Noble gas enrichment in the Jovian atmosphere via disk photoevaporation

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Table 3

Calculation results with desorption energy given by SMK2016.

No.	L_*[L_⊙]	α₀	Sc	f_IPE	FUV[G₀]	f_vfrag	Lifetime [Myr]	Ar ^a	Kr ^a	Xe ^a	BPF ^b
S1	0.1	0.01	1.0	0.25	10	✓	5.27	1.37	2.21	2.10
S2	0.1	0.01	1.0	0.25	10³	✓	5.24	1.36	2.17	2.09
S3	0.1	0.01	1.0	0.25	10⁵	✓	4.36	1.01	1.29	1.75
S4	0.1	0.04	0.1	0.1	10	✓	7.98	1.37	3.8	3.61
S5	0.1	0.04	1.0	0.1	10	✓	7.97	2.01	3.41	2.40
S6	0.3	0.04	0.1	0.1	10	✓	6.9	1.0	1.01	4.06
S7	0.3	0.04	1.0	0.1	10	✓	6.89	1.02	1.36	3.4
S8	1.0	0.01	0.1	0.25	10	✓	4.42	1.0	1.0	1.0	✓
S9	1.0	0.01	0.1	0.25	10		4.42	1.0	1.0	1.0	✓
S10	1.0	0.01	0.1	0.25	10³		4.36	1.0	1.0	1.0	✓
S11	1.0	0.04	0.1	0.25	10	✓	3.42	1.0	1.0	1.0
S12	1.0	0.04	0.1	0.1	10	✓	5.63	1.0	1.0	1.01
S13 (fiducial)	1.0	0.04	1.0	0.1	10	✓	5.62	1.0	1.0	1.3
S14	1.0	0.1	0.1	0.25	10	✓	2.85	1.0	1.0	1.0	✓

Notes. ^(a)Noble gas elements, ‘Ar’, ‘Kr’ and ‘Xe’, stand for the noble gas enrichment in the Jovian atmosphere, [Ar/H]_Jup/[Ar/H]_solar, [Kr/H]_Jup/[Kr/H]_solal and [Xe/H]_Jup/[Xe/H]_solar. ^(b)‘BPF’ stands for the bimodal planetesimal formation at the H₂O ice line and the silicate sublimation line.

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