{"total":29,"items":[{"citing_arxiv_id":"2606.21380","ref_index":54,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Theoretical consistency and phenomenology of supercooled cosmological phase transitions","primary_cat":"hep-ph","submitted_at":"2026-06-19T12:36:03+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"Applies high-T dimensional reduction for the first time to a classically scale-invariant model, computes NLO nucleation rate via determinants, and predicts LISA-detectable GW from supercooled PT in SU(2)cSM.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.09779","ref_index":2,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Higher-dimensional operators and Polyakov loop in hot Scalar QED from the heat kernel","primary_cat":"hep-ph","submitted_at":"2026-06-08T17:39:46+00:00","verdict":"UNVERDICTED","verdict_confidence":"UNKNOWN","novelty_score":5.0,"formal_verification":"none","one_line_summary":"Computes dimension-six operators in finite-temperature massive scalar QED via heat kernel methods and evaluates their combined effect with the Polyakov loop on first-order phase transition thermodynamics.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.06355","ref_index":71,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"$\\tt BlackHawk$ $\\tt v3.0$: Hawking Radiation from Regular Black Holes","primary_cat":"gr-qc","submitted_at":"2026-06-04T16:23:24+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"BlackHawk v3.0 adds Hawking temperatures and greybody factors for multiple regular black hole metrics to an existing public code via numerical routines.","context_count":1,"top_context_role":"background","top_context_polarity":"background","context_text":"13092, 130922D (2024), arXiv:2406.12917 [astro-ph.IM]. [68] R. Genzel, F. Eisenhauer, and S. Gillessen, Astron. Astrophys. Rev.32, 3 (2024), arXiv:2404.03522 [astro-ph.GA]. [69] M. Y. Khlopov, Res. Astron. Astrophys.10, 495 (2010), arXiv:0801.0116 [astro-ph]. [70] B. Carr, F. Kuhnel, and M. Sandstad, Phys. Rev. D94, 083504 (2016), arXiv:1607.06077 [astro-ph.CO]. [71] A. M. Green and B. J. Kavanagh, J. Phys. G48, 043001 (2021), arXiv:2007.10722 [astro-ph.CO]. [72] B. Carr and F. Kuhnel, Ann. Rev. Nucl. Part. Sci.70, 355 (2020), arXiv:2006.02838 [astro-ph.CO]. [73] P. Villanueva-Domingo, O. Mena, and S. Palomares-Ruiz, Front. Astron. Space Sci.8, 87 (2021), arXiv:2103.12087 [astro-ph.CO]. [74] B. Carr and F. Kuhnel, SciPost Phys."},{"citing_arxiv_id":"2606.04229","ref_index":69,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"A Deep Dive into Baryon Asymmetry -- the C2HDM","primary_cat":"hep-ph","submitted_at":"2026-06-02T21:26:27+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":4.0,"formal_verification":"none","one_line_summary":"New BSMPT implementation of baryon asymmetry computation using WKB transport equations with moment truncations and VEV profile solving, validated in the C2HDM with uncertainty and GW interplay analysis.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.01580","ref_index":9,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Primordial black holes spin from cosmological first-order phase transitions","primary_cat":"astro-ph.CO","submitted_at":"2026-06-01T02:26:19+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":7.0,"formal_verification":"none","one_line_summary":"The paper derives a quantitative relationship showing that the Kerr parameter a_* of PBHs from first-order phase transitions increases with latent heat α and decreases with transition rate β, reaching typical values of 10^{-3}.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2605.27727","ref_index":57,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"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":"2605.27231","ref_index":32,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"A Fast Method to Compute Scalar Induced Gravitational Waves on a Lattice with Primordial Non-Gaussianities","primary_cat":"astro-ph.CO","submitted_at":"2026-05-26T16:11:50+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":7.0,"formal_verification":"none","one_line_summary":"A new lattice method recasts SIGW integrals as FFT convolutions to compute fully non-Gaussian spectra in seconds with ~10% error on a radiation-dominated background.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2605.21477","ref_index":84,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Opening the Window of Ultra-Light PBHs by Exorcising the Poltergeist","primary_cat":"hep-ph","submitted_at":"2026-05-20T17:57:36+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"Incorporating the general-relativity mass tail df_PBH/d ln M ∝ M^3.78 smooths PBH evaporation, suppresses the scalar-induced GW signal by orders of magnitude, and reopens the ultra-light PBH window for the hot Big Bang.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2605.19336","ref_index":16,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"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 data.