We present a self-consistent model for the study of the structure of a neutron star in strong
magnetic fields. Starting from a microscopic Lagrangian, this model includes the effect of the …

Spectra of the neutral heavy mesons, η c (1 S, 2 S), J/ψ, ψ (2 S), η b (1 S, 2 S, 3 S), ϒ (1 S, 2
S, 3 S), D, D*, B, B*, B s and B s*, in a homogeneous magnetic field are analyzed by using a …

We discuss strange stars admixed with fermionic dark matter in the presence of a strong
magnetic field using the two-fluid Tolman-Oppenheimer-Volkov equations. We describe …

A bstract We consider chiral perturbation theory for SU (2) at finite temperature T in a
constant magnetic background B. We compute the thermal mass of the pions and the pion …

Lattice QCD Simulations in External Background Fields Page 1 Chapter 7 Lattice QCD
Simulations in External Background Fields Massimo D’Elia 7.1 Introduction The properties of …

A bstract We investigate the quark-meson model in a magnetic field using the functional
renormalization group equation beyond the local-potential approximation. Our truncation of …

We use chiral perturbation theory for SU (2) to compute the leading loop corrections to the
thermal mass of the pions and the pion decay constant in the presence of a constant …

We consider the quark-meson model with two quark flavors in a constant external magnetic
field B at finite-temperature T and finite baryon chemical potential μ B. We calculate the full …

The vacuum to nuclear matter phase transition is studied in the presence of a constant
external background magnetic field with the mean-field approximation in the Walecka …

We calculate the neutral pion mass in the presence of an external magnetic field of arbitrary
strength in the framework of the linear sigma model coupled to quarks at zero temperature …