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    <name>Article</name>
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              <text>Nonlinear radiated MHD flow of nanoliquids due to a rotating disk with irregular heat source and heat flux condition</text>
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              <text>AA7072-H&lt;sub&gt;2&lt;/sub&gt;O; Nanofluid; Nonlinear radiation; Rotating disk; Ti&lt;sub&gt;6&lt;/sub&gt;Al&lt;sub&gt;4&lt;/sub&gt;V</text>
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              <text>This research is made to visualize the nonlinear radiated flow of hydromagnetic nano-fluid induced due to rotation of the disk. The considered nano-fluid is a mixture of water and Ti6Al4V or AA7072 nano-particles. The various shapes of nanoparticles like lamina, column, sphere, tetrahedron and hexahedron are chosen in the analysis. The irregular heat source and nonlinear radiative terms are accounted in the law of energy. We used the heat flux condition instead of constant surface temperature condition. Heat flux condition is more relativistic and according to physical nature of the problem. The problem is made dimensionless with the help of suitable similarity constraints. The Runge-Kutta-Fehlberg scheme is adopted to find the numerical solutions of governing nonlinear ordinary differential systems. The solutions are plotted by considering the various values of emerging physical constraints. The effects of various shapes of nanoparticles are drawn and discussed.  2018 Elsevier B.V.</text>
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              <text>Mahanthesh B.; Gireesha B.J.; Shehzad S.A.; Rauf A.; Kumar P.B.S.</text>
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              <text>Physica B: Condensed Matter, Vol-537, pp. 98-104.</text>
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              <text>Elsevier B.V.</text>
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              <text>2018-01-01</text>
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              <text>&lt;a href="https://doi.org/10.1016/j.physb.2018.02.009" target="_blank" rel="noreferrer noopener"&gt;https://doi.org/10.1016/j.physb.2018.02.009&lt;/a&gt;
&lt;br /&gt;&lt;br /&gt;&lt;a href="https://www.scopus.com/inward/record.uri?eid=2-s2.0-85042006985&amp;amp;doi=10.1016%2Fj.physb.2018.02.009&amp;amp;partnerID=40&amp;amp;md5=cce3b2e5a9586fe7979723096e355ea0" target="_blank" rel="noreferrer noopener"&gt;https://www.scopus.com/inward/record.uri?eid=2-s2.0-85042006985&amp;amp;doi=10.1016%2fj.physb.2018.02.009&amp;amp;partnerID=40&amp;amp;md5=cce3b2e5a9586fe7979723096e355ea0&lt;/a&gt;</text>
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              <text>ISSN: 9214526; CODEN: PHYBE</text>
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              <text>Online</text>
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              <text>English</text>
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              <text>Mahanthesh B., Department of Mathematics, Christ University, Bangalore, 560029, India; Gireesha B.J., Department of Studies and Research in Mathematics, Kuvempu University, Shankaraghatta, Shimoga, 577 451, Karnataka, India; Shehzad S.A., Department of Mathematics, COMSATS Institute of Information Technology, Sahiwal, 57000, Pakistan; Rauf A., Department of Mathematics, COMSATS Institute of Information Technology, Sahiwal, 57000, Pakistan; Kumar P.B.S., Department of Studies and Research in Mathematics, Kuvempu University, Shankaraghatta, Shimoga, 577 451, Karnataka, India</text>
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