Evolution of energy density fluctuations in the presence of a magnetic field
arXiv:2506.13118 · doi:10.1016/j.jspc.2025.100246
Abstract
In this proceeding, we study the evolution of energy density fluctuations in the presence of a static and uniform magnetic field. By numerically solving the relativistic Boltzmann-Vlasov equation within the relaxation time approximation and performing the momentum mode analysis of different wavelength fluctuations, we show that the magnetic field increases the damping of mode oscillations. This causes a qualitative change in the fluctuations present in the system at the timescale required to achieve a local equilibrium state.
arXiv comment4 pages, 4 figures; Contribution to: 8th International Conference on Physics and Astrophysics of Quark Gluon Plasma (ICPAQGP 2023), Puri, Odisha, India
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