Study of Nonlinear Evolution of the Weibel-like Instability of Relativistic Electron Beams Relevant to Fast Ignition and Astrophysics
Relativistic laser matter interaction generates an intense fast electron beam with Mega ampere (MA) to Giga-ampere current. Such beam can propagate into high-density plasmas as background plasma electrons can provide sufficient return current to maintain charge and current neutrality. However, such system is subject to Weibel-like filamentation instabilities that break out the beam into filaments and generate intense magnetic fields. This could result in anomalous stopping and large angular spread of the electron beams, leading to a lower energy coupling to the fuel in the fast ignition (FI) scheme of inertial confinement fusion, therefore, of significant interest to FI. Understanding the nonlinear growth of the Weibel B-fields and its structure is also important to astrophysics as it is generally accepted to be responsible for relativistic collisionless shocks and cosmic rays and “jitter” radiation in gamma ray burst.