Oscillatons revisited
Abstract
In this paper, we study some interesting properties of a spherically symmetric oscillating soliton star made of a real time-dependent scalar field which is called an oscillaton. The known final configuration of an oscillaton consists of a stationary stage in which the scalar field and the metric coefficients oscillate in time if the scalar potential is quadratic. The differential equations that arise in the simplest approximation, that of coherent scalar oscillations, are presented for a quadratic scalar potential. This allows us to take a closer look at the interesting properties of these oscillating objects. The leading terms of the solutions considering a quartic and a cosh scalar potentials are worked in the so called stationary limit procedure. This procedure reveals the form in which oscillatons and boson stars may be related and useful information about oscillatons is obtained from the known results of boson stars. Oscillatons could compete with boson stars as interesting astrophysical objects, since they would be predicted by scalar field dark matter models.
Cite
@article{arxiv.gr-qc/0104093,
title = {Oscillatons revisited},
author = {L. Arturo Urena-Lopez},
journal= {arXiv preprint arXiv:gr-qc/0104093},
year = {2009}
}
Comments
10 pages REVTeX, 10 eps figures. Updated files to match version published in Classical and Quantum Gravity