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Constraining the Type of Central Engine of GRBs with Swift Data

  • Authors: Liang Li, Xue-Feng Wu, Wei-Hua Lei, Zi-Gao Dai, En-Wei Lian, and Felix Ryde

2018 The Astrophysical Journal Supplement Series 236 26.

  • Provider: AAS Journals

Caption: Figure 4.

Temporal decay indices α2 vs. α1 for our samples (excluding the internal plateau bursts). The three solid lines indicate the closure relations of three specific external shock models invoking energy injection with the parameter q = 0, as is expected in the BH/magnetar central engine models. The red, black, and blue solid lines are the models α2 = (3α1 + 3)/2 (νm < νx < νc; ISM); α2 = (3α1 + 1)/2 (νm < νx < νc; wind); and ﹩{\alpha }_{2}=(3{\alpha }_{1}+2)/2\,({\nu }_{m}\lt {\nu }_{x}\lt {\nu }_{c}﹩; ISM and wind).

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