PIRSA:23040084

Video URL

https://pirsa.org/23040084

The spherical ejecta of AT2017gfo

Sneppen, A. (2023). The spherical ejecta of AT2017gfo. Perimeter Institute for Theoretical Physics. https://pirsa.org/23040084

Sneppen, Albert. The spherical ejecta of AT2017gfo. Perimeter Institute for Theoretical Physics, Apr. 06, 2023, https://pirsa.org/23040084 

          @misc{ scivideos_PIRSA:23040084,
            doi = {10.48660/23040084},
            url = {https://pirsa.org/23040084},
            author = {Sneppen, Albert},
            keywords = {Strong Gravity},
            language = {en},
            title = {The spherical ejecta of AT2017gfo},
            publisher = {Perimeter Institute for Theoretical Physics},
            year = {2023},
            month = {apr},
            note = {PIRSA:23040084 see, \url{https://scivideos.org/pirsa/23040084}}
          }

Albert Sneppen Niels Bohr Institute

Talk numberPIRSA:23040084
DOI10.48660/23040084
Source RepositoryPIRSA
Collection
Talk Type Scientific Series
Subject

Abstract

The geometry of kilonovae is a key diagnostic of the physics of merging neutron stars with current hydrodynamical merger models typically showing aspherical ejecta. Previously, Sr II was identified in the spectrum of the only well-studied kilonova AT2017gfo, associated with the gravitational wave event GW170817. In this talk, we show that combining the strong Sr II P Cygni absorption-emission spectral feature and the blackbody nature of the kilonova spectrum, to determine that the kilonova is highly spherical at early epochs. Line shape analysis combined with the known inclination angle of the source also shows the same sphericity independently. The near-spherical geometry suggests early spectra of kilonovae may provide excellent precision cosmic distance measurements using the Expanding Photosphere Method.

Zoom link:  https://pitp.zoom.us/j/97287055430?pwd=bFVyeTRuZHVLcGlDdnhlK1d0OWE1Zz09