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In this work, we review how the mass and the width of the pole behave in a regime where temperature is below the critical chiral transition value. This is attained by considering a large- invariant Non-Linear Sigma Model (NLSM) such that we can study the dynamical generation of a resonance. Introducing thermal effects via the imaginary time formalism allows us to study the behavior of the pole and relate it to chiral restoration.

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