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20232026
most citedMagnetic seed generation by plasma heat flux in accretion disks

2 citations · 2 across the 10 of their papers we have counts for

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physics.plasm-ph2026

First Principles Magnetohydrodynamical Theory for the Expanding Box Model: Effects on Expansion-Induced Alfvén Wave Reflection

Sebastián Saldivia, Nicolás Villarroel-Sepúlveda, Sebastián Echeverría-Veas +2

The Expanding Box Model (EBM) has been widely employed to simulate multiscale plasma phenomena in the expanding solar wind by transforming the MHD equations to a co-moving, non-ine…

physics.plasm-ph2026

Knudsen number as a non-thermal parameter: possible origin of skewness in space plasma distributions

Iván Gallo-Méndez, Adolfo F. Viñas, Pablo S. Moya

Non-Maxwellian distributions and their origins in space plasma have attracted significant attention due to their prevalence and impact on various astrophysical and space-related ph…

physics.plasm-ph2025

Unifying Kappa Distribution Models for Non-Equilibrium Space Plasmas: A Superstatistical Approach Based on Moments

Abiam Tamburrini, Sergio Davis, Pablo S. Moya

From the perspective of non-equilibrium statistical mechanics, modeling the velocity distribution of particles in non-equilibrium, steady-state plasmas presents a significant chall…

physics.plasm-ph2025

The effect of plasma expansion on the dispersion properties of MHD waves

Sebastián Saldivia, Felipe A. Asenjo, Pablo S. Moya

In this work, we employ the set of ideal expanding magnetohydrodynamic (MHD) equations within the Expanding Box Model (EBM) framework to theoretically characterize the effects of r…

physics.plasm-ph2024

Dark energy as a battery for magnetic field generation in plasmas

Nicolás Villarroel-Sepúlveda, Pablo S. Moya, Felipe A. Asenjo +1

It is shown that in the spacetime dominated by a cosmological constant, in the far region of a Schwarzschild-de Sitter black hole, a seed magnetic field can be generated in an ambi…

physics.plasm-ph2024

Expanding CGL: The CGL double-adiabatic approximation in the Expanding Solar Wind

Sebastián Echeverría-Veas, Pablo S. Moya, Marian Lazar +2

Different in situ satellite observations within 0.3 to 1 AU from the Sun reveal deviations in the thermodynamics of solar wind expansion. Specifically, these deviations challenge t…