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

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

The irrotational solution presented <strong>in</strong> [8] was found by impos<strong>in</strong>g<br />

the Ansatz<br />

A word is <strong>in</strong> or<strong>de</strong>r concern<strong>in</strong>g that choice. It was <strong>in</strong>spired by the fact<br />

that, for a Newtonian fluid rotat<strong>in</strong>g rigidly, one has (with the<br />

appropriate <strong>de</strong>f<strong>in</strong>itions of <strong>and</strong> <strong>in</strong> the un<strong>de</strong>rly<strong>in</strong>g Eucli<strong>de</strong>an metric);<br />

it seemed then natural to impose (34) as a simplify<strong>in</strong>g assumption <strong>in</strong><br />

the irrotational case, with the role of taken over by Although this<br />

Ansatz did work as an aid <strong>in</strong> f<strong>in</strong>d<strong>in</strong>g the solution, we should bear <strong>in</strong> m<strong>in</strong>d,<br />

however, that is satisfied due to the fact that <strong>in</strong> the Newtonian<br />

case the vorticity l<strong>in</strong>es are straight l<strong>in</strong>es, whereas <strong>in</strong> a relativistic fluid<br />

one would expect a dynamical (multipole-like) distribution for or<br />

In or<strong>de</strong>r to arrive at the solution <strong>in</strong> [8], a further Ansatz of a more<br />

mathematical nature was imposed; the end result was that all the quantities<br />

of the solution, <strong>in</strong>clud<strong>in</strong>g the metric, can be written <strong>in</strong> terms of<br />

a s<strong>in</strong>gle function ( means here a coord<strong>in</strong>ate!), which satisfies the<br />

second-or<strong>de</strong>r ord<strong>in</strong>ary differential equation<br />

where is a constant, <strong>and</strong> sub<strong>in</strong>dices <strong>de</strong>note ord<strong>in</strong>ary <strong>de</strong>rivatives. Equation<br />

(35) can be transformed to a first-or<strong>de</strong>r one, which turns out to be<br />

an Abel equation of the first k<strong>in</strong>d. The (non-constant) angular velocity<br />

distribution for the rotat<strong>in</strong>g fluid is given by<br />

where <strong>and</strong> are constants. The equation of state is that of stiff matter,<br />

<strong>and</strong> the solution is of Petrov type I. The surface area of the body<br />

is f<strong>in</strong>ite. The solution admits no further Kill<strong>in</strong>g<br />

vectors.<br />

A few other differentially rotat<strong>in</strong>g <strong>in</strong>terior solutions have subsequently<br />

been found [10]. Needless to say, none of the differentially rotat<strong>in</strong>g<br />

<strong>in</strong>terior solutions with no extra Kill<strong>in</strong>g fields has yet been shown to admit<br />

a match<strong>in</strong>g asymptotically flat exterior vacuum field, a fact similar to<br />

that mentioned above for rigidly rotat<strong>in</strong>g solutions.<br />

4. VACUUM AS A “PERFECT FLUID”. THE<br />

“RIGID ROTATION” AND THE<br />

“IRROTATIONAL” GAUGES<br />

Equations (19)-(32) still hold when (<strong>and</strong> (33) becomes<br />

a trivial i<strong>de</strong>ntity.) One important difference, however, is the follow<strong>in</strong>g.

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