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  <channel rdf:about="http://digitalrepository.fccollege.edu.pk/handle/123456789/96">
    <title>DSpace Collection: Physics</title>
    <link>http://digitalrepository.fccollege.edu.pk/handle/123456789/96</link>
    <description>Physics</description>
    <items>
      <rdf:Seq>
        <rdf:li rdf:resource="http://digitalrepository.fccollege.edu.pk/handle/123456789/2603" />
        <rdf:li rdf:resource="http://digitalrepository.fccollege.edu.pk/handle/123456789/2602" />
        <rdf:li rdf:resource="http://digitalrepository.fccollege.edu.pk/handle/123456789/2190" />
        <rdf:li rdf:resource="http://digitalrepository.fccollege.edu.pk/handle/123456789/2189" />
      </rdf:Seq>
    </items>
    <dc:date>2026-06-22T18:50:12Z</dc:date>
  </channel>
  <item rdf:about="http://digitalrepository.fccollege.edu.pk/handle/123456789/2603">
    <title>Brief Communication: A modified Korteweg–de Vries equation for Rossby–Khantadze waves in a sheared zonal flow of the ionospheric E layer</title>
    <link>http://digitalrepository.fccollege.edu.pk/handle/123456789/2603</link>
    <description>Title: Brief Communication: A modified Korteweg–de Vries equation for Rossby–Khantadze waves in a sheared zonal flow of the ionospheric E layer
Authors: Zafar Kahlon, Dr. Laila; Amir Shah, Dr. Hassan; David Kaladze, Tamaz; Tul Ain, Qura; Assad Bukhari, Syed
Abstract: The system of non-linear equations for electromagnetic Rossby–Khantadze waves in a weakly ionized&#xD;
conductive ionospheric E-layer plasma with sheared zonal flow is given. Use of multiple-scale analysis&#xD;
allows reduction of an obtained set of equations to a (1C1)D non-linear modified KdV (mKdV) equation with&#xD;
cubic non-linearity describing the propagation of solitary Rossby–Khantadze solitons.
Description: The system of non-linear equations for electromagnetic Rossby–Khantadze waves in a weakly ionized&#xD;
conductive ionospheric E-layer plasma with sheared zonal flow is given. Use of multiple-scale analysis&#xD;
allows reduction of an obtained set of equations to a (1C1)D non-linear modified KdV (mKdV) equation with&#xD;
cubic non-linearity describing the propagation of solitary Rossby–Khantadze solitons.</description>
    <dc:date>2024-01-01T00:00:00Z</dc:date>
  </item>
  <item rdf:about="http://digitalrepository.fccollege.edu.pk/handle/123456789/2602">
    <title>Effect of trapping in coupled kinetic Alfven-acoustic waves in a partially degenerate plasma with quantizing magnetic !eld</title>
    <link>http://digitalrepository.fccollege.edu.pk/handle/123456789/2602</link>
    <description>Title: Effect of trapping in coupled kinetic Alfven-acoustic waves in a partially degenerate plasma with quantizing magnetic !eld
Authors: Zafar Kahlon, Dr. Laila; Masood, W; Iqbal, Zeeshan; Amir Shah, Dr. Hassan; A Bukhari, S; Asam, MT
Abstract: Inclusion of a quantizing magnetic !eld in a partially degenerate plasma has interesting effects on the&#xD;
propagation of solitary and nonlinear periodic structures in coupled kinetic Alfven acoustic waves. In&#xD;
this paper, we use two-potential theory to investigate the nonlinear structures using Sagdeev potential&#xD;
approach and further analyze it using nonlinear dynamical methods. It is shown that the existence of&#xD;
solitary structure is sensitive to small temperature effects and quantizing magnetic !eld in a dense&#xD;
plasma with adiabatically trapped electrons. The work presented here is useful in understanding the&#xD;
low frequency wave propagation in a dense astrophysical environment like white dwarf stars and in&#xD;
low beta laboratory plasmas e.g. intense laser-plasma interactions.
