PIRSA:21120008

The Multi-Messenger Milky Way

APA

Gossan, S. (2021). The Multi-Messenger Milky Way . Perimeter Institute. https://pirsa.org/21120008

MLA

Gossan, Sarah. The Multi-Messenger Milky Way . Perimeter Institute, Dec. 02, 2021, https://pirsa.org/21120008

BibTex

          @misc{ pirsa_21120008,
            doi = {10.48660/21120008},
            url = {https://pirsa.org/21120008},
            author = {Gossan, Sarah},
            keywords = {Strong Gravity},
            language = {en},
            title = {The Multi-Messenger Milky Way },
            publisher = {Perimeter Institute},
            year = {2021},
            month = {dec},
            note = {PIRSA:21120008 see, \url{https://pirsa.org}}
          }
          

Sarah Gossan Canadian Institute for Theoretical Astrophysics (CITA)

Collection
Talk Type Scientific Series
Subject

Abstract

The era of multi-messenger astronomy is well and truly upon us, with 90 compact binaries observed since the Advanced LIGO detectors saw first light in 2015. Despite our very own cosmic backyard, the Milky Way, being ripe with prospective sources for ground-based gravitational wave detectors, the closest source detected thus far (GW170817, the famed binary neutron star merger) was at a distance of 40 Mpc. In this talk, I will outline a number of prospective Galactic multi-messenger sources, and discuss several ways in which their detection over the next twenty years can be improved through both experimental and analytical techniques. 

Zoom Link: https://pitp.zoom.us/j/93664322641?pwd=VUoxbmFGZE1KczJ1RU1MR09TQ05Ldz09