Precision calculation of $N_{\text{eff}}$ with Neutrino Direct Simulation Monte Carlo

Abstract

Neutrino Direct Simulation Monte Carlo ($\nu$DSMC) is a Monte Carlo method for solving the neutrino Boltzmann equation in the early Universe, designed to track the evolution of cosmic neutrinos across a wide range of cosmological scenarios. We develop a complete $\nu$DSMC solver that consistently incorporates the effects of the electron mass, three-flavour neutrino oscillations, and finite-temperature QED corrections to the thermodynamics of the electromagnetic plasma. As a first application, we perform a high-precision calculation of neutrino decoupling in the standard cosmological model and obtain $N_{\text{eff}}=3.0439\pm 0.0006$, in excellent agreement with state-of-the-art results.

Version accepted for publication in Phys.Rev.D

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Cited by in corpus (2)

• Fast and Flexible Neutrino Decoupling Part I: The Standard Model
• Boltzmann Equation Solver for Thermalization