pith. sign in

arxiv: astro-ph/0107171 · v3 · submitted 2001-07-10 · 🌌 astro-ph · gr-qc

O(N) quintessence

classification 🌌 astro-ph gr-qc
keywords quintessencepotentialtextitballconditionformationaboveangular
0
0 comments X
read the original 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.

This paper has not been read by Pith yet.

discussion (0)

Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.