Abstract
We report on the first self-consistent numerical study of the feasibility of laser-driven relativistic pair shocks of prime interest for high-energy astrophysics. Using a QED-particle-in-cell code, we simulate the collective interaction between two counterstreaming electron-positron jets driven from solid foils by short-pulse (∼60 fs), high-energy (∼100 kJ) lasers. We show that the dissipation caused by self-induced, ultrastrong (>106 T) electromagnetic fluctuations is amplified by intense synchrotron emission, which enhances the magnetic confinement and compression of the colliding jets.
| Original language | English |
|---|---|
| Article number | 215003 |
| Journal | Physical Review Letters |
| Volume | 115 |
| Issue number | 21 |
| DOIs | |
| Publication status | Published - 17 Nov 2015 |
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