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    <name>Article</name>
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          <name>Title</name>
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              <text>Sensitivity analysis of heat transfer in nanoliquid with inclined magnetic field, exponential space-based heat source, convective heating, and slip effects</text>
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              <text>exponential space-related heat source parameter (ESHS); inclined magnetic field; nanofluid; nanoliquid; sensitivity analysis; slip effects</text>
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              <text>Sensitivity analysis of the rate of heat transport in the flow of nanoliquids over an elongated sheet using the response surface methodology (RSM) in combination with the face-centered central composite design. The flow is driven due to the velocity slip and the inclined magnetic field effects. Thermal analysis includes aspects of convective heating, Joule heating, viscous heating, and a space-dependent exponential heat source. The nanoliquid model consists of thermophoresis and random motion mechanisms. A set of coupled partial differential governance equations is rehabilitated into a set of ordinary differential equations using the appropriate transformation. Subsequent nonlinear problem is tackled numerically by utilizing finite difference code that employs the formula of four-stage Lobatto IIIa. The rate of heat transport is scrutinized by adopting RSM for three effectual parameters, namely magnetic field parameter ((Formula presented.)), angle of inclination ((Formula presented.)), and suction parameter (Formula presented.)). The velocity and temperature fields were found to be a decreasing function of an angle of inclination of the magnetic field. The velocity range is inversely related to the suction and flow aspects of velocity. Furthermore, the rate of heat transport is more sensitive to the suction parameter than to the magnetic field and to the angle of inclination of the magnetic field.  2020 Wiley Periodicals LLC</text>
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              <text>Mahanthesh B.; Thriveni K.</text>
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              <text>Heat Transfer, Vol-50, No. 3, pp. 2362-2379.</text>
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              <text>John Wiley and Sons Inc</text>
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              <text>2021-01-01</text>
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              <text>&lt;a href="https://doi.org/10.1002/htj.21982" target="_blank" rel="noreferrer noopener"&gt;https://doi.org/10.1002/htj.21982&lt;/a&gt;
&lt;br /&gt;&lt;br /&gt;&lt;a href="https://www.scopus.com/inward/record.uri?eid=2-s2.0-85092647375&amp;amp;doi=10.1002%2Fhtj.21982&amp;amp;partnerID=40&amp;amp;md5=0935e8a5128113851d9c69c242643bf3" target="_blank" rel="noreferrer noopener"&gt;https://www.scopus.com/inward/record.uri?eid=2-s2.0-85092647375&amp;amp;doi=10.1002%2fhtj.21982&amp;amp;partnerID=40&amp;amp;md5=0935e8a5128113851d9c69c242643bf3&lt;/a&gt;</text>
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              <text>ISSN: 26884534</text>
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              <text>English</text>
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              <text>Mahanthesh B., Department of Mathematics, CHRIST (Deemed to be University), Bangalore, Karnataka, India; Thriveni K., Department of Mathematics, CHRIST (Deemed to be University), Bangalore, Karnataka, India</text>
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