Description: Inclusion of a quantizing magnetic !eld in a partially degenerate plasma has interesting effects on the&#xD;
propagation of solitary and nonlinear periodic structures in coupled kinetic Alfven acoustic waves. In&#xD;
this paper, we use two-potential theory to investigate the nonlinear structures using Sagdeev potential&#xD;
approach and further analyze it using nonlinear dynamical methods. It is shown that the existence of&#xD;
solitary structure is sensitive to small temperature effects and quantizing magnetic !eld in a dense&#xD;
plasma with adiabatically trapped electrons. The work presented here is useful in understanding the&#xD;
low frequency wave propagation in a dense astrophysical environment like white dwarf stars and in&#xD;
low beta laboratory plasmas e.g. intense laser-plasma interactions.</description>
    <dc:date>2023-01-01T00:00:00Z</dc:date>
  </item>
  <item rdf:about="http://digitalrepository.fccollege.edu.pk/handle/123456789/2190">
    <title>The impact of quantized magnetic pressure on the stimulated Brillouin scattering of electromagnetic waves</title>
    <link>http://digitalrepository.fccollege.edu.pk/handle/123456789/2190</link>
    <description>Title: The impact of quantized magnetic pressure on the stimulated Brillouin scattering of electromagnetic waves
Authors: Rozina, Ch; Maroosh, A; Poedts, S; Shah, H. A.
Abstract: Within the frame work of Landau quantization theory of Fermi gas, we formulate here the exotic&#xD;
physics of magnetic stimulated Brillouin scattering instability (MSBS) arising due to the nonlinear&#xD;
interaction of high frequency electromagnetic waves(EMWs)with degenerate, strongly magnetized&#xD;
electron-ion plasma. Quantum magneto hydrodynamic model (QMHD)is followed to develop the&#xD;
basic differential equations of quantized magnetosonic waves(QMWs)in the presence of super strong&#xD;
magnetic (SSH) field, whereas Maxwell equations are used to derive the governing differential&#xD;
equation of pump EMWs. The nonlinear interaction of EMWs and QMWs is addressed by employing&#xD;
the phasor matching technique. The obtained dispersion relation of MSBS shows that for a fixed&#xD;
density of fermions, the SSH field alone suppresses the MSBS instability as a function of quantized&#xD;
magneto ion velocity (CHe) and the Alfven speed (VA) via three-wave decay and modulational&#xD;
instabilities. However, for particular condition the MSBS instability is found to increase as a function&#xD;
of SSH field. Next, the analytical results are verified numerically and graphically for soft x-rays in the&#xD;
environment of neutron star. The present MSBS analysis may be critical in neutron stars, radio pulsars&#xD;
and magnetars having super strong magnetic field i.e. even larger than the quantum threshold value&#xD;
i.e, H ∼ 4.4 × 1013G, or in any application where the enhancement or suppression of SBS may be&#xD;
important.</description>
    <dc:date>2023-08-16T00:00:00Z</dc:date>
  </item>
  <item rdf:about="http://digitalrepository.fccollege.edu.pk/handle/123456789/2189">
    <title>Fast and slow magnetosonic shock waves in non-Maxwellian plasmas</title>
    <link>http://digitalrepository.fccollege.edu.pk/handle/123456789/2189</link>
    <description>Title: Fast and slow magnetosonic shock waves in non-Maxwellian plasmas
Authors: Izhar, Navaira; Qureshi, M.N.S.; Shi, J.K.; Shah, H. A.
Abstract: Obliquely propagating nonlinear fast and slow magnetosonic wave modes in a hot non-Maxwellian dissipative plasma are investigated in the current work. Modified &#xD;
temperatures have been derived for the non-extensive Q- and (r, q)-distributions that correspond to the physical properties of such non-Maxwellian plasmas. The &#xD;
reductive perturbation technique has been employed to derive the linear dispersion relation (LDR) and Kadomstev-Petvashvilli-Burgers (KPB) equation for slow and &#xD;
fast magnetosonic wave modes in two dimensions. We then investigated the effect of non-extensive parameter Q, spectral indices (r, q) and kinematic viscosity ν on &#xD;
the LDR and nonlinear propagation of KPB shock profiles for both the slow and fast mode magnetosonic waves. We found that linear and nonlinear propagation of &#xD;
fast and slow magnetosonic wave modes have been considerably modified in such non-Maxwellian plasmas. The results presented here would depict a realistic &#xD;
picture of the propagation of linear and nonlinear fast and slow magnetosonic wave modes in non-Maxwellian plasmas.</description>
    <dc:date>2023-10-12T00:00:00Z</dc:date>
  </item>
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