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Marco Baldi

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The first hydrodynamical high-resolution N-body simulations for a weak<br />

DE-CDM VARIABLE interaction: [<strong>Baldi</strong>, arXiv:1005.2188]<br />

M / crit<br />

10 5<br />

10 4<br />

10 3<br />

10 2<br />

10 1<br />

Tuesday, July 6, 2010<br />

CDM<br />

EXP010a2<br />

EXP015a3<br />

EXP010e2<br />

EXP010e3<br />

EXP015e3<br />

z = 0.00000<br />

Resuts (IV): halo density profiles<br />

Density profiles for Group nr. 6<br />

M200(CDM) = 1.44298e+14 h -1 M O•<br />

N=2x512 3<br />

L=80Mpc/h<br />

Hydro<br />

10 100 1000<br />

r [ h -1 kpc ]<br />

<strong>Marco</strong> <strong>Baldi</strong> - MGADS, Strasbourg 16 VI 2010<br />

DENSITY PROFILES<br />

The combination of the friction<br />

term and of the mass variation of<br />

(coupled) CDM particles affects<br />

the virial equilibrium of collapsed<br />

objects.... BUT:<br />

If the coupling grows in time,<br />

there is also a decrease of the<br />

gravitational potential energy of<br />

halos. Two effects are competing,<br />

and can determine both shallower<br />

and steeper density profiles<br />

depending on the existence of a<br />

“Growing ϕMDE” phase.

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