Speaker
Prof.
Luca Baiotti
(The University of Osaka)
Description
After an overview of the current status of astrophysical observations and numerical simulations of binary neutron star mergers, I will present our ideas on how to possibly discriminate equations of state (EOSs) with a quark-hadron crossover with respect to EOSs with purely hadronic matter or with a first-order quark-hadron transition through gravitational waves emitted in binary neutron star mergers.
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Author
Prof.
Luca Baiotti
(The University of Osaka)