The phase diagram of neutral quark matter: The effect of neutrino trapping

نویسندگان

  • Stefan B. Rüster
  • Verena Werth
  • Michael Buballa
  • Igor A. Shovkovy
  • Dirk H. Rischke
چکیده

Stefan B. Rüster, ∗ Verena Werth, † Michael Buballa, ‡ Igor A. Shovkovy, § and Dirk H. Rischke ¶ Institut für Theoretische Physik, J.W. Goethe-Universität, D-60438 Frankfurt am Main, Germany Institut für Kernphysik, Technische Universität Darmstadt, D-64289 Darmstadt, Germany 3 Frankfurt Institute for Advanced Studies, J.W. Goethe-Universität, D-60438 Frankfurt am Main, Germany (Dated: November 3, 2006)

برای دانلود رایگان متن کامل این مقاله و بیش از 32 میلیون مقاله دیگر ابتدا ثبت نام کنید

ثبت نام

اگر عضو سایت هستید لطفا وارد حساب کاربری خود شوید

منابع مشابه

Color-Neutral Superconducting Quark Matter

We investigate the consequences of enforcing local color neutrality on the color superconducting phases of quark matter by utilizing the Nambu-JonaLasinio model supplemented by diquark and the t’Hooft six-fermion interactions. In neutrino free matter at zero temperature, color neutrality guarantees that the number densities of u, d, and s quarks in the Color-Flavor-Locked (CFL) phase will be eq...

متن کامل

Phase Diagram of Neutral Quark Matter at Moderate Densities

We discuss the phase diagram of moderately dense, locally neutral three-flavor quark matter using the framework of an effective model of quantum chromodynamics with a local interaction. The phase diagrams in the plane of temperature and quark chemical potential as well as in the plane of temperature and lepton-number chemical potential are discussed.

متن کامل

Phase diagram of neutral quark matter: Self-consistent treatment of quark masses

Theoretical studies suggest that quark matter at suffi ciently high densities and suffi ciently low temperatures may be a color superconductor. (For a review on color superconductivity see for example, Ref. [1].) In nature such conditions appear in the central regions of neutron stars. Therefore it is possible that matter is color superconducting in the cores of these objects. In compact stars ...

متن کامل

From Neutron Stars to Strange Stars

It is generally agreed that the tremendous densities reached in the centers of neutron stars provide a high pressure environment in which numerous particles processes are likely to compete with each other. These processes range from the generation of hyperons to quark deconfinement to the formation of kaon condensates and H-matter [1]. Another striking possibility concerns the formation of abso...

متن کامل

Quark-Hadron Phase Transitions in Young and Old Neutron Stars

The mixed phase of quarks and hadrons which might exist in the dense matter encountered in the varying conditions of temperature and trapped neutrino fraction in proto-neutron stars is studied. The extent that the mixed phase depends upon the thermodynamical parameters as well as on the stiffness of matter in the hadronic and quark phases is discussed. We show that hadronic equations of state t...

متن کامل

ذخیره در منابع من


  با ذخیره ی این منبع در منابع من، دسترسی به آن را برای استفاده های بعدی آسان تر کنید

عنوان ژورنال:

دوره   شماره 

صفحات  -

تاریخ انتشار 2006