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Shedding new light on Gamma-Ray Bursts with polarization data

Europe/Zurich
Other Institutes

Other Institutes

Campus Biotech Geneva
Description

During 2016 and 2017 the POLAR instrument detected a total 55 GRBs. It performed polarization measurements for a subset of these and the first results of this will soon be published to add to the first set of GRB polarization measurements performed by GAP earlier this decade. During this workshop the new POLAR results will be presented in detail while results of ongoing analysis projects will also be presented. This workshop serves to discus these new results, together with previous polarization measurements, in light of the different existing emission models.

The goal of the workshop is to produce a clear overview of the different existing theoretical predictions in the field and to discus these in light of these new results. The outcome of the discussions is foreseen to be part of an overview paper which will be organized during this workshop. A second goal is to define the most urgent open tasks within this upcoming field of astrophysics. Such tasks do not only concern theoretical work but also data analysis and hardware projects.

The workshop will take place in Geneva and will be attended by both experts in the field of GRB emission theory, general GRB experts and members of the POLAR collaboration.

A total of 15 participants from outside of Switzerland are invited and funding is available for both travel and accommodation for these participants. Additionally there is place for several other researchers from the field of GRB astrophysics who can contact the organizers in case they're interested in joining the meeting, the total number of participants is limited to 30.

 

The following topics will be covered:

- Recent GRB polarization measurements by GAP and POLAR

- Recent GRB afterglow polarization measurements

- Theoretical predictions of the polarization of GRB prompt and afterglow emission

- Implications of new measurement results on existing predictions

- Upcoming polarization results using existing data

- Focus of future theoretical work

- Focus of future analysis/measurements

 

Participants
  • Andrei Beloborodov
  • Andrii Neronov
  • Carole Mundell
  • Daisuke Yonetoku
  • Damien Bégué
  • Francesco Berlato
  • Hancheng Li
  • J. Michael Burgess
  • Jianchao Sun
  • Jirong Mao
  • Jochen Greiner
  • Jonathan Granot
  • Junjing Wang
  • Kenji Toma
  • Maria Munoz Salinas
  • Mark Pearce
  • Merlin Kole
  • Neal Gauvin
  • Nicolas Produit
  • Nirmal Iyer
  • Ramandeep Gill
  • Shuang-Nan Zhang
  • Teresa Tymieniecka
  • Thomas Siegert
  • Volodymyr Savchenko
  • Xin Wu
  • Yuan-Hao Wang
  • Zhengheng Li
    • 11:00 12:00
      Introduction: Introduction/Welcome

      Introduction by local organizers, introduction to the goals of the meeting

    • 12:00 13:00
      Lunch 1h

      Lunch at Campus Biotech

    • 13:00 14:00
      Measurements past and future: GAP results: overview

      Introduction to theoretical emission models

      • 13:00
        GRB prompt emission polarization measurements by GAP 1h
        Speaker: Prof. Daisuke Yonetoku
    • 14:00 15:00
      Measurements past and future: POLAR: the first science results

      Introduction to theoretical emission models

      • 14:00
        Detailed polarization measurements of 5 GRBs by POLAR 30m
        Speaker: Prof. Shuang-Nan Zhang (IHEP)
      • 14:30
        Details of the first POLAR analysis 30m
        Speaker: Mr Zhengheng Li (IHEP)
    • 15:00 15:30
      Coffee Break 30m
    • 15:30 16:15
      Measurements past and future: Polarization measurements without a Compton Telescope and not for GRBs

      Introduction to theoretical emission models

      • 15:30
        Polarization measurements without a Compton Telescope and not for GRBs 45m
        Speaker: Dr Thomas Siegert (MPE)
    • 16:15 17:15
      Measurements past and future: Polarization measurements of the afterglow

      Introduction to theoretical emission models

      • 16:15
        Polarization measurements of the GRB afterglow 1h
        Speaker: Prof. Carole Mundell
    • 10:00 11:45
      CERN visit

      Visit and tour of CERN

    • 11:45 13:15
      Lunch (back at biotech) 1h 30m
    • 13:15 14:45
      GRB: Prompt Emission Theories: Prompt emission Theory: Overview

      GRB prompt emission and predictions on overall GRB polarization

      • 13:15
        GRB Prompt Emission: an overview 45m
        Speaker: Prof. Kenji Toma (Tohoku University)
      • 14:00
        Polarization of GRB Prompt Emission: An overview 45m
        Speaker: Ramandeep Gill (CITA)
    • 14:45 15:15
      Coffee Break 30m
    • 15:15 18:00
      GRB: Prompt Emission Theories: Polarization Predictions Details

      GRB prompt emission and predictions on overall GRB polarization

      • 15:15
        Polarization Predictions of Photospheric Models 45m
        Speaker: Prof. Andrei Beloborodov
      • 16:00
        Synchrotron and Jitter Polarization Models towards POLAR Observations 45m
        Speaker: Prof. Jirong Mao (YNAO)
      • 16:45
        Discussion 1h 15m

        How do the theories presented today compare to the measured data?

        Are there clear problems with any of the existing models given recent results?

        Are we able to exclude any models?

