cc_controls

model_name

Name of supernova model to use when a star reaches the core-collapse stage. Possible values are rapid, delayed, startrack and combine. The first three can be found here (see Section 4), while a reference for the latter is this one.

model_name = 'rapid'

max_ns_mass

Maximum value for the mass of a neutron-star in solar masses. Needed for the prescriptions found in Fryer et al. paper.

max_ns_mass = 2.5d0

report_core_collapse

Flag to report on the terminal information of the core-collapse calculations

report_core_collapse = .false.

cc_data_directory

Name of the direcotry where core-collapse information will be saved.

cc_data_directory = 'cc_data'

filename_for_star_data

Name of the file containing information of the collapsing star at the core-collapse stage.

filename_for_star_data = 'star_at_core_collapse'

filename_for_binary_data

Name of the file with information of the binary system at core-collapse.

filename_for_binary_data = 'binary_at_core_collapse'