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                <text>Marangoni convection radiative flow of dusty nanoliquid with exponential space dependent heat source</text>
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                <text>Average Nusselt Number; Dusty Fluid; Exponential Space Dependent Heat Source; Marangoni Convection; Nano Fluid; Thermal Radiation</text>
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                <text>The flow of liquids submerged with nanoparticles is of significance to industrial applications, specifically in nuclear reactors and the cooling of nuclear systems to improve energy efficiency. The application of nanofluids in water-cooled nuclear systems can result in a significant improvement of their economic performance and/or safety margins. Therefore, in this paper, Marangoni thermal convective boundary layer dusty nanoliquid flow across a flat surface in the presence of solar radiation is studied. A two phase dusty liquid model is considered. Unlike classical temperature-dependent heat source effects, an exponential space-dependent heat source aspect is considered. Stretching variables are utilized to transform the prevailing partial differential system into a nonlinear ordinary differential system, which is then solved numerically via the Runge-Kutta-Fehlberg approach coupled with a shooting technique. The roles of physical parameters are focused in momentum and heat transport distributions. Graphical illustrations are also used to consider local and average Nusselt numbers. We examined the results under both linear and quadratic variation of the surface temperature. Our simulations established that the impact of Marangoni flow is useful for an enhancement of the heat transfer rate.  2017</text>
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                <text>Mahanthesh B.; Gireesha B.J.; PrasannaKumara B.C.; Shashikumar N.S.</text>
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                <text>Nuclear Engineering and Technology, Vol-49, No. 8, pp. 1660-1668.</text>
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                <text>Korean Nuclear Society</text>
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                <text>2017-01-01</text>
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                <text>&lt;a href="https://doi.org/10.1016/j.net.2017.08.015" target="_blank" rel="noreferrer noopener"&gt;https://doi.org/10.1016/j.net.2017.08.015&lt;/a&gt;
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                <text>All Open Access; Gold Open Access</text>
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                <text>ISSN: 17385733</text>
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                <text>Mahanthesh B., Department of Mathematics, Christ University, Bangalore, 560029, India, Department of Studies and Research in Mathematics, Kuvempu University, Shankaraghatta, Shimoga, 577451, Karnataka, India; Gireesha B.J., Department of Studies and Research in Mathematics, Kuvempu University, Shankaraghatta, Shimoga, 577451, Karnataka, India; PrasannaKumara B.C., Government First Grade College, Chikkamagaluru, Koppa, 577126, Karnataka, India; Shashikumar N.S., Department of Studies and Research in Mathematics, Kuvempu University, Shankaraghatta, Shimoga, 577451, Karnataka, India</text>
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                <text>Cattaneo-Christov heat flux on UCM nanofluid flow across a melting surface with double stratification and exponential space dependent internal heat source</text>
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              <elementText elementTextId="137001">
                <text>Brownian motion and thermophoresis; Cattaneo-Christov heat flux model; Melting surface; Thermal and solutal stratification; UCM fluid; Variable fluid properties</text>
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                <text>Melting and exponential space dependent internal heat source effects on magnetohydrodynamic of upper convected Maxwell liquid towards a horizontal flat surface are addressed. The combined effect of Brownian motion and thermophoresis in nanofluid modeling are retained. The Cattaneo-Christov heat flux model is imposed. Impacts of thermal and solutal stratifications are also accounted. A set of similarity variables are utilized to form ordinary differential system from the prevailing partial differential equations. The problem of ordinary differential system is analyzed numerically through Runge-Kutta-Fehlberg based shooting method. Graphical results of pertinent parameters on the velocity, temperature and nanoparticle concentration are studied. Skin friction coefficient, local Nusselt number and Sherwood number are also addressed.  2017</text>
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                <text>Mahanthesh B.; Gireesha B.J.; Raju C.S.K.</text>
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              <elementText elementTextId="137004">
                <text>Informatics in Medicine Unlocked, Vol-9, pp. 26-34.</text>
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              <elementText elementTextId="137005">
                <text>Elsevier Ltd</text>
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                <text>&lt;a href="https://doi.org/10.1016/j.imu.2017.05.008" target="_blank" rel="noreferrer noopener"&gt;https://doi.org/10.1016/j.imu.2017.05.008&lt;/a&gt;
&lt;br /&gt;&lt;br /&gt;&lt;a href="https://www.scopus.com/inward/record.uri?eid=2-s2.0-85024828009&amp;amp;doi=10.1016%2Fj.imu.2017.05.008&amp;amp;partnerID=40&amp;amp;md5=e11e0c4081b431068bee5cecc2b08822" target="_blank" rel="noreferrer noopener"&gt;https://www.scopus.com/inward/record.uri?eid=2-s2.0-85024828009&amp;amp;doi=10.1016%2fj.imu.2017.05.008&amp;amp;partnerID=40&amp;amp;md5=e11e0c4081b431068bee5cecc2b08822&lt;/a&gt;</text>
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              <elementText elementTextId="137008">
                <text>All Open Access; Gold Open Access</text>
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                <text>ISSN: 23529148</text>
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                <text>English</text>
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                <text>Mahanthesh B., Department of Mathematics, Christ University, Bangalore, 560058, India; Gireesha B.J., Department of Studies and Research in Mathematics, Kuvempu University, Shankaraghatta, Shimoga, 577 451, Karnataka, India; Raju C.S.K., Department of Mathematics, Garden City University, Bangalore, 560049, India</text>
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          <element elementId="50">
            <name>Title</name>
            <description>A name given to the resource</description>
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              <elementText elementTextId="133362">
                <text>Marangoni convection in Casson liquid flow due to an infinite disk with exponential space dependent heat source and cross-diffusion effects</text>
              </elementText>
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          <element elementId="49">
            <name>Subject</name>
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              <elementText elementTextId="133363">
                <text>Casson fluid; Cross-diffusion; Exponential space dependent heat source (ESHS); Joule heating; Magnetohydrodynamics; Marangoni convection</text>
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                <text>Present work aims to investigate the features of the exponential space dependent heat source (ESHS) and cross-diffusion effects in Marangoni convective heat mass transfer flow due to an infinite disk. Flow analysis is comprised with magnetohydrodynamics (MHD). The effects of Joule heating, viscous dissipation and solar radiation are also utilized. The thermal and solute field on the disk surface varies in a quadratic manner. The ordinary differential equations have been obtained by utilizing Von Km transformations. The resulting problem under consideration is solved numerically via Runge-Kutta-Fehlberg based shooting scheme. The effects of involved pertinent flow parameters are explored by graphical illustrations. Results point out that the ESHS effect dominates thermal dependent heat source effect on thermal boundary layer growth. The concentration and temperature distributions and their associated layer thicknesses are enhanced by Marangoni effect.  2018</text>
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                <text>Mahanthesh B.; Gireesha B.J.; Shashikumar N.S.; Hayat T.; Alsaedi A.</text>
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              <elementText elementTextId="133366">
                <text>Results in Physics, Vol-9, pp. 78-85.</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.rinp.2018.02.020" target="_blank" rel="noreferrer noopener"&gt;https://doi.org/10.1016/j.rinp.2018.02.020&lt;/a&gt;
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              <elementText elementTextId="133370">
                <text>All Open Access; Gold Open Access</text>
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                <text>ISSN: 22113797</text>
