The hardness–intensity correlation of photospheric emission from a structured jet for gamma-ray bursts
نویسندگان
چکیده
For many gamma-ray bursts (GRBs), hardness-intensity correlation (HIC) can be described by a power-law function, $E_{\rm p}\propto F^{\kappa}$, where p}$ is the peak energy of $\nu F_{\nu}$ spectrum, and $F$ instantaneous flux. In this paper, HIC non-dissipative photospheric emission from structured jet studied in different regimes. An intermediate photosphere, which contains both unsaturated saturated emissions introduced, we find positive $\kappa<1/4$ case. The same conclusion could generalized to hybrid without magnetic dissipations, or that with sub-photospheric dissipations fully thermalized. This may imply contribution peaking at $\sim1/2$ distribution observed $\kappa$ are mainly prompt GRBs synchrotron origin. Besides, photosphere give smaller low-energy photon index $\alpha$ than regime, naturally reproduce anti-correlation $\alpha-E_{\rm GRB pulse.
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ژورنال
عنوان ژورنال: Monthly Notices of the Royal Astronomical Society
سال: 2022
ISSN: ['0035-8711', '1365-8711', '1365-2966']
DOI: https://doi.org/10.1093/mnras/stac839