activity
20172021
most citedStellar equilibrium configurations of white dwarfs in the gravity

125 citations · 144 across the 3 of their papers we have counts for

collaborators

8 papers

gr-qc2021

Neutron stars in gravity with conserved energy-momentum tensor: Hydrostatic equilibrium and asteroseismology

Juan M. Z. Pretel, Sergio E. Jorás, Ribamar R. R. Reis +1

We investigate the equilibrium and radial stability of spherically symmetric relativistic stars, considering a polytropic equation of state (EoS), within the framework of

gr-qc2020

Fluid pulsation modes from strange stars in a higher-dimensional space-time

José D. V. Arbañil, César H. Lenzi, Manuel Malheiro

In this work, we make the first step to derive non-radial pulsation equations in extra dimensions and investigate how the - and -mode frequencies of strange quark stars, wi…

gr-qc2020

Stable relativistic polytropic objects with cosmological constant

José D. V. Arbañil, Pedro H. R. S. Moraes

The effects of the cosmological constant on the static equilibrium configurations and stability against small radial perturbations of relativistic polytropic spheres are investigat…

gr-qc20197 cited

Gravastar model in Randall-Sundrum braneworld

José D V Arbañil, Pedro H R S Moraes, Manuel Malheiro

In this work we derive a gravastar model in Randall-Sundrum II braneworld scenario. Gravastars (or gravitationally vacuum stars) were proposed by Mazur and Mottola as systems of gr…

gr-qc201912 cited

Extra dimensions' influence on the equilibrium and radial stability of strange quark stars

José D. V. Arbañil, Geanderson A. Carvalho, Ronaldo V. Lobato +2

We analyze the influence of extra dimensions on the static equilibrium configurations and stability against radial perturbations. For this purpose, we solve stellar structure equat…

gr-qc2018

Compact Astrophysical Objects in gravity

P. H. R. S. Moraes, J. D. V. Arbañil, G. A. Carvalho +4

In this article we study the hydrostatic equilibrium configuration of neutron stars (NSs) and strange stars (SSs), whose fluid pressure is computed from the equations of state $p=ω…