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                <text>English</text>
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                <text>Mahanthesh B., Department of Mathematics, Christ University, Bangalore, 560029, India, Department of Studies and Research in Mathematics, Kuvempu University, Shimoga, 577451, India; Gireesha B.J., Department of Studies and Research in Mathematics, Kuvempu University, Shimoga, 577451, India; Shashikumar N.S., Department of Studies and Research in Mathematics, Kuvempu University, Shimoga, 577451, India; Hayat T., Department of Mathematics, Quaid-i-Azam University 45320, Islamabad, 44000, Pakistan, Nonlinear Analysis and Applied Mathematics (NAAM) Research Group, Department of Mathematics, Faculty of Science, King Abdulaziz University, Jeddah, 21589, Saudi Arabia; Alsaedi A., Nonlinear Analysis and Applied Mathematics (NAAM) Research Group, Department of Mathematics, Faculty of Science, King Abdulaziz University, Jeddah, 21589, Saudi Arabia</text>
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                <text>Marangoni convective MHD flow of SWCNT and MWCNT nanoliquids due to a disk with solar radiation and irregular heat source</text>
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                <text>Carbon-water nanoliquids; Exponential space dependent heat source; Marangoni convection; MHD; Viscous dissipation</text>
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                <text>Present study addresses the Marangoni transport of dissipating SWCNT and MWCNT nanofluids under the influence of magnetic force and radiation. A novel exponential space dependent heat source is considered. The flow is generated due to a disk with surface tension created by thermal gradient. The partial differential equations system governing the flow of carbon-water nanoliquids and heat transfer through Marangoni convection is established. Subsequent system is reduced to nonlinear ordinary boundary value problem via generalized Karman transformations. Numerical solutions are developed of the arising nonlinear problem via Runge-Kutta based shooting approach. Impacts of embedded parameters are focused on Nusselt number, velocity and heat transport distributions through graphical illustrations. Our simulations figured out that the heat transfer rate increased via Marangoni convection; however it is decayed by applied magnetic force. The temperature of SWCNT-H2O nanoliquid dominates MWCNT-H2O nanoliquid.  2017 Elsevier B.V.</text>
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                <text>Mahanthesh B.; Gireesha B.J.; Shashikumar N.S.; Shehzad S.A.</text>
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              <elementText elementTextId="135221">
                <text>Physica E: Low-Dimensional Systems and Nanostructures, Vol-94, pp. 25-30.</text>
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              <elementText elementTextId="135222">
                <text>Elsevier B.V.</text>
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                <text>&lt;a href="https://doi.org/10.1016/j.physe.2017.07.011" target="_blank" rel="noreferrer noopener"&gt;https://doi.org/10.1016/j.physe.2017.07.011&lt;/a&gt;
&lt;br /&gt;&lt;br /&gt;&lt;a href="https://www.scopus.com/inward/record.uri?eid=2-s2.0-85025449715&amp;amp;doi=10.1016%2Fj.physe.2017.07.011&amp;amp;partnerID=40&amp;amp;md5=c42c2ab58fa1adb13a30aae88743f010" target="_blank" rel="noreferrer noopener"&gt;https://www.scopus.com/inward/record.uri?eid=2-s2.0-85025449715&amp;amp;doi=10.1016%2fj.physe.2017.07.011&amp;amp;partnerID=40&amp;amp;md5=c42c2ab58fa1adb13a30aae88743f010&lt;/a&gt;</text>
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                <text>ISSN: 13869477; CODEN: PELNF</text>
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                <text>Mahanthesh B., Department of Mathematics, Christ University, Bangalore, 560029, India, Department of Studies and Research in Mathematics, Kuvempu University, Shankaraghatta, Shimoga, 577451, Karnataka, India; Gireesha B.J., Department of Studies and Research in Mathematics, Kuvempu University, Shankaraghatta, Shimoga, 577451, Karnataka, India; Shashikumar N.S., Department of Studies and Research in Mathematics, Kuvempu University, Shankaraghatta, Shimoga, 577451, Karnataka, India; Shehzad S.A., Department of Mathematics, COMSATS Institute of Information Technology, Sahiwal, 57000, Pakistan</text>
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          <element elementId="50">
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              <elementText elementTextId="135899">
                <text>Nonlinear three-dimensional stretched flow of an Oldroyd-B fluid with convective condition, thermal radiation, and mixed convection</text>
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          <element elementId="49">
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              <elementText elementTextId="135900">
                <text>convective boundary condition; heat source/sink; nonlinear thermal convection; nonlinear thermal radiation; Oldroyd-B fluid</text>
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                <text>The effect of non-linear convection in a laminar three-dimensional Oldroyd-B fluid flow is addressed. The heat transfer phenomenon is explored by considering the non-linear thermal radiation and heat generation/absorption. The boundary layer assumptions are taken into account to govern the mathematical model of the flow analysis. Some suitable similarity variables are introduced to transform the partial differential equations into ordinary differential systems. The Runge-Kutta-Fehlberg fourth- and fifth-order techniques with the shooting method are used to obtain the solutions of the dimensionless velocities and temperature. The effects of various physical parameters on the fluid velocities and temperature are plotted and examined. A comparison with the exact and homotopy perturbation solutions is made for the viscous fluid case, and an excellent match is noted. The numerical values of the wall shear stresses and the heat transfer rate at the wall are tabulated and investigated. The enhancement in the values of the Deborah number shows a reverse behavior on the liquid velocities. The results show that the temperature and the thermal boundary layer are reduced when the non-linear convection parameter increases. The values of the Nusselt number are higher in the non-linear radiation situation than those in the linear radiation situation.  2017, Shanghai University and Springer-Verlag Berlin Heidelberg.</text>
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              <elementText elementTextId="135902">
                <text>Mahanthesh B.; Gireesha B.J.; Shehzad S.A.; Abbasi F.M.; Gorla R.S.R.</text>
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              <elementText elementTextId="135903">
                <text>Applied Mathematics and Mechanics (English Edition), Vol-38, No. 7, pp. 969-980.</text>
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              <elementText elementTextId="135904">
                <text>Springer Netherlands</text>
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                <text>&lt;a href="https://doi.org/10.1007/s10483-017-2219-6" target="_blank" rel="noreferrer noopener"&gt;https://doi.org/10.1007/s10483-017-2219-6&lt;/a&gt;
&lt;br /&gt;&lt;br /&gt;&lt;a href="https://www.scopus.com/inward/record.uri?eid=2-s2.0-85018304997&amp;amp;doi=10.1007%2Fs10483-017-2219-6&amp;amp;partnerID=40&amp;amp;md5=608abfa01073d3eafb391145fb0edf2d" target="_blank" rel="noreferrer noopener"&gt;https://www.scopus.com/inward/record.uri?eid=2-s2.0-85018304997&amp;amp;doi=10.1007%2fs10483-017-2219-6&amp;amp;partnerID=40&amp;amp;md5=608abfa01073d3eafb391145fb0edf2d&lt;/a&gt;</text>
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              <elementText elementTextId="135907">
                <text>Restricted Access</text>
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                <text>ISSN: 2534827; CODEN: AMMEE</text>
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              <elementText elementTextId="135910">
                <text>English</text>
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              <elementText elementTextId="135912">
                <text>Mahanthesh B., Department of Mathematics, Christ University, Bangalore, 560029, Karnataka, India, Department of Studies and Research in Mathematics, Kuvempu University, Shankarghatta, 577451, Karnataka, India; Gireesha B.J., Department of Studies and Research in Mathematics, Kuvempu University, Shankarghatta, 577451, Karnataka, India; Shehzad S.A., Department of Mathematics, COMSATS Institute of Information Technology, Sahiwal, 57000, Pakistan; Abbasi F.M., Department of Mathematics, COMSATS Institute of Information Technology, Islamabad, 44000, Pakistan; Gorla R.S.R., Department of Mechanical and Civil Engineering, Purdue University Northwest, Indiana, 46391, United States</text>
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  <item itemId="16272" public="1" featured="0">
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      <name>Article</name>
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          <element elementId="50">
