Cosmology
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- Alpha-Core Breakup in the Strong Decay of ΛΛ6He to a Deeply Bound H Dibaryon
- Updated 1.1% Precision Values of the Hubble Constant with Corrected Pantheon+ and Dark Energy Survey (DES)-DOVEKIE Type Ia Supernovae
- The Equivalence Principle in the Dark Sector in light of DESI
- Cosmological Constrained Axion-Portal Inelastic Dark Matter for the LZ Event
- Running Hubble Constant with the Redshift as a Marker of Evolutionary Dark Energy
- Caught by its own light: Wimpzillas, the LHAASO knee and the diffuse γ-ray sky
- A fast radio burst from a non-targeted low-frequency survey
- The WEFT project: I. The emergence of turbulence in a cosmic filament
- Limits on the Inferred Hubble Constant Bias from a Local McVittie Gravitational Field
- Cosmological information from field-level analysis in redshift space
- Bridging Between Statistical Mechanics and Black Hole Evolution: Theoretical Formalism
- Why Azimuthal Averaging Works in Halo Lensing: Symmetry and Power Counting for Nonlinear Shear and Magnification
- Galaxy Power Spectrum at Two-Loop Order: Implications for Weak Lensing Surveys and New Physics
- A Unified Halo Mass Function Across Dark Matter Models from High-Resolution Multi-Scale Simulations
- Scalable Dark Siren Cosmology with gwcosmo: GPU Acceleration, Validation and Systematics
- Optimising instrument concepts with Machine Learning: Application to CMB spectral distortion experiments
- B-sure. Part II. Scattering transforms as robustness test for tensor-to-scalar ratio detection from CMB observations
- Vanilla Scotogenic Model at the future Muon Collider
- Implementation of frequency-correlated noise in CMB component separation: Method, Validation, and Early Applications
- Toward Precision Kinetic Sunyaev-Zel'dovich Cosmology---1. The Matter - Momentum Bispectrum at One-Loop Order
- Using the Circumgalactic Medium of Dwarf Galaxies as a Calorimetric Dark Matter Detector
- Right Energy, Wrong Profile: Why the 43 GeV Cluster Line Is Unlikely to Be Dark Matter
- Gravitational Wave Bias in IllustrisTNG300 from Machine-Learned Population-Synthesis Calibrated Merger Rates
- Population III Host Candidates at z∼2: Strong He II λ1640 and Absent UV Metal Lines in HETDEX Lyα Emitters
- CMB-HD Foregrounds: Simulations, Source Detection, and Foreground Removal