Transients as Probes of Cosmic Domain Walls","primary_cat":"gr-qc","submitted_at":"2026-06-04T17:57:18+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"Two LIGO transients are consistent with domain wall signals from a shared scalar field but binary black hole models remain favored, with a morphological degeneracy identified.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2605.25625","ref_index":48,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Periodic orbits and gravitational waveforms around a Schwarzschild black hole with a cloud of strings embedded in perfect fluid dark matter","primary_cat":"gr-qc","submitted_at":"2026-05-25T09:28:15+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"Analysis of how string cloud parameter a and dark matter parameter α alter MBO, ISCO, periodic orbits indexed by q, and the gravitational waveforms generated by those orbits in a modified Schwarzschild spacetime.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2605.15330","ref_index":33,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"A metric solution for rotating black holes embedded in dark matter halos with central spikes","primary_cat":"gr-qc","submitted_at":"2026-05-14T18:51:56+00:00","verdict":"REJECT","verdict_confidence":"HIGH","novelty_score":6.0,"formal_verification":"none","one_line_summary":"A rotating black-hole metric with a dark-matter halo is derived, but the proposed halo profiles do not make the spacetime asymptotically flat as claimed.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2605.09250","ref_index":32,"ref_count":3,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Efficient and Stable Computation of Gravitational-Wave Fluxes from Generic Kerr Orbits via a Unified HeunC Framework","primary_cat":"gr-qc","submitted_at":"2026-05-10T01:28:01+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"A HeunC framework computes gravitational-wave fluxes from generic Kerr orbits with 10^{-11} relative errors and speedups of 3-60x over prior packages by eliminating auxiliary parameters via analytic continuation and adaptive quadrature.","context_count":1,"top_context_role":"background","top_context_polarity":"background","context_text":"and science applications of intermediate- and extreme mass- ratio inspirals, Classical Quantum Gravity24, R113 (2007), arXiv:astro-ph/0703495. [31] C. L. MacLeod and C. J. Hogan, Precision of Hubble constant derived using black hole binary absolute distances and statis- tical redshift information, Phys. Rev. D77, 043512 (2008), arXiv:0712.0618 [astro-ph]. [32] D. Laghi, N. Tamanini, W. Del Pozzo, A. Sesana, J. Gair, S. Babak, and D. Izquierdo-Villalba, Gravitational-wave cos- mology with extreme mass-ratio inspirals, Mon. Not. Roy. As- tron. Soc.508, 4512 (2021), arXiv:2102.01708 [astro-ph.CO]. [33] P. Auclairet al.(LISA Cosmology Working Group), Cosmol- ogy with the Laser Interferometer Space Antenna, Living Rev."},{"citing_arxiv_id":"2605.07187","ref_index":13,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Probing Gravitational Wave Signatures from Periodic Orbits of Regular Black Holes in Asymptotically Safe Gravity","primary_cat":"gr-qc","submitted_at":"2026-05-08T03:32:12+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":4.0,"formal_verification":"none","one_line_summary":"The quantum parameter ξ in an asymptotically safe regular black hole shifts the innermost stable orbit, enhances whirl behavior in periodic geodesics, and produces amplitude-modulated millihertz gravitational-wave strains whose peak amplitude grows with ξ, placing them inside the sensitivity bands预计","context_count":1,"top_context_role":"background","top_context_polarity":"background","context_text":"Danzmann, Class. Quant. Grav.14, 1399 (1997). [10] B. F. Schutz, Class. Quant. Grav.16, A131 (1999), arXiv:gr-qc/9911034. [11] J. R. Gair, L. Barack, T. Creighton, C. Cutler, S. L. Larson, E. S. Phinney, and M. Vallisneri, Class. Quant. Grav.21, S1595 (2004), arXiv:gr-qc/0405137. [12] P. Amaro-Seoaneet al.(LISA), (2017), arXiv:1702.00786 [astro-ph.IM]. [13] A. Maselli, N. Franchini, L. Gualtieri, T. P. Sotiriou, S. Barsanti, and P. Pani, Nature Astron.6, 464 (2022), arXiv:2106.11325 [gr-qc]. [14] W.-R. Hu and Y.-L. Wu, Natl. Sci. Rev.4, 685 (2017). [15] J. Luoet al.