Bulletin of the American Physical Society
71st Annual Meeting of the APS Division of Fluid Dynamics
Volume 63, Number 13
Sunday–Tuesday, November 18–20, 2018; Atlanta, Georgia
Session M02: Reacting Flows: Experiments
8:00 AM–9:57 AM,
Tuesday, November 20, 2018
Georgia World Congress Center
Room: B203
Chair: Subith Vasu, University of Central Florida
Abstract ID: BAPS.2018.DFD.M02.4
Abstract: M02.00004 : High Pressure Methane Ignition Delay Measurements under Supercritical Carbon Dioxide Conditions*
8:39 AM–8:52 AM
Presenter:
Miad Karimi
(Georgia Inst of Tech)
Authors:
Miad Karimi
(Georgia Inst of Tech)
Bradley Ochs
(Georgia Inst of Tech)
Wenting Sun
(Georgia Inst of Tech)
Devesh Ranjan
(Georgia Inst of Tech)
An inquiry to be investigated for supercritical carbon dioxide (sCO2) oxy-combustion is how well existing chemical kinetic models perform as no experimental data exists at relevant conditions. Autoignition delays are reported for CH4/O2/CO2 mixtures above the CO2 critical pressure (up to 200 bar) and for a temperature range of 1139 to 1433 K. Experiments reveal that a widely used kinetic model, GRI 3.0, underpredicts the ignition delay by a factor of 3 at 100 bar. However, kinetic models Aramco 2.0, USC Mech II, HP-Mech, and FFCM1 are capable of predicting autoignition delays though previously not validated at this pressure. At 100 bar, CH3 recombination to form C2H6 through CH3+CH3+M=C2H6+M becomes dominant compared to direct oxidation to form CH3O. The branching ratio of these two reaction pathways dictates the autoignition delay. The experimental results at 200 bar however, shows that only one chemical kinetics mechanism could capture the ignition behavior. Simulation results using Aramco 2.0 kinetics mechanism is determined to have a reasonable agreements to predict ignition delay times at 200 bar and a temperature range of 1139 K to 1250 K. No chemical effect from CO2 on autoignition was observed at supercritical conditions.
*U.S. Department of Energy-Award Number:DE-FE0025174
To cite this abstract, use the following reference: http://meetings.aps.org/link/BAPS.2018.DFD.M02.4
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