Table 3. Open in new tab Typical... | Oxford Academic

Table 3.

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Typical physical parameter values used in theoretical modelling of GRB afterglows.

Source	E_iso	γ₀	θ₀	n	p	\|$\xi ^2_{B}$\|	ξ_e	ϵ	θ_obs
	(erg)		(rad)	(cm⁻³)					(rad)
Standard GRBs^a	1.0 × 10⁵²	300	0.10	1.0	2.5	1.0 × 10⁻³	0.10	0	0
Failed GRBs^a	1.0 × 10⁵²	30	0.10	1.0	2.5	1.0 × 10⁻³	0.10	0	0
High-luminosity GRBs^a	1.0 × 10⁵⁴	300	0.10	1.0	2.5	1.0 × 10⁻³	0.10	0	0
Low-luminosity GRBs^a	1.0 × 10⁴⁹	300	0.10	1.0	2.5	1.0 × 10⁻³	0.10	0	0

Source	E_iso	γ₀	θ₀	n	p	\|$\xi ^2_{B}$\|	ξ_e	ϵ	θ_obs
	(erg)		(rad)	(cm⁻³)					(rad)
Standard GRBs^a	1.0 × 10⁵²	300	0.10	1.0	2.5	1.0 × 10⁻³	0.10	0	0
Failed GRBs^a	1.0 × 10⁵²	30	0.10	1.0	2.5	1.0 × 10⁻³	0.10	0	0
High-luminosity GRBs^a	1.0 × 10⁵⁴	300	0.10	1.0	2.5	1.0 × 10⁻³	0.10	0	0
Low-luminosity GRBs^a	1.0 × 10⁴⁹	300	0.10	1.0	2.5	1.0 × 10⁻³	0.10	0	0

^aRefer to Paper I.

Table 3.

Open in new tab

Typical physical parameter values used in theoretical modelling of GRB afterglows.

Source	E_iso	γ₀	θ₀	n	p	\|$\xi ^2_{B}$\|	ξ_e	ϵ	θ_obs
	(erg)		(rad)	(cm⁻³)					(rad)
Standard GRBs^a	1.0 × 10⁵²	300	0.10	1.0	2.5	1.0 × 10⁻³	0.10	0	0
Failed GRBs^a	1.0 × 10⁵²	30	0.10	1.0	2.5	1.0 × 10⁻³	0.10	0	0
High-luminosity GRBs^a	1.0 × 10⁵⁴	300	0.10	1.0	2.5	1.0 × 10⁻³	0.10	0	0
Low-luminosity GRBs^a	1.0 × 10⁴⁹	300	0.10	1.0	2.5	1.0 × 10⁻³	0.10	0	0

Source	E_iso	γ₀	θ₀	n	p	\|$\xi ^2_{B}$\|	ξ_e	ϵ	θ_obs
	(erg)		(rad)	(cm⁻³)					(rad)
Standard GRBs^a	1.0 × 10⁵²	300	0.10	1.0	2.5	1.0 × 10⁻³	0.10	0	0
Failed GRBs^a	1.0 × 10⁵²	30	0.10	1.0	2.5	1.0 × 10⁻³	0.10	0	0
High-luminosity GRBs^a	1.0 × 10⁵⁴	300	0.10	1.0	2.5	1.0 × 10⁻³	0.10	0	0
Low-luminosity GRBs^a	1.0 × 10⁴⁹	300	0.10	1.0	2.5	1.0 × 10⁻³	0.10	0	0

^aRefer to Paper I.