CORDIS Project
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This project focuses on simulating kilonovae resulting from binary neutron star mergers to better understand the physics of these events. By developing detailed models, it aims to link simulations with observations, enhancing knowledge of nucleosynthesis and the behavior of dense nuclear matter.
The merging of binary neutron stars produces an explosive kilonova transient, recently confirmed by the first ever detection of a kilonova, AT2017gfo, coincident with a gravitational wave signal, GW170817.
The wealth of observations provided by AT2017gfo offers the opportunity to probe the fundamental physics of binary neutron star mergers, including the incompletely known Equation of State of dense nuclear matter and rapid neutron capture nucleosynthesis (the r-process), which produces half of…
THE PROVOST, FELLOWS, FOUNDATION SCHOLARS & THE OTHER MEMBERS OF BOARD, OF THE COLLEGE OF THE HOLY & UNDIVIDED TRINITY OF QUEEN ELIZABETH NEAR DUBLIN
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