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[ascl:1806.005] Indri: Pulsar population synthesis toolset

Indri models the population of single (not in binary or hierarchical systems) neutron stars. Given a starting distribution of parameters (birth place, velocity, magnetic field, period), the code moves a set of stars through time (by evolving spin period and magnetic field) and space (flying inside Galactic potential). Upon completion of the evolution a set of observables (radio flux, position, dispersion measure or amplitude of gravitational wave and its geometrical orientation) is computed and can be compared with a radio survey such as the Parkes Multibeam Survey.

Code site:
https://github.com/cieslar/Indri
Appears in:
http://adsabs.harvard.edu/abs/2018arXiv180302397C
Bibcode:
2018ascl.soft06005C

ascl:1806.005
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