{"total":26,"items":[{"citing_arxiv_id":"2607.00349","ref_index":49,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Variability in Supermassive Black-Hole Accretion Rates in Fuzzy Dark Matter Cores due to Black-Hole Wandering","primary_cat":"astro-ph.CO","submitted_at":"2026-07-01T02:44:05+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"Numerical simulations find that black-hole wandering in FDM soliton cores produces intermittent accretion, limiting durable boosts except for ~10^7 solar mass seeds in low-sound-speed gas.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2607.00072","ref_index":39,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Precision Solar System Dynamics for Ultralight Dark Matter Search","primary_cat":"hep-ph","submitted_at":"2026-06-30T18:00:00+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":4.0,"formal_verification":"none","one_line_summary":"Current interplanetary range measurements could probe ultralight dark matter at masses around 10^{-15} eV if its solar system density were 10^5 times the local value.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.31629","ref_index":20,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Ultralight dark matter mixed with primordial black holes","primary_cat":"astro-ph.CO","submitted_at":"2026-06-30T13:13:03+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":4.0,"formal_verification":"none","one_line_summary":"In mixed ULDM-PBH halos the continuum PBH contribution alters soliton structure at the tens-of-percent level while discrete shot noise induces mode transitions too slow to matter on galactic timescales.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.30827","ref_index":14,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Time-dependent adaptive mesh refinement solver for the Gross-Pitaevskii-Poisson equations","primary_cat":"astro-ph.GA","submitted_at":"2026-06-29T18:57:36+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"A new AMR solver for the time-dependent GPP system is developed and validated on nonlinear test problems, preserving conservation laws and resolving wave features.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.26218","ref_index":38,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Dark Matter in Draco and Bo\\\"otes I: Hints of a Core in an Ultra-Faint Dwarf from Simulation-Based Inference","primary_cat":"astro-ph.GA","submitted_at":"2026-06-24T18:00:00+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":7.0,"formal_verification":"none","one_line_summary":"GraphNPE recovers a significantly lower central density for Boötes I consistent with a core while Draco remains marginally cuspy, and demonstrates that higher-order velocity moments reduce bias in dynamical modeling.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.25537","ref_index":189,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Probing the Fundamental Nature of Particle Dark Matter","primary_cat":"astro-ph.CO","submitted_at":"2026-06-24T08:13:20+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":2.0,"formal_verification":"none","one_line_summary":"Review summarizing radio searches for WIMP and ALP dark matter with SKA precursors and forecasts for SKA-Low and SKA-Mid telescopes.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.06394","ref_index":3,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Wave-Tide Locking in Thin Stellar Streams: A Phenomenological Mass Spectrometer for an Intermediate Ultralight Axion","primary_cat":"hep-ph","submitted_at":"2026-06-04T17:01:56+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"An analytic relation between tidal radius, gravitational Bohr radius, and axion de Broglie wavelength yields a mass estimator for intermediate ultralight axions of order 10^{-19} eV from observed stellar stream widths.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.01103","ref_index":26,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Self-gravitating quantum stars with a globally relevant Bohm potential","primary_cat":"hep-th","submitted_at":"2026-05-31T08:44:58+00:00","verdict":"CONDITIONAL","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"The equilibrium radius of self-gravitating dark fermion stars is determined by the fermion mass once the total mass is given, with the Bohm potential supplying outward pressure for heavier species and inward tension for lighter ones.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2605.29069","ref_index":12,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Equilibrium Core and Vortex Solutions of Bose Einstein Condensate Dark Matter around a Black Hole","primary_cat":"astro-ph.GA","submitted_at":"2026-05-27T20:19:49+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"Numerical construction of axisymmetric equilibrium core and vortex solutions for BECDM around a black hole using imaginary-time evolution, with stability assessed via turning-point criterion on enthalpy.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2605.27529","ref_index":10,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Existence of nonrelativistic $\\ell$- and multi-$\\ell$-boson stars and their radial stability","primary_cat":"math-ph","submitted_at":"2026-05-26T18:03:24+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"Existence of an infinite class of spherically-symmetric solutions to the multi-field Schrödinger-Poisson system is established via global minimization of the energy functional on rotationally invariant H1 functions with fixed L2 norms per component, with the minima shown to be orbitally stable.