On the possibility of rho-meson condensation in neutron stars
@article{Mallick2015OnTP, title={On the possibility of rho-meson condensation in neutron stars}, author={Ritam Mallick and Stefan Schramm and Veronica Dexheimer and Abhijit Bhattacharyya}, journal={Monthly Notices of the Royal Astronomical Society}, year={2015}, volume={449}, pages={1347-1351} }
The possibility of meson condensation in stars and in heavy-ion collisions has been discussed in the past. Here, we study whether rho meson condensation ($\rho^{-}$) can occur in very dense matter and determine the effect of strong magnetic fields on this condensation. We find that rho meson condensates can appear in the core of the neutron star assuming a rho mass which is reduced due to in-medium effects. We find that the magnetic field has a non-negligible effect in triggering condensation.
8 Citations
Neutron Stars—Possibilities and Limits for Exotic Phases
- Physics
- 2017
Neutron star physics has become one of the central topics of nuclear astrophysics. The extremely high densities in the core region of neutron stars potentially allow for exotic particles and phases…
On Manifestation of In-Medium Effects in Neutron Stars and Heavy-Ion Collisions
- Physics
- 2018
This review focuses on the demonstration of an interrelation between various in-medium effects, which are manifested in the phenomena occurring in neutron stars and heavy-ion collisions. More…
Possibility of $ \rho$ρ meson condensation in neutron stars: Unified approach of chiral SU(3) model and QCD sum rules
- Physics
- 2019
Abstract.In the present work the conjunction of chiral SU(3) model with QCD sum rules is employed to explore the possibility of $ \rho$ρ meson condensation in neutron stars. The quark and gluon…
Hyperons in Neutron Stars
- PhysicsUniverse
- 2021
I review the issues related to the appearance of hyperons in neutron star matter, focusing in particular on the problem of the maximum mass supported by hyperonic equations of state. I discuss the…
Exploring effects of magnetic field on the Hadron Resonance Gas
- Physics
- 2015
We present a study of the effects of magnetic fields on fluctuations and correlations in hadron resonance gas model. We find significant changes in the fluctuations of net baryon number, electric…
N ov 2 01 9 Vector-boson condensates , spin-triplet superfluidity of paired neutral and charged fermions , and 3 P 2 pairing of nucleons
- Physics
- 2019
After reminding of properties of the condensate of the complex scalar field in the external uniform magnetic field H focus is made on the study of phases of the complex neutral vector boson fields…
Vector-boson condensates, spin-triplet superfluidity of paired neutral and charged fermions, and
3P2
pairing of nucleons
- Physics
- 2019
After reminding of properties of the condensate of the complex scalar field in the external uniform magnetic field $H$ focus is made on the study of phases of the complex neutral vector boson fields…
References
SHOWING 1-10 OF 49 REFERENCES
Medium modifications to the omega -meson mass in the Walecka model.
- PhysicsPhysical review. C, Nuclear physics
- 1994
This work calculates the effective mass of the [omega] meson in nuclear matter in a relativistic random-phase approximation to the Walecka model and reports a reduction in the meson mass of about 170 MeV at nuclear-matter saturation density.
Hybrid stars in a strong magnetic field
- Physics
- 2012
We study the effects of high magnetic fields on the particle population and equation of state of hybrid stars using an extended hadronic and quark SU(3) non-linear realization of the sigma model. In…
Magnetic moment of the rho-meson in QCD sum rules: alpha s -corrections
- Physics
- 2003
The magnetic moment of the rho-meson is calculated in the framework of QCD sum rules in external fields. Perturbative corrections are taken into account. Bare loop calculations (parton model) give…
Kaon properties in (proto-)neutron star matter
- Physics
- 2009
Abstract.The modification of kaon and antikaon properties in the interior of (proto-)neutron stars is investigated using a chiral SU(3) model. The parameters of the model are fitted to nuclear-matter…