activity
20132026
most citedStellar equilibrium configurations of compact stars in gravity

307 citations · 1k across the 27 of their papers we have counts for

collaborators

30 papers

astro-ph.SR2026

Tidal Properties of White Dwarfs Admixed with Fermionic Dark Matter

G. A. Carvalho, J. D. V. Arbañil, I. A. Lacerda +1

This study investigates the impact of fermionic dark matter (DM) on the structural and tidal properties of white dwarfs (WDs). Using a two-fluid general relativistic framework, we…

astro-ph.SR2026

Rotating strange dwarfs and their indistinguishability from white dwarfs

Edson Otoniel, José D. V. Arbañil, Geanderson A. Carvalho +1

We investigate the structure of strange dwarfs, modeled as hybrid compact stars composed of a self bound strange quark matter core surrounded by a white dwarf like crust, within a…

astro-ph.SR2025★ 2 cited

Dark Matter in White Dwarfs: Implications for Their Structure

Sílvia P. Nunes, José D. V. Arbañil, Juan M. Z. Pretel +1

White Dwarfs (WDs), the final evolutionary stage of most stars, are frequently modeled considering only a dense plasma matter. However, their potential interaction with dark matter…

gr-qc2025

Examining the influence of anisotropy on the fundamental mode of nonradial oscillation in neutron stars on a complete general relativistic scheme

José D. V. Arbañil, Gabriel O. Cavalheiro, Victor B. T. Alves +3

The anisotropic influence on the -mode frequency of oscillations and dimensionless tidal deformability of neutron stars is analyzed by employing the nonradial oscillation equati…

astro-ph.HE2025★ 1 cited

Effects of light-mass fermionic dark matter on the equilibrium and stability of white dwarfs

G. A. Carvalho, J. D. V. Arbañil, J. G. Coelho

White dwarfs (WDs) can be used as laboratories to test strong gravity and high-density regimes, once their equation of state is not so uncertain as the one of neutron stars. This m…

astro-ph.SR2025★ 3 cited

Exploring Temperature Influences on Gravitational Wave Production in Binary White Dwarfs

Sílvia P. Nunes, José D. V. Arbañil, César H. Lenzi +1

This study investigates the conditions under which gravitational waves (GWs) are emitted during the merger of hot white dwarfs (WDs) in a binary system. Traditionally, these system…

gr-qc2024★ 5 cited

Dark energy effects on realistic neutron stars

Juan M. Z. Pretel, Sergio B. Duarte, José D. V. Arbañil +2

By considering realistic equations of state (EoSs) to describe the ordinary matter of the stellar crust, in this study, we explore the effect of a dark energy core, made of Chaplyg…

astro-ph.SR2024

Gravitational wave seismology of charged strange stars in the Cowling approximation: the fluid pulsation modes

José D. V. Arbañil, César H. Lenzi, Juan M. Z. Pretel +1

In this work we study, within the framework of Cowling approximation, the effect of the electric charge on the gravitational wave frequency of fluid oscillation modes of strange qu…

hep-ph2024

Gravitational wave asteroseismology of dark matter hadronic stars

C. V. Flores, C. H. Lenzi, M. Dutra +2

The influence of the dark matter mass~() and the Fermi momentum~($k_{F}^{\dm}$) on the -mode oscillation frequency, damping time parameter, and tidal deformability of had…

gr-qc2023★ 1 cited

Compact stars in scalar-tensor theories with a single-well potential and the corresponding theory

Juan M. Z. Pretel, Sergio E. Jorás, Ribamar R. R. Reis +2

The macroscopic properties of compact stars in modified gravity theories can be significantly different from the general relativistic (GR) predictions. Within the gravitational con…

astro-ph.HE2023★ 17 cited

Fluid pulsation modes and tidal deformability of anisotropic strange stars in light of the GW event

José D. V. Arbañil, Cesar V. Flores, César H. Lenzi +1

The effects of the anisotropy on the fluid pulsation modes adopting the so-called Cowling approximation and tidal deformability of strange quark stars are investigated by using the…

astro-ph.HE2023★ 5 cited

Phase transition and stiffer core fluid in neutron stars: Effects on stellar configurations, dynamical stability, and tidal deformability

José D. V. Arbañil, Lucas S. Rodrigues, César H. Lenzi

In this work, we investigate the influence of the phase transition and a stiffer fluid in neutron stars' cores on the static equilibrium configuration, dynamical stability, and tid…

gr-qc2022★ 21 cited

Charged quark stars in metric gravity

Juan M. Z. Pretel, José D. V. Arbañil, Sergio B. Duarte +2

We provide the modified TOV equations for the hydrostatic equilibrium of charged compact stars within the metric gravitational background. We adopt the MIT bag model EoS for…

gr-qc2021★ 18 cited

Tidal deformability and radial oscillations of anisotropic polytropic spheres

José D. V. Arbañil, Grigoris Panotopoulos

We compute the equilibrium, the fundamental eigenfrequency of oscillations modes, and quadrupolar tidal deformability of anisotropic polytropic spheres. These studies are respectiv…

astro-ph.SR2021★ 20 cited

The structure and stability of massive hot white dwarfs

Sílvia P. Nunes, José D. V. Arbañil, Manuel Malheiro

We investigate the structure and stability against radial oscillations, pycnonuclear reactions, and inverse -decay of hot white dwarfs. We regard that the fluid matter is made u…

gr-qc2021★ 54 cited

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★ 7 cited

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-qc2019★ 7 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-qc2019★ 12 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★ 3 cited

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…

astro-ph.SR2018★ 20 cited

White dwarfs with a surface electrical charge distribution: Equilibrium and stability

G. A. Carvalho, José D. V. Arbañil, R. M. Marinho +1

The equilibrium configuration and the radial stability of white dwarfs composed of charged perfect fluid are investigated. These cases are analyzed through the results obtained fro…

gr-qc2017★ 22 cited

Relativistic polytropic spheres with electric charge: Compact stars, compactness and mass bounds, and quasiblack hole configurations

José D. V. Arbañil, Vilson T. Zanchin

We study the static stellar equilibrium configurations ofuncharged and charged spheres composed by a relativistic polytropic fluid, and compare with those of spheres composed by a…

gr-qc2017★ 125 cited

Stellar equilibrium configurations of white dwarfs in the gravity

G. A. Carvalho, R. V. Lobato, P. H. R. S. Moraes +4

In this work we investigate the equilibrium configurations of white dwarfs in a modified gravity theory, na\-mely, gravity, for which and stand for the Ricci scala…