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Irreversibility analysis of magneto-thermogravitational convection of radiative hybrid nanofluid in a U-shaped curvilinear porous container with a T-shaped baffle

  • Samrat Hansda,
  • Anirban Chattopadhyay,
  • Swapan K. Pandit,
  • Mikhail A. Sheremet

摘要

In this study, we investigate the intricate dynamics of magneto-thermogravitational convection conjugated with entropy generation analysis within a U-shaped porous enclosure, enriched with the inclusion of a T-shaped cold baffle and a radiative hybrid nanofluid. Our investigation focuses on a configuration where a segment of the lower border is maintained at a warm temperature, while the rest of the border is subjected to adiabatic conditions, with the outer boundaries kept cold. Notably, we introduce a novel element to this setup: a T-shaped cooled baffle positioned at the cavity’s geometric center, introducing complexity to the U-shaped porous structure. The governing Navier–Stokes equations are effectively worked out by employing a higher-order compact technique. Rigorous validation of our in-house program against established experimental and computational benchmarks ensures the reliability of our simulations. Our analysis scrutinizes the impact of key parameters, including the Darcy number ( \(10^{-4} \le Da \le 10^{-2}\) 10 - 4 D a 10 - 2 ), Hartmann number ( \(0 \le Ha \le 50\) 0 H a 50 ), inclination of angle ( \(0^{0} \le \gamma \le 90^{0}\) 0 0 γ 90 0 ), Rayleigh number ( \(10^{4} \le Ra \le 10^{6}\) 10 4 R a 10 6 ), volumetric heat source/sink coefficient ( \(-10 \le Q \le 10\) - 10 Q 10 ), radiation parameter ( \(1 \le Rd \le 10\) 1 R d 10 ), length of the heater ( \(0.2 \le b \le 0.8\) 0.2 b 0.8 ) and solid volume fraction ( \(0.0 \le \phi _{\text{hnp}} \le 0.04\) 0.0 ϕ hnp 0.04 ) of the hybrid nanofluid. Visualization of our computed results through streamlines, isotherms, \(Nu_{\text{avg}}\) N u avg , \(E_\text{T}\) E T and Be offers deeper insights into the heat transfer phenomena. Optimal heat transfer conditions are identified at specific parameter combinations, such as \(b=0.2\) b = 0.2 , \(Ra=10^{6}\) R a = 10 6 , \(Da=10^{-2}\) D a = 10 - 2 , \(Ha=0\) H a = 0 , \(\gamma =90^{0}\) γ = 90 0 , \(Rd=10\) R d = 10 , \(Q=-10\) Q = - 10 and \(\phi _{\text{hnp}}=0.04\) ϕ hnp = 0.04 . Conversely, maximum total entropy generation occurs under different conditions, notably at \(b=0.8\) b = 0.8 , \(Ra=10^{6}\) R a = 10 6 , \(Da=10^{-2}\) D a = 10 - 2 , \(Ha=0\) H a = 0 , \(\gamma =90^{0}\) γ = 90 0 , \(Rd=10\) R d = 10 , \(Q=10\) Q = 10 and \(\phi _{\text{hnp}}=0.0\) ϕ hnp = 0.0 . Our outcomes allow a deeper understanding of convective energy transport phenomena in complex porous geometries with implications for various engineering applications.