2010
DOI: 10.3367/ufne.0180.201001b.0055
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Nonlinear aspects of quantum plasma physics

Abstract: Dense quantum plasmas are ubiquitous in planetary interiors and in compact astrophysical objects (e.g., the interior of white dwarf stars, in magnetars, etc.), in semiconductors and micromechanical systems, as well as in the next-generation intense laser–solid density plasma interaction experiments and in quantum X-ray free-electron lasers. In contrast to classical plasmas, quantum plasmas have extremely high plasma number densities and low temperatures. Quantum plasmas are composed of electrons, positrons and… Show more

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Cited by 514 publications
(328 citation statements)
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References 218 publications
(298 reference statements)
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“…The field of quantum plasma physics [1][2][3][4][5] has considerable interest having risen recently in connection with its potential applications in modern technology, in emerging miniaturization techniques. In quantum plasmas, due to inter-fermion distances much lower than its de Broglie wavelength and the influence of the Pauli exclusion rule, many quantum effects such as electron-tunnelling, degeneracy pressure and Landau quantization may occur [6][7][8].…”
Section: Introductionmentioning
confidence: 99%
“…The field of quantum plasma physics [1][2][3][4][5] has considerable interest having risen recently in connection with its potential applications in modern technology, in emerging miniaturization techniques. In quantum plasmas, due to inter-fermion distances much lower than its de Broglie wavelength and the influence of the Pauli exclusion rule, many quantum effects such as electron-tunnelling, degeneracy pressure and Landau quantization may occur [6][7][8].…”
Section: Introductionmentioning
confidence: 99%
“…The figure shows the dispersion characteristic of the quantum Langmuir wave frequency ω versus the wave vector k, which is described by the equation (9). The green branch of dispersion is presented the classical high frequency Langmuir wave, the red and blue branches characterize the Coulomb exchange interactions and quantum Bohm potential influence, where n0e 10 21 cm −3 , η = 1.…”
Section: Figmentioning
confidence: 99%
“…Here, the quantum mechanics comes into the picture due to (1) overlapping of electron wave functions owing to the Heisenberg uncertainty principle, leading to electron tunneling though the quantum Bohm potential (also referred to as the quantum recoil effect 6 ), and (2) electron exchange and electron correlations because of the electronone-half spin effect. Thus, there are new equations of state 19,20 (the degenerate electron pressure that relates the Fermi electron temperature and the electron number density), new quantum forces involving the electron exchange and electron correlation potentials, 21 as well as the Bohm potential 1,5,7,8 and electron-one-half spin effects. 22,23 Inclusion of these forces in the collective behavior of the dense quantum plasma plays a significant role, since the physical phenomena appear on the atomic and nanoscales.…”
Section: Introductionmentioning
confidence: 99%
“…[1][2][3][4][5][6][7][8] It is concerned with the collective behavior of charged particles in dense plasmas in which the electrons are degenerate and the ions non-degenerate. Such dense plasmas are found in astrophysical settings [9][10][11] (e.g., in the cores of white dwarf stars and magnetars) and in warm dense matter, 12 in planetary systems 13 (e.g., in the core of Jupiter), in intense laser-solid compressed density plasma experiments for inertial confined fusion (ICF), 14 and in quantum free-electron-laser (Q-FEL) systems 15,16 for producing coherent x-rays, as well as in metallic thin films/nanostructures 18 and semiconductor devices.…”
Section: Introductionmentioning
confidence: 99%