Stimulated Raman scattering of ultra intense hollow Gaussian beam in relativistic plasma
Effect of relativistic nonlinearity on stimulated Raman scattering (SRS) of laser beam propagating carrying null intensity in center [hollow Gaussian beam (HGB)] is studied in collisionless plasma. The construction of the equations is done employing the fluid theory which is developed with partial d...
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Veröffentlicht in: | Laser and particle beams 2015-09, Vol.33 (3), p.489-498 |
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description | Effect of relativistic nonlinearity on stimulated Raman scattering (SRS) of laser beam propagating carrying null intensity in center [hollow Gaussian beam (HGB)] is studied in collisionless plasma. The construction of the equations is done employing the fluid theory which is developed with partial differential equation and Maxwell's equations. The phenomenon of SRS is shown along with the excitation of seed plasma wave considering relativistic nonlinearity. The power of plasma wave is observed for higher order of HGB. The Raman back reflectivity is studied numerically for various orders of hollow Gaussian laser beam (HGLB) and the numerical analysis shows that these parameters play vital role on reflectivity characteristics. It is observed that the Raman back reflectivity is less for the higher order of HGLB. |
doi_str_mv | 10.1017/S0263034615000488 |
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The construction of the equations is done employing the fluid theory which is developed with partial differential equation and Maxwell's equations. The phenomenon of SRS is shown along with the excitation of seed plasma wave considering relativistic nonlinearity. The power of plasma wave is observed for higher order of HGB. The Raman back reflectivity is studied numerically for various orders of hollow Gaussian laser beam (HGLB) and the numerical analysis shows that these parameters play vital role on reflectivity characteristics. 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It is observed that the Raman back reflectivity is less for the higher order of HGLB.</description><subject>Collisionless plasmas</subject><subject>Gaussian beams (optics)</subject><subject>Investigations</subject><subject>Laser beams</subject><subject>Lasers</subject><subject>Localization</subject><subject>Magnetic fields</subject><subject>Mathematical analysis</subject><subject>Maxwell's equations</subject><subject>Nonlinearity</subject><subject>Numerical analysis</subject><subject>Partial differential equations</subject><subject>Particle beams</subject><subject>Plasma waves</subject><subject>Propagation</subject><subject>Raman scattering</subject><subject>Raman spectra</subject><subject>Reflectance</subject><subject>Reflectivity</subject><subject>Relativistic effects</subject><subject>Relativistic 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Beams</addtitle><date>2015-09-01</date><risdate>2015</risdate><volume>33</volume><issue>3</issue><spage>489</spage><epage>498</epage><pages>489-498</pages><issn>0263-0346</issn><eissn>1469-803X</eissn><abstract>Effect of relativistic nonlinearity on stimulated Raman scattering (SRS) of laser beam propagating carrying null intensity in center [hollow Gaussian beam (HGB)] is studied in collisionless plasma. The construction of the equations is done employing the fluid theory which is developed with partial differential equation and Maxwell's equations. The phenomenon of SRS is shown along with the excitation of seed plasma wave considering relativistic nonlinearity. The power of plasma wave is observed for higher order of HGB. The Raman back reflectivity is studied numerically for various orders of hollow Gaussian laser beam (HGLB) and the numerical analysis shows that these parameters play vital role on reflectivity characteristics. 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subjects | Collisionless plasmas Gaussian beams (optics) Investigations Laser beams Lasers Localization Magnetic fields Mathematical analysis Maxwell's equations Nonlinearity Numerical analysis Partial differential equations Particle beams Plasma waves Propagation Raman scattering Raman spectra Reflectance Reflectivity Relativistic effects Relativistic plasmas Scattering |
title | Stimulated Raman scattering of ultra intense hollow Gaussian beam in relativistic plasma |
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