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Nonplanar solitons in a degenerate multi-species plasma

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dc.contributor.author Shah, M. G.
dc.contributor.author Mamun, A. A.
dc.contributor.author Hossen, M. R.
dc.date.accessioned 2018-09-04T05:01:41Z
dc.date.accessioned 2019-05-27T09:57:16Z
dc.date.available 2018-09-04T05:01:41Z
dc.date.available 2019-05-27T09:57:16Z
dc.date.issued 2015-05-06
dc.identifier.uri http://hdl.handle.net/20.500.11948/3034
dc.description.abstract The nonlinear propagation of cylindrical and spherical positron-acoustic solitary waves (PASWs) in an unmagnetized, collisionless, relativistic, degenerate plasma system that consists of nonrelativistic inertial cold positrons, relativistic degenerate electron and hot positron fluids, and positively-charged immobile ions has been investigated theoretically. By using a reductive perturbation technique, we derive the Korteweg-de Vries (K-dV) equation. The solitary wave solution has been numerically analyzed to comprehend the localized electrostatic disturbances. We observed that the effects of the degenerate pressure, relativity, and the number densities of inertial cold positrons, hot positrons, electrons, and positively-charged static ions notably modify the fundamental features of the cylindrical and the spherical PASWs. The implications of our results for dense plasmas in astrophysical compact objects (e.g., non-rotating white dwarfs, neutron stars, etc.) are briefly discussed. Full Text Link: https://doi.org/10.3938/jkps.66.1239 en_US
dc.language.iso en en_US
dc.publisher Springer en_US
dc.subject Positron-acoustic waves en_US
dc.subject Solitary waves en_US
dc.subject Compact objects en_US
dc.subject Degenerate pressure en_US
dc.subject K-dV equation en_US
dc.subject Relativistic factors en_US
dc.title Nonplanar solitons in a degenerate multi-species plasma en_US
dc.type Article en_US


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