Author
Listed:
- Li, Haoran
- Jia, Ming
- Ding, Rui
- Li, Xinyi
- Zhang, Zonghan
- Zhang, Yanzhi
Abstract
The Kelvin-Helmholtz Rayleigh-Taylor (KH-RT) model, widely used for spray breakup simulations, relies on some idealized assumptions (e.g., neglect fuel viscosity and surface tension), necessitating case-specific manual tuning that introduces substantial prediction uncertainties in spray simulations. This is critical because spray simulation accuracy directly impacts the in-cylinder mixture formation, combustion, and ultimately the performance predictions of power equipment. To address this issue, this study establishes a data-driven correlation between the breakup length constant Cb and two key parameters (i.e., ambient density ρg and fuel kinematic viscosity νl) through Non-dominated Sorting Genetic Algorithm II (NSGA-II), which can be expressed as Cb = 0.075⋅νl3⋅ln(ρg)+4.74. The proposed correlation is first verified by the analytical solution of Cb, demonstrating good agreement in both magnitude and trend. Furthermore, large-scale validation using 563 cases was conducted, confirming that spray features of the eight fuels (i.e., diesel, gasoline, biodiesel, DME, methanol, PODE, ammonia, and n-butanol) under various conditions can be accurately captured by the improved KH-RT model without manual parameter tuning. The impacts of fuel properties and ambient conditions on breakup length, along with their influences on spray development, were finally investigated. The improved KH-RT model eliminates empirical parameter tuning, significantly reducing both computational time and spray prediction uncertainties, thereby improving power equipment performance predictions.
Suggested Citation
Li, Haoran & Jia, Ming & Ding, Rui & Li, Xinyi & Zhang, Zonghan & Zhang, Yanzhi, 2025.
"An improved Kelvin-Helmholtz Rayleigh-Taylor (KH-RT) breakup model with wide fuel applicability based on data-driven techniques,"
Energy, Elsevier, vol. 334(C).
Handle:
RePEc:eee:energy:v:334:y:2025:i:c:s0360544225033031
DOI: 10.1016/j.energy.2025.137661
Download full text from publisher
As the access to this document is restricted, you may want to
for a different version of it.
Corrections
All material on this site has been provided by the respective publishers and authors. You can help correct errors and omissions. When requesting a correction, please mention this item's handle: RePEc:eee:energy:v:334:y:2025:i:c:s0360544225033031. See general information about how to correct material in RePEc.
If you have authored this item and are not yet registered with RePEc, we encourage you to do it here. This allows to link your profile to this item. It also allows you to accept potential citations to this item that we are uncertain about.
We have no bibliographic references for this item. You can help adding them by using this form .
If you know of missing items citing this one, you can help us creating those links by adding the relevant references in the same way as above, for each refering item. If you are a registered author of this item, you may also want to check the "citations" tab in your RePEc Author Service profile, as there may be some citations waiting for confirmation.
For technical questions regarding this item, or to correct its authors, title, abstract, bibliographic or download information, contact: Catherine Liu (email available below). General contact details of provider: http://www.journals.elsevier.com/energy .
Please note that corrections may take a couple of weeks to filter through
the various RePEc services.