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Cited article:

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Spin period evolution of Vela pulsar based on the wind emission: Application to the long period radio pulsars GPM J1839‐10 (P = 21 min) and GLEAM‐X J1627 (P = 18 min)

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Inferring neutron star properties with continuous gravitational waves

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Monthly Notices of the Royal Astronomical Society 521 (2) 2103 (2023)
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Evolution of Spin Period and Magnetic Field of the Crab Pulsar: Decay of the Braking Index by the Particle Wind Flow Torque

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Revisiting the Magnetic Field Distribution of Normal Pulsars: Implications for the Multiple Origins for Neutron Stars

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Pulsar braking and the P–$\dot{P}$ diagram

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Monthly Notices of the Royal Astronomical Society 467 (3) 3493 (2017)
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45 years of rotation of the Crab pulsar

A. G. Lyne, C. A. Jordan, F. Graham-Smith, et al.
Monthly Notices of the Royal Astronomical Society 446 (1) 857 (2015)
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THE BRAKING INDEX OF PSR J1734–3333 AND THE MAGNETAR POPULATION

C. M. Espinoza, A. G. Lyne, M. Kramer, R. N. Manchester and V. M. Kaspi
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https://doi.org/10.1088/2041-8205/741/1/L13