0000000000493905

AUTHOR

Fabio D. Lora-clavijo

showing 2 related works from this author

Anisotropic quark stars with an interacting quark equation of state

2019

A deep exploration of the parameter space that relates the interacting equation of state with the bag constant B, and the interaction parameter a, is fundamental for the construction of diverse models of quark stars. In particular, the anisotropy of quark stars with a well-motivated quantum chromodynamics (QCD) equation of state is presented here. The contribution of the fourth order corrections parameter ($\mathrm{a}$) of the QCD perturbation on the radial and tangential pressure generate significant effects on the mass-radius relation and the stability of the quark star. An adequate set of solutions for several values of the bag factor and the interaction parameter are used in order to ca…

Quantum chromodynamicsQuarkPhysicsParticle physicsEquation of stateHigh Energy Physics::LatticeHigh Energy Physics::PhenomenologyAnisotropicPerturbation (astronomy)FOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Parameter spaceWeak interactionGeneral Relativity and Quantum CosmologyCompact spaceQuark starQuark starsAnisotropic Quark stars Equation of stateHigh Energy Physics::ExperimentAnisotropy
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Magnetised tori with magnetic polarisation around Kerr black holes: variable angular momentum discs

2023

Analytical models of magnetised, geometrically thick discs are relevant to understand the physical conditions of plasma around compact objects and to explore its emitting properties. This has become increasingly important in recent years in the light of the Event Horizon Telescope observations of Sgr A* and M87. Models of thick discs around black holes usually consider constant angular momentum distributions and do not take into account the magnetic response of the fluid to applied magnetic fields. We present a generalisation of our previous work on stationary models of magnetised accretion discs with magnetic polarisation (Pimentel et al. 2018). This extension is achieved by accounting for…

High Energy Astrophysical Phenomena (astro-ph.HE)83C57 76W05 85A30 83C55FOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Astrophysics - High Energy Astrophysical PhenomenaGeneral Relativity and Quantum Cosmology
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