Ion acoustic solitons in dense magnetized plasmas with nonrelativistic degenerate electrons and positrons

• Autor(a) principal: Sadiq, Safeer
• Data de Publicação: 2014
• Outros Autores: Mahmood, Shahzad, Haque, Q., Ali, Munazza Zulfiqar
• Tipo de documento: Artigo
• Idioma: eng
• Título da fonte: Repositório Institucional da UFRGS
• Texto Completo: http://hdl.handle.net/10183/108040
• topic: Plasmas relativisticos; Plasmas astrofisicos; Sólitons em plasmas; Pulsars; Relações de dispersão; Ondas íon-acústicas em plasmas; Atmosferas estelares; Plasmas; Pulsars: general; Stars: atmospheres; Waves

The propagation of electrostatic waves in a densemagnetized electron–positron–ion (EPI) plasma with nonrelativistic and ultrarelativistic degenerate electrons and positrons is investigated. The linear dispersion relation is obtained for slow and fast electrostatic waves in the EPI plasma. The limiting cases for ion acoustic wave (slow) and ion cyclotron wave (fast) are also discussed. Using the reductive perturbation method, two-dimensional propagation of ion acoustic solitons is found for both the nonrelativistic and ultrarelativistic degenerate electrons and positrons. The effects of positron concentration, magnetic field, and mass of ions on ion acoustic solitons are shown in numerical plots. The proper form of Fermi temperature for nonrelativistic and ultrarelativistic degenerate electrons and positrons is employed, which has not been used in earlier published work. The present investigation is useful for the understanding of linear and nonlinear electrostatic wave propagation in the dense magnetized EPI plasma of compact stars. For illustration purposes, we have applied our results to a pulsar magnetosphere.