Magnetic inclination alignment with timescale proportional to B to the minus two suppresses observed numbers of strong-field neutron stars, unifying pulsars and magnetars under one log-uniform initial B distribution.
Title resolution pending
2 Pith papers cite this work. Polarity classification is still indexing.
2
Pith papers citing it
fields
astro-ph.HE 2years
2026 2verdicts
UNVERDICTED 2representative citing papers
Numerical and analytical modeling of polar-cap processes in magnetic white dwarfs finds pair creation viable only for P ≲ 100 s and B_d ≲ 10^10 G, rendering it difficult to sustain in observed objects.
citing papers explorer
-
A Log-Uniform Initial Magnetic Field Distribution Explains Pulsar and Magnetar Populations through Magnetic Inclination Alignment
Magnetic inclination alignment with timescale proportional to B to the minus two suppresses observed numbers of strong-field neutron stars, unifying pulsars and magnetars under one log-uniform initial B distribution.
-
Study for curvature radiation and magnetic pair creation process on polar-cap region of magnetic white dwarf
Numerical and analytical modeling of polar-cap processes in magnetic white dwarfs finds pair creation viable only for P ≲ 100 s and B_d ≲ 10^10 G, rendering it difficult to sustain in observed objects.