Statistical modeling of cavitation inception
Abstract
Details
- Title: Subtitle
- Statistical modeling of cavitation inception
- Creators
- Mehedi Hasan Bappy
- Contributors
- Pablo Carrica (Advisor)Jiajia Li (Advisor)Joseph Katz (Committee Member)Ching-Long Lin (Committee Member)James Buchholz (Committee Member)George Constantinescu (Committee Member)
- Resource Type
- Dissertation
- Degree Awarded
- Doctor of Philosophy (PhD), University of Iowa
- Degree in
- Mechanical Engineering
- Date degree season
- Spring 2022
- DOI
- 10.17077/etd.006449
- Publisher
- University of Iowa
- Number of pages
- xvi, 155 pages
- Copyright
- Copyright 2022 Mehedi Hasan Bappy
- Language
- English
- Description bibliographic
- Includes bibliographical references (pages 149-155).
- Public Abstract (ETD)
Cavitation is the phenomenon of bubbles growing when the liquid pressure drops below vapor pressure. Cavitation is mostly undesirable and fluid engineering systems are often designed to avoid it, so proper prediction of the cavitation inception point is important. This thesis presents a cavitation inception model that includes pressure fluctuations at the sub-grid scale (SGS) level in CFD simulations. As turbulence models look to predict the momentum transfer at the resolved scales by approximating the SGS turbulence behavior, the model presented in this thesis seeks to predict the cavitation inception at the SGS level. To this end, the SGS flow field is modeled as homogeneous isotropic turbulence (HIT), dependent on the unresolved turbulence Taylorscale Reynolds number Reλ. Direct numerical simulations (DNS) of HIT up to Reλ = 240 were performed, tracking nuclei with sizes between 0.1 and 150 μm and solving the Rayleigh-Plesset equation on the time histories of the nuclei to predict bubble cavitation rates at different absolute pressures. The behavior of the pressure on the nuclei in HIT was studied, including pressure probability density functions, low-pressure event frequency and duration, and effect of nuclei size on these parameters. It is found that low-pressure events are more likely as Reλ and the nuclei size increase. A table providing cavitation rate as a function of Reλ, nuclei radius, turbulent kinetic energy dissipation rate, and pressure was generated to use for predicting cavitation inception in complex CFD problems. The model can predict the effect of unresolved pressure fluctuations, which typically increases the cavitation inception number when compared to CFD predictions that use the minimum flow pressure to predict inception, but it can also predict a lower cavitation inception number for highly resolved LES simulations where very low pressure events are rare and small in volume. The model was tested for high Reλ HIT turbulence and a backward facing step, showing satisfactory comparisons with experiments.
- Academic Unit
- Mechanical Engineering
- Record Identifier
- 9984271254402771