Non-relativistic collisionless shocks in unmagnetized electron-proton plasmas

Details Non-relativistic collisionless shocks in unmagnetized electron-proton plasmas Non-relativistic collisionless shocks in unmagnetized electron-proton plasmas

Apr 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008aps..apr8he042k&link_type=abstract

American Physical Society, 2008 APS April Meeting and HEDP/HEDLA Meeting, April 11-15, 2008, abstract #8HE.042

Astronomy and Astrophysics

Astrophysics

Scientific paper

We show that collisionless shocks with non-relativistic propagation speed can be driven even in unmagnetized electron-proton plasmas by using two-dimensional particle-in-cell simulations. We performed a series of simulations for flow velocities of 0.9c, 0.45c, 0.2c and 0.1c with a reduced proton to electron mass ratio of 20 and observed formation of collisionless shocks in all cases. In these shocks, the Weibel-type instability generates strong magnetic fields within the shock transition layer. The generated magnetic fields provide an effective dissipation mechanism for the upstream plasma which enables the shocks to form without background magnetic fields. Since non-relativistic shocks are frequently driven in weakly magnetized electron-proton plasmas in the universe associated with various astrophysical phenomena (e.g., supernova explosions), this kind of shocks mediated by the Weibel instability can exist in the universe. In addition, thanks to the self-similarity in the basic equations of collisionless plasma, there is a possibility to generate such shocks in a laboratory with high-power laser facilities by scaling the quantities.

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