Marco Baldi
Marco Baldi
Marco Baldi
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m c<br />
1.4<br />
1.3<br />
1.2<br />
1.1<br />
1.0<br />
Features of interacting dark energy<br />
1) MASS VARIATION<br />
of coupled matter particles<br />
Mass correction for different coupled dark energy models<br />
CDM ( = 0, c=0)<br />
RP1 ( = 0.143, c=0.04)<br />
RP2 ( = 0.143, c=0.08)<br />
RP3 ( = 0.143, c=0.12)<br />
RP4 ( = 0.143, c=0.16)<br />
RP5 ( = 0.143, c=0.2)<br />
0.9<br />
0 10 20 30 40 50<br />
z<br />
Tuesday, July 6, 2010<br />
<strong>Marco</strong> <strong>Baldi</strong> - MGADS, Strasbourg 16 VI 2010<br />
2) MODIFIED EXPANSION<br />
due to the Early DE component
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