| Article ID | Journal | Published Year | Pages | File Type |
|---|---|---|---|---|
| 1839504 | Nuclear Physics A | 2007 | 4 Pages |
Abstract
The normal phase of dense quark matter allows a systematic low energy expansion even in the strong coupling regime relevant for the physics of compact stars. I present the main ideas that lead to this conclusion and discuss how the expansion can be used to obtain qualitative strong coupling results for bulk properties of dense matter.
Related Topics
Physical Sciences and Engineering
Physics and Astronomy
Nuclear and High Energy Physics