(TianQin), Class. Quant. Grav.33, 035010 (2016), arXiv:1512.02076 [astro-ph.IM]. [16] Y. Gong, J. Luo, and B. Wang, Nature Astron.5, 881"},{"citing_arxiv_id":"2604.13614","ref_index":86,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Scalarizations of magnetized Reissner-Nordstr\\\"om black holes induced by parity-violating and parity-preserving interactions","primary_cat":"gr-qc","submitted_at":"2026-04-15T08:27:26+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"Magnetic fields lower the scalarization threshold for electromagnetic and gravitational Chern-Simons couplings but produce opposite trends on the two Gauss-Bonnet branches, with nonlinear terms converting exponential growth into bounded oscillations.","context_count":1,"top_context_role":"background","top_context_polarity":"background","context_text":"the Supermassive Black Hole,\" Astrophys. J. Lett.875, L1 (2019) [arXiv:1906.11238 [astro-ph.GA]]. [85] A. Maselli, N. Franchini, L. Gualtieri, T. P. Sotiriou, S. Barsanti and P. Pani, \"Detecting fundamental fields with LISA observations of gravitational waves from ex- treme mass-ratio inspirals,\" Nature Astron.6, no.4, 464-470 (2022) [arXiv:2106.11325 [gr-qc]]. [86] K. Akiyamaet al.[Event Horizon Telescope], \"First Sagittarius A* Event Horizon Telescope Results. I. The Shadow of the Supermassive Black Hole in the Center of the Milky Way,\" Astrophys. J. Lett.930, no.2, L12 (2022) [arXiv:2311.08680 [astro-ph.HE]]. [87] K. Bronnikov, N. O. Santos and A. Wang, \"Cylindrical Systems in General Relativity,\" Class. Quant."},{"citing_arxiv_id":"2604.06053","ref_index":142,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Probing Kerr Symmetry Breaking with LISA Extreme-Mass-Ratio Inspirals","primary_cat":"gr-qc","submitted_at":"2026-04-07T16:41:35+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"LISA EMRIs can constrain deviations from Kerr equatorial symmetry to 10^{-2} and axial symmetry to 10^{-3} using Analytic Kludge waveforms and Fisher analysis.","context_count":1,"top_context_role":"background","top_context_polarity":"background","context_text":"Singh, A. Chowdhuri, and A. Bhat- tacharyya, Exploring waveforms with non-GR devia- tions for extreme mass-ratio inspirals, JCAP10, 047, arXiv:2405.18508 [gr-qc]. [141] A. Maselli, N. Franchini, L. Gualtieri, and T. P. Sotiriou, Detecting scalar fields with Extreme Mass Ratio Inspirals, Phys. Rev. Lett.125, 141101 (2020), arXiv:2004.11895 [gr-qc]. [142] A. Maselli, N. Franchini, L. Gualtieri, T. P. Sotiriou, S. Barsanti, and P. Pani, Detecting fundamental fields with LISA observations of gravitational waves from extreme mass-ratio inspirals, Nature Astron.6, 464 (2022), arXiv:2106.11325 [gr-qc]. [143] M. Della Rocca, S. Barsanti, L. Gualtieri, and A. Maselli, Extreme mass-ratio inspirals as probes"},{"citing_arxiv_id":"2603.25084","ref_index":96,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Particle motions and gravitational waveforms in rotating black hole spacetimes of loop quantum gravity","primary_cat":"gr-qc","submitted_at":"2026-03-26T06:38:36+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"The LQG parameter ξ enlarges equatorial bound orbit energy ranges, confines off-equatorial trajectories, and produces larger deviations from Kerr waveforms in EMRI models for two rotating LQG black holes, though signals fall below detector sensitivities.","context_count":1,"top_context_role":"background","top_context_polarity":"background","context_text":"Babak, H. Fang, J. R. Gair, K. Glampedakis, and S. A. Hughes, 'Kludge' gravitational waveforms for a test-body orbiting a Kerr black hole, Phys. Rev. D 75, 024005 (2007), [Erratum: Phys.Rev.D 77, 04990 (2008)], arXiv:gr-qc/0607007. [95] E. Poisson and C. M. Will, Gravity: Newtonian, Post-Newtonian, Relativistic (Cambridge University Press, 2014). [96] A. J. K. Chua, C. J. Moore, and J. R. Gair, Aug- mented kludge waveforms for detecting extreme-mass- ratio inspirals, Phys. Rev. D96, 044005 (2017), arXiv:1705.04259 [gr-qc]. [97] J. D. E. Creighton and W. G. Anderson, Gravitational-wave physics and astronomy: An introduction to theory, experiment and data analysis (Wiley-VCH, Berlin, 2011). [98] L."