This is a preview of subscription content, log in via an institution to check access.
Access this chapter
Tax calculation will be finalised at checkout
Purchases are for personal use only
Notes
- 1.
This is a very relaxed constraint, as in reality the radius \(w_0\) of the beam should be larger than the radius of the atomic ensemble \(\sigma _t\) to yield a more uniform intensity profile across the cloud. For a ratio \(w_0/\sigma _t = a\), the temperature limit scales with \(1/a^2\).
References
Brown DD, Freise A (2014) Finesse. http://www.gwoptics.org/finesse
Dovale Álvarez M, Brown DD, Jones AW, Mow-Lowry CM, Miao H, Freise A (2017) Fundamental limitations of cavity-assisted atom interferometry. Phys Rev A 96:053820
Riou I, Mielec N, Lefèvre G, Prevedelli M, Landragin A, Bouyer P, Bertoldi A, Geiger R, Canuel B (2017) A marginally stable optical resonator for enhanced atom interferometry. J Phys B 50:155002
Abitan H, Skettrup T (2004) Laser resonators with several mirrors and lenses with the bow-tie laser resonator with compensation for astigmatism and thermal lens effects as an example. J Opt A Pure Appl Opt 7:7–20
Habraken SJM, Nienhuis G (2007) Modes of a twisted optical cavity. Phys Rev A 75:033819
Author information
Authors and Affiliations
Corresponding author
Rights and permissions
Copyright information
© 2019 Springer Nature Switzerland AG
About this chapter
Cite this chapter
Álvarez, M.D. (2019). 4-Mirror Large-Waist Cavity with Tuneable Stability for Enhanced Atom Interferometry. In: Optical Cavities for Optical Atomic Clocks, Atom Interferometry and Gravitational-Wave Detection. Springer Theses. Springer, Cham. https://doi.org/10.1007/978-3-030-20863-9_8
Download citation
DOI: https://doi.org/10.1007/978-3-030-20863-9_8
Published:
Publisher Name: Springer, Cham
Print ISBN: 978-3-030-20862-2
Online ISBN: 978-3-030-20863-9
eBook Packages: Physics and AstronomyPhysics and Astronomy (R0)