Cosmology
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- The Origin of the Fermi Halo-like Emission: A New Model of the Fermi Bubbles
- Matter-Antimatter Asymmetry from Dirac-Majorana Flip-Flop
- Primordial black holes as a natural consequence of scale-invariance
- Interpretation of Nanohertz Gravitational Waves via Cosmic Strings in Post-BBN Matter and Kination Domination
- Impact of site-dependent noise configurations on Einstein Telescope science at low frequency
- Heavy Higgsino Dark Matter With Low Reheating in View of the LZ High-Recoil Event
- Matter Flavor Conversion Mediated by Pseudo-Sterile States as the Possible Origin of Neutrino Oscillation Anomalies
- Exploring neutrino loss with diffuse astrophysical neutrino fluxes
- Constraints on Primordial Oscillatory Features from the Power Spectrum and Bispectrum of Redshift-Space Galaxy Clustering in DESI DR1
- Phenomenology of axion-meson mixing and scattering processes
- Scatter, bias, and chaos of satellite orbits in triaxial dark matter haloes
- Growth, geometry, and early-universe split of the matter density parameter Ωm
- Fermi-eROSITA cross-correlations suggest annihilation lines of ∼70 GeV WIMPs
- A simple solution to the monopole problem: SU(5) GUT with symmetry breaking into special subgroup
- The decay rate of metastable cosmic strings beyond the thin-string approximation
- Cosmological perturbations of TDiff fields
- Gravitational wave emission from nonspherical collapse in an early matter-dominated era using N-body simulations
- Coverage is not enough: Frequentist tests of simulation-based inference for primordial non-Gaussianity
- A time-varying speed of light and implications for the evolution of the universe, Part I: Establishing a variable light speed model
- A new standard model of cosmology: Time-varying fundamental constants and the evolution of the universe
- Revisiting self-interacting dark matter with DESI DR2 baryon acoustic oscillation observations
- Studying generalized polytropic and warm dark matter in NGC 5055
- Is Dark Matter Really Matter?
- Calibration-induced Systematics in SALT3 Training and Their Impact on Dark Energy Constraints from Stage IV Supernova Surveys
- Unified dark sector and Hubble-tension alleviation in scalar–vector–tensor gravity