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Transitional millisecond pulsars

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arxiv 2010.09060 v2 pith:LIO7K5TT submitted 2020-10-18 astro-ph.HE

Alessandro Papitto , Domitilla de Martino This is my paper · ORCID
classification astro-ph.HE
keywords millisecondpulsarstransitionalbinariesradiosystemstightaccreting
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Millisecond pulsars in tight binaries have recently opened new challenges in our understanding of physical processes governing the evolution of binaries and the interaction between astrophysical plasma and electromagnetic fields. Transitional systems that showed changes from rotation-powered to accretion powered states and vice versa have bridged the populations of radio and accreting millisecond pulsars, eventually demonstrating the tight evolutionary link envisaged by the recycling scenario. A decade of discoveries and theoretical efforts have just grasped the complex phenomenology of transitional millisecond pulsars from the radio to the gamma-ray band. This review summarises the main properties of the three transitional millisecond pulsars discovered so far, as well as of candidates and related systems, discussing the various models proposed to cope with the multifaceted behaviour.

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Forward citations

Cited by 5 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. SRG/eROSITA X-ray selected cataclysmic variable candidates observed in SDSS-V DR20

    astro-ph.SR 2026-07 conditional novelty 6.0 of 10

    eROSITA-selected SDSS-V DR20 spectroscopy yields 587 cataclysmic variables (274 known), including new nearby systems, AM CVns, and a low-accretion-rate polar.

  2. Fast optical spectroscopic observations of PSR J1023+0038 over one orbital period

    astro-ph.HE 2026-07 accept novelty 6.0 of 10

    Full-orbit minute-cadence optical spectroscopy of PSR J1023+0038 reveals short-timescale line variability and asymmetric Doppler maps consistent with outflows.

  3. An energy approach to pulsar-disc interaction: disc stability and implications for transitional millisecond pulsars

    astro-ph.HE 2025-05 conditional novelty 5.0 of 10

    Axisymmetric SPH-MHD simulations show accretion discs around oblique millisecond pulsars are disrupted when the inner disc radius lies well beyond the light cylinder, confirming the Ekşi and Alpar stability diagram.

  4. Understanding the Neutron Star Population with the SKAO Telescopes

    astro-ph.HE 2026-07 accept novelty 3.5 of 10

    SKAO AA* and AA4 surveys are projected to discover thousands of ordinary pulsars and ~800–1000 MSPs, enabling population synthesis, mass measurements and tests of gravity and emission physics.

  5. Probing Neutron Star Interiors and the Properties of Cold Ultra-dense Matter with the SKAO

    astro-ph.HE 2026-07 accept novelty 3.5 of 10

    SKAO's sensitivity, surveys and sub-arraying will deliver tighter NS mass, MoI, spin, glitch and precession constraints that, with X-ray and GW data, probe cold ultra-dense matter.

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