On the Formation of Inner Vacuum Gaps in Radio Pulsars

@article{Gil2002OnTF,
  title={On the Formation of Inner Vacuum Gaps in Radio Pulsars},
  author={J. Gil and G. Melikidze},
  journal={The Astrophysical Journal},
  year={2002},
  volume={577},
  pages={909-916}
}
The problem of formation of the Ruderman-Sutherland-type inner vacuum gap in neutron stars with Ω 1 (where Ti is the critical temperature above which Fe ions will not be bound at the surface and Ts is the actual temperature of the polar cap surface heated by the back flow of relativistic electrons) that the inner vacuum gap can form, provided that the actual surface magnetic field is extremely strong (Bs 1013 G) and curved ( < 106 cm), irrespective of the value of dipolar component measured… Expand
Drifting subpulses and inner acceleration regions in radio pulsars
Two modes of partially screened gap
Can the Inner Gap Sparking Take Place in Millisecond Pulsars
...
1
2
3
4
...

References

SHOWING 1-10 OF 38 REFERENCES
Charge Densities above Pulsar Polar Caps
Three Modes of Pulsar Inner Gap
Non-stationary pair plasma in a pulsar magnetosphere and the two-stream Instability
  • E. Asseo, George I. Melikidze
  • Physics
  • 1998
Particle acceleration and radio emission above pulsar polar caps
...
1
2
3
4
...