The Effect of Pair Cascades on the High-Energy Spectral Cutoff in Gamma-Ray Bursts

Abstract

The highly luminous and variable prompt emission in Gamma-Ray Bursts (GRBs) arises in an ultra-relativistic outflow. The exact underlying radiative mechanism shaping its non-thermal spectrum is still uncertain, making it hard to determine the outflow's bulk Lorentz factor $\Gamma$. GRBs with spectral cutoff due to pair production ($\gamma \gamma \to e^{+}{e}^{-}$) at energies $E_c\gtrsim 10$MeV are extremely useful for inferring $\Gamma$. We find that when the emission region has a high enough compactness, then as it becomes optically thick to scattering, Compton downscattering by non-relativistic $e^{\pm }$-pairs can shift the spectral cutoff energy well below the self-annihilation threshold, $E_{\mathrm{sa}}=\Gamma m_e{c}^2/(1+z)$. We treat this effect numerically and show that $\Gamma$ obtained assuming $E_c=E_{\mathrm{sa}}$ can under-predict its true value by as much as an order of magnitude.

5 pages, 3 figures, Accepted for publication in MNRAS Letters

References in corpus (2)

• The Physics of Gamma-Ray Bursts and Relativistic Jets
• Non-thermal Gamma-ray Emission from Delayed Pair Breakdown in a Magnetized and Photon-rich Outflow

Cited by in corpus (9)

• When Did the Remnant of GW170817 Collapse to a Black Hole?
• Temporal Evolution of Prompt GRB Polarization
• GRB Spectrum from Gradual Dissipation in a Magnetized Outflow
• Insights into the physics of GRBs from the high-energy extension of their prompt emission spectra
• Physical origin of GeV emission in the early phase of GRB 170405A: Clues from emission onsets with multi-wavelength observations
• Very High Energy Emission and Cascade Radiation of Gamma-Ray Burst Afterglows: Homogeneous Versus Wind External Media
• Understanding the Impact of Semi-numeric Reionization Models when using CNNs
• Nanophotonics for pair production
• Plasmas in Gamma-Ray Bursts: particle acceleration, magnetic fields, radiative Processes and environments