Two-Photon Methods for Astrometric Gravitational Wave Detection

          @misc{ scivideos_PIRSA:24110041,
            doi = {10.48660/24110041},
            url = {https://pirsa.org/24110041},
            author = {Stankus, Paul},
            keywords = {Cosmology},
            language = {en},
            title = {Two-Photon Methods for Astrometric Gravitational Wave Detection},
            publisher = {Perimeter Institute for Theoretical Physics},
            year = {2024},
            month = {nov},
            note = {PIRSA:24110041 see, \url{https://scivideos.org/pirsa/24110041}}
          }
          

Abstract

With the observation of gravitational waves (GW's) at high, kilohertz frequencies by LIGO and the evidence for GW's at low, nanohertz frequencies from NANOGrav there is a new emphasis on exploring the GW landscape at intermediate frequency ranges. Beyond the two measurement methods used in these observations, i.e. laser metrology in LIGO and pulsar timing offsets in NANOGrav, we have been developing a third approach of observing astrometric GW signatures, which is very well suited to the intermediate microhertz frequency range. While astrometric GW observations have been discussed in the context of survey missions, e.g. GAIA, this presentation will exhibit a potentially superior approach using long baseline two-photon interferometry, with both space-based and ground-based platforms. The practicalities of a near-future experiment will be particularly highlighted