Using the KEPLER hydrodynamics code , 464 models of thermonuclear X-ray bursters were performed across a range of accretion rates and compositions .
We present the library of simulated burst profiles from this sample , and examine variations in the simulated lightcurve for different model conditions .
We find that the recurrence time varies as a power law against accretion rate , and measure its slope while mixed H/He burning is occurring for a range of metallicities , finding the power law gradient to vary from \eta = 1.1 to 1.24 .
We also identify the accretion rates at which mixed H/He burning stops and a transition occurs to different burning regimes .
We also explore how varying the accretion rate and metallicity affects burst morphology in both the rise and tail .