Conveners
Plenary 9: Neutron Star Mergers
- Akif Baha Balantekin (University of Wisconsin-Madison)
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Dr Jocelyn Read (CSU Fullerton)02/06/2018, 14:00PNAPlenaryNeutron stars host the densest stable matter in the universe. Accurately modeling their multi-messenger astrophysics relies on a detailed description of the equation of state above nuclear density. Astronomical observations, including binary pulsar dynamics, x-ray bursts and timing, and gravitational-wave observations, can in turn be used to constrain the properties of this dense matter. On...Go to contribution page
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Dr Kenta Hotokezaka (Princeton University)02/06/2018, 14:35PNAPlenaryA neutron star merger, GW170817, was discovered by Advanced LIGO. The gravitational wave signal is followed by electromagnetic counterparts in multi-wavelength including GRB 170817A, kilonova, and non-thermal synchrotron afterglow. These emissions are produced by outflows launched in the merger. I will talk about the properties of different components of merger outflows and implications of...Go to contribution page
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Daniel Kasen (UC Berkeley/LBNL)02/06/2018, 15:10PNAPlenaryThe recent detection of gravitational waves and associated electromagnetic emission from a binary neutron star merger has illuminated the physics of strong gravity and dense matter, and addressed long standing questions as to the origin of the heaviest elements in the universe. I will review our physical understanding of compact object mergers — grounded in theoretical calculations and...Go to contribution page