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This is a Quantitative Study study.

Binary population synthesis of the Galactic canonical pulsar population

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Binary population synthesis models radio and γ-ray pulsar populations, highlighting natal kick effects.

Models demonstrate strong agreement with observed radio and γ-ray pulsar populations in the Galaxy.
The reproduction of the radio-loud to radio-quiet γ-ray pulsar ratio aligns well with catalogued data.
Analysis identifies a correlation between pulsar latitude and spin-down luminosity due to natal kicks at birth.
Findings support the idea of low spin-down luminosity pulsars potentially emitting weak γ-rays.

Song et al. (2025) studied this question.

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