Simultaneous Acceleration of Protons and Electrons at Nonrelativistic Quasiparallel Collisionless Shocks
arXiv:1412.0672 · doi:10.1103/PhysRevLett.114.085003
Abstract
We study diffusive shock acceleration (DSA) of protons and electrons at nonrelativistic, high Mach number, quasiparallel, collisionless shocks by means of self-consistent 1D particle-in-cell simulations. For the first time, both species are found to develop power-law distributions with the universal spectral index in momentum space, in agreement with the prediction of DSA. We find that scattering of both protons and electrons is mediated by right-handed circularly polarized waves excited by the current of energetic protons via non-resonant hybrid (Bell) instability. Protons are injected into DSA after a few gyro-cycles of shock drift acceleration (SDA), while electrons are first pre-heated via SDA, then energized via a hybrid acceleration process that involves both SDA and Fermi-like acceleration mediated by Bell waves, before eventual injection into DSA. Using the simulations we can measure the electron/proton ratio in accelerated particles, which is of paramount importance for explaining the cosmic ray fluxes measured at Earth and the multi-wavelength emission of astrophysical objects such as supernova remnants, radio supernovae, and galaxy clusters. We find the normalization of electron power-law is that of the protons for strong nonrelativistic shocks.
5 pages, 4 figures, accepted to PRL (some updates)
References in corpus (8)
- Circumstellar Emission from Type Ib and Ic Supernovae
- A kinetic approach to cosmic ray induced streaming instability at supernova shocks
- Non-Thermal Electron Acceleration in Low Mach Number Collisionless Shocks. I. Particle Energy Spectra and Acceleration Mechanism
- Simulations and Theory of Ion Injection at Non-relativistic Collisionless Shocks
- Non-Thermal Electron Acceleration in Low Mach Number Collisionless Shocks. II. Firehose-Mediated Fermi Acceleration and its Dependence on Pre-Shock Conditions
- Simulations of Ion Acceleration at Non-relativistic Shocks. III. Particle Diffusion
- Cosmic ray acceleration at perpendicular shocks in supernova remnants
- Particle-in-cell simulations of particle energization via shock drift acceleration from low Mach number quasi-perpendicular shocks in solar flares
Cited by in corpus (49)
- Turbulence and Particle Acceleration in Giant Radio Haloes: the Origin of Seed Electrons
- Time-resolved hadronic particle acceleration in the recurrent Nova RS Ophiuchi
- Electron Surfing and Drift Accelerations in a Weibel-dominated High-Mach-number Shock
- A Nova Outburst Powered by Shocks
- Relativistic electrons produced by foreshock disturbances
- Probing Acceleration and Turbulence at Relativistic Shocks in Blazar Jets
- Electron energy partition across interplanetary shocks: I. Methodology and Data Product
- Collisionless shock heating of heavy ions in SN 1987A
- Electron Preacceleration in Weak Quasi-perpendicular Shocks in High-beta Intracluster Medium
- Point-source and diffuse high-energy neutrino emission from Type IIn supernovae
- PIC Simulation Methods for Cosmic Radiation and Plasma Instabilities
- A radio-emitting outflow produced by the tidal disruption event AT2020vwl
- dHybridR: a Hybrid--Particle-in-Cell Code Including Relativistic Ion Dynamics
- The contribution of winds of star clusters to the Galactic cosmic-ray population
- Radiative Supernova Remnants and Supernova Feedback
- Post-Merger Jets from Supermassive Black Hole Coalescences as Electromagnetic Counterparts of Gravitational Wave Emission
- Radio relics radio emission from multi-shock scenario
- Non-thermal particle acceleration at highly oblique non-relativistic shocks
- Characteristics of Interplanetary Discontinuities in the Inner Heliosphere Revealed by Parker Solar Probe
- Morphology of radio relics II: Properties of polarised emission
- Particle acceleration and magnetic field amplification in massive young stellar object jets
- Radio Emission from Accreting Isolated Black Holes in Our Galaxy
- Non-linear diffusive shock acceleration: A recipe for injection of electrons
- The Magnetohydrodynamic-Particle-In-Cell Module in Athena++: Implementation and Code Tests
- Revealing an unexpectedly low electron injection threshold via reinforced shock acceleration
- Particle Acceleration in Mildly Relativistic Outflows of Fast Energetic Transient Sources
- The evolution of cosmic ray electrons in the cosmic web: seeding by AGN, star formation and shocks
- A formation mechanism for "Wrong Way" Radio Relics
- Radio emission from tidal disruption events produced by the collision between super-Eddington outflows and the circumnuclear medium
- A Numerical Study of the Impact of Jet Magnetic Topology on Radio Galaxy Evolution
- Local acceleration of protons to 100 keV in a quasi-parallel bow shock
- CMB foreground measurements through broad-band radio spectro-polarimetry: prospects of the SKA-MPG telescope
- The impact of low luminosity AGN on their host galaxies: A radio and optical investigation of the kpc-scale outflow in MaNGA 1-166919
- Electron Energization in Quasi-Parallel Shocks: Test-Particle-Electrons in a Proton Driven Turbulence
- Magnetic Field Amplification and Particle Acceleration in Weakly Magnetized Trans-relativistic Electron-ion Shocks
- Cosmic ray acceleration and non-thermal emission from fast luminous optical transient sources
- The radio spectra of SN 2020oi: Effects of radiative cooling on the deduced source properties
- Energy Dissipation in Strong Collisionless Shocks: The Crucial Role of Ion-to-Electron Scale Separation in Particle-in-Cell Simulations
- Kinetic Simulation on Electron, Proton and Helium Acceleration in a Nonrelativistic Quasiparallel shock
- Luminous Fast Blue Optical Transients as "Failed" Gravitational-wave Sources: Helium CoreBlack Hole Mergers Following Delayed Dynamical Instability
- Proton Acceleration by Collisionless Shocks in Supermassive Black Hole Coronae: Implications for High-Energy Neutrinos
- PeV particle acceleration and non-thermal emission in the `minimalist' model of the extended jets in W50/SS433
- Very High Energy Gamma Rays from Ultra Fast Outflows
- Numerical Modeling of Relativistic Effects in Synchrotron-Emitting Shocks
- Long-term evolution of a supernova remnant hosting a double neutron star binary
- Non-linear Diffusive Shock Acceleration of Cosmic Rays -- Quasi-thermal and Non-thermal Particle Distributions
- Suppressed diffusion and gamma-ray emission from the Cygnus bubble
- The structure of cluster merger shocks: turbulent width and the electron heating timescale
- Revisiting Disk Winds in Active Galactic Nuclei as an Origin of Cosmic Gamma-ray and Neutrino Backgrounds