Video URL
https://pirsa.org/21050025A nuclear physics - multi-messenger astronomy analysis of binary neutron star mergers - Tim Dietrich
APA
Dietrich, T. (2021). A nuclear physics - multi-messenger astronomy analysis of binary neutron star mergers - Tim Dietrich. Perimeter Institute for Theoretical Physics. https://pirsa.org/21050025
MLA
Dietrich, Tim. A nuclear physics - multi-messenger astronomy analysis of binary neutron star mergers - Tim Dietrich. Perimeter Institute for Theoretical Physics, May. 27, 2021, https://pirsa.org/21050025
BibTex
@misc{ scivideos_PIRSA:21050025, doi = {10.48660/21050025}, url = {https://pirsa.org/21050025}, author = {Dietrich, Tim}, keywords = {Strong Gravity}, language = {en}, title = {A nuclear physics - multi-messenger astronomy analysis of binary neutron star mergers - Tim Dietrich}, publisher = {Perimeter Institute for Theoretical Physics}, year = {2021}, month = {may}, note = {PIRSA:21050025 see, \url{https://scivideos.org/index.php/pirsa/21050025}} }
Tim Dietrich Max Planck Institute for Gravitational Physics (Albert Einstein Institute)
Abstract
We discuss how we can use numerical-relativity simulations to derive gravitational-wave and electromagnetic models describing the binary neutron star coalescence. We show how these models can be used within a multi-messenger framework to derive new constraints on the neutron-star equation of state and the Hubble constant. For this purpose, we analyze the gravitational wave signal GW170817 and its electromagnetic counterparts AT2017gfo and GRB170817A, together with X-ray observations by NICER, radio observations of massive pulsars, and nuclear theory computations. Similarly, we also discuss that a non-detection of a kilonova for the second binary neutron-star merger detection GW190425 placed constraints on the properties of the system.
Zoom Link: https://pitp.zoom.us/j/99911822549?pwd=NXNNMWJVOUhMTGJSSGYwWUN2NEcxQT09