},{"citing_arxiv_id":"2601.02904","ref_index":32,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Probing the nature of Einstein nonlinear Maxwell Yukawa black hole through gravitational wave forms from periodic orbits and quasiperiodic oscillations","primary_cat":"gr-qc","submitted_at":"2026-01-06T10:41:13+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":4.0,"formal_verification":"none","one_line_summary":"Gravitational waveforms from periodic orbits and QPOs around ENLMY black holes are derived and used with MCMC to constrain the Yukawa parameter and charge for microquasars and the galactic center.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2512.16322","ref_index":17,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"First-time assessment of glitch-induced bias and uncertainty in inference of extreme mass ratio inspirals","primary_cat":"gr-qc","submitted_at":"2025-12-18T09:03:38+00:00","verdict":"ACCEPT","verdict_confidence":"MODERATE","novelty_score":7.0,"formal_verification":"none","one_line_summary":"Moderately mitigated glitch streams induce negligible to minor biases (0.04–0.6σ) in EMRI parameters while weakly mitigated streams with higher-SNR events can reach ~1σ biases, making EMRI inference more robust than for MBHBs.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2512.11911","ref_index":16,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Gravitational radiations from periodic orbits around a black hole in the effective field theory extension of general relativity","primary_cat":"gr-qc","submitted_at":"2025-12-11T01:04:43+00:00","verdict":"REJECT","verdict_confidence":"MODERATE","novelty_score":4.0,"formal_verification":"none","one_line_summary":"EFTGR black-hole periodic orbits follow the (z,w,v) taxonomy and emit zoom-whirl waveforms whose phase, not amplitude, is sensitive to the EFTGR coupling ϵ1.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2510.17967","ref_index":18,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Scalar fields around black hole binaries in LIGO-Virgo-KAGRA","primary_cat":"gr-qc","submitted_at":"2025-10-20T18:00:02+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"Semi-analytic waveform model for scalar environments around black hole binaries is validated against numerical relativity and applied to LIGO-Virgo-KAGRA data to obtain upper limits on scalar densities with tentative evidence in GW190728.","context_count":1,"top_context_role":"background","top_context_polarity":"background","context_text":"of ultralight dark matter to supermassive black holes and binaries, Phys. Rev. D102, 063022 (2020), arXiv:2009.00012 [gr-qc]. [17] B. J. Kavanagh, D. A. Nichols, G. Bertone, and D. Gag- gero, Detecting dark matter around black holes with gravitational waves: Effects of dark-matter dynamics on the gravitational waveform, Phys. Rev. D102, 083006 (2020), arXiv:2002.12811 [gr-qc]. [18] A. Maselli, N. Franchini, L. Gualtieri, T. P. Sotiriou, S. Barsanti, and P. Pani, Detecting fundamental fields with LISA observations of gravitational waves from ex- treme mass-ratio inspirals, Nature Astron.6, 464 (2022), arXiv:2106.11325 [gr-qc]. [19] A. Coogan, G. Bertone, D. Gaggero, B. J. Kavanagh, and D. A. Nichols, Measuring the dark matter environments"},{"citing_arxiv_id":"2510.11793","ref_index":55,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Black hole mergers beyond general relativity: a self-force approach","primary_cat":"gr-qc","submitted_at":"2025-10-13T18:00:08+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":7.0,"formal_verification":"none","one_line_summary":"Self-force theory is extended to compute merger and ringdown waveforms in beyond-GR black hole binaries under the extreme mass-ratio approximation, with first calculations of self-force corrections to the merger waveform.","context_count":1,"top_context_role":"background","top_context_polarity":"background","context_text":"δGαβ[h] is the linearized Einstein tensor on the back- ground gαβ; δ2Gαβ[h, h] is the second-order Einstein ten- sor, quadratic in hαβ; and the term quadratic in φ is the stress-energy tensor of the scalar field. The Dirac δ4 source terms are the particle's Detweiler stress-energy tensor [95, 96] and charge distribution, which we write in 1 Strictly speaking, Ref. [ 55] obtained these field equations from the variational principles δ(SEH + SbGR)/δgαβ + δSpp/δ˜gαβ = 0 and δ(SEH + SbGR)/δφ + δSpp/δφR = 0, which will be rigorously derived elsewhere [89]. See also Refs. [90-92]. 2 As a consequence, dCS is indistinguishable from GR at this order because in dCS the secondary will possess a scalar dipole but not a scalar monopoleq[93, 94]."}],"limit":50,"offset":0}