{"total":10,"items":[{"citing_arxiv_id":"2606.28482","ref_index":51,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Strongest constraints on dark acoustic oscillations from the Lyman-alpha forest","primary_cat":"astro-ph.CO","submitted_at":"2026-06-26T18:00:00+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":7.0,"formal_verification":"none","one_line_summary":"First constraints from Ly-alpha forest limit DAO participation to at most 30% of dark matter for peaks below 50 h/Mpc at 95% CL using a deep kernel emulator of simulations.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.26234","ref_index":33,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Lyman-Alpha Forest and its Cross-Correlation with High-Redshift Galaxies in Effective Field Theory at the Field Level","primary_cat":"astro-ph.CO","submitted_at":"2026-06-24T18:00:02+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"An EFT-based field-level forward model for the Lyman-alpha forest matches simulations at the percent level on quasi-linear scales and generates mocks for DESI and DESI-II analyses.","context_count":1,"top_context_role":"background","top_context_polarity":"unclear","context_text":"Haehnelt, J. S. Bolton, M. Molaro, E. Puchwein et al.,Unveiling Dark Matter free-streaming at the smallest scales with high redshift Lyman-alpha forest,arXiv e-prints(2023) arXiv:2309.04533 [2309.04533]. 45 [32] M. Zaldarriaga,Searching for Fluctuations in the Intergalactic Medium Temperature Using the LyαForest, ApJ564 (2002) 153 [astro-ph/0102205]. [33] A. A. Meiksin,The physics of the intergalactic medium,Reviews of Modern Physics81(2009) 1405 [0711.3358]. [34] M. McQuinn,The Evolution of the Intergalactic Medium, ARA&A54(2016) 313 [1512.00086]. [35] M. Viel, J. Lesgourgues, M. G. Haehnelt, S. Matarrese and A. Riotto,Can Sterile Neutrinos Be Ruled Out as Warm Dark Matter Candidates?, Phys. Rev. Lett."},{"citing_arxiv_id":"2606.23791","ref_index":64,"ref_count":2,"confidence":0.9,"is_internal_anchor":false,"paper_title":"One Generator, Any Process: LLM-Conditioning for the LHC","primary_cat":"hep-ph","submitted_at":"2026-06-22T18:00:02+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"LLM embeddings condition a generative transformer to enable faster convergence, better performance, and generalization to unseen LHC processes using a single model.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.17155","ref_index":41,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Freeze-in and ultra-relativistic freeze-out during general reheating scenarios","primary_cat":"hep-ph","submitted_at":"2026-06-15T18:00:08+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":7.0,"formal_verification":"none","one_line_summary":"Derives analytic relic yields for dark matter production in general reheating scenarios parametrized by equation-of-state ω, cooling index α, interaction scale Λ and temperature power n, organized by two critical temperature exponents.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.06969","ref_index":54,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Lyman-$\\alpha$ forest constraints on pure and mixed fuzzy dark matter","primary_cat":"astro-ph.CO","submitted_at":"2026-06-05T06:57:12+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"Lyman-alpha forest data yield m_FDM > 1.9e-21 eV (95% CL) for pure FDM and f_FDM upper limits of 0.07-0.65 for mixed FDM at log10(m_FDM/eV) = -23 to -21.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2510.17977","ref_index":67,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Growth of Structure in Multi-species Wave Dark Matter","primary_cat":"astro-ph.CO","submitted_at":"2025-10-20T18:00:10+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":7.0,"formal_verification":"none","one_line_summary":"Derives the power spectrum evolution and cross-spectra for arbitrary multi-species wave and particle dark matter, incorporating free-streaming, Jeans scales, and intrinsic fluctuations.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2510.15046","ref_index":9,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Multi-species Dark Matter with Warmth and Randomness","primary_cat":"astro-ph.CO","submitted_at":"2025-10-16T18:03:25+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":7.0,"formal_verification":"none","one_line_summary":"Presents a general analytic framework based on truncated BBGKY hierarchy solved via Volterra equations for computing power spectra in multi-species dark matter with finite velocity dispersion and Poisson fluctuations.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2506.12131","ref_index":35,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Early Growth of Structure in Warm Wave Dark Matter","primary_cat":"astro-ph.CO","submitted_at":"2025-06-13T18:00:01+00:00","verdict":"CONDITIONAL","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"Derives suppression of adiabatic perturbations and scale-dependent growth of isocurvature power in warm wave dark matter, verifies with Schrödinger-Poisson simulations, and proposes an analytic halo mass function.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2411.07970","ref_index":152,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"MUltiplexed Survey Telescope (MUST) Science White Paper I: Overview of Large-Scale Structure Cosmology in the Era of Stage-V Spectroscopic Surveys","primary_cat":"astro-ph.CO","submitted_at":"2024-11-12T17:51:21+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":4.0,"formal_verification":"none","one_line_summary":"MUST is a planned 6.5m Stage-V spectroscopic survey telescope targeting 100M+ galaxies and quasars to z~5.5 for large-scale structure cosmology studies.","context_count":1,"top_context_role":"background","top_context_polarity":"background","context_text":"cial model corresponding to the CDM limit (m X → ∞). In this case, we constrain the lower bound of the WDM parti- cle mass. An optimistic survey covering 14,000 deg 2 would yield the most stringent lower bound onm X to date, with a 95% CL limit of 10.5 keV . Even a conservative 10,000 deg2 survey would achievem X >7.6 keV , exceeding the current strongest Lyαforest-only constraint ofm X >5.7 keV [152]. 4 6 8 10 12 mX [keV] Stellar stream: GD-1 + Pal 5 Lyα: SDSS + XQ-100 Lyα: [5,000 deg 2] Lyα: HIRES + UVES Lensed quasar: JWST MW satellite: DES + PS1 Lyα: [10,000 deg 2] Lyα: [14,000 deg 2] Figure 13Warm dark matter constraints. Arrows indicate the allowed parameter space (lower bounds) at the 95% confidence level (CL), which ex- tend towards infinity, corresponding to the CDM limit-the fiducial model"},{"citing_arxiv_id":"2407.01690","ref_index":38,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Structure-wide dark matter density depletion induced by local degeneracies","primary_cat":"astro-ph.GA","submitted_at":"2024-07-01T18:02:11+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"Degeneracy-induced depletion from fermionic DM in subhalos creates structure-wide low-density cores consistent with observations, linking profile diversity to formation history.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null}],"limit":50,"offset":0}