            <name>Title</name>
            <description>A name given to the resource</description>
            <elementTextContainer>
              <elementText elementTextId="124488">
                <text>Analysis of a magnetic field and Hall effects in nanoliquid flow under insertion of dust particles</text>
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          </element>
          <element elementId="49">
            <name>Subject</name>
            <description>The topic of the resource</description>
            <elementTextContainer>
              <elementText elementTextId="124489">
                <text>boundary layer flow; dusty fluid; Hall current; magnetohydrodynamics; mixed convection; nanoparticles</text>
              </elementText>
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          <element elementId="41">
            <name>Description</name>
            <description>An account of the resource</description>
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              <elementText elementTextId="124490">
                <text>In this study, the two-phase hydromagnetic flow of a viscous liquid through a suspension of dust and nanoparticles is considered. The influence of the Hall current is also taken into account. The similarity variables are utilized to transform the problem into one independent variable. The obtained expressions in one independent variable are solved through the RungeKuttaFehlberg scheme connected with the shooting procedure. The computed results are sketched for employing multiple values of physical constraints on the temperature and velocity of the nanofluid and dust phase. The characterization of various nanoparticles like Cu, Al2O3, TiO2, and Ag on velocities and temperatures of both phases is made through plots. A comparative analysis in the limiting approach is presented to justify the present solution methodology. The range of emerging parameters is taken as 0 ? l ? 3, 0.1 ? ?t ? 3, 0 ? m ? 2.5, 0 ? M2 ? 2, 0.1 ? ?v ? 3, 0 ? ? ? 0.4, and ?0.8 ? ? ? 0.8. From the study, it is revealed that ?t has theopposite effect on the temperature of dust and nanofluid phases. The Hall parameter mraisesthe profiles of velocities in the nanoliquid and dust phases. Also, it is found that the transverse velocities h(?) and H((?) andtemperatures ?(?) and ?p(?) rise for larger ?.  2020 Wiley Periodicals, Inc.</text>
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              <elementText elementTextId="124491">
                <text>Mahanthesh B.; Gireesha B.J.; Shehzad S.A.; Ibrar N.; Thriveni K.</text>
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            <description>A related resource from which the described resource is derived</description>
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              <elementText elementTextId="124492">
                <text>Heat Transfer, Vol-49, No. 3, pp. 1632-1648.</text>
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              <elementText elementTextId="124493">
                <text>John Wiley and Sons Inc</text>
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                <text>2020-01-01</text>
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                <text>&lt;a href="https://doi.org/10.1002/htj.21682" target="_blank" rel="noreferrer noopener"&gt;https://doi.org/10.1002/htj.21682&lt;/a&gt;
&lt;br /&gt;&lt;br /&gt;&lt;a href="https://www.scopus.com/inward/record.uri?eid=2-s2.0-85096188948&amp;amp;doi=10.1002%2Fhtj.21682&amp;amp;partnerID=40&amp;amp;md5=bba313589b1a1af5b1f5ce131a4a3327" target="_blank" rel="noreferrer noopener"&gt;https://www.scopus.com/inward/record.uri?eid=2-s2.0-85096188948&amp;amp;doi=10.1002%2fhtj.21682&amp;amp;partnerID=40&amp;amp;md5=bba313589b1a1af5b1f5ce131a4a3327&lt;/a&gt;</text>
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            <description>Information about rights held in and over the resource</description>
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              <elementText elementTextId="124496">
                <text>Restricted Access</text>
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                <text>ISSN: 26884534</text>
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              <elementText elementTextId="124499">
                <text>English</text>
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                <text>Mahanthesh B., Department of Mathematics, CHRIST (Deemed to be University), Bangalore, India; Gireesha B.J., Department of Studies and Research in Mathematics, Kuvempu University, Shimoga, India; Shehzad S.A., Department of Mathematics, COMSATS University Islamabad, Sahiwal, Pakistan; Ibrar N., Department of Mathematics, Faculty of Science, University of Sargodha, Sargodha, Pakistan; Thriveni K., Department of Mathematics, CHRIST (Deemed to be University), Bangalore, India</text>
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  <item itemId="16896" public="1" featured="0">
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          <description>The Dublin Core metadata element set is common to all Omeka records, including items, files, and collections. For more information see, http://dublincore.org/documents/dces/.</description>
          <elementContainer>
            <element elementId="50">
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              <description>A name given to the resource</description>
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                  <text>Articles</text>
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      <name>Article</name>
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          <element elementId="50">
            <name>Title</name>
            <description>A name given to the resource</description>
            <elementTextContainer>
              <elementText elementTextId="133181">
                <text>Nonlinear radiated MHD flow of nanoliquids due to a rotating disk with irregular heat source and heat flux condition</text>
              </elementText>
            </elementTextContainer>
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          <element elementId="49">
            <name>Subject</name>
            <description>The topic of the resource</description>
            <elementTextContainer>
              <elementText elementTextId="133182">
                <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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            <description>An account of the resource</description>
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              <elementText elementTextId="133183">
                <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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          <element elementId="39">
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            <description>An entity primarily responsible for making the resource</description>
            <elementTextContainer>
              <elementText elementTextId="133184">
                <text>Mahanthesh B.; Gireesha B.J.; Shehzad S.A.; Rauf A.; Kumar P.B.S.</text>
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            <name>Source</name>
            <description>A related resource from which the described resource is derived</description>
            <elementTextContainer>
              <elementText elementTextId="133185">
                <text>Physica B: Condensed Matter, Vol-537, pp. 98-104.</text>
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            <name>Publisher</name>
            <description>An entity responsible for making the resource available</description>
            <elementTextContainer>
              <elementText elementTextId="133186">
                <text>Elsevier B.V.</text>
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            <name>Date</name>
            <description>A point or period of time associated with an event in the lifecycle of the resource</description>
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              <elementText elementTextId="133187">
                <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;
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                <text>ISSN: 9214526; CODEN: PHYBE</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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                <text>Nonlinear radiative flow of casson nanoliquid past a cone and wedge with magnetic dipole: Mathematical model of renewable energy</text>
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              <elementText elementTextId="132625">
                <text>Casson fluid; Internal heat source; Magnetic dipole; Nanoparticles; Nonlinear solar radiation</text>
