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- W3035422341 abstract "We can probe observationally and reproduce theoretically intricate properties of the Crab Nebula nearest to the pulsar - The Inner Knot. The tiny knot is indeed a bright spot on the surface of a quasi-stationary magnetic relativistic shock that accelerates particles. It is required that the part of the wind that produces the Inner Knot has low magnetization; thus, it is not a site of gamma-ray flares. We develop a model of particle acceleration during explosive reconnection events in relativistic highly magnetized plasma and apply the model to explain the Crab gamma-ray flares. Particles are efficiently accelerated by charge-starved DC-type electric fields during initial stages of magnetic flux merges. By implication, the magnetic reconnection is an important, and possibly dominant process of particle acceleration in high energy astrophysical sources." @default.
- W3035422341 created "2020-06-19" @default.
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- W3035422341 date "2017-01-01" @default.
- W3035422341 modified "2023-09-24" @default.
- W3035422341 title "What we recently learnt about Crab: structure of the wind, the shock, flares and reconnection" @default.
- W3035422341 hasPublicationYear "2017" @default.
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