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.
L., Linares M., Homan J., Chakrabarty D.
1 Pith paper cite this work. Polarity classification is still indexing.
1
Pith paper citing it
fields
astro-ph.HE 1years
2025 1verdicts
CONDITIONAL 1representative citing papers
citing papers explorer
-
An energy approach to pulsar-disc interaction: disc stability and implications for transitional millisecond pulsars
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.