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      KCI등재 SCI SCIE SCOPUS

      Modeling of Modified Electron-acoustic Solitary Waves in a Relativistic Degenerate Plasma

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      https://www.riss.kr/link?id=A104321014

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      다국어 초록 (Multilingual Abstract)

      The modeling of a theoretical and numerical study on the nonlinear propagation of modifiedelectron-acoustic (mEA) solitary waves has been carried out in an unmagnetized, collisionless, relativistic,degenerate quantum plasma (containing non-relativistic degenerate inertial cold electrons,both non-relativistic and ultra-relativistic degenerate hot electron and inertial positron fluids, andpositively-charged static ions). A reductive perturbation technique is used to derive the planar andthe nonplanar Korteweg-de Vries (K-dV) equations, which admit a localized wave solution for thesolitary profile. The solitary wave’s characteristics are found to have been influenced significantlyforin the non-relativistic and the ultra-relativistic limits. The mEA solitary waves are also foundto have been significantly modified due to the effects of the degenerate pressure and the numberdensities of this dense plasma’s constituents. The properties of the planar K-dV solitary wave arequite different from those of the nonplanar K-dV solitary wave. The relevance of our results toastrophysical objects (like white dwarfs and neutron stars), which are of scientific interest, is brieflymentioned.
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      The modeling of a theoretical and numerical study on the nonlinear propagation of modifiedelectron-acoustic (mEA) solitary waves has been carried out in an unmagnetized, collisionless, relativistic,degenerate quantum plasma (containing non-relativisti...

      The modeling of a theoretical and numerical study on the nonlinear propagation of modifiedelectron-acoustic (mEA) solitary waves has been carried out in an unmagnetized, collisionless, relativistic,degenerate quantum plasma (containing non-relativistic degenerate inertial cold electrons,both non-relativistic and ultra-relativistic degenerate hot electron and inertial positron fluids, andpositively-charged static ions). A reductive perturbation technique is used to derive the planar andthe nonplanar Korteweg-de Vries (K-dV) equations, which admit a localized wave solution for thesolitary profile. The solitary wave’s characteristics are found to have been influenced significantlyforin the non-relativistic and the ultra-relativistic limits. The mEA solitary waves are also foundto have been significantly modified due to the effects of the degenerate pressure and the numberdensities of this dense plasma’s constituents. The properties of the planar K-dV solitary wave arequite different from those of the nonplanar K-dV solitary wave. The relevance of our results toastrophysical objects (like white dwarfs and neutron stars), which are of scientific interest, is brieflymentioned.

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      참고문헌 (Reference)

      1 W. H. Lee, 632 : 421-, 2005

      2 S. Tasnim, 19 : 033706-, 2012

      3 H. R. Pakzad, 352 : 185-, 2014

      4 E. F. El-Shamy, 338 : 279-, 2012

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      8 D. B. Blaschke, 96 : 140402-, 2006

      9 P. Helander, 90 : 135004-, 2003

      10 M. Murklund, 78 : 591-, 2006

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      2 S. Tasnim, 19 : 033706-, 2012

      3 H. R. Pakzad, 352 : 185-, 2014

      4 E. F. El-Shamy, 338 : 279-, 2012

      5 J. -N. Han, 20 : 072109-, 2013

      6 M. R. Hossen, 44 : 673-, 2014

      7 B. Kozlovsky, 604 : 892-, 2004

      8 D. B. Blaschke, 96 : 140402-, 2006

      9 P. Helander, 90 : 135004-, 2003

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      49 M. S. Zobaer, 343 : 675-, 2013

      50 A. A. Mamun, 290 : 173-, 2001

      51 P. Chatterjee, 339 : 261-, 2012

      52 J. -N. Han, 21 : 012102-, 2014

      53 F. C. Michel, "Theory of Neutron Star Magnetospheres" University of Chicago Press 1990

      54 M. R. Hossen, "Nonlinear excitations in degenerate quantum plasmas" Lap-lambert Academic Publishing 2014

      55 S. L. Shapiro, "Black Holes, White Dwarfs, and Neutron Stars" John Wiley and Sons 1983

      56 H. R. Millar, "Active Galactive Nuclei" Springer 1987

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      2023 평가예정 해외DB학술지평가 신청대상 (해외등재 학술지 평가)
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      기준연도 WOS-KCI 통합IF(2년) KCIF(2년) KCIF(3년)
      2016 0.47 0.15 0.31
      KCIF(4년) KCIF(5년) 중심성지수(3년) 즉시성지수
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