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Accretion Models of Gamma‐Ray Bursts

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Figure

Fig. 1.— Contours of ta bold dashed line. The three dotted lines correspond to three important transitions, computedwith the analytical approximations ofgas-pressure-dominated NDAF to a degeneracy-pressure-dominated NDAF (equation 31), and (iii)the transit
Fig. 2.— Contours of accretion efficiency ξThe contour levels correspond to log = macc/md in the rout-md plane for m3 = 1 and α−1 = 1
Fig. 3.— Contours of accretion efficiency ξ = ˙m/m ˙inj in the rout- ˙minj (in solar masses per second)plane

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