COMPUTATION OF SYNTHETIC SPECTRA FROM SIMULATIONS OF RELATIVISTIC SHOCKS

Particle-in-cell (PIC) simulations of relativistic shocks are in principle capable of predicting the spectra of photons that are radiated incoherently by the accelerated particles. The most direct method evaluates the spectrum using the fields given by the Liénard-Wiechart potentials. However, for r...

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Main Authors: Reville, B, Kirk, J
Format: Journal article
Language:English
Published: Institute of Physics Publishing 2010
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author Reville, B
Kirk, J
author_facet Reville, B
Kirk, J
author_sort Reville, B
collection OXFORD
description Particle-in-cell (PIC) simulations of relativistic shocks are in principle capable of predicting the spectra of photons that are radiated incoherently by the accelerated particles. The most direct method evaluates the spectrum using the fields given by the Liénard-Wiechart potentials. However, for relativistic particles this procedure is computationally expensive. Here we present an alternative method that uses the concept of the photon formation length. The algorithm is suitable for evaluating spectra both from particles moving in a specific realization of a turbulent electromagnetic field or from trajectories given as a finite, discrete time series by a PIC simulation. The main advantage of the method is that it identifies the intrinsic spectral features and filters out those that are artifacts of the limited time resolution and finite duration of input trajectories. © 2010. The American Astronomical Society. All rights reserved. Printed in the U.S.A.
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spelling oxford-uuid:3efc9a23-e268-4297-ab48-d000dc0c2d672022-03-26T14:29:07ZCOMPUTATION OF SYNTHETIC SPECTRA FROM SIMULATIONS OF RELATIVISTIC SHOCKSJournal articlehttp://purl.org/coar/resource_type/c_dcae04bcuuid:3efc9a23-e268-4297-ab48-d000dc0c2d67EnglishSymplectic Elements at OxfordInstitute of Physics Publishing2010Reville, BKirk, JParticle-in-cell (PIC) simulations of relativistic shocks are in principle capable of predicting the spectra of photons that are radiated incoherently by the accelerated particles. The most direct method evaluates the spectrum using the fields given by the Liénard-Wiechart potentials. However, for relativistic particles this procedure is computationally expensive. Here we present an alternative method that uses the concept of the photon formation length. The algorithm is suitable for evaluating spectra both from particles moving in a specific realization of a turbulent electromagnetic field or from trajectories given as a finite, discrete time series by a PIC simulation. The main advantage of the method is that it identifies the intrinsic spectral features and filters out those that are artifacts of the limited time resolution and finite duration of input trajectories. © 2010. The American Astronomical Society. All rights reserved. Printed in the U.S.A.
spellingShingle Reville, B
Kirk, J
COMPUTATION OF SYNTHETIC SPECTRA FROM SIMULATIONS OF RELATIVISTIC SHOCKS
title COMPUTATION OF SYNTHETIC SPECTRA FROM SIMULATIONS OF RELATIVISTIC SHOCKS
title_full COMPUTATION OF SYNTHETIC SPECTRA FROM SIMULATIONS OF RELATIVISTIC SHOCKS
title_fullStr COMPUTATION OF SYNTHETIC SPECTRA FROM SIMULATIONS OF RELATIVISTIC SHOCKS
title_full_unstemmed COMPUTATION OF SYNTHETIC SPECTRA FROM SIMULATIONS OF RELATIVISTIC SHOCKS
title_short COMPUTATION OF SYNTHETIC SPECTRA FROM SIMULATIONS OF RELATIVISTIC SHOCKS
title_sort computation of synthetic spectra from simulations of relativistic shocks
work_keys_str_mv AT revilleb computationofsyntheticspectrafromsimulationsofrelativisticshocks
AT kirkj computationofsyntheticspectrafromsimulationsofrelativisticshocks