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Home All issues Volume 665 (September 2022) A&A, 665 (2022) A129 Full HTML
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Table 1.

Simulation properties for simulations with an AGN.

Simulation Initial Jet energy fgrad Thermal CR CR streaming CR streaming
name B field fraction conduction diffusion advection heating
HYDRO No 100% kinetic 0.2 No No No No
MHDc Yes 100% kinetic 0.2 Yes No No No
CRc_dsh Yes 10% kinetic, 90% CR 0.2 Yes Yes Yes Yes
CRc_dsh_weakcr Yes 90% kinetic, 10% CR 0.2 Yes Yes Yes Yes
CRc Yes 10% kinetic, 90% CR 0.2 Yes No No No
CRc_d Yes 10% kinetic, 90% CR 0.2 Yes Yes No No
CRc_s Yes 10% kinetic, 90% CR 0.2 Yes No Yes No
CRc_h Yes 10% kinetic, 90% CR 0.2 Yes No No Yes
CRc_ds Yes 10% kinetic, 90% CR 0.2 Yes Yes Yes No
CRc_dh Yes 10% kinetic, 90% CR 0.2 Yes Yes No Yes
CRc_sh Yes 10% kinetic, 90% CR 0.2 Yes No Yes Yes
CRc_dsh_f0.5 Yes 10% kinetic, 90% CR 0.5 Yes Yes Yes Yes
CRc_dsh_f1 Yes 10% kinetic, 90% CR 1 Yes Yes Yes Yes
CRc_dsh_f1_2* Yes 10% kinetic, 90% CR 1 Yes Yes Yes Yes
CRc_dsh_1 Yes 10% kinetic, 90% CR 0.2 Yes Yes Yes Yes
CRc_dsh_2 Yes 10% kinetic, 90% CR 0.2 Yes Yes Yes Yes

Notes. All simulations have a total cluster mass of 8 × 1014 M⊙ and an BH with a mass of originally 1.6 × 1010 M⊙. All MHD simulations treat electrons and ions separately, while the non-MHD simulation (HYDRO) has only one temperature (and no CR). fgrad stands for the strength of the gradient descent for the BH (see Sect. 3.6.1). The asterisk in CRc_dsh_f1_2* indicates that the sub-grid drag force from gas and stars is turned off.

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