activity
20222026
most citedPonderomotive forces in unmagnetized plasmas described by Kappa distribution functions

8 citations · 8 across the 9 of their papers we have counts for

collaborators

9 papers

astro-ph.CO2026

Dark energy and negative compressibility of the Universe: A study based on cosmic equations of state

Felipe A. Asenjo, Ósmar Rodríguez, Ariel Órdenes Morales +1

All cosmological models are defined through energy and matter, which describe the evolution of the targeted Universe. Whether the content is simple or complex, it can be defined th…

gr-qc2026

Reconnection of Gravitational Fields

Luca Comisso, Felipe A. Asenjo

In a tetrad formulation of general relativity, an ideal Ohm-type condition for the gravitational field implies the conservation of gravitational fluxes and the preservation of the…

gr-qc2026

Frozen-In Gravitational Fields

Felipe A. Asenjo, Maricarmen A. Winkler, Luca Comisso

Spacetime can undergo complex nonlinear evolution, as governed by the Einstein field equations, and a central challenge is to understand the geometric structures that arise, persis…

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.space-ph2026

Non-thermal plasma density redistribution in planetary magnetospheres due to ion-cyclotron waves

Joaquín Espinoza-Troni, Felipe A Asenjo, Pablo S Moya

Planetary magnetospheres exhibit diverse environments where Ultra-low frequency (ULF) pulsations induce nonlinear ponderomotive effects. Since suprathermal populations modeled by K…

astro-ph.SR2026

Dispersive Properties of MHD Waves in the Expanding Solar Wind for a Parker Spiral Geometry

Sebastián Saldivia, Felipe Asenjo, Pablo S. Moya

In this work, we quantify the effects of solar wind expansion on the dispersive properties of the three normal modes of ideal MHD using the Expanding Box Model, under a background…

physics.plasm-ph2025

Laser-Driven Annular Shock Waves as Laboratory Analogues of CDM Cosmologies and Cosmological Gravitational Waves

Felipe A. Asenjo, Felipe Veloso, Julio C. Valenzuela

We demonstrate that the experimental evolution of an annular, laser-driven plasma shock wave, expanding over time and undergoing self-interaction gives rise to multiple shock struc…

physics.plasm-ph2025

Electromagnetic plasma waves in Big Bounce and Big Crunch cosmologies

Felipe A. Asenjo

We study the exact dynamics of electromagnetic waves in cold electron-positron plasma in the simplest background of Big Bounce and Big Crunch cosmologies. We show that these waves…

physics.plasm-ph2022★ 8 cited

Ponderomotive forces in unmagnetized plasmas described by Kappa distribution functions

Joaquín Espinoza-Troni, Felipe A Asenjo, Pablo S Moya

The Washimi and Karpman ponderomotive interaction due to electromagnetic waves propagation is investigated for unmagnetized plasmas described by a isotropic Kappa distribution. We…