2012/01/16 by Nikitas Stamatopoulos, Stamatopoulos, Nikitas · 1 citation
Earth and Planetary Sciences · Physics and Astronomy · #Atmospheric Ozone and Climate #Computational Physics (physics.comp-ph) #Cosmology and Nongalactic Astrophysics (astro-ph.CO) #FOS: Physical sciences #Geophysics and Gravity Measurements #High Energy Physics - Theory (hep-th) #Ionosphere and magnetosphere dynamics
paper · pdf · doi:10.48550/arxiv.1201.3368
openalex publication_date 2012/01/16 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28
We calculate the lattice dispersion relation for three dimensional simulations of scalar fields. We argue that the mode frequency of scalar fields on the lattice should not be treated as a function of the magnitude of its wavevector but rather of its wavevector decomposition in Fourier space. Furthermore, we calculate how the lattice dispersion relation differs depending on the way that spatial derivatives are discretized when using finite difference methods in configuration space. For applications that require the mode frequency as an average function of the magnitude of the wavevector, we show how to calculate the radially averaged lattice dispersion relation. Finally, we use the publicly available framework LATTICEEASY to show that wrong treatment of dispersion relations in simulations of preheating leads to an inaccurate description of parametric resonance, which results in incorrect calculations of particle number densities during thermalization after inflation.