In this work, we study the possibility of finite-time future cosmological singularities appearing in $f(R,T)$ gravity, where $R$ is Ricci scalar and $T$ trace stress-energy tensor. We present theory both geometrical dynamically equivalent scalar-tensor representation obtain respective equations motion. a background Friedmann-Lema\^{i}tre-Robertson-Walker (FLRW) universe with an arbitrary curvat...

Recent advances in nuclear theory combined with new astrophysical observations have led to the need for specific theoretical models that actually apply phenomena on dense-matter physics. At same time, quantum chromodynamics (QCD) predicts existence of non-nucleonic degrees freedom at high densities neutron-star matter, such as quark matter. Within a confining matter model, which consists homoge...