Off-axis afterglow light curves from high-resolution hydrodynamical jet simulations

Hendrik J. Van Eerten, Andrew I. MacFadyen, Weiqun Zhang

    Research output: Chapter in Book/Report/Conference proceedingConference contribution

    Abstract

    Numerical jet simulations serve a valuable role in calculating gamma-ray burst afterglow emission beyond analytical approximations. Here we present the results of high resolution 2D simulations of decelerating relativistic jets performed using the RAM adaptive mesh refinement relativistic hydrodynamics code. We have applied a separate synchrotron radiation code to the simulation results in order to calculate light curves at frequencies varying from radio to X-ray for observers at various angles from the jet axis. We provide a confirmation from radio light curves from simulations rather than from a simplified jet model for earlier results in the literature finding that only a very small number of local Ibc supernovae can possibly harbor an orphan afterglow. Also, recent studies have noted an unexpected lack of observed jet breaks in the Swift sample. Using a jet simulation with physical parameters representative for an average Swift sample burst, such as a jet half opening angle of 0.1 rad and a source redshift of z = 2.23, we have created synthetic light curves at 1.5 keV with artifical errors while accounting for Swift instrument biases as well. A large set of these light curves have been generated and analyzed using a Monte Carlo approach. Single and broken power law fits are compared. We find that for increasing observer angle, the jet break quickly becomes hard to detect. This holds true even when the observer remains well within the jet opening angle. We find that the odds that a Swift light curve from a randomly oriented 0.1 radians jet at z = 2.23 will exhibit a jet break at the 3σ level are only 12 percent. The observer angle therefore provides a natural explanation for the lack of perceived jet breaks in the Swift sample.

    Original languageEnglish (US)
    Title of host publicationGamma Ray Bursts 2010, GRB 2010
    Pages173-176
    Number of pages4
    Volume1358
    DOIs
    StatePublished - 2011
    EventGamma Ray Bursts 2010, GRB 2010 - Annapolis, MD, United States
    Duration: Nov 1 2010Nov 4 2010

    Other

    OtherGamma Ray Bursts 2010, GRB 2010
    CountryUnited States
    CityAnnapolis, MD
    Period11/1/1011/4/10

    Fingerprint

    afterglows
    light curve
    high resolution
    simulation
    harbors
    gamma ray bursts
    supernovae
    bursts
    synchrotron radiation
    hydrodynamics

    Keywords

    • Bursts
    • Gamma-rays
    • Hydrodynamics
    • Methods
    • Numerical
    • Relativity

    ASJC Scopus subject areas

    • Physics and Astronomy(all)

    Cite this

    Van Eerten, H. J., MacFadyen, A. I., & Zhang, W. (2011). Off-axis afterglow light curves from high-resolution hydrodynamical jet simulations. In Gamma Ray Bursts 2010, GRB 2010 (Vol. 1358, pp. 173-176) https://doi.org/10.1063/1.3621765

    Off-axis afterglow light curves from high-resolution hydrodynamical jet simulations. / Van Eerten, Hendrik J.; MacFadyen, Andrew I.; Zhang, Weiqun.

    Gamma Ray Bursts 2010, GRB 2010. Vol. 1358 2011. p. 173-176.

    Research output: Chapter in Book/Report/Conference proceedingConference contribution

    Van Eerten, HJ, MacFadyen, AI & Zhang, W 2011, Off-axis afterglow light curves from high-resolution hydrodynamical jet simulations. in Gamma Ray Bursts 2010, GRB 2010. vol. 1358, pp. 173-176, Gamma Ray Bursts 2010, GRB 2010, Annapolis, MD, United States, 11/1/10. https://doi.org/10.1063/1.3621765
    Van Eerten HJ, MacFadyen AI, Zhang W. Off-axis afterglow light curves from high-resolution hydrodynamical jet simulations. In Gamma Ray Bursts 2010, GRB 2010. Vol. 1358. 2011. p. 173-176 https://doi.org/10.1063/1.3621765
    Van Eerten, Hendrik J. ; MacFadyen, Andrew I. ; Zhang, Weiqun. / Off-axis afterglow light curves from high-resolution hydrodynamical jet simulations. Gamma Ray Bursts 2010, GRB 2010. Vol. 1358 2011. pp. 173-176
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