activity
20102026
most citedA light strange star in the remnant HESS J1731-347: minimal consistency checks

68 citations · 176 across the 13 of their papers we have counts for

collaborators

15 papers

astro-ph.HE2026

The Galactic Black Hole mass distribution

L S. Rocha, N. Pires, L. M. de Sá +8

The population of extragalactic black holes has been significantly expanded and better understood since the first detection of gravitational waves. Over the past decade, approximat…

astro-ph.HE2026

The mass of the neutron star in 4U 1820-30 revisited

Marcio G B de Avellar, Jorge E Horvath, Nathalia D Pires +7

We revisit the mass of the neutron star in the ultracompact binary 4U 1820--30 in light of a recently reported transient absorption feature at about 3.8 keV, interpreted as a gravi…

astro-ph.HE2024

Evolution of long-period compact radio sources driven by winds

J. E. Horvath, Lucas M. de Sá, Lívia S. Rocha +3

We address in this work the nature and evolution of the long-period compact star sources, which has recently added several unexpected members. The central hypothesis is that partic…

astro-ph.HE2023★ 15 cited

Mass Distribution and Maximum Mass of Neutron Stars: Effects of Orbital Inclination Angle

Lívia S. Rocha, Jorge E. Horvath, Lucas M. de Sá +3

Matter at ultra-high densities finds a physical realization inside neutron stars. One key property is their maximum mass, which has far-reaching implications for astrophysics and t…

cs.DC2023

A visão da BBChain sobre o contexto tecnológico subjacente à adoção do Real Digital

Marcio G B de Avellar, Alexandre A S Junior, André H G Lopes +3

We explore confidential computing in the context of CBDCs using Microsoft's CCF framework as an example. By developing an experiment and comparing different approaches and performa…

astro-ph.HE2023★ 68 cited

A light strange star in the remnant HESS J1731-347: minimal consistency checks

J. E. Horvath, L. S. Rocha, L. M. de Sá +5

Context: Recently, Doroshenko and collaborators reported a very low-mass compact star, a Central Compact Object named XMMU J173203.3-344518 inside the supernova remnant HESS J1731-…

astro-ph.HE2021

Sudden discharge of young charged magnetars as a new model for FRBs

Marcio G. B. de Avellar, Pedro P. B. Beaklini, Sílvia P. Nunes +2

We propose a new model for Fast Radio Bursts (FRBs) based on a sudden discharge of a charged young magnetar, caused by the short falling timescale of oppositely charged particles o…

astro-ph.HE2021★ 5 cited

Fast Radio Bursts as crustal dynamical events induced by magnetic field evolution in young magnetars

J. E. Horvath, P. H. R. S. Moraes, M. G. B. de Avellar +1

We revisit in this work a model for repeating Fast Radio Bursts based of the release of energy provoked by the magnetic field dynamics affecting a magnetar's crust. We address the…

astro-ph.HE2016★ 13 cited

Phase lags of quasi-periodic oscillations across source states in the low-mass X-ray binary 4U 1636-53

Marcio G B de Avellar, Mariano Méndez, Diego Altamirano +2

While there are many dynamical mechanisms and models that try to explain the origin and phenomenology of the quasi-periodic oscillations (QPOs) seen in the X-ray light curves of lo…

astro-ph.SR2015

Trends of Stellar Entropy along Stellar Evolution

Marcio G. B. de Avellar, Rodrigo A. de Souza, Jorge E. Horvath

This paper is devoted to discuss the difference in the thermodynamic entropy budget {\it per baryon} in each type of stellar object found in Universe. We track and discuss the actu…

astro-ph.SR2013★ 3 cited

Statistical measure of complexity in compact stars with global charge neutrality

Rodrigo Alvares de Souza, Marcio Guilherme Bronzato de Avellar, Jorge Ernesto Horvath

Recently, it has been suggested that a critical electrical field arises during the gravitational collapse of massive stars leading to a vacuum polarization. This, in turn, leads to…

astro-ph.SR2013★ 1 cited

Entropy, Disequilibrium and Complexity in Compact Stars: An information theory approach to understand their Composition

Marcio G B de Avellar, Jorge E Horvath

The composition of neutron stars is an issue that has been studied for decades. Yet we do not know exactly what these very compact objects are made of. At this stage of the technol…

astro-ph.HE2013★ 37 cited

Time lags of the kilohertz quasi-periodic oscillations in the low-mass X-ray binaries 4U 1608--52 and 4U 1636--53

M. G. B. de Avellar, M. Méndez, A. Sanna +1

(abridged) We studied the energy and frequency dependence of the Fourier time lags and intrinsic coherence of the kHz QPOs in the NS LMXBs 4U 1608-52 and 4U 1636-53 using RXTE data…

astro-ph.SR2011★ 24 cited

Self-bound models of compact stars and recent mass-radius measurements

M. G. B. de Avellar, J. E. Horvath, L. Paulucci

The exact composition of a specific class of compact stars, historically referred to as "neutron stars", is still quite unknown. Possibilities ranging from hadronic to quark degree…

astro-ph.HE2010★ 10 cited

Exact and Quasi-exact Models of Strange Stars

M. G. B. Avellar, J. E. Horvath

We construct and compare a variety of simple models for strange stars, namely, hypothetical self-bound objects made of a cold stable version of the quark-gluon plasma. Exact, quasi…