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                <text>Solar energy is an important source of energy for all the living things. Other sources of energy such as electricity and heat can be converted from solar radiation. The recent advanced technologies are utilized to convert solar energy into electricity. In this direction, nanoliquids are quite useful because they directly absorb or scatter solar radiation. Nanofluids are selected to be best aspirant for the development of renewable energy. They are successfully utilized in the processes of renewable energy. Due to such importance of nanofluids, we investigate the effects of nanoparticles on nonlinear convective and radiative flow of Casson liquid. Two cases are considered namely flow due to a cone and flow due to a wedge. In addition to traditional temperature dependent heat source aspect an exponential space dependent heat source effect is examined. Explicitly heat/mass transfer mechanism is analysed due to prescribed linear surface temperature/particles volume fraction. Problem formulation is presented using conservation laws of mass, momentum, energy and nanoparticles volume fraction under boundary layer approximations. The solutions to the dimensionless problem are computed via Runge-Kutta-Fehlberg based shooting method. Results are plotted and examined. The exponential space dependent and thermal dependent heat source aspects are dominates on thermal field. Further, heat and mass transfer rates are higher in case of flow created by cone than flow created by wedge. The liquid velocity is higher in the case of flow due to wedge than flow due to cone case.  2018 by American Scientific Publishers All rights reserved.</text>
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                <text>Mahanthesh B.; Gireesha B.J.; Sheikholeslami M.; Shehzad S.A.; Kumar P.B.S.</text>
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              <elementText elementTextId="132628">
                <text>Journal of Nanofluids, Vol-7, No. 6, pp. 1089-1100.</text>
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              <elementText elementTextId="132629">
                <text>American Scientific Publishers</text>
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                <text>2018-01-01</text>
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                <text>&lt;a href="https://doi.org/10.1166/jon.2018.1546" target="_blank" rel="noreferrer noopener"&gt;https://doi.org/10.1166/jon.2018.1546&lt;/a&gt;
&lt;br /&gt;&lt;br /&gt;&lt;a href="https://www.scopus.com/inward/record.uri?eid=2-s2.0-85047860979&amp;amp;doi=10.1166%2Fjon.2018.1546&amp;amp;partnerID=40&amp;amp;md5=6b2931cd01cd324ee2949db8db7f6334" target="_blank" rel="noreferrer noopener"&gt;https://www.scopus.com/inward/record.uri?eid=2-s2.0-85047860979&amp;amp;doi=10.1166%2fjon.2018.1546&amp;amp;partnerID=40&amp;amp;md5=6b2931cd01cd324ee2949db8db7f6334&lt;/a&gt;</text>
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                <text>ISSN: 2169432X</text>
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                <text>Mahanthesh B., Department of Mathematics, Christ University, Bangalore, 560029, India, Department of Studies and Research in Mathematics, Kuvempu University, Shankaraghatta, Shimoga, 577451, Karnataka, India; Gireesha B.J., Department of Mathematics, Christ University, Bangalore, 560029, India; Sheikholeslami M., Department of Mechanical Engineering, Babol Noshirvani University of Technology, Babol, 47148-71167, Iran; Shehzad S.A., Department of Mathematics, COMSATS Institute of Information Technology, Sahiwal, 57000, Pakistan; Kumar P.B.S., Department of Mathematics, Christ University, Bangalore, 560029, India</text>
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      <name>Article</name>
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        <elementContainer>
          <element elementId="50">
            <name>Title</name>
            <description>A name given to the resource</description>
            <elementTextContainer>
              <elementText elementTextId="131275">
                <text>Magnetohydrodynamic squeezing two-phase flow of particulate suspension in a rotating channel with transpiration cooling</text>
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          <element elementId="49">
            <name>Subject</name>
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              <elementText elementTextId="131276">
                <text>dusty liquid; fluidparticle suspension; Magnetohydrodynamics; rotation; squeezing flow; two-phase flow</text>
              </elementText>
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          <element elementId="41">
            <name>Description</name>
            <description>An account of the resource</description>
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                <text>This article addresses the time-dependent two-phase magnetohydrodynamic squeezing flow of dusty liquid. The fluid flow is considered in a rotating channel. The flow is constructed by squeezing of an upper plate and stretching of the lower plate and relevant equations are obtained. Numerical results are computed by utilizing shooting method along with the RKFehlberg scheme. The obtained solutions are validated by comparison with the existing analytical solutions. The effects of pertinent parameters on velocities of both phases are comprehensively discussed through graphical results. The numerical values of shear stress of both phases at lower and upper walls are also tabulated. Furthermore, the slope of the linear regression line through data points is determined in order to quantify the increase/decrease. Numerical simulations disclosed that the normal and transverse velocities are decreased due to stronger Coriolis force. It is also established that the velocities of the fluid phase are higher than that of the dust phase  IMechE 2018.</text>
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              <elementText elementTextId="131278">
                <text>Mahanthesh B.; Gireesha B.J.; Thammanna G.T.; Hayat T.; Alsaedi A.</text>
              </elementText>
            </elementTextContainer>
          </element>
          <element elementId="48">
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            <elementTextContainer>
              <elementText elementTextId="131279">
                <text>Proceedings of the Institution of Mechanical Engineers, Part C: Journal of Mechanical Engineering Science, Vol-233, No. 4, pp. 1224-1235.</text>
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          <element elementId="45">
            <name>Publisher</name>
            <description>An entity responsible for making the resource available</description>
            <elementTextContainer>
              <elementText elementTextId="131280">
                <text>SAGE Publications Ltd</text>
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            <name>Date</name>
            <description>A point or period of time associated with an event in the lifecycle of the resource</description>
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              <elementText elementTextId="131281">
                <text>2019-01-01</text>
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                <text>&lt;a href="https://doi.org/10.1177/0954406218771725" target="_blank" rel="noreferrer noopener"&gt;https://doi.org/10.1177/0954406218771725&lt;/a&gt;
&lt;br /&gt;&lt;br /&gt;&lt;a href="https://www.scopus.com/inward/record.uri?eid=2-s2.0-85047409262&amp;amp;doi=10.1177%2F0954406218771725&amp;amp;partnerID=40&amp;amp;md5=98e167f63b09be7de04b4322e6a46283" target="_blank" rel="noreferrer noopener"&gt;https://www.scopus.com/inward/record.uri?eid=2-s2.0-85047409262&amp;amp;doi=10.1177%2f0954406218771725&amp;amp;partnerID=40&amp;amp;md5=98e167f63b09be7de04b4322e6a46283&lt;/a&gt;</text>
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          <element elementId="47">
            <name>Rights</name>
            <description>Information about rights held in and over the resource</description>
            <elementTextContainer>
              <elementText elementTextId="131283">
                <text>Restricted Access</text>
              </elementText>
            </elementTextContainer>
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              <elementText elementTextId="131284">
                <text>ISSN: 9544062; CODEN: PMCSE</text>
              </elementText>
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            <name>Format</name>
            <description>The file format, physical medium, or dimensions of the resource</description>
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            <description>A language of the resource</description>
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              <elementText elementTextId="131286">
                <text>English</text>
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              <elementText elementTextId="131288">
                <text>Mahanthesh B., Department of Mathematics, Christ University, Bengaluru, Karnataka, India, Department of Studies and Research in Mathematics, Kuvempu University, Shankaraghatta, Shimoga, Karnataka, India; Gireesha B.J., Department of Studies and Research in Mathematics, Kuvempu University, Shankaraghatta, Shimoga, Karnataka, India; Thammanna G.T., Department of Studies and Research in Mathematics, Kuvempu University, Shankaraghatta, Shimoga, Karnataka, India; Hayat T., Department of Mathematics, Quaid-I-Azam University, Islamabad, Pakistan, Nonlinear Analysis and Applied Mathematics (NAAM) Research Group, Department of Mathematics, Faculty of Science, King Abdulaziz University, Jeddah, Saudi Arabia; Alsaedi A., Nonlinear Analysis and Applied Mathematics (NAAM) Research Group, Department of Mathematics, Faculty of Science, King Abdulaziz University, Jeddah, Saudi Arabia</text>
