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Dark Energy in f(R) Gravity - Indiana University

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Compatibility with observations I<br />

<br />

Use<br />

f(R) observations<br />

A. G. Riess et al., Astrophys. J. 607, 665 (2004)<br />

SNLS<br />

X clusters<br />

Gold<br />

ΛCDM<br />

Z t=-0.56+0.07-0.04<br />

j=1

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