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Radio Pulsar Sub-Populations (II) : The Mysterious RRATs

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arxiv 2201.00295 v2 pith:AHOG6DAT submitted 2022-01-02 astro-ph.HE

Abhishek , Namrata Malusare , Tanushree N , Gayathri Hegde , Sushan Konar This is my paper · ORCID
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keywords rratrratsconjecturesneutronotherpopulationpulsarsradio
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Several conjectures have been put forward to explain the RRATs, the newest subclass of neutron stars, and their connections to other radio pulsars. This work discusses these conjectures in the context of the characteristic properties of the RRAT population. Contrary to expectations, it is seen that - a) the RRAT population is statistically un-correlated with the nulling pulsars, and b) the RRAT phenomenon is unlikely to be related to old age or death-line proximity. It is perhaps more likely that the special emission property of RRATs is a signature of them being later evolutionary phases of other types of neutron stars which may have resulted in restructuring of the magnetic fields.

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Cited by 2 Pith papers

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

  1. Timing and statistical analysis of single-pulse search pulsar discoveries from the PALFA survey

    astro-ph.HE 2026-08 conditional novelty 6.0 of 10

    Timing solutions for five PALFA rotating radio transients, spin periods for two more, and Bayesian energy and wait-time fits that support log-normal burst energies and near-Poisson burst times.

  2. 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.

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