Cosmology
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- Heavy Dark Baryons as Self-Interacting Dark Matter: A GeV-Scale Coincidence
- Heavy Dark Baryons at Large N: Self-Interactions across All Scales
- The Simons Observatory: Design and Initial Performance of the Detector Readout System for the Large-Aperture Telescope
- Primordial Tensor Signatures and Gravitational Wave Constraints in Lorentz Violating Inflation with Non-Canonical Kinetics
- Stacked strong and weak lensing united: Improved measurement of the stellar and dark matter distributions in massive early-type galaxies at z∼ 0.5
- Metastable Dark Energy on the Phantom Brane
- Infrared Screening of the Cosmological Constant
- Do DESI-DR2 BAO data imply a coupling of dark matter and dark energy?
- Modeling Uncertainties in Modified Gravity Predictions for the Stochastic Gravitational-Wave Background
- A Consistent Implementation of Cluster Strong Lensing in Cosmological Simulation Light Cones
- A truncation test of the DESI evolving dark energy signal: three supernova calibrations compared
- Recovering Subtle Cosmological Information with the Zel’dovich-inspired Transform
- Testing ΛCDM versus Dynamical Dark Energy in 1 Yr: A DESI Spectroscopic Follow-up Program for Rubin Supernovae
- An improved standardization framework for Type II-P supernovae using a hierarchical Bayesian approach
- Is DESI Seeing Dynamical Dark Energy, or a Cosmic Glitch in Gravity?
- Optimization Procedure of the Baffle of the GroundBIRD Telescope to Mitigate Stray Light
- Everything Everywhere All At Once: A Hierarchical Framework for Mapping Anisotropies in the Local Universe
- Close Pulsar Pairs See Dark Matter Substructure through the Gravitational-Wave Background
- Toward Detecting the Moving Lens Effect with Optical Spectroscopy
- AdS - de Sitter transition in interacting dark energy models
- Fisher and DALI posterior approximations for testing gravity with gravitational waves
- Constraints on Complex Electroweak WIMPs from Solar Capture
- How collective modes terminate in the dispersion relation of neutrino plasmas
- Searching for BSM Experimental Signatures with Large Lagrangian Models
- A Strong Cosmologically Coupled Mass Growth Solution in Linearized General Relativity