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  <item itemId="16867" public="1" featured="0">
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          <elementContainer>
            <element elementId="50">
              <name>Title</name>
              <description>A name given to the resource</description>
              <elementTextContainer>
                <elementText elementTextId="64">
                  <text>Articles</text>
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            </element>
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      <name>Article</name>
      <description>Faculty Publications -Articles</description>
    </itemType>
    <elementSetContainer>
      <elementSet elementSetId="1">
        <name>Dublin Core</name>
        <description>The Dublin Core metadata element set is common to all Omeka records, including items, files, and collections. For more information see, http://dublincore.org/documents/dces/.</description>
        <elementContainer>
          <element elementId="50">
            <name>Title</name>
            <description>A name given to the resource</description>
            <elementTextContainer>
              <elementText elementTextId="132777">
                <text>Nonlinear convection in nano Maxwell fluid with nonlinear thermal radiation: A three-dimensional study</text>
              </elementText>
            </elementTextContainer>
          </element>
          <element elementId="49">
            <name>Subject</name>
            <description>The topic of the resource</description>
            <elementTextContainer>
              <elementText elementTextId="132778">
                <text>Maxwell fluid; Nanoparticles; Non-linear convection; Nonlinear density temperature (NDT); Nonlinear thermal radiation; Three dimensional flow</text>
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            </elementTextContainer>
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              <elementText elementTextId="132779">
                <text>The combined effects of nonlinear thermal convection and radiation in 3D boundary layer flow of non-Newtonian nanofluid are scrutinized numerically. The flow is induced by the stretching of a flat plate in two lateral directions. The mechanism of heat and mass transport under thermophoretic and Brownian motion is elaborated via implementation of the thermal convective condition. The prevailing two-point nonlinear boundary value problem is reduced to a two-point ordinary differential problem by employing suitable similarity transformations. The solutions are computed by the implementation of homotopic scheme. At the end, a comprehensive parametric study has been conducted to analyze the typical trend of the solutions. It is found that the nanoparticle volume fraction and temperature profiles are stronger for the case of solar radiation in comparison with problem without radiation.  2017 Faculty of Engineering, Alexandria University</text>
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            <name>Creator</name>
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            <elementTextContainer>
              <elementText elementTextId="132780">
                <text>Mahanthesh B.; Gireesha B.J.; Thammanna G.T.; Shehzad S.A.; Abbasi F.M.; Gorla R.S.R.</text>
              </elementText>
            </elementTextContainer>
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              <elementText elementTextId="132781">
                <text>Alexandria Engineering Journal, Vol-57, No. 3, pp. 1927-1935.</text>
              </elementText>
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            <name>Publisher</name>
            <description>An entity responsible for making the resource available</description>
            <elementTextContainer>
              <elementText elementTextId="132782">
                <text>Elsevier B.V.</text>
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            <name>Date</name>
            <description>A point or period of time associated with an event in the lifecycle of the resource</description>
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              <elementText elementTextId="132783">
                <text>2018-01-01</text>
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              <elementText elementTextId="132784">
                <text>&lt;a href="https://doi.org/10.1016/j.aej.2017.03.037" target="_blank" rel="noreferrer noopener"&gt;https://doi.org/10.1016/j.aej.2017.03.037&lt;/a&gt;
&lt;br /&gt;&lt;br /&gt;&lt;a href="https://www.scopus.com/inward/record.uri?eid=2-s2.0-85018788652&amp;amp;doi=10.1016%2Fj.aej.2017.03.037&amp;amp;partnerID=40&amp;amp;md5=ab2fa8856f092ed84bfca11d6243514d" target="_blank" rel="noreferrer noopener"&gt;https://www.scopus.com/inward/record.uri?eid=2-s2.0-85018788652&amp;amp;doi=10.1016%2fj.aej.2017.03.037&amp;amp;partnerID=40&amp;amp;md5=ab2fa8856f092ed84bfca11d6243514d&lt;/a&gt;</text>
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            <name>Rights</name>
            <description>Information about rights held in and over the resource</description>
            <elementTextContainer>
              <elementText elementTextId="132785">
                <text>All Open Access; Gold Open Access</text>
              </elementText>
            </elementTextContainer>
          </element>
          <element elementId="46">
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            <description>A related resource</description>
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              <elementText elementTextId="132786">
                <text>ISSN: 11100168</text>
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            </elementTextContainer>
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            <name>Format</name>
            <description>The file format, physical medium, or dimensions of the resource</description>
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              <elementText elementTextId="132787">
                <text>Online</text>
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            </elementTextContainer>
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            <description>A language of the resource</description>
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              <elementText elementTextId="132788">
                <text>English</text>
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                <text>Mahanthesh B., Department of Mathematics, Christ University, Bangalore, 560029, India, Department of Studies and Research in Mathematics, Kuvempu University, Shankaraghatta 577451, Shimoga, Karnataka, India; Gireesha B.J., Department of Studies and Research in Mathematics, Kuvempu University, Shankaraghatta 577451, Shimoga, Karnataka, India; Thammanna G.T., Department of Studies and Research in Mathematics, Kuvempu University, Shankaraghatta 577451, Shimoga, Karnataka, India; Shehzad S.A., Department of Mathematics, COMSATS Institute of Information Technology, Sahiwal, 57000, Pakistan; Abbasi F.M., Department of Mathematics, COMSATS Institute of Information Technology, Islamabad, 44000, Pakistan; Gorla R.S.R., Department of Mechanical &amp;amp; Civil Engineering, Purdue University Northwest, Westville, 1401 S. U.S. 42, United States</text>
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                <text>Dynamics of magneto-nano third-grade fluid with brownian motion and thermophoresis effects in the pressure type die</text>
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                <text>The non-transient dynamics of the non-Newtonian third-grade liquid driven by pressure type die in the presence of nanoparticles is studied. The fluid is dissipating and its properties are taken as unvarying. The governing partial differential equations system is developed and they are numerically solved after non-dimensionalization. The significance of pertinent parameters on flow fields is analyzed and discussed. The thermal field shows dual behaviour in the flow domain due to the impact of magnetism, Brownian motion and thermophoresis.  2019 by American Scientific Publishers All rights reserved.</text>
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                <text>Mahanthesh B.; Joseph T.V.</text>
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                <text>Journal of Nanofluids, Vol-8, No. 4, pp. 870-875.</text>
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                <text>&lt;a href="https://doi.org/10.1166/jon.2019.1642" target="_blank" rel="noreferrer noopener"&gt;https://doi.org/10.1166/jon.2019.1642&lt;/a&gt;
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                <text>ISSN: 2169432X</text>
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                <text>Mahanthesh B., Department of Mathematics, Christ [Deemed to be University], Bangalore, 560029, India; Joseph T.V., Department of Mathematics, Christ [Deemed to be University], Bangalore, 560029, India</text>
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                <text>Nonlinear convective and radiated flow of tangent hyperbolic liquid due to stretched surface with convective condition</text>
