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Short range correlations (SRC) have been known to be an important aspect ofnuclear theory for some time. Recent works have re-ignited interest on thistopic, particularly due to the fact that it has recently been demonstrated thatSRC may be responsible for breaking pairing gaps in nuclear matter. In thiswork we revisit the concept of SRC for beta equilibrated matter in neutronstars. We construct two equivalent models, with and without SRC and proceed toinvestigate the thermal evolution of stars described by such models. We showthat SRC play a major role in the thermal evolution of neutron stars. It willbe shown that while the SRC largely leaves the macroscopic properties of thestar unaltered, it significantly alters the proton fraction, thus leading to anearly onset of the direct Urca (DU) process, which in turns leads to starsexhibiting much faster cooling.

Short-range correlation effects on the neutron star cooling