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Exact Solutions and Scalar Fields in Gravity - Instituto Avanzado de ...

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The FRW Universes with Barotropic Fluids <strong>in</strong> Jordan–Brans–Dicke Theory<br />

<strong>and</strong><br />

The l<strong>in</strong>e element for the FRW metric <strong>in</strong> coord<strong>in</strong>ates is<br />

where is the scale factor, <strong>and</strong> or st<strong>and</strong>s for positive,<br />

vanish<strong>in</strong>g or negative space curvature, respectively.<br />

For a perfect fluid <strong>in</strong> a FRW cosmology its ord<strong>in</strong>ary, but nonl<strong>in</strong>ear field<br />

equations comprise the two unknown variables <strong>and</strong><br />

is the field equation, together with<br />

where overdots st<strong>and</strong> for time <strong>de</strong>rivatives.<br />

2. BAROTROPIC FLUIDS<br />

The equation with dist<strong>in</strong>guish barotropic<br />

fluids. The conservation equation<br />

yields<br />

However <strong>in</strong>stead of I use <strong>in</strong> this section the “time parameter<br />

<strong>de</strong>f<strong>in</strong>ed by with With it, the field equation is<br />

once formally <strong>in</strong>tegrated<br />

where is an <strong>in</strong>tegration constant, <strong>and</strong><br />

93

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