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            <name>Subject</name>
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              <elementText elementTextId="136875">
                <text>Heat source; Nonlinear convection; Nonlinear thermal radiation; Numerical solution; Tangent hyperbolic fluid</text>
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                <text>The current study compacts with effect of nonlinear convection and radiation on tangent hyperbolic fluid flow of through a convectively heated vertical surface. The converted set of boundary layer equations are solved numerically by Runge-Kutta-Fehlberg method. The effect of various pertinent parameters on flow and heat transfer characteristics are discussed with tabulated numerical values and deliberate figures. Additionally, the skin friction coefficient and Nusselt number are also presented. We noticed that, the skin friction factor and heat transfer rates are higher in presence of nonlinear convection than its absence. Further, velocity profile decreases by increasing power law index but establishes opposite results for skin friction.  2017</text>
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                <text>Mahanthesh B.; Kumar P.B.S.; Gireesha B.J.; Manjunatha S.; Gorla R.S.R.</text>
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              <elementText elementTextId="136878">
                <text>Results in Physics, Vol-7, pp. 2404-2410.</text>
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              <elementText elementTextId="136879">
                <text>Elsevier B.V.</text>
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                <text>&lt;a href="https://doi.org/10.1016/j.rinp.2017.07.012" target="_blank" rel="noreferrer noopener"&gt;https://doi.org/10.1016/j.rinp.2017.07.012&lt;/a&gt;
&lt;br /&gt;&lt;br /&gt;&lt;a href="https://www.scopus.com/inward/record.uri?eid=2-s2.0-85024928797&amp;amp;doi=10.1016%2Fj.rinp.2017.07.012&amp;amp;partnerID=40&amp;amp;md5=1567e7a7f16ae36a70544d9b466842c5" target="_blank" rel="noreferrer noopener"&gt;https://www.scopus.com/inward/record.uri?eid=2-s2.0-85024928797&amp;amp;doi=10.1016%2fj.rinp.2017.07.012&amp;amp;partnerID=40&amp;amp;md5=1567e7a7f16ae36a70544d9b466842c5&lt;/a&gt;</text>
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              <elementText elementTextId="136882">
                <text>All Open Access; Gold Open Access</text>
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                <text>ISSN: 22113797</text>
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                <text>Mahanthesh B., Department of Mathematics, Christ University, Bangalore, 560058, India; Kumar P.B.S., Department of Studies and Research in Mathematics, Kuvempu University, Shankaraghatta-577 451, Shimoga, Karnataka, India; Gireesha B.J., Department of Studies and Research in Mathematics, Kuvempu University, Shankaraghatta-577 451, Shimoga, Karnataka, India; Manjunatha S., Department of Engineering Mathematics, Faculty of Engineering, Christ University, Mysore Road, Bengaluru, 560074, India; Gorla R.S.R., Department of Mechanical and Civil Engineering, Purdue University, Northwest, Westville, 46391, IN, United States</text>
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              <elementText elementTextId="124153">
                <text>Significance of exponential space- and thermal-dependent heat source effects on nanofluid flow due to radially elongated disk with Coriolis and Lorentz forces</text>
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          <element elementId="49">
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            <description>The topic of the resource</description>
            <elementTextContainer>
              <elementText elementTextId="124154">
                <text>Buongiorno model; Exponential heat source; Nanofluid; Radial magnetic field; Rotating disk; Shooting method</text>
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                <text>In this paper, the nanofluid flow near an infinite disk which stretches in the radial direction in the presence of exponential space-based heat source (ESHS) and thermal-based heat source (THS) is investigated. The Brownian motion and thermophoresis effects are accounted to study the nanofluids. Effects of radial magnetism and the Coriolis force are also deployed. The pertinent nonlinear equations are approximated under boundary layer notion and modified von Km transformations. The subsequent nonlinear differential system is treated via shooting method. The impacts of controlling parameters on flow profiles are discussed and depicted with the aid of graphs. Results show that as the ESHS and THS parameters increase, the thermal field increases. However, ESHS phenomenon is highly influential than THS phenomenon on energy transport and its gradient. Further, it is found that thermophoresis slip mechanism has more effect on heat transport rate than the Brownian motion.  2019, Akadiai Kiad Budapest, Hungary.</text>
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                <text>Mahanthesh B.; Lorenzini G.; Oudina F.M.; Animasaun I.L.</text>
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                <text>Journal of Thermal Analysis and Calorimetry, Vol-141, No. 1, pp. 37-44.</text>
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                <text>&lt;a href="https://doi.org/10.1007/s10973-019-08985-0" target="_blank" rel="noreferrer noopener"&gt;https://doi.org/10.1007/s10973-019-08985-0&lt;/a&gt;
&lt;br /&gt;&lt;br /&gt;&lt;a href="https://www.scopus.com/inward/record.uri?eid=2-s2.0-85075329951&amp;amp;doi=10.1007%2Fs10973-019-08985-0&amp;amp;partnerID=40&amp;amp;md5=7be1b546d57dcdfbf52e55f11854f2d3" target="_blank" rel="noreferrer noopener"&gt;https://www.scopus.com/inward/record.uri?eid=2-s2.0-85075329951&amp;amp;doi=10.1007%2fs10973-019-08985-0&amp;amp;partnerID=40&amp;amp;md5=7be1b546d57dcdfbf52e55f11854f2d3&lt;/a&gt;</text>
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                <text>ISSN: 13886150; CODEN: JTACF</text>
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                <text>Mahanthesh B., Department of Mathematics, CHRIST (Deemed to be University), Bangalore, 560029, India; Lorenzini G., Department of Engineering and Architecture, University of Parma, Parco Area Delle Scienze 181/A, Parma, 43124, Italy; Oudina F.M., Department of Physics, Faculty of Sciences, University of 20 ao 1955 - Skikda, B.P 26 Road El-Hadaiek, Skikda, 21000, Algeria; Animasaun I.L., Fluid Dynamics Research Group, Department of Mathematical Sciences, Federal University of Technology, Akure, Nigeria</text>
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                <text>Effects of chemical reaction and partial slip on the three-dimensional flow of a nanofluid impinging on an exponentially stretching surface</text>
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                <text>The three-dimensional mixed convection boundary layer flow of a nanofluid induced by an exponentially stretching sheet is numerically investigated in the presence of thermal radiation, heat source/sink and first-order chemical reaction effects. The adopted nanofluid model incorporates the effects of Brownian motion and thermophoresis into the mathematical model. The first-order velocity slip boundary conditions are also taken into account. The governing boundary layer equations are transformed into a set of nonlinear ordinary differential equations by employing suitable similarity variables. The resultant equations are solved numerically using the Runge-Kutta-Fehlberg method. Obtained solutions are compared with previous results in a limiting sense from the literature, demonstrating an excellent agreement. To show the typical trend of the solutions, a parametric study is conducted. The axial velocity, transverse velocity, temperature and nanoparticle volume fraction profiles as well as the skin-friction coefficient, Nusselt and Sherwood numbers are demonstrated graphically as a representative set of numerical results and discussed comprehensively.  2017, SocietItaliana di Fisica and Springer-Verlag Berlin Heidelberg.</text>
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                <text>European Physical Journal Plus, Vol-132, No. 3</text>
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                <text>Mahanthesh B., Department of Mathematics, Christ University, Bangalore-29, Karnataka, India, Department of Studies and Research in Mathematics, Kuvempu University, Shimoga, Shankaraghatta, 577451, Karnataka, India; Mabood F., Department of Mathematics, University of Peshawar, Peshawar, Pakistan; Gireesha B.J., Department of Studies and Research in Mathematics, Kuvempu University, Shimoga, Shankaraghatta, 577451, Karnataka, India; Gorla R.S.R., Department of Mechanical and Civil engineering, Purdue University, Northwest, Westville, 46391, IN, United States</text>
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                <text>Flow of nanoliquid past a vertical plate with novel quadratic thermal radiation and quadratic Boussinesq approximation: Sensitivity analysis</text>
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              <elementText elementTextId="122066">
