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• W4384338367 abstract "We investigate the geometry of the magnetic field of rotation-powered pulsars. A new method for calculating an angle ($beta$) between the spin and magnetic dipole axes of a neutron star (NS) in the ejector stage is considered within the frame of the magnetic dipole energy loss mechanism. We estimate the surface magnetic field strength ($B_{rm ns}$) for a population of known neutron stars in the radio pulsar (ejector) stage. The evaluated $B_{rm ns}(beta)$ may differ by an order of magnitude from the values without considering the angle $beta$. It is shown that $B_{rm ns}(beta)$ lies in the range $10^{8}$--$10^{14},text{G}$ for a known population of short and middle periodic radio pulsars." @default.
• W4384338367 created "2023-07-15" @default.
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• W4384338367 date "2023-07-14" @default.
• W4384338367 modified "2023-09-27" @default.
• W4384338367 title "Estimates of the Surface Magnetic Field Strength of Radio Pulsars" @default.
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• W4384338367 doi "https://doi.org/10.3390/universe9070334" @default.
• W4384338367 hasPublicationYear "2023" @default.
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