Published January 21, 2000
| Published
Journal Article
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Polarization evolution in strong magnetic fields
- Creators
- Heyl, Jeremy S.
- Shaviv, Nir J.
Abstract
Extremely strong magnetic fields change the vacuum index of refraction. Although this polarization-dependent effect is small for typical neutron stars, it is large enough to decouple the polarization states of photons travelling within the field. The photon states evolve adiabatically and follow the changing magnetic field direction. The combination of a rotating magnetosphere and a frequency-dependent-state decoupling predicts polarization phase lags between different wavebands, if the emission process takes place well within the light cylinder. This QED effect may allow observations to distinguish between different pulsar-emission mechanisms and to reconstruct the structure of the magnetosphere.
Additional Information
© 2000 Royal Astronomical Society. Accepted 1999 September 1; Received 1999 June 28; in original form 1999 February 1. Article first published online: 4 Apr. 2002.Attached Files
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Additional details
- Eprint ID
- 27947
- Resolver ID
- CaltechAUTHORS:20111123-112839566
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2011-11-23Created from EPrint's datestamp field
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2021-11-09Created from EPrint's last_modified field