1978
DOI: 10.1086/156144
|View full text |Cite
|
Sign up to set email alerts
|

Potential drops above pulsar polar caps - Ultrarelativistic particle acceleration along the curved magnetic field

Help me understand this report

Search citation statements

Order By: Relevance

Paper Sections

Select...
1
1
1

Citation Types

2
81
0

Year Published

1981
1981
2015
2015

Publication Types

Select...
5
4

Relationship

0
9

Authors

Journals

citations
Cited by 124 publications
(83 citation statements)
references
References 0 publications
2
81
0
Order By: Relevance
“…The secondary plasma-generation condition determines its height. Another model, based on the assumption of free particle escape from the neutron star surface,was first studied by Arons' group (Fawley et al 1977;Scharlemann et al 1978;Arons & Scharlemann 1979), and recently in more detail by Istomin & Sobyanin (2011a,b); Medin & Lai (2010);Timokhin (2010) ;Chen & Beloborodov (2013) and Timokhin & Arons (2013).…”
Section: Electron-positron Generationmentioning
confidence: 99%
“…The secondary plasma-generation condition determines its height. Another model, based on the assumption of free particle escape from the neutron star surface,was first studied by Arons' group (Fawley et al 1977;Scharlemann et al 1978;Arons & Scharlemann 1979), and recently in more detail by Istomin & Sobyanin (2011a,b); Medin & Lai (2010);Timokhin (2010) ;Chen & Beloborodov (2013) and Timokhin & Arons (2013).…”
Section: Electron-positron Generationmentioning
confidence: 99%
“…Further out, the usual effects of field line curvature (one way or the other) need to be included. By contrast MT follow the approach of Jon Arons and colleagues (Fawley et al 1977;Scharlemann et al 1978): they assume that v stays equal to c. (They do not discuss the initial acceleration by a super-GJ density from v < c to v « c, an essential feature of the Arons et al solution). The continuity condition (11) then requires ap e oc B on a streamline.…”
Section: Gmdr 2 J Fr G \[Rmentioning
confidence: 99%
“…Study of polar cap relativstic particle acceleration in the 1970's had led to the conclusion that acceleration of a space charge limited particle beam from the stellar surface with energy/particle high enough to emit magnetically convertible curvature gamma rays occurs because of curvature of the magnetic field (Scharlemann et al 1978, Arons andScharlemann 1979). In a curved B field, matching of the beam charge density to the Goldreich-Julian density occurs only at the surface.…”
Section: Polar Accelerationmentioning
confidence: 99%