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2605.17813","ref_index":15,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"ACT Data and Positive Running of the Spectral Index for Scalar Theory and Modified Gravity","primary_cat":"gr-qc","submitted_at":"2026-05-18T03:39:26+00:00","verdict":null,"verdict_confidence":null,"novelty_score":null,"formal_verification":null,"one_line_summary":null,"context_count":1,"top_context_role":"background","top_context_polarity":"background","context_text":"Another indirect confirmation of the inflationary regime will be the detection of a stochastic primordial gravitational wave background, and the future gravitational wave experiments will operate in frequency bands that will probe the inflationary gravitational waves [6-14]. NANOGrav already verified a stochastic gravitational wave background back in 2023 [15], but inflation itself cannot generate such a signal [16, 17]. Thus the next ten years will be extremely important for modern theoretical physics. Recently, the Atacama Cosmology Telescope (ACT) [18, 19] combined with the DESI data [20] stirred things up in CMB-related cosmology. Already the DESI data found interesting phenomena [21-25], that added up to the already known tensions of the Λ-Cold-Dark-Matter model [26-31]."},{"citing_arxiv_id":"2605.15197","ref_index":40,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Primordial Black Hole from Tensor-induced Density Fluctuation: First-order Phase Transitions and Domain Walls","primary_cat":"astro-ph.CO","submitted_at":"2026-05-14T17:59:55+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"Tensor perturbations from first-order phase transitions and domain wall annihilation induce curvature fluctuations at second order that form primordial black holes, allowing asteroid-mass PBHs to comprise all dark matter for specific parameter ranges with associated gravitational wave peaks in LISA,","context_count":1,"top_context_role":"background","top_context_polarity":"background","context_text":"(EPTA, InPTA:), Astron. Astrophys.678, A50 (2023), arXiv:2306.16214 [astro-ph.HE]. [38] G. Agazie et al. (NANOGrav), Astrophys. J. Lett.951, L8 (2023), arXiv:2306.16213 [astro-ph.HE]. [39] A. Afzal et al. (NANOGrav), Astrophys. J. Lett.951, L11 (2023), [Erratum: Astrophys.J.Lett. 971, L27 (2024), Erratum: Astrophys.J. 971, L27 (2024)], arXiv:2306.16219 [astro-ph.HE]. [40] J. Antoniadis et al. (EPTA, InPTA:), Astron. Astrophys.678, A50 (2023), arXiv:2306.16214 [astro-ph.HE]. [41] D. J. Reardon et al., Astrophys. J. Lett.951, L6 (2023), arXiv:2306.16215 [astro-ph.HE]. [42] H. Xu et al., Res. Astron. Astrophys.23, 075024 (2023), arXiv:2306.16216 [astro-ph.HE]. [43] A. G. Riess et al., Astrophys. J. Lett.934, L7 (2022), arXiv:2112."},{"citing_arxiv_id":"2605.15176","ref_index":1,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Matching higher-dimensional operators at finite temperature for general models","primary_cat":"hep-ph","submitted_at":"2026-05-14T17:57:40+00:00","verdict":"CONDITIONAL","verdict_confidence":"LOW","novelty_score":8.0,"formal_verification":"none","one_line_summary":"The authors automate matching of generic 3D dimension-five and -six operators for arbitrary models, implemented in an extension of DRalgo with public code and examples for scalar-Yukawa, hot QCD, and the full Standard Model.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2605.14088","ref_index":36,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Single field matter bounce with dark energy era: comparison with CMB Planck 2018 data and best fit parameters","primary_cat":"astro-ph.CO","submitted_at":"2026-05-13T20:14:23+00:00","verdict":"CONDITIONAL","verdict_confidence":"LOW","novelty_score":4.0,"formal_verification":"none","one_line_summary":"A matter bounce model driven by a scalar field with exponential potential fits Planck 2018 CMB data comparably to inflationary ΛCDM, with the potential slope λ directly setting the scalar spectral index ns.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2605.09250","ref_index":42,"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":"are evaluated through the separable Teukolsky equation [48- 51] for the Weyl scalarsψ0 andψ 4 [52]. This master equation naturally decomposes into coupled ordinary differential equa- tions for the angular and radial coordinates-commonly re- ferred to as the angular Teukolsky equation (ATE) and radial Teukolsky equation (RTE). The multiscale expansion strat- egy [42, 53-55] then separates the problem into a computa- tionally expensive offline data-generation step and a rapid on- line interpolation step, enabling efficient waveform construc- tion. Substantial efforts have been devoted to computing these GW fluxes for increasingly generic orbital geometries. On the numerical side, Hughes pioneered a framework that employs a"},{"citing_arxiv_id":"2604.20768","ref_index":21,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Primordial Magnetogenesis and Gravitational Waves from ALP-assisted Phase Transition","primary_cat":"hep-ph","submitted_at":"2026-04-22T16:57:22+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"ALP-assisted first-order phase transitions can explain observed intergalactic magnetic fields and produce detectable gravitational waves, linking cosmology with particle physics searches.","context_count":1,"top_context_role":"background","top_context_polarity":"background","context_text":"Space-based interferome- ters, such as LISA [16], DECIGO [23] and BBO [13] are sensitive to the mHz-dHz regime, while ground-based detectors like the Einstein Telescope (ET) [14] and Cosmic Explorer (CE) [19] will probe higher frequencies, typically in the 10-10 3 Hz range, and PTA exper- iments, including the Square Kilometre Array (SKA) [18], THEIA [25] andµ-ARES [21] provide complementary coverage at lower frequencies in the nHz-µHz range. Throughout this analysis, we assume a benchmark observation time oft obs = 4 years for interferometer- based detectors andt obs = 20 years for PTA-based detectors and SNR>10 to be a GW detection threshold. 