In 1D neutron star burst models, rotation at up to 80% of break-up reduces peak density and pressure, shortens recurrence times by up to about 14%, broadens light curves by up to about 125%, and shifts nucleosynthesis endpoints by up to five mass units.
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Type I X-Ray Burst Models With Rotation
In 1D neutron star burst models, rotation at up to 80% of break-up reduces peak density and pressure, shortens recurrence times by up to about 14%, broadens light curves by up to about 125%, and shifts nucleosynthesis endpoints by up to five mass units.