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Diego Saez-Gomez

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Cosmological evolution<br />

in viable f(R)<br />

Hu-Sawicki and Nojiri-Odintsov model<br />

Deceleration parameter<br />

Cosmological evolution in viable modified gravity 9<br />

q = −aä/ȧ 2 DSG, Class.Quant.Grav. 30 095008 (2013)<br />

0.4<br />

0.2<br />

0.0<br />

HS<br />

NO<br />

CDM<br />

0.5<br />

0.0<br />

HS<br />

NO<br />

CDM<br />

0.2<br />

0.4<br />

0.5<br />

0.6<br />

0.8<br />

1.0<br />

1.0<br />

1.0 0.5 0.0 0.5 1.0<br />

z<br />

"CDM initial (a) conditions<br />

1.0 0.5 0.0 0.5 1.0<br />

z<br />

Phantom (b) initial conditions<br />

Figure 3: Evolution of the deceleration parameter q = −aä/ȧ 2 for the models F HS (R) and F NO (R)

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