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Probing the equation of state of dense matter: neutron-star properties and multi-messenger constraints

Mar. 13 - 14:30 - 2025

Speaker: Anthea Fantina (Grand Accélérateur National d’Ions Lourds)

Title : Probing the equation of state of dense matter: neutron-star properties and multi-messenger constraints

Abstract: Neutron stars are unique laboratories to probe matter in extreme conditions that cannot be currently reproduced on Earth. The determination of their equation of state (EoS) is a challenge, but it is particularly important since it allows to relate different global neutron-star properties and to link the prediction of astrophysical observables to microphysical properties of dense matter. In this presentation, I will give a brief introduction on the dense-matter EoS, and specifically on the EoS for neutron stars. Various constraints will be discussed and the prediction of neutron-star observables obtained with a large variety of EoSs by performing Bayesian analyses will be presented in connection with recent (multi-messenger) astrophysical observations.

 

Room: Sala de Reuniões e Seminários (2-8.3, 2nd Floor of Physics Building)

 

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