                <text>Modified Buongiorno model; Nanofluid; Nonlinear Boussinesq approximation; Quadratic thermal radiation; Response surface methodology; Sensitivity analysis</text>
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                <text>The effects of quadratic thermal radiation and quadratic Boussinesq approximation are investigated on the heat transport of a 36 nm Al2O3 ? H2O nanofluid over a vertical plate. The modified Buongiorno model is used in the analysis that includes the effectual thermophysical properties of the nanofluid and the key slip mechanisms. Experimentally verified correlations are used for the thermophysical properties. The reduced nonlinear differential problem is solved numerically by the Finite Difference Method (FDM). Flow profiles are displayed and analyzed for changes in dimensionless parameters. Further, the heat transfer flux at the wall is analyzed for interactive impacts of the buoyancy ratio, Brownian random motion, and thermophoresis parameters using the face-centered Central Composite Design (CCD) of the Response Surface Methodology (RSM). A sensitivity analysis is carried out for the heat transfer flux of the nanoliquid. Quadratic thermal radiation was found to improve the temperature profile. Furthermore, the mechanisms of Brownian random motion and thermophoresis have a negative sensitivity towards the rate of heat transfer. In various thermal applications like solar collectors, the density variation in terms of temperature differences is significantly high. Such phenomena can be accurately modeled by utilizing the quadratic Boussinesq approximation and the novel quadratic thermal radiation aspect.  2020 Elsevier Ltd</text>
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                <text>Mahanthesh B.; Mackolil J.</text>
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              <elementText elementTextId="122069">
                <text>International Communications in Heat and Mass Transfer, Vol-120</text>
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&lt;br /&gt;&lt;br /&gt;&lt;a href="https://www.scopus.com/inward/record.uri?eid=2-s2.0-85096471091&amp;amp;doi=10.1016%2Fj.icheatmasstransfer.2020.105040&amp;amp;partnerID=40&amp;amp;md5=38f3e1586362ae23c467840a919c49d0" target="_blank" rel="noreferrer noopener"&gt;https://www.scopus.com/inward/record.uri?eid=2-s2.0-85096471091&amp;amp;doi=10.1016%2fj.icheatmasstransfer.2020.105040&amp;amp;partnerID=40&amp;amp;md5=38f3e1586362ae23c467840a919c49d0&lt;/a&gt;</text>
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                <text>ISSN: 7351933; CODEN: IHMTD</text>
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                <text>Mahanthesh B., Department of Mathematics, CHRIST (Deemed to be University), Bengaluru, 560029, Karnataka, India; Mackolil J., Department of Mathematics, CHRIST (Deemed to be University), Bengaluru, 560029, Karnataka, India</text>
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          <element elementId="50">
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            <description>A name given to the resource</description>
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              <elementText elementTextId="117052">
                <text>Response surface optimization of heat transfer rate in Falkner-Skan flow of ZnO ? EG nanoliquid over a moving wedge: Sensitivity analysis</text>
              </elementText>
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          <element elementId="49">
            <name>Subject</name>
            <description>The topic of the resource</description>
            <elementTextContainer>
              <elementText elementTextId="117053">
                <text>Falkner-Skan flow; Nanoliquid; Response surface methodology; Sensitivity analysis</text>
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              <elementText elementTextId="117054">
                <text>In this work, the optimization of the heat transfer rate in the Falkner-Skan flow of ethylene glycol-based ZnO nanoliquid passing through a moving wedge is performed using the Response Surface Methodology (RSM). The experimentally estimated nanoliquid properties are included in the calculations for realistic modeling. The heat transfer rate is optimized through the use of the numerical experiment based on the face-centered central composite design (CCF). The sensitivity of the heat transfer rate is evaluated using the obtained quadratic model. The impact of the relevant parameters is displayed graphically using the finite difference method-based solution procedure and analyzed in detail. The interactive impacts of the key parameters are also evaluated using three-dimensional surface plots. The maximum sensitivity of the heat transfer rate is towards the moving wedge parameter. The optimized rate of heat transfer occurs at the high levels of the radiation aspect, moving wedge parameter, and nanoparticle volume fraction. The interactive impacts of the nanoparticles volume fraction and the Falkner-Skan index were found to be non-linear. The movement of the wedge was found to have a significant impact on both the flow field and the rate of heat transfer.  2021 Elsevier Ltd</text>
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                <text>Mahanthesh B.; Mackolil J.; Mallikarjunaiah S.M.</text>
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              <elementText elementTextId="117056">
                <text>International Communications in Heat and Mass Transfer, Vol-125</text>
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              <elementText elementTextId="117057">
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                <text>&lt;a href="https://doi.org/10.1016/j.icheatmasstransfer.2021.105348" target="_blank" rel="noreferrer noopener"&gt;https://doi.org/10.1016/j.icheatmasstransfer.2021.105348&lt;/a&gt;
&lt;br /&gt;&lt;br /&gt;&lt;a href="https://www.scopus.com/inward/record.uri?eid=2-s2.0-85106566886&amp;amp;doi=10.1016%2Fj.icheatmasstransfer.2021.105348&amp;amp;partnerID=40&amp;amp;md5=8d8a6d26be1f3e5174a59c780629e358" target="_blank" rel="noreferrer noopener"&gt;https://www.scopus.com/inward/record.uri?eid=2-s2.0-85106566886&amp;amp;doi=10.1016%2fj.icheatmasstransfer.2021.105348&amp;amp;partnerID=40&amp;amp;md5=8d8a6d26be1f3e5174a59c780629e358&lt;/a&gt;</text>
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                <text>Mahanthesh B., Department of Mathematics, CHRIST (Deemed to be University), Bengaluru, 560029, Karnataka, India; Mackolil J., Department of Mathematics, CHRIST (Deemed to be University), Bengaluru, 560029, Karnataka, India; Mallikarjunaiah S.M., Department of Mathematics and Statistics, Texas A&amp;amp;M University-Corpus Christi, Corpus Christi, 78412, TX, United States</text>
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          <element elementId="50">
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            <elementTextContainer>
              <elementText elementTextId="121981">
                <text>Significance of quadratic thermal radiation and quadratic convection on boundary layer two-phase flow of a dusty nanoliquid past a vertical plate</text>
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          <element elementId="49">
            <name>Subject</name>
            <description>The topic of the resource</description>
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              <elementText elementTextId="121982">
                <text>Boundary layer flow; Dusty fluid; Magnetohydrodynamics; Nanoliquid; Quadratic Boussinesq approximation; Quadratic thermal radiation</text>
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              <elementText elementTextId="121983">
                <text>Boundary layer two-phase flow of particulate Al2O3-H2O nanoliquid over a vertical flat plate is studied numerically subjected to the aspects of quadratic thermal convection and quadratic thermal radiation. The Khanafer-Vafai-Lightstone monophasic nanofluid model (KVL model) and Saffman's dusty fluid model are used for the equations governing the flow of dusty nanoliquids. The quadratic Boussinesq approximation is used together with the Prandtl's boundary layer approximation. The non-linear problem is treated with the finite difference method. Surface plots and streamlines are presented to visualize the results. A comparison of linear thermal radiation, quadratic thermal radiation, and nonlinear thermal radiation is performed. Among the three types of radiation, the greatest heat transfer is observed in nonlinear thermal radiation followed by quadratic thermal radiation and linear thermal radiation. Also, in the presence of quadratic convection, the heat transport, and velocity field get enhanced. It is found that the presence of Al2O3 nanoparticles of 3% volume concentration in particulate water effectively advances the heat transport of the system. However, heat transport gets reduced by increasing the mass fraction of dust particles. Furthermore, in the presence of a transverse magnetic field, the velocity of the dusty nanoliquid gets reduced.  2020</text>
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                <text>Mahanthesh B.; Mackolil J.; Radhika M.; Al-Kouz W.; Siddabasappa</text>
