{"total":23,"items":[{"citing_arxiv_id":"2607.01697","ref_index":66,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Gravitational Waves from Multiple First-Order Phase Transitions in a Scenario with Early Matter Domination","primary_cat":"hep-ph","submitted_at":"2026-07-02T04:41:30+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":4.0,"formal_verification":"none","one_line_summary":"Early matter domination with time-dependent decay rates produces multiple first-order phase transitions whose gravitational wave signatures encode the transition and reheating temperatures.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.27526","ref_index":79,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Dynamics of Relativistic Binaries in Structured and Stochastic Environments: A Lagrange-Fourier-Hansen Framework","primary_cat":"gr-qc","submitted_at":"2026-06-25T20:19:24+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"A new framework projects perturbations onto resonant frequencies via Hansen coefficients to produce efficient coupled ODEs for orbital elements in GW-driven relativistic binaries, demonstrated on tidal fields and accretion disks.","context_count":1,"top_context_role":"background","top_context_polarity":"background","context_text":"Barausse and L. 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LISA","primary_cat":"astro-ph.GA","submitted_at":"2026-06-09T17:11:19+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"Models directional galactic GW background with Doppler effects from Milky Way kinematics and shows via Fisher forecast that neglecting rotation produces observable biases in LISA parameter inference.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.04998","ref_index":14,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Self-force calculations with numerical relativity methods","primary_cat":"gr-qc","submitted_at":"2026-06-03T15:16:34+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"A new numerical relativity-inspired method achieves exponential convergence for scalar self-force calculations in Kerr spacetime on circular equatorial orbits up to near-extremal spins and the ISCO.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2605.29305","ref_index":3,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Recoil-regulated extreme mass-ratio inspirals in AGN disks","primary_cat":"astro-ph.HE","submitted_at":"2026-05-28T03:36:28+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"Recoil kicks and binary interactions in AGN disks suppress EMRI formation except in young systems, predicting LISA rates of 1-30 per year dominated by low-mass AGNs.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2605.28804","ref_index":71,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Whispers of Supergravity in Gravitational Wave Backgrounds: Determining the Gravitino Mass from Cosmic Thermal History","primary_cat":"astro-ph.CO","submitted_at":"2026-05-27T17:55:42+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"Gravitino masses in the 100 TeV to 10^10 TeV range can be inferred from two frequency features in the stochastic gravitational wave spectrum produced by an early matter-dominated phase.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2605.27727","ref_index":50,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Reconstructing ACT-compatible and GW170817-compatible Einstein-Gauss-Bonnet Inflation from the Observational Indices","primary_cat":"gr-qc","submitted_at":"2026-05-26T22:02:09+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":4.0,"formal_verification":"none","one_line_summary":"Four Einstein-Gauss-Bonnet inflationary models are reconstructed from a chosen tensor-to-scalar ratio and shown to satisfy ACT and GW170817 constraints including scalar perturbation amplitude.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2605.19336","ref_index":9,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Recombination Thickness as an Uncertainty in Inflationary Observables","primary_cat":"astro-ph.CO","submitted_at":"2026-05-19T04:19:44+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"Finite recombination thickness introduces Gaussian smoothing in ln k to the primordial power spectrum, producing non-trivial differences between TT and EE spectral indices that may be detectable in future CMB 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Refs. [100, 119] have demonstrated that the PNG atfNL order can induce significant anisotropies in the SIGW background, with further investigations extending to PNG atg NL order in Refs. [101, 102]. Regarding non-Gaussianity in the SIGW background, Ref. [119] provided an approximate expression for the angular bispectrum associated with PNG atf NL order, while a compre- hensive analysis of the angular bispectrum and trispectrum for PNG up tog NL order was presented in Ref. [148]. These studies underscore that the SIGW non-Gaussianity results from the squeezed PNG, suggesting that the angular bispectrum and trispectrum of SIGWs"},{"citing_arxiv_id":"2002.04615","ref_index":23,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"New Sensitivity Curves for Gravitational-Wave Signals from Cosmological Phase Transitions","primary_cat":"hep-ph","submitted_at":"2020-02-11T19:00:01+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":7.0,"formal_verification":"none","one_line_summary":"Defines peak-integrated sensitivity curves (PISCs) that fold in the expected spectral shape of gravitational waves from cosmological phase transitions and supplies semianalytical fits plus public data for major detectors.","context_count":1,"top_context_role":"background","top_context_polarity":"background","context_text":"Lumma, and M. Pauly, Phase transitions in the early universe, arXiv:2008.09136. [21] D. J. 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