Probing modified gravity in cosmic filaments

Alex Ho; Max Gronke; Bridget Falck; David F. Mota

doi:10.1051/0004-6361/201833899

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Volume 619 (November 2018)

A&A, 619 (2018) A122

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Table 1.

Model parameters of the simulation runs.

Name	\|f_R0\|	n	λ_ϕ^a (Mpc h⁻¹)	γ_max^b
fofr4	10⁻⁴	1	∼23.7	4/3
fofr5	10⁻⁵	1	∼7.5	4/3
fofr6	10⁻⁶	1	∼2.3	4/3

Name	a_ssb	β	L^a (Mpc h⁻¹)	γ_max^b
symm_A	0.50	1.0	1.0	∼1.75
symm_B	0.33	1.0	1.0	∼1.93
symm_C	0.50	2.0	1.0	∼7.00
symm_D	0.25	1.0	1.0	∼1.97

Notes. The values to the left of the vertical line are the model input parameters, and values to the right of it are derived physical properties which help to interpret our results.

^(a)

Range of the fifth force in vacuum.

^(b)

Maximum enhancement of gravity.

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