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

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94 EXACT SOLUTIONS AND SCALAR FIELDS IN GRAVITY<br />

obeys the follow<strong>in</strong>g “dynamic” equation<br />

together with its constra<strong>in</strong>t<br />

Its solutions <strong>de</strong>term<strong>in</strong>e the way these mo<strong>de</strong>ls exp<strong>and</strong> via the scale factor<br />

function which, from Eq.(11), is given by<br />

Eq.(12) whose <strong>in</strong>tegral is<br />

together with Eq.(13) turn out the follow<strong>in</strong>g solutions. For k= 0,<br />

with<br />

while <strong>and</strong> rema<strong>in</strong> un<strong>de</strong>term<strong>in</strong>ed. Therefore, for the FRW flat<br />

space three different cosmic solutions exist, dist<strong>in</strong>guished by the sign of<br />

the discrim<strong>in</strong>ant which <strong>de</strong>pends the coupl<strong>in</strong>g parameter<br />

<strong>and</strong> through on the equation of state. For the discrim<strong>in</strong>ants<br />

the scalar field has two branches: one with an<br />

<strong>in</strong>creas<strong>in</strong>g function of time, <strong>and</strong> the other with a <strong>de</strong>creas<strong>in</strong>g function<br />

of time [7].<br />

For spaces one obta<strong>in</strong>s a similar solution:

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