PIRSA:15020125

Optical frequency standards for gravitational wave detection

Vutha, A. (2015). Optical frequency standards for gravitational wave detection. Perimeter Institute. https://pirsa.org/15020125

Vutha, Amar. Optical frequency standards for gravitational wave detection. Perimeter Institute, Feb. 12, 2015, https://pirsa.org/15020125 

          @misc{ pirsa_PIRSA:15020125,
            doi = {10.48660/15020125},
            url = {https://pirsa.org/15020125},
            author = {Vutha, Amar},
            keywords = {Strong Gravity},
            language = {en},
            title = {Optical frequency standards for gravitational wave detection},
            publisher = {Perimeter Institute},
            year = {2015},
            month = {feb},
            note = {PIRSA:15020125 see, \url{https://pirsa.org}}
          }

Amar Vutha University of Toronto

DOI 10.48660/15020125
Collection
Talk Type Scientific Series
Subject

Abstract

Gravitational waves (GW) imprint apparent Doppler shifts on the frequency of photons propagating between an emitter and detector of light. This forms the basis of a method to detect mHz GW using Doppler velocimetry between pairs of satellites [1]. The crucial component in such GW detectors is the frequency standard on board the emitting and receiving satellites. I will discuss how recent developments in atomic clock technology have led to devices that could be sufficiently sensitive to probe astrophysically interesting sources. I will present a design for a robust, space-capable optical frequency standard [2], that is being developed at York.

References

[1] JW Armstrong, Living Rev. Relativity 9, (2006), 1 [2] AC Vutha, arXiv:1501.01733 (2015)