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Subphotospheric Turbulence as a Heating Mechanism in Gamma-Ray Bursts

  • Authors: Jonathan Zrake, Andrei M. Beloborodov, and Christoffer Lundman

2019 The Astrophysical Journal 885 30.

  • Provider: AAS Journals

Caption: Figure 2.

Upper panel: turbulence cascade spectrum v() in the presence of Compton damping. The blue curve shows the cascade in a jet with optical depth ﹩\tau ={{\ell }}_{0}/{{\ell }}_{\star }={10}^{3}﹩ and the heating parameter ξ = 0.2; it has a viscous cutoff at ﹩{{\ell }}_{\mathrm{damp}}\gt {{\ell }}_{\star }﹩. The red curve shows a similar cascade when τ = 10 and ξ = 0.01; it does not cut off and extends to microscopic plasma scales ﹩{\ell }\ll {{\ell }}_{\star }﹩. In both cases, the jet has enthalpy w ≈ 2ξ (see the text). Bottom panel: comparison of the cascade timescale tturb() = /v() (the blue and red curves show the same models as in the upper panel) with the Compton damping timescale ﹩{t}_{\mathrm{damp}}({\ell })﹩ (black curve). Compton damping prevents the cascade from entering the shaded region where ﹩{t}_{\mathrm{turb}}\gt {t}_{\mathrm{damp}}﹩.

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