Wave-Particle Interactions in Astrophysical Plasmas
Dissipation processes derived from the kinetic theory of gases (shear viscosity and heat conduction) are employed to examine the solar wind that interacts with planetary ionospheres. The purpose of this study is to estimate the mean free path of wave-particle interactions that produce a continuum response in the plasma behavior.
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Modelling the impact of energetic electrons on electron-acoustic instabilities and HF/UHF wave propagation in the ionospheric-like plasmas. [PDF]
Ebadi D, Barzegar S.
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Dynamical Casimir Effect Under the Action of Gravitational Waves. [PDF]
de Oliveira G, Moreira TH, Céleri LC.
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Direct observations of cross-scale energy transfer driven by multiple-ion interactions in space plasmas. [PDF]
Liu ZY, Zong QG, Wang S, Zhou XZ, Yue C.
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Experimental and numerical investigation of elastic wave dispersion and attenuation induced by coal particle damping. [PDF]
Chen H +5 more
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Topological states in chain of interacting electrons. [PDF]
Karnaukhov IN, Krasovskii EE.
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Enhanced dust removal via the synergy of a standing wave acoustic field and high-pressure spray: An integrated experimental and numerical study. [PDF]
Wu S +7 more
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Large-scale optical trapping using a gradient-thickness protected microbottle resonator. [PDF]
Li Y +10 more
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Gravitational form factors of the Higgs boson. [PDF]
Beißner P +3 more
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A low-circuit-depth quantum computing approach to the nuclear shell model. [PDF]
Sarma C, Stevenson PD.
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