Please use this identifier to cite or link to this item:
http://hdl.handle.net/2289/1451
Title: | Vacuum gaps in pulsars and PSR J2144-3933 |
Authors: | Gil, Janusz Mitra, D. |
Keywords: | Magnetic Fields, Stars: Pulsars: General, Radiation Mechanisms: Nonthermal |
Issue Date: | 20-Mar-2001 |
Publisher: | The University of Chicago Press for the American Astronomical Society |
Citation: | Astrophysical Journal, 2001, Vol.550, p383-391 |
Abstract: | In this paper we revisit the radio pulsar death line problem within the framework of curvature radiation and/or the inverse Compton scattering-induced vacuum gap model above neutron star polar caps. Our special interest is in the recently detected pulsar PSR J2144-3933 with extremal period 8.5 s, which lies far beyond conventional death lines. We argue that the formation of vacuum gaps requires a complicated multipolar surface magnetic field, with a strength Bs typically much higher than the surface dipolar component Bd and a radii of curvature R much smaller than the neutron star radius R=106 cm. Such a multipolar surface field is also consistent with death lines including the extremal pulsar PSR J2144-3933. Since vacuum gap models produce sparks, our paper naturally supports the spark related models of subpulse drift phenomenon as well as the spark-associated models of coherent pulsar radio emission. |
URI: | http://hdl.handle.net/2289/1451 |
ISSN: | 0004-637X 1538-4357(Online) |
Alternative Location: | http://dx.doi.org/10.1086/319714 |
Copyright: | (2001) by the American Astronomical Society. |
Appears in Collections: | Research Papers (A&A) |
Files in This Item:
File | Description | Size | Format | |
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2001.APJ.550.P383.pdf | 9p. | 187.4 kB | Adobe PDF | View/Open |
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