A combination of rotochemical heating with a large pairing gap and vortex creep explains the observed temperatures of PSR J0437-4715 and PSR B0950+08 while remaining consistent with upper limits on three other old pulsars.
P., Frantsuzova, A., Gourgouliatos, K
2 Pith papers cite this work. Polarity classification is still indexing.
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Population synthesis of normal radio pulsars finds that exponential magnetic field decay with timescale 8.3 Myr reproduces observed distributions of P, P-dot, DM and flux better than power-law decay.
citing papers explorer
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Neutron star heating vs. HST observations
A combination of rotochemical heating with a large pairing gap and vortex creep explains the observed temperatures of PSR J0437-4715 and PSR B0950+08 while remaining consistent with upper limits on three other old pulsars.
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Pulsar Population Synthesis with Magnetorotational Evolution: Constraining the Decay of Magnetic field
Population synthesis of normal radio pulsars finds that exponential magnetic field decay with timescale 8.3 Myr reproduces observed distributions of P, P-dot, DM and flux better than power-law decay.