The Novel Mechanism of Pair Creation in Pulsar Magnetospheres
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In this paper we study the possibility of efficient pair production in a pulsar’s magnetosphere. It has been shown that by means of relativistic centrifugal force the electrostatic field exponentially amplifies. As a result the field approaches the Schwinger limit leading to a pair creation process in the light cylinder area where the effects of rotation are very efficient. Analysing the parameters of the normal period (∼1 s) pulsars we found that the process is so efficient that the number density of electron–positron pairs exceeds the Goldreich–Julian density by five orders of magnitude.
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2016 ◽
Vol 31
(02n03)
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pp. 1641031
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2011 ◽
Vol 696
(3)
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pp. 201-206
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2012 ◽
Vol 29
(2)
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pp. 021102
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2021 ◽
Vol 36
(02)
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pp. 2150011
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2015 ◽
Vol 2
(5)
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pp. 56
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