Cosmology
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- BICEP/Keck XXII: Analysis of the South Pole Atmosphere for CMB Observations
- Calculating the squeezed bispectrum in stochastic inflation by Monte Carlo simulation
- Measuring peculiar velocity and tomographic redshift dipole with DESI DR1 catalogs
- Comment on `Measuring the Hubble Constant Using Strongly Lensed Gravitational Wave Signals'
- Universal CMB Phase Coherence from Single-Field Inflation
- Gravitational Backreaction in de Sitter: A Canonical ADM Approach
- Double-peaked Ly α emission during reionization requires nearby voids and a favourable local ionizing background
- Anisotropy of Satellite Galaxies-I: Contrasting Correlations with Central Galaxy, Host Halo, and Large-Scale Filament Structures
- SPT-3G D1: Foreground-Robust Lensing Templates for Primordial Gravitational Wave Searches
- Upper Limits on the Isotropic Gravitational-Wave Background from the first part of LIGO, Virgo, and KAGRA's fourth Observing Run
- Exact Solutions of Maxwell Vacuum Equations in Null Homogeneous Petrov Spaces with Non-Solvable Motion Groups
- The Ontological Origin of the Universe and Maximal Existence
- Higgsino Dark Matter Interpretation of the LUX-ZEPLIN 248 keV Nuclear-Recoil Event
- Is MOND an Emergent Effective Law of a Complex Dark Matter Sector?
- Area-product universality in multi-horizon black hole entropy
- Singlet Extended Mirror Standard Model World as Dark Matter and Gravitational Waves Imprints of a High Scale Mirror Phase Transitions
- Stasis Combs: Gravitational-Wave Signatures of Recurrent Cosmological Stasis
- Multiparameter sensing of axion dark matter with superconducting-qubit networks
- A Non-Singular Cyclic Universe from Modified Gravity
- Study of dynamical dark energy using DESI DR2 BAO, CMB, and Type Ia Supernovae data
- A Six-Parameter Teleparallel Cosmology Beyond ΛCDM: Sign-Changing Torsional Dark Energy and Implications for H0
- f(T,ℒm) Cosmology Embedded in a Viscous Barotropic Fluid
- The role of anisotropy in f(Q) gravity: insights from cosmological observations
- Investigating the coincidence problem with Interacting Dark Energy Models
- Probing dark energy dynamics through a new CPL-type Om(z) parametrization in FLRW Universe