Half the Neutron Stars
About this episode
The episode discusses a study suggesting that magnetars constitute about half of all neutron stars, challenging previous assumptions.
Today's episode — S05E191, Friday September 11, 2026: Main story: A population-synthesis study published in Nature Astronomy on 10 September argues that magnetars make up roughly half of all neutron stars, not the one-in-a-hundred implied by the catalogues. Celsa Pardo-Araujo and Nanda Rea (Institute of Space Sciences, ICE-CSIC, Barcelona) with Michele Ronchi (ASTRON) and Vanessa Graber (Royal Holloway) modelled the whole isolated-neutron-star population as one family rather than four separate classes, evolving spin-down, magneto-thermal decay and Galactic dynamics together, then filtering the simulated population the way real surveys filter the sky. Of the 24 known neutron stars younger than 2,000 years, magnetars and central compact objects are about 59%; the derived birth fraction averages ~50% (40–70% or 30–50% depending on the assumed birth-field distribution, which peaks at 1–2.5 × 10^14 gauss). Two consequences: the Galactic core-collapse supernova rate has to be higher than assumed, around two per century, and magnetar central-engine models for superluminous supernovae, gamma-ray burst plateaus and fast radio bursts finally have the supply to work. Caveats: it is a model…
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