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Light and GW Emission from the First Detected BNS Merger

Light and GW Emission from the First Detected BNS Merger

Discussion on GW170817 at the Compact Objects Group Meeting, CCA Flatiron Institute

Matteo Cantiello

October 20, 2017
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  1. Light and GW Emission from the First Detected BNS Merger

    Artist depict of a massive binary system (NASA). Overlaid: MESA evolutionary tracks LIGO Scientific Collaboration and Virgo Collaboration (LVC), PRL 2017 LVC+FERMI+… ApJL 2017 (MultiMessengerPaper)
  2. Artist depict of a massive binary system (NASA). Overlaid: MESA

    evolutionary tracks LIGO Scientific Collaboration and Virgo Collaboration (LVC), PRL 2017 Instrumental glitch in the Livingston detector data. Similar glitches are registered roughly once every few hours in each of the LIGO detectors with no temporal correlation between the LIGO sites. Their cause remains unknown.
  3. Artist depict of a massive binary system (NASA). Overlaid: MESA

    evolutionary tracks LIGO Scientific Collaboration and Virgo Collaboration (LVC), PRL 2017 Frequency evolution Chirp mass Strain Amplitude
  4. Announcement on 16 October 2017. Madness! Artist depict of a

    massive binary system (NASA). Overlaid: MESA evolutionary tracks 1 PRL, 7 Nature papers, 9 Science, 40 ApJ/ApJL, 5 MNRAS and many more
  5. GW170817, EM170817 Artist depict of a massive binary system (NASA).

    Overlaid: MESA evolutionary tracks LIGO Scientific Collaboration and Virgo Collaboration (LVC), PRL 2017 LVC+FERMI+… ApJL 2017 (MultiMessengerPaper)