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20162026
most citedTwo-solar-mass hybrid stars: a two model description with the Nambu-Jona-Lasinio quark model

56 citations · 213 across the 15 of their papers we have counts for

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6 papers · 1 filter

nucl-th2022

Hybrid stars with large strange quark cores

Márcio Ferreira, Renan Câmara Pereira, Constança Providência

The possible existence of hybrid stars is studied using several multi-quark interaction channels. The hadronic phase consists of an equation of state (EoS) with presently accepted…

nucl-th2021★ 2 cited

Hybrid stars from a constrained equation of state

Márcio Ferreira, Renan Câmara Pereira, Constança Providência

We determine, within a meta-model, the properties of the nuclear matter equation of state (EoS) that allow for a phase transition to deconfinement matter. It is shown that the prop…

nucl-th2021★ 18 cited

Hybrid stars with large strange quark cores constrained by GW170817

Márcio Ferreira, Renan Câmara Pereira, Constança Providência

We analyze the impact of several multi-quark interaction channels on the properties of hybrid stars. Four and eight vector interactions were included in the NJL model to de…

nucl-th2020★ 34 cited

Quark matter in light neutron stars

Márcio Ferreira, Renan Câmara Pereira, Constança Providência

Higher-order repulsive interactions are included in the three-flavor NJL model in order to describe the quark phase of an hybrid star. The effect of 4-quark and 8-quark vector-isos…

nucl-th2020★ 44 cited

Neutron stars with large quark cores

Márcio Ferreira, Renan Câmara Pereira, Constança Providência

We describe charge-neutral neutron star matter in equilibrium using hybrid equations of state, where a first-order phase transition from hadronic to quark matter is realized. T…

nucl-th2016★ 56 cited

Two-solar-mass hybrid stars: a two model description with the Nambu-Jona-Lasinio quark model

Renan Câmara Pereira, Pedro Costa, Constança Providência

Hybrid stars with a quark phase described by the NambuJona-Lasinio model are studied. The hadron-quark model used to determine the stellar matter equation of state favors the ap…