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LOFF, the inhomogeneous “faces” of color superconductivity

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Presentation on theme: "LOFF, the inhomogeneous “faces” of color superconductivity"— Presentation transcript:

1 LOFF, the inhomogeneous “faces” of color superconductivity
Marco Ruggieri Università degli Studi di Bari Conversano, 16 – 20 Giugno 2005

2 High density QCD Color Superconductivity
Hadrons at very high density and low temperature: deconfinement. Degrees of freedom: quarks and gluons. Quarks fill large Fermi surfaces. One gluon exchange is attractive in the color antisymmetric channel. Color Superconductivity

3 Pairing with zero total momentum
BCS color superconductivity Superficie di Fermi Fermi Surface BCS: Usare la figura della sfera di fermi per parlare degli impulsi utili per al dinamica. Pairing with zero total momentum

4 BCS color superconductivity 2
Phases characterized by diquark condensation: Superconductive Normal

5 In nature……… Fermi momenta of the quarks can be different, because:
Weak equilibrium Non-zero masses of the quarks Electrical and color neutrality How can this affect BCS superconductivity ?

6 Different Fermi momenta
u d From now on I consider only two flavor quark matter It is difficult to form pairs with total zero momentum

7 Inhomogeneous gap parameter
Pairs with non-zero total momenum Inhomogeneous gap parameter LOFF phase

8 Cristallography of the LOFF phase
One can make the following general ansatz: Usually the wave vectors are choosen along the direction of vertices of regular poliedra Cristallography

9 Interesting cristallographic structures
P=8 Face centered cube (F.C.C.) P=6 Body centered cube (B.C.C.)

10 Smearing of the gap parameter
My goal is to see which is the LOFF structure realized in quark matter. I can do this by comparing the free energy of the various structures. How can I compute such a free energy ? Gap equation = Free energy

11 Comparison of the free energies
One wave BCC FCC Dire che la procdura di smearing può essere ripetuta per le diverse strutture. BCS LOFF (Ruggieri et al )

12 LOFF and compact stars ? LOFF, gCFL CFL (if densities are high enough)
Mantel + hadron superfluid If quark matter is present in the core of a neutron star, then the LOFF phase could be realized there. LOFF, gCFL CFL (if densities are high enough)

13 If LOFF, how can it contribuite to the thermodynamics ?
Gapless fermion dispersion laws LOFF BCS Fermions are relevant for the thermodynamical properties. Spatial symmetries are spontaneously broken Phonons

14 Conlusions and open questions
Different Fermi momenta: pairs with non-zero momemtum. Cristallography of the LOFF phase: smearing approximation. LOFF with three flavors. Transport coefficients. Applications to condensed matter.

15 References In this talk I presented results obtained in collaboration with: R. Casalbuoni, M. Ciminale, R. Gatto, M. Mannarelli, G. Nardulli. Thanks to all of them. Thanks also to: V. Laporta, N. Ippolito, John Petrucci and, last but not least, M. La Calamita.


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