Phases of nuclear matter are crucial in the determination of physical properties of neutron
stars (NS). In the core of NS, the density and pressure become so large that the nuclear …

In the late age of developing quantum mechanics, Lev Landau made great efforts to
understand the nature of matter, even stellar matter, by applying the quantum theory. Ninety …

Tidal deformation of neutron star with multiquark core is calculated using nuclear and
multiquark equations of state. The equation of state of the multiquark phase from the …

The quadrupole normal-mode oscillation frequency fn of a multiquark star are computed for
n= 1–5. At the transition from low to high density multiquark in the core region, the first two …

Moment of inertia (I), rotational (tidal) Love number (λ (rot)), and quadrupole moment (Q) of
slowly rotating massive neutron stars (NSs) with holographic multiquarks (MQs) core are …

We study thermodynamic properties of the multiquark nuclear matter. The dependence of
the equation of state on the colour charges is explored both analytically and numerically in …

We consider contributions of the open-string singlet (OSS) interaction to the proton–proton
scattering. Modelling baryon and meson as instanton and open string in the effective QCD …

We review the holographic multiquark states in the deconfined quark‐gluon plasma. Nuclear
matter can become deconfined by extremely high temperature and/or density. In the …

Tidal deformation of neutron star with multiquark core is calculated using nuclear and
multiquark equations of state. The equation of state of the multiquark phase from the …

We study the magnetic properties of the coloured multiquark states in the quark-gluon
plasma where the gluons are deconfined and the chiral symmetry is still broken, using the …