Prospects of Prompt Gamma-Ray Burst Polarimetry with POLAR-2

TL;DR

POLAR-2 aims to measure gamma-ray burst polarization with high precision, enabling insights into emission mechanisms and jet physics by utilizing advanced spectro-polarimetric techniques on synthetic data.

Contribution

This paper demonstrates the potential of POLAR-2's High-energy Polarimetry Detector to constrain physical parameters of GRB emission models through novel time-resolved spectro-polarimetric analysis.

Findings

Can constrain polarization degree to about 2.2% for bright GRBs.

Allows distinguishing between different emission models.

Provides insights into magnetic field and jet structure.

Abstract

The dominant radiation mechanism that powers the prompt $\gamma$-ray emission in gamma-ray bursts (GRBs) remains poorly understood. High quality, time- and energy-resolved linear polarization measurements of prompt $\gamma$-ray photons can distinguish between synchrotron and inverse-Compton processes and provide crucial constraints on the outflow properties. This will be achieved by POLAR-2 that is proposed as a dedicated GRB polarimeter and successor to POLAR. The High-energy Polarimetry Detector (HPD) is one of the three instruments of POLAR-2 that features significantly improved sensitivity in the $(40-1000)$\,keV energy range and a detection area four times larger than that of POLAR. Here we demonstrate the capabilities of the HPD to constrain key physical model parameters by creating and fitting to synthetic sources using a time-resolved spectro-polarimetric theoretical model of prompt GRB emission. The time-resolved spectral and polarization fits are performed using a novel technique featuring maximum likelihood over an unbinned (in time and energy) list of detected events. The constrained model parameters directly relate to the underlying source physics that would reveal an accelerating, coasting or decelerating emission region. For a pulse fluence of $\mathcal{F}=10^{-5}\mathcal{F}_{-5}\,{\rm erg\,cm^{-2}}$ and higher we can constrain the time-integrated polarization degree to an absolute accuracy ($1\,\sigma$) of about $2.2\mathcal{F}_{-5}^{\,-1/2}$ per cent, as long as source photons dominate over the background. In bright GRBs, such unprecedented accuracy at these energies will allow to distinguish between different models for the prompt GRB emission mechanism and constrain the magnetic field geometry, jet angular structure and outflow composition.