The short-range and tensor correlations associated to realistic nucleon-nucleon interactions induce a population of high-momentum components in the many-body nuclear wave function. We study the impact of such high-momentum components on bulk observables associated to isospin asymmetric matter. The kinetic part of the symmetry energy is strongly reduced by correlations when compared to the non-interacting case. The origin of this behavior is elucidated using realistic interactions with different short-range and tensor structures. The existence of high-momentum components in the nuclear many-body wave function is a well-established property both from an experimental [1,2] and a theoretical points of view [3,4]. Short-range correlated pairs have been studied in detail at electron scattering facilities [5]. Two-nucleon knock-out reactions have identified the predominance of isospin I = 0 correlated pairs [2], an effect that has been related to the tensor component of the nucleon-nucleon (NN) interaction [6,7].The enhanced effect of correlations on neutron-proton (np) pairs with respect to neutronneutron (nn) pairs suggests that correlations can be increased (or even tuned) in isospin asymmetric systems, where a different number of np and nn pairs exist. Our microscopic many-body calculations indicate that the dependence of short-range and tensor correlations on the isospin asymmetry of the system, α = (N − Z)/(N + Z), is well understood from general theoretical principles [8]. One-body occupations, for instance, follow a systematic trend: neutrons become less depleted as the system becomes more neutron-rich, while the proton depletion increases [8,9].Here, rather than looking at microscopic properties, we want to quantify the effect that NN correlations have on the bulk properties of isospin asymmetric systems. By analysing the energy of symmetric, asymmetric and neutron matter obtained within a realistic many-body approach, we will draw conclusions on the impact of correlations on asymmetric systems.We will focus our attention on the symmetry energy, which characterises the properties of isospin-rich nuclei as well as neutron stars [10].To quantify the effect of correlations in a meaningful way, we use a many-body approximation that includes consistently short-range and tensor correlations. The ladder approximation, implemented within the self-consistent Green's functions (SCGF) approach, provides a microscopic description of these effects via a fully dressed propagation of nucleons in nuclear matter [4]. This is achieved by (a) computing the scattering of particles via a T -matrix (or effective interaction) in the medium, (b) extracting a self-energy out of the effective interaction and (c) using Dyson's equation to build two-body propagators which are subsequently inserted in the scattering equation [8,11]. To solve the close set of equations, an iterative numerical procedure is a must. Recent advances have allowed implementations both at zero [12] and at finite temperature [13] using fully realistic NN i...