Thermomagnetic correlation lengths of strongly interacting matter in

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Thermomagnetic correlation lengths of strongly interacting matter in the Nambu-Jona-Lasinio model M. Loewe Pontificia

Thermomagnetic correlation lengths of strongly interacting matter in the Nambu-Jona-Lasinio model M. Loewe Pontificia Universidad Católica de Chile and CCTVAL UTFSM, Valparaíso, January, 2018.

This talk is based on the following articles: Thermomagnetic correlations lengths of strongle interacting

This talk is based on the following articles: Thermomagnetic correlations lengths of strongle interacting matter in the Nambu-Jona-Lasinio model, Phys. Rev. D 96 (2017) 034007, by. A. Ayala, L. A. Hernández, M. Loewe, A. Raya, J. C. Rojas, and R. Zamora Thermomagnetic properties of the strong coupling in the local Nambu. Jona-Lasinio model. PHys. Rev. D 94 (2016) 054019, by A. Ayala, C. A. Dominguez, L. A. Hernandez, M. Loewe, A. Raya, J. C. Rojas and C. Villavicencio I acknowledge support from: FONDECYT 1170107 and PIA/BASAL FB 0821

Here we will use the Nambu-Jona-Lasinio model (NJL) for discussing strongly interacting matter under

Here we will use the Nambu-Jona-Lasinio model (NJL) for discussing strongly interacting matter under the influence of a magnetic field. In the mean field approximation where and We get, then, the “gap equation”

The light quark condensate is given by The effect of the magnetic field is

The light quark condensate is given by The effect of the magnetic field is reflected in the dressing of the quark propagator. Once we take thermomagnetic condensates from Lattice we have information about M(B, T)and G(B, T).

Schwinger’s proper time representation of the fermionic propagator

Schwinger’s proper time representation of the fermionic propagator

We have chosen the homogeneous magnetic field to point in the z-direction. We use

We have chosen the homogeneous magnetic field to point in the z-direction. We use the “symmetric gauge” and we defined We introduce finite temperature in the Matsubara formalism

In this way where The model is not renormalizable. We isolate the vacuum contribution

In this way where The model is not renormalizable. We isolate the vacuum contribution which has to be regularized. It is the only divergent term. The thermomagnetic contribution turns out to be finite.

The vacuum contribution The thermomagnetic contribution

The vacuum contribution The thermomagnetic contribution

In the previous expression M = M (B, T), such that when B, T

In the previous expression M = M (B, T), such that when B, T → 0, M → M 0. To fix the vacuum values of the condensate and the dynamical generted mass, we choose the ultraviolet cutoff such that the model reproduces the Physical mass of the pion and of the pion decay constant. Two set of parameters for τ0, condensate and M 0

The effective Coupling

The effective Coupling

Among different quantities, we may calculate the pseudocritical temperature. This is the value of

Among different quantities, we may calculate the pseudocritical temperature. This is the value of T that maximizes the chiral susceptibility To compare with the lattice results it is necessary to rescale the temperature.

To get a better physical understanding about IMC, we will proceed to study the

To get a better physical understanding about IMC, we will proceed to study the correlation function between two test quarks, with the same quantum numbers, in coordinate space

For T well beyond Tc = 176 Me. V, both correlation distances increase monotonically.

For T well beyond Tc = 176 Me. V, both correlation distances increase monotonically. For lower values of T there is a turnover behavior where the correlation lengths start off decreasing slightly , increasing then again and, finally, decreasing for larger values of B. The behavior is totally differente (just decreasing) if we take M constant (instead of M(B, T)). There is a competition between B and T: The tightening induced by the classical force and the random thermal motion.

Conclusions The correlation length is an interesting object for analyzing thermomagnetico effects in strongly

Conclusions The correlation length is an interesting object for analyzing thermomagnetico effects in strongly correlated matter. When the correlation distances increases, the test charges are further apart and correspondingly their interaction becomes weaker. For large temperatures more particles pop up from vacuum contributing to screen the interaction between the test particles