The neutrino signal from protoneutron star accretion and black hole formation

Open Access

Table 1:

Thermodynamic conditions of the PNSs in Fig. 4, comparing the central data (a) with the maximum temperature (b).
EoS	T	$\rho$	Y $_{\rm e}$
	[MeV]	10¹⁴ [g/cm³]
eos1 (a)	29.78	12.0	0.299
eos1 (b)	96.05	5.86	0.270
eos2 (a)	50.27	9.16	0.297
eos2 (b)	92.04	4.37	0.271

Source LaTeX | All tables | In the text

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