Abstract
In the present research a simplified mathematical model for the solar thermal collectors is considered in the form of non-uniform unsteady stretching surface. The non-Newtonian Maxwell nanofluid model is utilized for the working fluid along with slip and convective boundary conditions and comprehensive analysis of entropy generation in the system is also observed. The effect of thermal radiation and variable thermal conductivity are also included in the present model. The mathematical formulation is carried out through a boundary layer approach and the numerical computations are carried out for Cuwater and TiO2-water nanofluids. Results are presented for the velocity, temperature and entropy generation profiles, skin friction coefficient and Nusselt number. The discussion is concluded on the effect of various governing parameters on the motion, temperature variation, entropy generation, velocity gradient and the rate of heat transfer at the boundary.
| Original language | English |
|---|---|
| Pages (from-to) | 123-136 |
| Number of pages | 14 |
| Journal | Central European Journal of Physics |
| Volume | 16 |
| Issue number | 1 |
| DOIs | |
| State | Published - 2018 |
| Externally published | Yes |
Bibliographical note
Publisher Copyright:© 2018 R. Sikora et al.
UN SDGs
This output contributes to the following UN Sustainable Development Goals (SDGs)
-
SDG 7 Affordable and Clean Energy
Keywords
- Maxwell-nanofluid
- Solar energy
- entropy generation
- partial slip
- thermal collectors
- thermal radiation
- variable thermal conductivity
ASJC Scopus subject areas
- General Physics and Astronomy
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