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

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

authors <strong>and</strong> became a start<strong>in</strong>g po<strong>in</strong>t for different multidimensional generalizations.<br />

Here we consi<strong>de</strong>r a more general class of exact solutions <strong>in</strong> a D–<br />

dimensional mo<strong>de</strong>l with scalar fields <strong>and</strong> fields of forms, <strong>in</strong>spired by<br />

mo<strong>de</strong>rn unified mo<strong>de</strong>ls. Such generalization is <strong>in</strong>ten<strong>de</strong>d to study general<br />

gravitational <strong>and</strong> cosmological properties of these mo<strong>de</strong>ls. Clear, that<br />

most of their symmetries are not preserved <strong>in</strong> arbitrary dimensions, but<br />

are recovered <strong>in</strong> 10 or 11. Among our solutions, there are solutions with<br />

harmonic functions obta<strong>in</strong>ed by the null–geo<strong>de</strong>sic method suggested by<br />

G. Neugebauer <strong>and</strong> D. Kramer <strong>in</strong> [2]. We also consi<strong>de</strong>r exact spherically<br />

symmetric, cosmological <strong>and</strong> black hole configurations with<br />

All of them have a general structure s<strong>in</strong>ce m<strong>in</strong>or restrictions on parameters<br />

of the mo<strong>de</strong>l are imposed. We also present PPN parameters for<br />

4–dimensional section of the metric with the aim of study<strong>in</strong>g new observational<br />

w<strong>in</strong>dows to unified mo<strong>de</strong>ls <strong>and</strong> extra dimensions [3, 4, 5].<br />

2. THE MODEL<br />

We consi<strong>de</strong>r the mo<strong>de</strong>l governed by the action<br />

where is the metric on the manifold M, dim M = D,<br />

is a vector from dilatonic scalar fields, is a non–<br />

<strong>de</strong>generate matrix<br />

is a on a D–dimensional manifold M,<br />

is a cosmological constant <strong>and</strong> is a 1–form on<br />

In (0) we <strong>de</strong>note<br />

where is some f<strong>in</strong>ite set.<br />

In the mo<strong>de</strong>ls with one time all when the signature of the<br />

metric is (–1, +1,..., +1).<br />

2.1. ANSATZ FOR COMPOSITE P-BRANES<br />

Let us consi<strong>de</strong>r the manifold <strong>and</strong> metric as

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