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Table 1.

Properties of the two detected quasi-bound levels, v = 2,  J = 29 and v = 1,  J = 31, of H2 and their emission spectrum.

Transition λ A Ar τd
label (cm−1) (μm) (s−1) (s−1) (s) (K)
2 − 0 O(31) 1387.04 7.2096 2.704E−11 5.482E−06 8.130E12 676.0
2 − 0 Q(29) 4165.40 2.4007 4.592E−08 5.482E−06 8.130E12 676.0
2 − 0 S(27) 7034.45 1.4216 2.240E−07 5.482E−06 8.130E12 676.0
2 − 1 Q(29) 1944.67 5.1423 3.947E−07 5.482E−06 8.130E12 676.0
2 − 1 S(27) 4590.29 2.1785 2.944E−06 5.482E−06 8.130E12 676.0
2 − 2 S(27) 2399.19 4.1681 1.873E−06 5.482E−06 8.130E12 676.0
2 − 3 S(27) 489.60 20.4248 2.582E−10 5.482E−06 8.130E12 676.0
1 − 0 Q(31) 1974.02 5.0658 2.452E−07 5.219E−06 4.083E06 1520.5
1 − 0 S(29) 4752.38 2.1042 2.101E−06 5.219E−06 4.083E06 1520.5
1 − 1 S(29) 2531.65 3.9500 2.872E−06 5.219E−06 4.083E06 1520.5
1 − 2 S(29) 586.98 17.0364 4.963E−10 5.219E−06 4.083E06 1520.5

Notes. is the computed transition frequency; λ is the corresponding vacuum wavelength. A is the sum of the electric quadrupole and the magnetic dipole contributions to the Einstein radiative emission coefficients of the transition from Roueff & Abgrall (2022). Ar is the total radiative decay probability, and τd is the dissociation lifetime of the upper level. is the quasi-bound upper level energy expressed in K above the dissociation limit.

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