Boson Stars: Early History and Recent Prospects
Abstract
Boson stars are descendants of the so-called geons of Wheeler, except that they are built from scalar particles instead of electromagnetic fields. If scalar fields exist in nature, such localized configurations kept together by their self-generated gravitational field can form within Einstein's general relativity. In the case of complex scalar fields, an absolutely stable branch of such non-topological solitons with conserved particle number exists. Our present surge stems from the speculative possibility that these compact objects could provide a considerable fraction of the non-baryonic part of dark matter. In any case, they may serve as a convenient "laboratory" for studying numerically rapidly rotating bodies in general relativity and the generation of gravitational waves.
Cite
@article{arxiv.gr-qc/9801063,
title = {Boson Stars: Early History and Recent Prospects},
author = {Eckehard W. Mielke and Franz E. Schunck},
journal= {arXiv preprint arXiv:gr-qc/9801063},
year = {2007}
}
Comments
20 pages, 1 Postscript figure, LaTeX, uses mprocl.sty