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Entropy, complexity and disequilibrium in compact stars
(ELSEVIER SCIENCE BVAMSTERDAM, 2012)
We used the statistical measurements of information entropy, disequilibrium and complexity to infer a hierarchy of equations of state for two types of compact stars from the broad class of neutron stars, namely, with ...
Delta baryons and diquark formation in the cores of neutron stars
(American Physical Society, 2020-09-09)
We investigate the hadron-quark phase transition in cold neutron stars in light of (i) the observed limits on the maximum-mass of heavy pulsars, (ii) constraints on the tidal properties inferred from the gravitational waves ...
Pion mass effects on axion emission from neutron stars through NN bremsstrahlung processes
(ELSEVIER SCIENCE BV, 2009)
The rates of axion emission by nucleon-nucleon bremsstrahlung are calculated with the inclusion of the full momentum contribution from a nuclear one pion exchange (OPE) potential. The contributions of the neutron-neutron ...
Uma introdução ao modelo da hadrodinâmica quântica para estudo das estrelas de nêutronsAn introduction to the quantum hadrodynamics model for study of neutron stars
(Universidade Federal do Rio Grande do NorteBrasilUFRNFísica Bacharelado, 2021)
On the mass distribution of neutron stars
(WILEY-BLACKWELL, 2011)
The distribution of masses for neutron stars is analysed using the Bayesian statistical inference, evaluating the likelihood of the proposed Gaussian peaks by using 54 measured points obtained in a variety of systems. The ...
Neutron stars in Scalar-Tensor-Vector Gravity
(Springer, 2017-02)
Scalar-Tensor-Vector Gravity (STVG), also referred as Modified Gravity (MOG), is an alternative theory of the gravitational interaction. Its weak field approximation has been successfully used to describe Solar System ...