Impact of CFL Quark Matter on the Cooling of Compact Stars

Details Impact of CFL Quark Matter on the Cooling of Compact Stars Impact of CFL Quark Matter on the Cooling of Compact Stars

2003-03-10

arxiv.org/abs/hep-ph/0303073v1

Physics

High Energy Physics

High Energy Physics - Phenomenology

7 pages. Talk presented at 2002 International Workshop "On Strong Coupling Gauge Theories And Effective Field Theories" (SCGT

Scientific paper

The cooling mechanism of compact stars with quark cores in the color-flavor locked phase is discussed. It is argued that the high thermal conductivity of the quark core plays a key role in the stellar cooling. It implies that the cooling time of compact stars with color-flavor locked quark cores is similar to that of ordinary neutron stars, unless the star is almost completely made of color-flavor locked quark matter.

Affiliated with

Also associated with

No associations

Rating

Impact of CFL Quark Matter on the Cooling of Compact Stars does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Impact of CFL Quark Matter on the Cooling of Compact Stars, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Impact of CFL Quark Matter on the Cooling of Compact Stars will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-283963