Work

On the decay of the magnetic fields of single radio pulsars

Year: 1992

Type: article

Abstract: We investigate the statistical evidence for the decay of the magnetic field of single radio pulsars. We perform population syntheses for different assumed values for the time scale of field decay using a Monte Carlo method. We allow for the selection effects in pulsar surveys and compare the synthesized populations with the observed pulsars. We take account of the finite scale height of the distribution in the Galaxy of free electrons, which determine the dispersion measure and hence the apparent distance of radio pulsars. Our simulations give much better agreement with the observations if the time scale for the field decay is assumed to be longer than the typical active life time of a radio pulsar. This indicates that no significant field decay occurs in single radio pulsars.

Source: UvA-DARE (University of Amsterdam)

Authors: D. Bhattacharya, R. A. M. J. Wijers, J.W. Hartman, F. Verbunt

Institutions: National Aeronautics and Space Administration, University of California, Santa Barbara, University of Amsterdam, Utrecht University

Language: English

Topic: Pulsars and Gravitational Waves Research

Subfield: Astronomy and Astrophysics

Field: Physics and Astronomy

Domain: Physical Sciences

Open Access status: green

OpenAlex ID: W2199151736

FWCI: 2.158

Cites:

Cited by: 28

Related to: 10