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<Article>
<Journal>
<PublisherName>OICC Press</PublisherName>
<JournalTitle>Journal of Theoretical and Applied Physics</JournalTitle>
<Issn>2251-7235</Issn>
<Volume>18</Volume>
<Issue>6</Issue>
<PubDate PubStatus="epublish">
<Year>2024</Year>
<Month>12</Month>
<Day>30</Day>
</PubDate>
</Journal>
<ArticleTitle>Laser-magnetized plasma interaction: inverse bremsstrahlung absorption with non-Maxwellian electrons</ArticleTitle>
<VernacularTitle></VernacularTitle>
<FirstPage>1</FirstPage>
<LastPage>6</LastPage>
<ELocationID EIdType="doi">10.57647/j.jtap.2024.1806.72</ELocationID>
<Language>EN</Language>
<AuthorList>
<Author>
<FirstName>Narges</FirstName>
<LastName>Firouzi-Farrashbandi</LastName>
<Affiliation>Department of Physics Education, Farhangian University, Tehran, Iran</Affiliation>
<Identifier Source="ORCID">https://orcid.org/0000-0002-8242-1153</Identifier>
</Author>
<Author>
<FirstName>Mohammad</FirstName>
<LastName>Eslami-Kalantari</LastName>
<Affiliation>Department of Physics, Yazd University, Yazd, Iran</Affiliation>
<Identifier Source="ORCID">https://orcid.org/0000-0002-8502-1796</Identifier>
</Author>
<Author>
<FirstName>Abdelaziz</FirstName>
<LastName>Sid</LastName>
<Affiliation>Laboratory of Physics of Radiations and Their Interaction with Matter (PRIMALAB), Department of Physics, Faculty of Matter Sciences, University of Batna 1, Batna, Algeria</Affiliation>
<Identifier Source="ORCID">https://orcid.org/0000-0001-9859-5185</Identifier>
</Author>
</AuthorList>
<PublicationType>Journal Article</PublicationType>
<History>
<PubDate PubStatus="received">
<Year>2024</Year>
<Month>12</Month>
<Day>30</Day>
</PubDate>
</History>
<Abstract>In this paper, q-parameterized nonextensive distribution is used to investigate various faces of the laser-magnetized plasma interactions including Inverse Bremsstrahlung Absorption (IBA). IBA process serves as an important way of delivering laser energy to plasma in laser fusion interactions. To do this, the Fokker-Planck equation and the q-nonextensive distribution function are used while a magnetic field is taken into account. As the maximum electron velocity in the limit of &amp;nbsp;goes to infinity, the q-nonextensive distribution function reduces to the standard Maxwelle-Boltzmann distribution. In this case, Laser and plasma parameters such as electron temperature, laser wavelength and nonextensivity degree are studied on IBA in magnetized plasma. Considering the existence of a static magnetic field, it is indicated that the IBA increases in the critical layer with a decrease in the laser wavelength and the strength of non-extensivity (q). But IBA varies slowly with the static magnetic field. Some instability can occur through the inverse bremsstrahlung absorption.</Abstract>
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<Param Name="value">Fusion</Param>
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<Object Type="keyword">
<Param Name="value">Magneto-inertial</Param>
</Object>
<Object Type="keyword">
<Param Name="value">Plasma</Param>
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<Object Type="keyword">
<Param Name="value">Inverse bremsstrahlung</Param>
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<Object Type="keyword">
<Param Name="value">q-nonextensive</Param>
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<Object Type="keyword">
<Param Name="value">Fokker-Planck</Param>
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</Article>
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