Dense stellar matter in asymptotically free gauge theories: I. The high density limit |
| |
| Authors: | M.B. Kislinger P.D. Morley |
| |
| Affiliation: | Enrico Fermi Institute and Department of Physics, University of Chicago, Chicago, Illinois, 60637 USA |
| |
| Abstract: | In asymptotically free gauge theories perturbation theory may be used to obtain the behavior of dense stellar matter. The criteria for the determination of ?crit, the minimum density above which perturbation theory is valid, are presented. The asymptotic form for the quark-gluon thermodynamic potential is given. |
| |
| Keywords: | |
| 本文献已被 ScienceDirect 等数据库收录！ |
|
