Atom interferometric gravitational wave detection using heterodyne laser links

J. M. Hogan, D. M. S. Johnson, S. Dickerson, T. Kovachy, A. Sugarbaker, S.-w. Chiow, P. W. Graham, M. A. Kasevich, B. Saif, S. Rajendran, P. Bouyer, B. D. Seery, L. Feinberg, and R. Keski-Kuha, General Relativity and Gravitation 43

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The properties of the atomic proof-masses are regular (all atoms are identical) and knowable (well defined magnetic susceptibility). They are immune from charging events

Cited in the paper.

Concurrent interferometers can be implemented using different initial velocities so that each interferometer is addressable with a unique Doppler shift. Strategies for efficient allocation of Doppler bandwidth for LMT interferometers are discussed in [ 19 ]

Cited in the paper.

The description here is of a transition from the ground to excited state. For transitions from excited to ground, the signs of all the phase shifts are flipped

Cited in the paper.

Assumes a conventional π / 2 − π − π / 2 \pi/2-\pi-\pi/2 N ​ ℏ ​ k N\hbar k LMT sequence and a perturbation frequency ω = π / T \omega=\pi/T equal to the peak GW response frequency

Cited in the paper.

See, for example, [ 20 ]

Cited in the paper.

See Eq. 6 of Ref. [ 2 ] . Here we neglect averaging over the cloud. Averaging would further relax requirements at short wavelengths

Cited in the paper.

See, for example, the analysis in Refs. [ 2 , 4 ]

Cited in the paper.

J.M. Hogan, (to be published)

Cited in the paper.

P. W. Graham, J. M. Hogan, M. A. Kasevich, and S. Rajendran, Physical Review Letters 110

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2014

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T. Kovachy, J. M. Hogan, A. Sugarbaker, S. M. Dickerson, C. A. Donnelly, C. Overstreet, and M. A. Kasevich, (2014) , arXiv:1407.6995

Original

2014

Later among the works it cites.