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R. O. Gomes

Researcher at Frankfurt Institute for Advanced Studies

Publications -  45
Citations -  617

R. O. Gomes is an academic researcher from Frankfurt Institute for Advanced Studies. The author has contributed to research in topics: Neutron star & Stars. The author has an hindex of 13, co-authored 44 publications receiving 422 citations. Previous affiliations of R. O. Gomes include Universidade Federal do Rio Grande do Sul & Goethe University Frankfurt.

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GW190814 as a massive rapidly rotating neutron star with exotic degrees of freedom

Veronica Dexheimer, +5 more
- 22 Feb 2021 - 
TL;DR: In this article, the authors investigate the possibility of producing massive neutron stars from a few different equation of state models that contain exotic degrees of freedom, such as hyperons and quarks.
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What do we learn about vector interactions from GW170817

Veronica Dexheimer, +3 more
- 01 Mar 2019 - 
TL;DR: In this article, the role played by vector-isovector meson interaction in dense matter present in the interior of neutron stars in the light of new measurements made during the double neutron-star merger GW170817.
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Constraining Strangeness in Dense Matter with GW170817

R. O. Gomes, +3 more
- 04 Jun 2019 - 
TL;DR: In this paper, the authors show how the modeling of strangeness content in dense matter affects the properties of isolated neutrons stars and the tidal deformation in binary systems and show that hybrid stars can only exist if a phase transition takes place at low densities close to saturation.
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Many-body Forces in the Equation of State of Hyperonic Matter

R. O. Gomes, +4 more
- 14 Jul 2015 - 
TL;DR: In this article, an extended version of the formalism proposed originally by Taurines et al. was introduced, which considers the effects of many-body forces simulated by nonlinear self-couplings and meson-meson interaction contributions.
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What is the magnetic field distribution for the equation of state of magnetized neutron stars

Veronica Dexheimer, +5 more
- 10 Oct 2017 - 
TL;DR: In this paper, the authors report a realistic calculation of the magnetic field profile for the equation of state inside strongly magnetized neutron stars, and they find that magnetic fields increase relatively slowly with increasing baryon chemical potential (or baryons density) of magnetized matter.