You are not logged in to this journal. Log in    |   Subscription Information

Phys. Rev. D 74, 094019 (2006) [32 pages]

Crystallography of three-flavor quark matter

Krishna Rajagopal1,2 and Rishi Sharma1
1Center for Theoretical Physics, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
2Nuclear Science Division, MS 70R319, Lawrence Berkeley National Laboratory, Berkeley, California 94720, USA

Received 5 June 2006; published 17 November 2006

We analyze and compare candidate crystal structures for the crystalline color superconducting phase that may arise in cold, dense but not asymptotically dense, three-flavor quark matter. We determine the gap parameter Delta and free energy Omega(Delta) for many possible crystal structures within a Ginzburg-Landau approximation, evaluating Omega(Delta) to order Delta6. In contrast to the two-flavor case, we find a positive Delta6 term and hence an Omega(Delta) that is bounded from below for all the structures that we analyze. This means that we are able to evaluate Delta and Omega as a function of the splitting between Fermi surfaces for all the structures we consider. We find two structures with particularly robust values of Delta and the condensation energy, within a factor of 2 of those for the CFL phase which is known to characterize QCD at asymptotically large densities. The robustness of these phases results in their being favored over wide ranges of density. However, it also implies that the Ginzburg-Landau approximation is not quantitatively reliable. We develop qualitative insights into what makes a crystal structure favorable, and use these to winnow the possibilities. The two structures that we find to be most favorable are both built from condensates with face-centered cubic symmetry: in one case, the <ud> and <us> condensates are separately face-centered cubic; in the other case <ud> and <us> combined make up a face-centered cube.

©2006 The American Physical Society

URL: http://link.aps.org/doi/10.1103/PhysRevD.74.094019
DOI: 10.1103/PhysRevD.74.094019
PACS: 12.38.-t; 12.38.Mh; 26.60.+c; 74.20.-z
  • 12.38.-t
    Quantum chromodynamics
  • 12.38.Mh
    Quark–gluon plasma
  • 26.60.+c
    Nuclear matter aspects of neutron stars
  • 74.20.-z
    Theories and models of superconducting state
  • YEAR: 2006

REFERENCES (52)

For access to fully linked references, you need to log in. For access to fully linked references, you need to Log in.

CITING ARTICLES

For access to citing articles, you need to log in.
For access to citing articles, you need to Log in.



A new free weekly publication from APS

Physics - A new free weekly publication from APS
Please visit physics.aps.org
 
Article Tools