Testing the Field Correlator Method with astrophysical constraints

Details Testing the Field Correlator Method with astrophysical constraints Testing the Field Correlator Method with astrophysical constraints

2009-01-08

arxiv.org/abs/0901.1035v1

PoS Confinement8:149,2008

Physics

High Energy Physics

High Energy Physics - Phenomenology

5 pages, 3 figures, published in the Proceedings of the 8th Conference on Quark Confinement and Hadron Spectrum, Mainz (German

Scientific paper

We study the structure of hybrid stars with the Field Correlator Method, extended to the zero temperature limit, for the quark phase. For the hadronic phase, we use the microscopic Brueckner-Hartree- Fock many-body theory. The comparison with the neutron star mass phenomenology puts serious constraints on the currently adopted values of the gluon condensate $G_2 \simeq 0.006-0.007 \rm {GeV^4}$, and the large distance static $Q \bar Q$ potential.

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