POSYDON is a next-generation single and binary-star population synthesis code incorporating full stellar structure and evolution modeling with the use of MESA.
In some cases, CC1 or CC2 occurs twice in the evolutionary pathway, after which the model ends, for example, ZAMS_CC1_CC1. This is a result of the model failing in step_SN due to the following error: The SN type is not ECSN neither CCSN.
This is a result from the interpolator in the step_HMS_HMS returning None for the SN_type, associated with the star undergoing the collapse. This is unexpected, because these stars are sufficiently massive to undergo a CC- or ECSN.
Moreover, the interpolator is predicting that this system becomes a BH.
Manually performing the collapse returns that this system should undergo a CCSN.
The questions we would like to get clear before fixing these systems:
Is the interpolator incorrectly predicting the SN type?
If so, how should this be handled? Should these systems manually be recalculated? Should the interpolator be retrained?
In some cases,
CC1
orCC2
occurs twice in the evolutionary pathway, after which the model ends, for example,ZAMS_CC1_CC1
. This is a result of the model failing instep_SN
due to the following error:The SN type is not ECSN neither CCSN.
This is a result from the interpolator in the
step_HMS_HMS
returning None for theSN_type
, associated with the star undergoing the collapse. This is unexpected, because these stars are sufficiently massive to undergo a CC- or ECSN. Moreover, the interpolator is predicting that this system becomes a BH. Manually performing the collapse returns that this system should undergo a CCSN.The questions we would like to get clear before fixing these systems: