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

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

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The <strong>in</strong>fluence of scalar fields <strong>in</strong> protogalactic <strong>in</strong>teractions 215<br />

theory of gravity, <strong>in</strong>clud<strong>in</strong>g a number of topics: merg<strong>in</strong>gs [16, 17], mix<strong>in</strong>g<br />

processes [18], simulation of s<strong>in</strong>k<strong>in</strong>g satellites [19], <strong>and</strong> mass <strong>and</strong><br />

energy lost <strong>in</strong> tidal <strong>in</strong>teractions [20], among others. However, we ma<strong>de</strong><br />

our calculations with<strong>in</strong> the framework of scalar-tensor theories, <strong>in</strong> the<br />

Newtonian limit, to <strong>in</strong>vestigate the <strong>in</strong>fluence of massive scalar fields on<br />

the dynamics.<br />

This paper is organized as follows: In section 2 we present the Newtonian<br />

approximation of a typical scalar field theory. In section 3, we<br />

present our mo<strong>de</strong>ls of protogalaxies, the <strong>in</strong>itial conditions, <strong>and</strong> the results.<br />

The conclusions are <strong>in</strong> section 4.<br />

2. SCALAR FIELDS AND THE NEWTONIAN<br />

APPROXIMATION<br />

We consi<strong>de</strong>r a typical scalar field theory given by the follow<strong>in</strong>g Lagrangian<br />

from which we get the gravity equations,<br />

<strong>and</strong> the scalar field equation<br />

We expect to have nowadays small <strong>de</strong>viations of the scalar fields<br />

around the background <strong>de</strong>f<strong>in</strong>ed here as If we <strong>de</strong>f<strong>in</strong>e<br />

the Newtonian approximation gives [21]<br />

where we have done<br />

<strong>and</strong>

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