6 Results In this section, we present the phenomenological implications of the supercooled PT in the"},{"citing_arxiv_id":"2604.19197","ref_index":6,"ref_count":2,"confidence":0.9,"is_internal_anchor":false,"paper_title":"CP-violating multi-field phase transitions and gravitational waves in a hidden NJL sector","primary_cat":"hep-ph","submitted_at":"2026-04-21T08:07:06+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"Multi-field tunneling analysis in a CP-violating NJL model yields a slow transition (β/H ~ 100) whose stochastic gravitational-wave signal is detectable by μAres and insensitive to the CP angle.","context_count":1,"top_context_role":"background","top_context_polarity":"background","context_text":"for the value ofκ turb, we takeκ turb ≈(5∼10)%κ sw. 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Petiteau, and A."},{"citing_arxiv_id":"2604.11893","ref_index":10,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Relativistic signatures of scalar dark matter in extreme-mass-ratio inspirals","primary_cat":"gr-qc","submitted_at":"2026-04-13T18:00:05+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"Relativistic metric backreaction from scalar dark matter clouds in EMRIs produces dominant polar gravitational wave corrections for Mμ ≲ 0.12, exceeding axial and scalar radiation channels at small separations.","context_count":1,"top_context_role":"background","top_context_polarity":"background","context_text":"Next Generation Global Gravitational Wave Observa- tory: The Science Book (2021), arXiv:2111.06990 [gr-qc]. [8] M. Colpi, K. Danzmann, M. Hewitson,et al.(LISA), LISA Definition Study Report (2024), arXiv:2402.07571 [astro-ph.CO]. [9] P. A. Seoane, J. Andrews, M. A. Sedda,et al. 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Holley-Bockelmann, D."},{"citing_arxiv_id":"2604.06053","ref_index":20,"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":"unclear","context_text":"(LISA), Astrophysics with the Laser Interferometer Space Antenna, Living Reviews in Rela- tivity26, 2 (2023), arXiv:2203.06016 [gr-qc]. [19] D. Laghi, N. Tamanini, W. Del Pozzo, A. Sesana, J. Gair, S. Babak, and D. Izquierdo-Villalba, Gravitational-wave cosmology with extreme mass-ratio inspirals, Mon. Not. R. Astron. Soc.508, 4512 (2021), arXiv:2102.01708 [astro-ph.CO]. [20] P. Auclairet al.(LISA Cosmology Working Group), Cosmology with the Laser Interferometer Space An- tenna, Living Reviews in Relativity26, 5 (2023), arXiv:2204.05434 [astro-ph.CO]. [21] J. R. Gair, M. Vallisneri, S. L. Larson, and J. G. Baker, Testing General Relativity with Low-Frequency, Space- Based Gravitational-Wave Detectors, Living Reviews in"},{"citing_arxiv_id":"2604.06009","ref_index":29,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Are Black Holes Fuzzballs? Probing Horizon-Scale Structure with LISA","primary_cat":"hep-th","submitted_at":"2026-04-07T16:05:27+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"LISA can constrain non-axisymmetric mass quadrupole deformations at the 10^{-3} level and axisymmetric mass octupole deformations at the 10^{-2} level in EMRI signals to test fuzzball proposals.","context_count":1,"top_context_role":"background","top_context_polarity":"background","context_text":"Amaro-Seoaneet al.(LISA), Laser Interferometer Space Antenna, (2017), arXiv:1702.00786 [astro-ph.IM]. [27] M. Colpiet al., LISA Definition Study Report, (2024), arXiv:2402.07571 [astro-ph.CO]. [28] P. A. Seoaneet al.(LISA), Astrophysics with the Laser Interferometer Space Antenna, Living Reviews in Rela- tivity26, 2 (2023), arXiv:2203.06016 [gr-qc]. [29] P. 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Arunet al.(LISA), New horizons for fundamental"},{"citing_arxiv_id":"2511.21488","ref_index":13,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Bayesian analysis of the complex singlet model with phase transition gravitational waves","primary_cat":"hep-ph","submitted_at":"2025-11-26T15:21:11+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":3.0,"formal_verification":"none","one_line_summary":"Bayesian forecasts for the Taiji detector constrain complex singlet model parameters through electroweak phase transition gravitational wave signals.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2511.16748","ref_index":10,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"LISA as a probe of pre-big-bang physics: a nested sampling analysis","primary_cat":"gr-qc","submitted_at":"2025-11-20T19:01:34+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"Nested sampling analysis indicates LISA could constrain H1, m, sigma_i and beta in the pre-big-bang model to relative uncertainties of about 18 percent under favorable conditions when including foregrounds.