Modeling Dense Particle Flow in Multistage and Obstructed Flow Receivers Using High Fidelity Simulations
DOI:
https://doi.org/10.52825/solarpaces.v2i.805Keywords:
Concentrating Solar Power, Particles, Falling Particle Receiver, CFD-DEM, Multistage Receiver, Obstructed Flow Receiver, Dense Particle FlowAbstract
Particles are a leading contender for next-generation, concentrating solar power technologies, and the design of the particle receiver is critical to minimize the levelized cost of electricity. Falling particle receivers (FPRs) are a viable receiver concept, but many new designs feature complex particle obstructions that include dense discrete phase flows. This creates additional challenges for modeling as particle-to-particle interactions (i.e., collisions) and particle drag become more complex. To improve upon existing modeling strategies, a CFD-DEM simulation capability was created by coupling two independent codes: Sierra/Fuego and LAMMPS. A suitable receiver model was then defined using a traditional continuum-based model for the air and a granular model for the particle curtain. A sensitivity study was executed using this model to determine the relevance of different granular model inputs on important quantities of interest in obstructed flow FPRs: the particle velocity and curtain opacity. The study showed that the granular model inputs had little effect on the particle velocity magnitude and curtain opacity after an obstruction.
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Copyright (c) 2024 Brantley Mills, Flint Pierce, Eldwin Djajadiwinata, Rageh Saeed, Shaker Alaqel, Nader Saleh
This work is licensed under a Creative Commons Attribution 4.0 International License.
Accepted 2024-07-10
Published 2024-08-28
Funding data
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Solar Energy Technologies Office
Grant numbers 39637 -
Department of Energy National Nuclear Security Administration Laboratory Residency Graduate Fellowship
Grant numbers DE-NA0003525