The mass distribution in the outskirts of clusters of galaxies as a probe of the theory of gravity

Open Access

Table 1.

Samples of simulated clusters.

z	ΛCDM-L			ΛCDM-I			ΛCDM-H
	Size	M_200c	MAR (Γ_dyn)	Size	M_200c	MAR (Γ_dyn)	Size	M_200c	MAR (Γ_dyn)
		[10¹⁴ h⁻¹ M_⊙]	[10³ h⁻¹ M_⊙] yr⁻¹		[10¹⁴ h⁻¹ M_⊙]	[10³ h⁻¹ M_⊙] yr⁻¹		[10¹⁴ h⁻¹ M_⊙]	[10³ h⁻¹ M_⊙] yr⁻¹
0.00	2755			407			41
0.09	2656			323			20
0.20	2467			275			21
0.30	2110			233			17
0.40	2046			151
0.50	1730			104
0.60	1481			87
0.69	1272			51
0.79	1067			32
0.89	862			22
1.00	646			11

z	fR4-L			fR4-I			fR4-H
	Size	M_200c	MAR (Γ_dyn)	Size	M_200c	MAR (Γ_dyn)	Size	M_200c	MAR (Γ_dyn)
		[10¹⁴ h⁻¹ M_⊙]	[10³ h⁻¹ M_⊙] yr⁻¹		[10¹⁴ h⁻¹ M_⊙]	[10³ h⁻¹ M_⊙] yr⁻¹		[10¹⁴ h⁻¹ M_⊙]	[10³ h⁻¹ M_⊙] yr⁻¹

0.00	3301			652			58
0.09	3249			550			55
0.20	3105			432			40
0.30	2919			334			30
0.40	2717			256
0.50	2351			203
0.60	2115			135
0.69	1742			95
0.79	1534			57
0.89	1256			34
1.00	1039			23

Notes. The upper (lower) table is for ΛCDM (fR4).

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