Reply to comment on "Equation of state of dense and magnetized fermion system"
arXiv:1110.0420 · doi:10.1103/PhysRevC.85.039802
Abstract
A Comment [1] to our recent article [2], expressed criticism on our estimate of the maximum magnetic field that can exist inside a neutron star and on the pressure anisotropy we found for a magnetized gas of fermions. These two points are relevant for the physics of neutron stars. With our reply we attempt not only to address the Comment's criticisms, but for the sake of the reader's understanding, we also try to clarify the connection between our and some literature's results mentioned in the comment.
References in corpus (3)
Cited by in corpus (9)
- The influence of strong magnetic fields on proto-quark stars
- Stability of super-Chandrasekhar magnetic white dwarfs
- Thermodynamics of Neutrons in a Magnetic Field and its Implications for Neutron Stars
- Magnetic fields in anisotropic relativistic stars
- Thermodynamic Behaviour of Magnetized QGP within the Self-Consistent Quasiparticle Model
- Anisotropic pressure of magnetized quark matter with anomalous magnetic moment
- Thermomagnetic properties and Debye Screening for magnetized quark-gluon Plasma using the extended self-consistent quasiparticle model
- On the role of the Vacuum Energy in the Thermodynamics of Neutron Matter
- The spin-polarized ferromagnetic state of a cold Fermi gas