Plasma Shocks and Instabilities in Relativistic Jets of Gamma-ray Bursts

  • a project financed from the government budget through the STAR-C3 program of the ROmanian Space Agency (ROSA)
  • period: 20 July 2017 - 19 July 2018

Research team:

Summary:


Gamma-ray bursts are short flashes of high energy photons that reach the Earth from cosmological distances, the origin and mechanism of which are the focus of intense research and debate. There is a general understanding that gamma-ray bursts and their afterglows are produced in shocks resulting from collisions of shells within relativistic jets from black holes as they propagate and interact with the ambient medium. Particle-in-cell simulations enable us to study collisionless shock structure and instability growth in various plasma conditions that lead to particle acceleration, magnetic field generation, and emission of radiation. Among relativistic plasma processes, much less is known about the velocity shear processes such as the kinetic Kelvin-Helmholtz and mushroom instabilities. The main goal of this research project is to unveil the nature of the processes at work in relativistic jets of gamma-ray bursts. We will perform 3-dimensional relativistic particle-in-cell simulations of both electron-proton and electron-positron plasmas, for unmagnetized and magnetized jets, to reveal the role of kinetic Kelvin-Helmholtz and mushroom instabilities in these extreme astrophysical phenomena. We will self-consistently calculate the radiation spectra and spectral evolution. These calculations will provide a link between jet plasma properties and the observed radiation from gamma-ray burst jets. The proposed project will also involve the training of an undergraduate student by combining education and research aspects. Our project directly ties with the ESA's Cosmic Vision to look for clues to the processes at work in gamma-ray bursts and provides numerical simulation support for observational data from present and future ESA’s missions, such as INTGRAL, XMM-Newton, and Athena.

References:

Dutan, I., Nishikawa, K.-I., Mizuno, Y., et al. 2017, International Astronomical Union Proc., IAU Symposium, 324, 199
Nishikawa, K.-I., Frederiksen, J. T., Nordlung, A., et al. 2016, ApJ, 820, 94
Nishikawa, K.-I., Hardee, P. E., Dutan, I., et al. 2014, ApJ, 793, 60
Nishikawa, K.-I., Zhang, B., Dutan, I., et al. 2013, Ann. Geophys., 31, 1535
Nishikawa, K.-I., Niemiec, J., Hardee, P., et al. 2009, ApJ, 698, L10

Articles:

Conferences, meetings, and talks:

Special events at the ISS:

  • Intensive Course: May 21-25, 2018
    Location: Institute of Space Science, Auditorium
    Instructor: Dr. Ken-Ichi Nishikawa (Department of Physics, University of Alabama in Huntsville, USA)
    Title: Computational Methods for Kinetic Processes in Plasma Physics
    List of Participants [pdf]
    [video 1] [video 2] [video 3] [video 4] [video 5] [video 6] [video 7]

  • ISS Seminar: Wednesday, May 23rd, 2018 -- 11:00 am
    Location: Institute of Space Science, Auditorium
    Speaker: Dr. Athina Meli
    (University of Liege, Belgium and Athens Institute for Education and Research, Greece)
    Title: The High Energy Universe: Ultra-high-energy Cosmic Rays, Active Galactic Nuclei, and Gamma-ray Bursts

  • ISS Seminar: Monday, May 21st, 2018 -- 11:00 am
    Location: Institute of Space Science, Auditorium
    Speaker: Dr. Ken-Ichi Nishikawa (Department of Physics, University of Alabama in Huntsville, USA)
    Title: Reconnection and Associated Flares in Global Relativistic Jets containing Helical Magnetic Fields with Particle-in-cell Simulations
    [video]