Particle Acceleration by Pickup Process Upstream of Relativistic Shocks

نویسندگان

چکیده

Abstract Particle acceleration at magnetized purely perpendicular relativistic shocks in electron–ion plasmas is studied by means of two-dimensional particle-in-cell simulations. Magnetized with the upstream bulk Lorentz factor γ 1 ≫ are known to emit intense electromagnetic waves from shock front, which induce electrostatic plasma (wakefield) and transverse filamentary structures region via stimulated/induced Raman scattering filamentation instability, respectively. The wakefield filaments inject a fraction incoming particles into particle process, once decoupled flow wakefield, picked up again flow. picked-up accelerated motional electric field. maximum attainable estimated as γ max , e ∼ α 1 3 for electrons ,i}\sim (1+{m}_{e}{\gamma }_{1}/{m}_{i}){\gamma }_{1}^{2}$?> i ( + m stretchy="true">/ stretchy="false">) 2 ions, where α ∼ 10 determined our simulation results. can increase weakly if sufficiently large. This result indicates that highly astrophysical such external gamma-ray bursts be an efficient accelerator.

برای دانلود رایگان متن کامل این مقاله و بیش از 32 میلیون مقاله دیگر ابتدا ثبت نام کنید

اگر عضو سایت هستید لطفا وارد حساب کاربری خود شوید

منابع مشابه

Particle Acceleration at Relativistic Shocks

I review the current status of Fermi acceleration theory at relativistic shocks. I first discuss the relativistic shock jump conditions, then describe the nonrelativistic Fermi mechanism and the differences introduced by relativistic flows. I present numerical calculations of the accelerated particle spectrum, and examine the maximum energy attainable by this process. I briefly consider the min...

متن کامل

Particle acceleration and relativistic shocks

Observations of both gamma-ray burst sources and certain classes of active galaxy indicate the presence of relativistic shock waves and require the production of high energy particles to explain their emission. In this paper we first review the basic theory of shock waves in relativistic hydrodynamics and magneto-hydrodynamics, emphasising the astrophysically interesting cases. This is followed...

متن کامل

Particle Acceleration in Relativistic Collisionless Shocks: Fermi Process at Last?

We present evidence that relativistic shocks propagating in unmagnetized plasmas can selfconsistently accelerate particles. We use long-term two-dimensional particle-in-cell simulations to study the well-developed shock structure in unmagnetized pair plasma. The particle spectrum downstream of such a shock consists of two components: a relativistic Maxwellian, with characteristic temperature se...

متن کامل

Particle Acceleration at Multiple Internal Relativistic Shocks

Relativistic shocks provide an efficient method for high-energy particle acceleration in many astrophysical sources. Multiple shock systems are even more effective and of importance, for example, in the internal shock model of gamma-ray bursts. We investigate the reacceleration of pre-existing energetic particles at such relativistic internal shocks by the first order Fermi process of pitch ang...

متن کامل

Nonlinear Particle Acceleration in Relativistic Shocks

Monte Carlo techniques are used to model nonlinear particle acceleration in parallel collisionless shocks of various speeds, including mildly relativistic ones. When the acceleration is efficient, the backreaction of accelerated particles modifies the shock structure and causes the compression ratio, r, to increase above test-particle values. Modified shocks with Lorentz factors, γ0 . 3, can ha...

متن کامل

ذخیره در منابع من


  با ذخیره ی این منبع در منابع من، دسترسی به آن را برای استفاده های بعدی آسان تر کنید

ژورنال

عنوان ژورنال: The Astrophysical Journal

سال: 2022

ISSN: ['2041-8213', '2041-8205']

DOI: https://doi.org/10.3847/1538-4357/ac38aa