        Speaker: Dr Damien Bégué (MPE)
    • 19:00 21:00
      Conference Dinner 2h
    • 09:30 12:30
      Future prospects: Polarimetry with 170817A: afterglow models
      • 09:30
        Polarization measurements of the afterglow 1h
        Speaker: Prof. Carole Mundell
      • 10:30
        Review of the GRB afterglow polarization and recent work on GRB 170817A 45m
        Speaker: Prof. Jonathan Granot
      • 11:15
        GRB 170817A afterglow measurements 30m
        Speaker: Prof. Carole Mundell
      • 11:45
        Theoretical interpretation of the detected circular polarization and the polarimetry of kilonova 170817 45m
        Speaker: Prof. Kenji Toma (Tohoku University)
    • 12:30 13:15
      Lunch 45m
    • 13:15 13:45
      Discussions: What do we need from future instruments?
      • 13:15
        What do we need from future instruments? 30m

        In light of the discussions from yesterday, what type of measurements are most important for the future? Energy dependence, time dependence? Do we prefer many "ok" measurements or do we prefer a few very detailed ones (quantity vs quality)?

        What are the lessons learned from previous missions which can benefit the future ones?

        Speaker: Nicolas Produit (Universite de Geneve (CH))
    • 13:45 14:10
      Future prospects: GAP2
      • 13:45
        Future prospects with GAP2 20m
        Speaker: Prof. Daisuke Yonetoku
    • 14:10 14:35
      Future prospects: POLAR-2
      • 14:10
        POLAR-2 20m
        Speaker: Merlin Reynaard Kole (Universite de Geneve (CH))
    • 14:35 15:00
      Future prospects: SPHiNX
    • 15:00 15:30
      Coffee Break 30m
    • 15:30 16:00
      Future prospects: eXTP
      • 15:30
        Polarization measurements with the eXTP mission 20m
        Speaker: Prof. Shuang-Nan Zhang (IHEP)
    • 16:00 17:00
      Discussions: What do we need from theory?
    • 19:00 21:00
      Dinner (@ Bain de Paquis) 2h
    • 09:30 09:45
      Data Analysis: GRB localization: importance for polarization

      Ongoing data analysis projects

      • 09:30
        The importance of localization 15m
        Speaker: Merlin Reynaard Kole (Universite de Geneve (CH))
    • 09:45 10:15
      Data Analysis: GRB localization with POLAR

      Ongoing data analysis projects

      • 09:45
        GRB Localization with POLAR 30m
        Speaker: Mr Yuanhao Wang
    • 10:15 11:10
      Data Analysis: GRB localization with BALROG

      Ongoing data analysis projects

      • 10:15
        POLARIZATION ANALYSIS FOR REAL INSTRUMENTS 20m

        The future of x-ray polarimetry looks bright. Unfortunately, the sources we look at are not. Low and high count measurements both require proper statistical treatment and the literature on polarization statistics is derived from regularity conditions designed for optical measurements. I will discuss these approaches and present a new approach appropriate for both idealized and real x-ray polarimeters. Additionally, I will show that concepts such as "bias" are purely the result of improper statistical treatment.

        Speaker: Dr J. Michael Burgess (MPE)
      • 10:35
        The BALROG for GRB localization 35m
        Speaker: Mr Francesco Berlato (MPE)
    • 11:10 11:30
      Data Analysis: Future plans with POLAR data: Geneva

      Ongoing data analysis projects

      • 11:10
        Plans for future analysis POLAR data in Geneva 20m
        Speaker: Merlin Reynaard Kole (Universite de Geneve (CH))
    • 11:30 12:00
      Data Analysis: Future plans with POLAR data: IHEP

      Ongoing data analysis projects

      • 11:30
        Plans for GRB analysis with POLAR data at IHEP 30m
        Speaker: Jianchao Sun (Institute of High Energy Physics, Chinese Academy of Sciences)
    • 12:00 13:00
      Lunch 1h
    • 13:00 14:00
      Novel Analysis methods: Forward folding polarization data
      • 13:00
        Synchrotron emission and polarization 1h

        We present the first joint fits of POLAR and GBM using proper likelihoods, a new forward-folding technique, and physical models. We will discuss the approach, the software (3ML) that enabled this analysis and the physical framework within which we interpret our results.

        Speaker: Dr J. Michael Burgess (MPE)
    • 14:00 15:00
      Novel Analysis methods: CDCI: Plans for online analysis tools for polarization data
    • 15:00 15:30
      Coffee Break 30m
    • 15:30 16:15
      Novel Analysis methods: CDCI: POLAR data demonstration
    • 16:15 17:15
      Novel Analysis methods: Discussion: What do we need to make polarization analysis accessible?
      • 16:15
        How do we make polarization analysis open? 1h

        With the increase in available polarization data it becomes possible to make this data public and allow any interested party to perform analysis on it. This requires simple, transparent thoroughly tested public tools as well as data in easy to use formats.

        We aim to discus here what people from the theory and analysis community would like to do with public polarization data and how we can best provide such tools.

        Speaker: Merlin Reynaard Kole (Universite de Geneve (CH))
    • 09:30 11:15
      Final discussions: Planning future projects
    • 11:15 11:30
      Final discussions: Closing