Résumé
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.
| langue originale | Anglais |
|---|---|
| Numéro d'article | 215003 |
| journal | Physical Review Letters |
| Volume | 115 |
| Numéro de publication | 21 |
| Les DOIs | |
| état | Publié - 17 nov. 2015 |
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