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2511.02612","ref_index":11,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Model Parameter Reconstruction of Electroweak Phase Transition with TianQin and LISA: Insights from the Dimension-Six Model","primary_cat":"hep-ph","submitted_at":"2025-11-04T14:35:27+00:00","verdict":"CONDITIONAL","verdict_confidence":"LOW","novelty_score":4.0,"formal_verification":"none","one_line_summary":"Simulations show TianQin and LISA can reconstruct the dimension-six model parameter Λ to sub-percent statistical precision for strong signals using Fisher, Bayesian sampling, and machine learning on data with noise and foregrounds.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2511.00996","ref_index":13,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Measuring gravitational wave spectrum from electroweak phase transition and Higgs self-couplings","primary_cat":"hep-ph","submitted_at":"2025-11-02T16:07:09+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"Frequency-domain simulations of the Taiji mission, including noise and foregrounds, demonstrate that the stochastic gravitational wave background from an electroweak phase transition can constrain Higgs cubic and quartic self-couplings in a singlet-extended Standard Model despite degeneracies.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2509.03360","ref_index":18,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"The Early Career Workshop of GR-Amaldi 2025","primary_cat":"physics.soc-ph","submitted_at":"2025-08-30T17:29:12+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":1.0,"formal_verification":"none","one_line_summary":"The paper reports on the aims, activities, and conclusions of an early-career workshop focused on scientific overviews, transferable skills, and networking in gravitational physics.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2507.08737","ref_index":51,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Quantum production of gravitational waves after inflation","primary_cat":"gr-qc","submitted_at":"2025-07-11T16:40:04+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":7.0,"formal_verification":"none","one_line_summary":"Scalar metric perturbations after inflation break conformal invariance and induce quantum production of gravitons, generating a GW spectrum that peaks near GHz frequencies for standard primordial scalar power spectra.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2506.22921","ref_index":34,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Statistic threshold of distinguishing the environmental effects and modified theory of gravity with multiple massive black-hole binaries","primary_cat":"gr-qc","submitted_at":"2025-06-28T15:12:50+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":4.0,"formal_verification":"none","one_line_summary":"The paper derives statistic thresholds to distinguish dynamical friction from dark matter spikes, extra dimension theory, and varying G theory using -4 PN order GW corrections in massive black hole binary inspirals across different astronomical models.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2506.15496","ref_index":25,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Thermodynamical uncertainties for primordial black holes from cosmological phase transitions","primary_cat":"hep-ph","submitted_at":"2025-06-18T14:34:48+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"A state-of-the-art thermodynamic analysis of supercooled phase transitions yields a universal lower bound β/H_* ≃ 5 and shows that viable PBH dark-matter parameter space in classically conformal gauge-Higgs theories is severely limited by percolation and QCD constraints.","context_count":1,"top_context_role":"background","top_context_polarity":"background","context_text":"arXiv:hep-ph/9605288. 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Okada, and Y."},{"citing_arxiv_id":"2505.22066","ref_index":16,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Cosmic Strings as Dynamical Dark Energy: Novel Constraints","primary_cat":"astro-ph.CO","submitted_at":"2025-05-28T07:45:53+00:00","verdict":"CONDITIONAL","verdict_confidence":"LOW","novelty_score":4.0,"formal_verification":"none","one_line_summary":"Cosmic string networks are constrained to less than ~1% of the energy density using CMB+BAO+SN data, with some models preferring mildly negative densities but no Bayesian evidence favoring them over LambdaCDM.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2311.01300","ref_index":275,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"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":"rest mass energy and eventually disappear. Together the string elements generate a stochastic GW background [246-268] and GW bursts [252, 254, 258, 259, 264, 265, 268- 274]. Detection and measurement of the string-generated gravitational waves by LISA will be informative for cosmology and high energy physics (see the whitepaper from the 29 LISA Cosmology Working Group for a summary [275]). The physics of CSs is sensitive to (1) the set of fields to which the string couples, (2) whether the strings are global or local, (3) the ratio of the characteristic string width to curvature scale. Here, we assume that the strings are minimally coupled (they interact with each other but only radiate gravitational waves), local and well-described in the"}],"limit":50,"offset":0}