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2605.23206","ref_index":42,"ref_count":2,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Yukawa-Screened Bose-Star Condensation","primary_cat":"hep-ph","submitted_at":"2026-05-22T03:48:41+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":3.0,"formal_verification":"none","one_line_summary":"Yukawa screening in the YSP system broadens Bose-star profiles and delays condensation, matching a screened kinetic formula after fitting one normalization parameter.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2605.17211","ref_index":51,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Constraints on Self-Interacting Fuzzy Dark Matter from the Stellar Kinematics of the Dwarf Galaxy Leo II","primary_cat":"astro-ph.CO","submitted_at":"2026-05-17T01:00:54+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"Using Jeans analysis of Leo II stellar kinematics, the paper constrains the fuzzy dark matter mass m_a and self-interaction parameter f_a, finding 95% CL lower limits on m_a in the (1-10)×10^{-22} eV range for |f_a^{-1}| ≲ 10^{-14} GeV^{-1}.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2605.12589","ref_index":12,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Tunneling and tidal stripping in multifield ultralight dark matter halos","primary_cat":"hep-ph","submitted_at":"2026-05-12T18:00:00+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":7.0,"formal_verification":"none","one_line_summary":"A semiclassical tunneling model shows that two-field ultralight DM halos have stability bounds that can be relaxed for some density-mass ratios but become more stringent across much of the parameter space compared to single-field cases.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2605.03477","ref_index":6,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Self-Interaction Bounds on Ultralight Dark Matter Couplings to Matter","primary_cat":"hep-ph","submitted_at":"2026-05-05T08:05:54+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"Self-interaction bounds from cosmology constrain ultralight dark matter couplings to neutrinos, electrons, and light quarks via unavoidable quantum loop corrections.","context_count":1,"top_context_role":"background","top_context_polarity":"background","context_text":"043541, [arXiv:1610.08297]. [3] E. G. M. Ferreira,Ultra-light dark matter,Astron. Astrophys. Rev.29(2021), no. 1 7, [arXiv:2005.03254]. [4] D. Antypas et al.,New Horizons: Scalar and Vector Ultralight Dark Matter,arXiv:2203.14915. [5] W. Hu, R. Barkana, and A. Gruzinov,Cold and fuzzy dark matter,Phys. Rev. Lett.85(2000) 1158-1161, [astro-ph/0003365]. [6] H.-Y . Schive, T. Chiueh, and T. Broadhurst,Cosmic Structure as the Quantum Interference of a Coherent Dark Wave,Nature Phys.10(2014) 496-499, [arXiv:1406.6586]. [7] N. Bar, D. Blas, K. Blum, and S. Sibiryakov,Galactic rotation curves versus ultralight dark matter: Implications of the soliton-host halo relation,Phys. Rev. D98(2018), no. 8 083027, [arXiv:1805."},{"citing_arxiv_id":"2605.02172","ref_index":19,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Constraints on Ultralight Scalar and Dark Photon Dark Matter from PPTA-DR3 and EPTA-DR2","primary_cat":"astro-ph.CO","submitted_at":"2026-05-04T03:05:51+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":4.0,"formal_verification":"none","one_line_summary":"Bayesian analysis of PPTA-DR3 and EPTA-DR2 finds no statistically significant ULDM signals and sets 95% CL upper limits on scalar and dark photon dark matter, improving prior bounds in most mass ranges.","context_count":1,"top_context_role":"background","top_context_polarity":"background","context_text":"Hui, \"Wave Dark Matter,\" Annu. Rev. Astron. Astrophys.59, 247 (2021), arXiv:2101.11735. [17] E. G. M. Ferreira, \"Ultra-light dark matter,\" Astron. Astrophys. Rev.29, 7 (2021), arXiv:2005.03254. [18] H.-Y. Schive, T. Chiueh, and T. Broadhurst, \"Cosmic structure as the quantum interference of a coherent dark wave,\" Nature Physics10, 496 (2014), arXiv:1406.6586. [19] H.-Y. Schive, M.-H. Liao, T.-P. Woo, S.-K. Wong, T. Chiueh, T. Broadhurst, and W. Y. P. Hwang, \"Understanding the Core- Halo Relation of Quantum Wave Dark Matter from 3D Simula- tions,\" Phys. Rev. Lett.113, 261302 (2014), arXiv:1407.7762. [20] J. Zhang, Y.-L. Sming Tsai, J.-L. Kuo, K. Cheung, and M.-C. Chu, \"Ultralight Axion Dark Matter and Its Impact on Dark"},{"citing_arxiv_id":"2604.26393","ref_index":13,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Tidal Heating of Stellar Clusters in Fuzzy Dark Matter Halos","primary_cat":"astro-ph.CO","submitted_at":"2026-04-29T08:02:13+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"Simulations reveal tidal heating dominates stellar cluster evolution in low-mass fuzzy dark matter halos, suppressed by reduced soliton mass and tidal stripping, so halo structure must be modeled to constrain the fuzzy dark matter particle mass.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2604.23353","ref_index":19,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Testing Scalar Field Dark Matter models in M31 galaxy through the Rotation Curve analysis","primary_cat":"astro-ph.CO","submitted_at":"2026-04-25T15:39:47+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":4.0,"formal_verification":"none","one_line_summary":"Fuzzy dark matter with smooth cored halos provides the most consistent description of M31's rotation curve among scalar field models when paired with a two-bulge baryonic configuration.","context_count":1,"top_context_role":"background","top_context_polarity":"background","context_text":"In particular, SFDM halos are expected to form hierarchically in a manner similar to CDM, while condensation processes inside structures naturally lead to galactic-scale cores [15-18] One of the most studied