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- W3023164448 abstract "We perform numerical simulations of the dynamics of magnetized and highly relativistic pulsar-like winds produced by long-lasting central engines in Gamma Ray Bursters (GRB). The very fast wind interacts with the initial relativistically expanding GRB outflow, creating a multiple-shock structure. Depending on the parameters of the model (the energy of the initial explosion, the outside density, the wind power, the delay time for the switch-on of the wind, and the magnetization of the wind) a variety of temporal behaviors can be produced. In certain regimes the dynamics of such secondary engine-driven shocks is self-similar." @default.
- W3023164448 created "2020-05-13" @default.
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- W3023164448 date "2020-04-29" @default.
- W3023164448 modified "2023-09-26" @default.
- W3023164448 title "Dynamics of long-lasting relativistic winds in Gamma Ray Bursters" @default.
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