Published August 15, 2017 | Version v1
Journal article

Thermodynamic analysis of a solar dish receiver using different nanofluids

  • 1. Department of Mechanic of Biosystems Engineering, University of Mohaghegh Ardabili, Ardabil (Iran, Islamic Republic of)
  • 2. Department of Mechanic of Biosystems Engineering, Tarbiat Modares University, Tehran (Iran, Islamic Republic of)
  • 3. Department of Renewable Energies, Faculty of New Sciences & Technologies, University of Tehran, Tehran (Iran, Islamic Republic of)

Description

Nanofluid application as the working fluid is proposed as a way for improving the solar system performance. In this study, a dish concentrator with a cylindrical cavity receiver was numerically modeled. Four different nanofluids including Al2O3/thermal oil, Cu/thermal oil, SiO2/thermal oil, and TiO2/thermal oil, were investigated as the working fluid of the solar system. The effects of the nanoparticles concentration in the range of 0–5% on the first and second law of the thermodynamic were considered in this study. The results indicated that the thermal efficiency decreased with increasing nanoparticle volume concentration. Also, the calculated results showed that the obtained exergy and efficiency of exergy improved by increasing the nanofluid concentrations. And it can be concluded from results that the entropy generation reduced with increasing nanofluid concentrations. The Bejan number increased with enhancing the nanoparticles volume fraction. In general Cu/thermal oil nanofluid has best exergy manner among the investigated nanofluid in the cylindrical cavity receiver. - Highlights: • A cylindrical cavity receiver was numerically modeled with different nanofluids. • The first and second law of the thermodynamic were investigated. • The system performance was considered using four different nanofluids. • Al2O3, Cu, SiO2, and TiO2 were investigated as the nanoparticles. • Thermal oil was used as the base fluid.

Availability note (English)

Available from http://dx.doi.org/10.1016/j.energy.2017.05.016

Additional details

Identifiers

DOI
10.1016/j.energy.2017.05.016;
PII
S0360-5442(17)30762-4;

Publishing Information

Journal Title
Energy (Oxford)
Journal Volume
133
Journal Page Range
p. 749-760
ISSN
0360-5442
CODEN
ENEYDS

Optional Information

Copyright
Copyright (c) 2017 Elsevier Science B.V., Amsterdam, The Netherlands, All rights reserved.