O(N) quintessence
Astrophysics
2009-11-06 v3 General Relativity and Quantum Cosmology
Abstract
We study a new class of quintessence models, in which the scalar field possesses a O(\textit{N}) internal symmetry. We give a critical condition of instability for the potential against Q ball formation. We find that the most widely used potentials of quintessence don't satisfy the above condition, and therefore the O(\textit{N}) quintessence with these potential will not lead to the Q ball formation. It is worth noting that O(\textit{N}) quintessence with cosine-type potential is especially interesting in that the angular contribution is not negligible.
Keywords
Cite
@article{arxiv.astro-ph/0107171,
title = {O(N) quintessence},
author = {Xin-zhou Li and Jian-gang Hao and Dao-jun Liu},
journal= {arXiv preprint arXiv:astro-ph/0107171},
year = {2009}
}
Comments
9 pages, 1 figure, this updated version will appear in Class. Quantum Grav