Cosmology
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- CosmoAgent: AI Agent for Theoretical Cosmology
- The Loud Tail of the Supermassive Black Hole Binary Population: Multimessenger Candidates and Prospects for SKAO
- Tracing the Cosmic Origins: Machine Learning Reconstruction of the Primordial Density Field from EoR Observations
- Effective reheating in Gauss--Bonnet inflation with μ(ϕ,X) coupling
- Extra-dimensional Origins of Chemical Potentials at the Cosmological Collider
- Toward Bayesian photometric cosmic chronometers: Application to VIPERS
- Is MOND an effect of cosmic frame-dragging à la Mach?
- Testing the direction of dark sector interaction using late-time datasets
- Probing the sensitivity of dark energy dynamics to equation of state parametrization flexibility
- Finite-distance effects and scalar suppression in massive gravity
- Semi-Analytic Predictions for Strong-Lensing Perturbers in Cold and Self-Interacting Dark Matter
- Physics-Informed Neural Networks vs U-Net: Application to thermal dust emission recovery in the microwave
- Cluster connectivity in DES Y3 data: impact on galaxy properties
- AMICO galaxy clusters in KiDS-1000: Cosmological constraints from the two-point correlation function
- Prospects of Detecting Cosmological Domain Walls in the Cosmic Microwave Background
- Non-Markovian Cosmology with Causal Memory Kernels
- Direct detection of right-handed fermionic dark matter: electron-recoil measurements in Xe atoms
- AXIS Could Have Accessed Dark Matter Decays
- Odd radio circle J1555+2726: Observational evidence for shock re-acceleration of fossil plasma
- Sound-Horizon-Agnostic Forecast for Constraints on H0 and Σmν from BAO, CMB Lensing, Supernovae and LSST-like Galaxy Lensing
- A Robust Estimator for the Lyman-α Forest 1D Power Spectrum at High Redshift
- QUIJOTE scientific results - XII. Characterization of the polarized synchrotron emission at the power spectrum level in the QUIJOTE-MFI wide survey
- Gravitational Wave Diffractive Images Reveal the Structure of Astrophysical Objects
- Robust paths to primordial B modes in the presence of polarised point source contamination
- A cosmic filament catalog for COSMOS-Web Data Release 1 across 0.5 < z < 3.5