Verification of the diffusive shock acceleration in Mrk 501
arXiv:1806.00325 · doi:10.1093/mnras/sty1323
Abstract
The present work considers a plane shock front propagating along a cylindrical jet. Electrons experience the diffusive shock acceleration around the shock front, and subsequently drift away into the downstream flow in which they emit most of their energy. Assuming a proper boundary condition at the interface between the shock zone and the downstream zone, we solve the transport equation for the electrons in the downstream flow zone, where the combined effects of escape, synchrotron and IC cooling in the Thomson regime are taken into account. Using the electron spectrum obtained in this manner we calculate the multi-wavelength spectral energy distribution of Mrk 501 in the synchrotron self-Compton scenario. We check numerically if the Klein-Nishina cross-section could be approximated to the Thomsom regime. We consider whether the model results yield physically reasonable parameters, and further discuss some of implications of the model results. It suggests that the process of diffusive shock acceleration operates in the outflow of Mrk 501.
arXiv comment8 pages, 3 figures, 1 table, accepted for publication in MNRAS
References in corpus (66)
- Unified Schemes for Radio-Loud Active Galactic Nuclei
- Particle acceleration by ultra-relativistic shocks: theory and simulations
- Variable VHE gamma-ray emission from Markarian 501
- Constraints on the Physical Parameters of TeV Blazars
- The power of blazar jets
- Constraining Emission Models of Luminous Blazar Sources
- Log-parabolic spectra and particle acceleration in the BL Lac object Mkn 421: spectral analysis of the complete BeppoSAX wide band X-ray data set
- Fermi-LAT Observations of Markarian 421: the Missing Piece of its Spectral Energy Distribution
- Particle acceleration at ultrarelativistic shocks: an eigenfunction method
- Synchrotron Self-Compton Analysis of TeV X-ray Selected BL Lacertae Objects
- Swift observations of the very intense flaring activity of Mrk 421 during 2006: I. Phenomenological picture of electron acceleration and predictions for the MeV/GeV emission
- Stochastic Acceleration and the Evolution of Spectral Distributions in SSC Sources: A Self Consistent Modeling of Blazars' Flares
- Analytical solutions for energy spectra of electrons accelerated by nonrelativistic shock-waves in shell type supernova remnants
- Insights Into the High-Energy Gamma-ray Emission of Markarian 501 from Extensive Multifrequency Observations in the Fermi Era
- Extreme synchrotron BL Lac objects
- TeV BL Lac objects at the dawn of the Fermi era
- Klein-Nishina Effects in the Spectra of Non-Thermal Sources Immersed in External Radiation Fields
- Parsec Scale Properties of Markarian 501
- Klein-Nishina Effects on Optically Thin Synchrotron and Synchrotron Self-Compton Spectrum
- Log-parabolic spectra and particle acceleration in blazars. III: SSC emission in the TeV band from Mkn 501
- Relativistic Shocks: Particle Acceleration and Magnetization
- Rapid variability in the synchrotron self Compton model for blazars
- The structure and emission model of the relativistic jet in the quasar 3C 279 inferred from radio to high-energy gamma-ray observations in 2008-2010
- An evolutionary scenario for blazar unification
- Simultaneous observations of PKS 2155-304 with H.E.S.S., Fermi, RXTE and ATOM: spectral energy distributions and variability in a low state
- A Study of High Energy Emission from the TeV blazar Mrk 501 during Multiwavelength Observations in 1996
- The spectrum of particles accelerated in relativistic, collisionless shocks
- Diffusive Acceleration of Particles at Oblique, Relativistic, Magnetohydrodynamic Shocks
- Stochastic particle acceleration and synchrotron self--Compton radiation in TeV blazars
- Equipartition Gamma-Ray Blazars and the Location of the Gamma-Ray Emission Site in 3C 279
- Energetics of Tev Blazars and Physical Constraints on their Emission Regions
- Spectral Energy Distribution of Markarian 501: Quiescent State vs. Extreme Outburst
- Cosmic ray acceleration at oblique shocks
- Diffusive Shock Acceleration in Unmodified Relativistic, Oblique Shocks
- Probing Acceleration and Turbulence at Relativistic Shocks in Blazar Jets
- Multiwavelength observations of Mrk 501 in 2008
- The jet of Markarian 501 from millions of Schwarzschild radii down to a few hundreds
- Synchrotron and inverse-Compton emission from blazar jets I: a uniform conical jet model
- Electron Acceleration and Time Variability of High Energy Emission from Blazars
- Multiband variability studies and novel broadband SED modeling of Mrk 501 in 2009
- The curvature of spectral energy distribution of blazars
- Ultra High Energy Cosmic Rays
- Emitting electrons spectra and acceleration processes in the jet of Mrk 421: from low state to giant flare state
- Relaxational effects in radiating stellar collapse
- Shock acceleration of electrons in the presence of synchrotron losses: I. test particle theory
- Fourier Analysis of Blazar Variability
- Very hard gamma-ray emission from a flare of Mrk 501
- TeV variability in blazars: how fast can it be?
- The Sub-Luminal Parsec-scale Jet of Mkn 501
- Multiwavelength Properties of Blazars
- Discerning the -ray emitting region in the flat spectrum radio quasars
- Evidence for the Secondary Emission as the Origin of Hard Spectra in TeV Blazars
- Significant Limb-Brightening in the Inner Parsec of Markarian 501
- The physical parameters of Markarian 501 during flaring activity
- Multi-frequency, Multi-Epoch Study of Mrk 501: Hints for a two-component nature of the emission
- Rapid TeV Flaring in Markarian 501
- Very High Energy outburst of Markarian 501 in May 2009
- Emitting electrons and source activity in Markarian 501
- Diffusive shock acceleration in radiation dominated environments
- "Leading blob" model in a stochastic acceleration scenario: the case of the 2009 flare of Mkn~501
- Modelling the variability of 1ES1218+30.4
- X-ray and gamma-ray variability of Mrk 421
- Synchrotron Self-Compton Emission by Relativistic Electrons under Stochastic Acceleration: Application to Mrk 421 and Mrk 501
- A Steady-State Spectral Model For Electron Acceleration And Cooling In Blazar Jets: Application To 3C 279
- Electron Acceleration in Pulsar-Wind Termination Shocks: An Application to the Crab Nebula Gamma-Ray Flares
- Electrostatic Potentials in Supernova Remnant Shocks
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- A time-dependent particle acceleration and emission model: Understanding the particle spectral evolution and blazar flares
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