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              <elementText elementTextId="121985">
                <text>International Communications in Heat and Mass Transfer, Vol-120</text>
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                <text>Mahanthesh B., Department of Mathematics, CHRIST (Deemed to be University), Bengaluru, 560029, India; Mackolil J., Department of Mathematics, CHRIST (Deemed to be University), Bengaluru, 560029, India; Radhika M., Department of Mathematics, Government First Grade College, KGF, 563122, India; Al-Kouz W., Mechanical Engineering Department, Prince Mohammad bin Fahd University, Al Khobar, 31952, Saudi Arabia; Siddabasappa, Department of Mathematics, Government Science College, Bengaluru, 560019, India</text>
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                <text>Statistical analysis of stagnation-point heat flow in Williamson fluid with viscous dissipation and exponential heat source effects</text>
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                <text>exponential heat source; probable error; regression analysis; stagnation-point flow; viscous dissipation; Williamson fluid</text>
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                <text>This analysis explores the effect of the novel exponential space-dependent heat generation factor on the stagnation-point Williamson fluid flow over a stretchable surface. The heat transport phenomenon is carried out by the addition of viscous and Ohmic dissipations. Similarity transformations are applied to the nonlinear system of partial differential expressions that arise by the flow. The nonlinear ordinary differential system hence obtained is solved to visualize the role of different constraints graphically. Statistical methods such as correlation, probable error, and regression are utilized. The probable error is evaluated to calculate the reliability of the computed correlation factors. The study reveals that the velocity phenomenon is reduced by incrementing the Weissenberg parameter. The velocity of the hydromagnetic liquid is lesser than the velocity of magnetohydrodynamic fluid flow. Also, the higher heat generation factor gives a boost to the temperature of the flowing material.  2020 Wiley Periodicals LLC</text>
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                <text>Mahanthesh B.; Mackolil J.; Shehzad S.A.</text>
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                <text>ISSN: 26884534</text>
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                <text>Mahanthesh B., Department of Mathematics, CHRIST (Deemed to be University), Bengaluru, India; Mackolil J., Department of Mathematics, CHRIST (Deemed to be University), Bengaluru, India; Shehzad S.A., Department of Mathematics, COMSATS University Islamabad, Sahiwal, Pakistan</text>
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                <text>Exponential heat source effects on the stagnation-point heat transport of Williamson nanoliquid with nonlinear Boussinesq approximation</text>
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          <element elementId="49">
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                <text>correlation and probable error; exponential space-dependent heat source; nanofluid; nonlinear Boussinesq approximation; Williamson fluid</text>
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                <text>The nonlinear two-point partial differential boundary value problem associated with the nano-pseudoplastic material flow and heat transport subject to nonlinear Boussinesq approximation is computed and explored statistically. Heat transportation features are analyzed by the consideration of an exponential space-related heat source and the Buongiorno model of nanofluids. The boundary-driven expressions of the physical phenomenon are coupled and highly complicated due to the consideration of nonlinear convection terms. Reasonable variables are employed to reform the partial differential equations into a system of ordinary differential expressions and are solved numerically. Furthermore, correlation and regression techniques are employed for the statistical evaluation of the phenomenon. The probable error is implemented to calculate the reliability of the computed correlation factors. The exponential index and Schmidt number are positively correlated with the reduced skin friction coefficient whereas the other parameters are negatively correlated with it. The heat transfer rate is improved predominantly by the nonlinear thermal convection parameter. The temperature is enhanced by the intensification of the exponential-based heat source factor. The temperature and concentration profiles are boosted by incrementing the Biot number values.  2021 Wiley Periodicals LLC</text>
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                <text>Mahanthesh B.; Mackolil J.; Shehzad S.A.; Al-Kouz W.</text>
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                <text>Heat Transfer, Vol-50, No. 7, pp. 6645-6664.</text>
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                <text>&lt;a href="https://doi.org/10.1002/htj.22196" target="_blank" rel="noreferrer noopener"&gt;https://doi.org/10.1002/htj.22196&lt;/a&gt;
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                <text>Mahanthesh B., Department of Mathematics, CHRIST (Deemed to be University), Bengaluru, Karnataka, India; Mackolil J., Department of Mathematics, CHRIST (Deemed to be University), Bengaluru, Karnataka, India; Shehzad S.A., Department of Mathematics, COMSATS University Islamabad, Sahiwal, Pakistan; Al-Kouz W., Mechatronics Engineering Department, German Jordanian University, Amman, Jordan</text>
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          <element elementId="50">
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                <text>Two-phase flow of dusty Casson fluid with Cattaneo-Christov heat flux and heat source past a cone, wedge and plate</text>
              </elementText>
            </elementTextContainer>
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          <element elementId="49">
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              <elementText elementTextId="134589">
                <text>Casson fluid; Cattaneo-Christov heat flux; Cone; Dusty fluid; Exponential space-based heat source; Wedge</text>
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                <text>This article addresses the boundary layer flow and heat transfer in Casson fluid submerged with dust particles over three different geometries (vertical cone, wedge and plate). The aspects of Cattaneo-Christov heat flux and exponential space-based heat source (ESHS) are also accounted. At first, the partial differential equations are transformed into a set of ordinary differential equations via appropriate similarity transformations. Resulting equations are solved via shooting method coupled with the Runge-Kutta-Fehlberg-45 integration scheme. The consequences of dimensionless parameters on velocity and temperature fields of both fluid and dust particles phase are analyzed. The rate of increment/decrement in the skin friction as well as the Nusselt number for various values of physical parameters are also estimated via slope of linear regression line using data points.  2018 Trans Tech Publications, Switzerland.</text>
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              <elementText elementTextId="134591">
                <text>Mahanthesh B.; Makinde O.D.; Gireesha B.J.; Krupalakshmi K.L.; Animasaun I.L.</text>
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                <text>Defect and Diffusion Forum, Vol-387, pp. 625-639.</text>
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                <text>Trans Tech Publications Ltd</text>
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&lt;br /&gt;&lt;br /&gt;&lt;a href="https://www.scopus.com/inward/record.uri?eid=2-s2.0-85056525077&amp;amp;doi=10.4028%2Fwww.scientific.net%2FDDF.387.625&amp;amp;partnerID=40&amp;amp;md5=c892bc97ad7b34aa51f65819d7ca6abf" target="_blank" rel="noreferrer noopener"&gt;https://www.scopus.com/inward/record.uri?eid=2-s2.0-85056525077&amp;amp;doi=10.4028%2fwww.scientific.net%2fDDF.387.625&amp;amp;partnerID=40&amp;amp;md5=c892bc97ad7b34aa51f65819d7ca6abf&lt;/a&gt;</text>
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                <text>ISSN: 10120386; CODEN: DDAFE</text>
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              <elementText elementTextId="134599">
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                <text>Mahanthesh B., Department of Mathematics, Christ University, Bangalore, 560029, India; Makinde O.D., Faculty of Military Science, Stellenbosch University, Saldanha, 7395, South Africa; Gireesha B.J., Department of Studies and Research in Mathematics, Kuvempu University, Shankaraghatta, Shimoga, 577 451, Karnataka, India; Krupalakshmi K.L., Department of Studies and Research in Mathematics, Kuvempu University, Shankaraghatta, Shimoga, 577 451, Karnataka, India; Animasaun I.L., Department of Mathematical Sciences, Federal University of Technology, Akure, Nigeria</text>
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