realizations is fuzzy dark matter (FDM), in which the wave nature of the SF leads to the formation of a central solitonic core surrounded by an extended halo [19, 20]. Other SF realizations include Bose-Einstein condensate (BEC) DM [21] and multistate SF configurations (mSFDM) [22], which may produce more complex density structures depending on the superposition of quantum states. Testing such models against observational data is essential for assessing their viability. RC analyses serve as a particularly useful laboratory for this purpose, since SF halos often predict characteristic deviations from standard"},{"citing_arxiv_id":"2604.15240","ref_index":53,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Boson star-black hole binaries: initial data and head-on collisions","primary_cat":"gr-qc","submitted_at":"2026-04-16T17:15:14+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"A one-body conformal-factor correction stabilizes boson star-black hole initial data, enabling gravitational-wave analysis that shows higher multipoles can discriminate mixed mergers from pure black-hole binaries.","context_count":1,"top_context_role":"background","top_context_polarity":"background","context_text":"modes, ergoregions and nonlinear instabilities of ultra- compact objects,\" Phys. Rev. D90, 044069 (2014), arXiv:1406.5510 [gr-qc]. [52] Gareth Arturo Marks, Seppe J. Staelens, Tamara Evstafyeva, and Ulrich Sperhake, \"Long-Term Sta- ble Nonlinear Evolutions of Ultracompact Black-Hole Mimickers,\" Phys. Rev. Lett.135, 131402 (2025), arXiv:2504.17775 [gr-qc]. [53] Seppe J. Staelens, \"Search for growing angular modes in ultracompact boson star evolutions,\" J. Phys. Conf. Ser.3177, 012046 (2026), arXiv:2508.19460 [gr-qc]. [54] Tamara Evstafyeva, Nils Siemonsen, and William E. East, \"Assessing the stability of ultracompact spinning boson stars with nonlinear evolutions,\" Phys. Rev. D 113, 044024 (2026), arXiv:2508."},{"citing_arxiv_id":"2604.08053","ref_index":52,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Constraining Ultralight Scalar Dark Matter in the Galactic Center with the S2 Orbit","primary_cat":"hep-ph","submitted_at":"2026-04-09T10:02:09+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"Using S2 star periastron precession, the work constrains ultralight scalar dark matter mass ratios to below 10^{-3} or 1 and improves quadratic coupling bounds for masses 10^{-20} to 10^{-18} eV.","context_count":1,"top_context_role":"background","top_context_polarity":"background","context_text":"arXiv:1908.10370 [gr-qc]. [50] D. Baumann, H. S. Chia, R. A. Porto, and J. Stout, Gravitational Collider Physics, Phys. Rev. D101, 083019 (2020), arXiv:1912.04932 [gr-qc]. [51] H.-Y. Schive, T. Chiueh, and T. Broadhurst, Cos- mic Structure as the Quantum Interference of a Co- herent Dark Wave, Nature Phys.10, 496 (2014), arXiv:1406.6586 [astro-ph.GA]. [52] H.-Y. Schive, M.-H. Liao, T.-P. Woo, S.-K. Wong, T. Chi- ueh, T. Broadhurst, and W. Y. P. Hwang, Understanding the Core-Halo Relation of Quantum Wave Dark Mat- ter from 3D Simulations, Phys. Rev. Lett.113, 261302 (2014), arXiv:1407.7762 [astro-ph.GA]. [53] P.-H. Chavanis, Mass-radius relation of self-gravitating Bose-Einstein condensates with a central black hole, Eur."},{"citing_arxiv_id":"2603.06329","ref_index":7,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Effects of Self-Interaction and of an Ideal Gas in Binary Mergers of Bosonic Dark Matter Cores","primary_cat":"astro-ph.CO","submitted_at":"2026-03-06T14:41:26+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"Self-interaction changes the energy-mass scaling of BECDM core mergers from E proportional to minus M cubed to milder forms, altering mass retention, while an ideal gas only modifies the gravitational background without changing the bosonic scaling.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2602.11512","ref_index":27,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Stone Skipping Black Holes in Ultralight Dark Matter Solitons","primary_cat":"astro-ph.CO","submitted_at":"2026-02-12T03:12:31+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":7.0,"formal_verification":"none","one_line_summary":"Black holes in ultralight dark matter solitons undergo quasi-periodic stone-skipping orbits driven by soliton dipole excitations, modifying inspiral dynamics when the black hole is much lighter than the soliton.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2512.14921","ref_index":23,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"$\\ell$-Boson stars in anti-de Sitter spacetime","primary_cat":"gr-qc","submitted_at":"2025-12-16T21:19:59+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"ℓ-boson stars are constructed and their properties studied in asymptotically anti-de Sitter spacetime.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2510.17977","ref_index":27,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"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":28,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"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":27,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"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":"2406.13394","ref_index":55,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Gravitational Wave Birefringence from Fuzzy Dark Matter","primary_cat":"gr-qc","submitted_at":"2024-06-19T09:38:13+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"Fuzzy dark matter induces frequency-dependent amplitude birefringence in gravitational waves with periodic time modulation set by the scalar mass, but no velocity birefringence.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null}],"limit":50,"offset":0}