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• W4284992407 endingPage "087105" @default.
• W4284992407 startingPage "087105" @default.
• W4284992407 abstract "A three-dimensional Thomas–Fermi dense anisotropic magnetized plasma having Fermi–Dirac distributed ions and electrons as well as classical fluid negative dust impurities is considered to analyze oblique modulational instability (MI) and head-on collisions among dust-acoustic dark solitons. The Chew–Golberger–Low description is employed to define the anisotropic dust pressure. The linear analysis is investigated. It is found that for larger wavelengths, the pressure anisotropy has a strong effect on the wave frequency. Following the multiscale reductive perturbation technique, a (3 + 1)-dimensional nonlinear Schrödinger equation is derived. Also, the MI criterion is identified, and the regions of (un)stable modulated waves are determined precisely. In addition to that, (un)stable domains of the modulated structures as well as the profile of the dust-acoustic rogue waves are found to be strongly affected by dust grain density, pressure anisotropy, and the strength of the magnetic field. In the stable regions, the face-to-face dark soliton collision and their phase shifts as well as their analytical trajectories are reported by applying the extended Poincare–Lighthill–Kuo method. Numerical analysis reveals that the phase shifts increase with dust concentration but decrease with dust pressure anisotropy. The present results may be applicable in exploring the nonlinear wave dynamics and solitary wave interactions in dense astrophysical plasmas especially to white dwarfs, interiors of the neutron stars, and magnet stars." @default.
• W4284992407 created "2022-07-11" @default.
• W4284992407 creator A5001959794 @default.
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• W4284992407 creator A5073214349 @default.
• W4284992407 date "2022-08-01" @default.
• W4284992407 modified "2023-09-23" @default.
• W4284992407 title "Three-dimensional rogue waves and dust-acoustic dark soliton collisions in degenerate ultradense magnetoplasma in the presence of dust pressure anisotropy" @default.
• W4284992407 cites W1656232303 @default.
• W4284992407 cites W1967717972 @default.
• W4284992407 cites W1967809128 @default.
• W4284992407 cites W1971670048 @default.
• W4284992407 cites W1980882379 @default.
• W4284992407 cites W1981987637 @default.
• W4284992407 cites W1992191817 @default.
• W4284992407 cites W2001220107 @default.
• W4284992407 cites W2010353305 @default.
• W4284992407 cites W2010438536 @default.
• W4284992407 cites W2010725877 @default.
• W4284992407 cites W2013541534 @default.
• W4284992407 cites W2013843436 @default.
• W4284992407 cites W2018444028 @default.
• W4284992407 cites W2018568869 @default.
• W4284992407 cites W2018747001 @default.
• W4284992407 cites W2020373581 @default.
• W4284992407 cites W2023464924 @default.
• W4284992407 cites W2023896836 @default.
• W4284992407 cites W2026187717 @default.
• W4284992407 cites W2027824283 @default.
• W4284992407 cites W2028397752 @default.
• W4284992407 cites W2030667491 @default.
• W4284992407 cites W2030669316 @default.
• W4284992407 cites W2034058745 @default.
• W4284992407 cites W2034725572 @default.
• W4284992407 cites W2044846126 @default.
• W4284992407 cites W2050639649 @default.
• W4284992407 cites W2057765389 @default.
• W4284992407 cites W2058291823 @default.
• W4284992407 cites W2061605946 @default.
• W4284992407 cites W2062862365 @default.
• W4284992407 cites W2064436329 @default.
• W4284992407 cites W2071138577 @default.
• W4284992407 cites W2072974685 @default.
• W4284992407 cites W2073774189 @default.
• W4284992407 cites W2081937115 @default.
• W4284992407 cites W2082140050 @default.
• W4284992407 cites W2084141000 @default.
• W4284992407 cites W2087768396 @default.
• W4284992407 cites W2088971356 @default.
• W4284992407 cites W2090537396 @default.
• W4284992407 cites W2091087178 @default.
• W4284992407 cites W2095287124 @default.
• W4284992407 cites W2109738443 @default.
• W4284992407 cites W2115809190 @default.
• W4284992407 cites W2127853869 @default.
• W4284992407 cites W2129762139 @default.
• W4284992407 cites W2150837901 @default.
• W4284992407 cites W2155140415 @default.
• W4284992407 cites W2160958037 @default.
• W4284992407 cites W2234254766 @default.
• W4284992407 cites W2259214054 @default.
• W4284992407 cites W2268020843 @default.
• W4284992407 cites W2316386143 @default.
• W4284992407 cites W2418547924 @default.
• W4284992407 cites W2548273632 @default.
• W4284992407 cites W2790487275 @default.
• W4284992407 cites W2790945006 @default.
• W4284992407 cites W2892181390 @default.
• W4284992407 cites W2922246531 @default.
• W4284992407 cites W2981095792 @default.
• W4284992407 cites W2981636431 @default.
• W4284992407 cites W2992310557 @default.
• W4284992407 cites W2999160148 @default.
• W4284992407 cites W3000169322 @default.
• W4284992407 cites W3008503414 @default.
• W4284992407 cites W3008547377 @default.
• W4284992407 cites W3020874505 @default.
• W4284992407 cites W3091160786 @default.
• W4284992407 cites W3095834425 @default.
• W4284992407 cites W3098022040 @default.
• W4284992407 cites W3125340439 @default.
• W4284992407 cites W3130887518 @default.
• W4284992407 cites W3176492829 @default.
• W4284992407 cites W3204275631 @default.
• W4284992407 cites W3208703841 @default.
• W4284992407 cites W3208964815 @default.
• W4284992407 cites W4205684785 @default.
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• W4284992407 doi "https://doi.org/10.1063/5.0096990" @default.
• W4284992407 hasPublicationYear "2022" @default.
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