TY - JOUR
T1 - Realization of a gain with electromagnetically induced transparency system using non-degenerate Zeeman sublevels in 87Rb
AU - Zhou, Minchuan
AU - Zhou, Zifan
AU - Shahriar, Selim M.
N1 - Funding Information:
This work was supported by DARPA through the slow light program under Grant No. FA9550-07-C-0030 and by AFOSR under Grants No. FA9550-10-01-0228 and No. FA9550-09-01-682-0652.
Publisher Copyright:
© 2017 Elsevier B.V.
PY - 2017/11/1
Y1 - 2017/11/1
N2 - Previously, we had proposed an optically-pumped five-level Gain EIT (GEIT) system, which has a transparency dip superimposed on a gain profile and exhibits a negative dispersion suitable for the white-light-cavity signal-recycling (WLC-SR) scheme of the interferometric gravitational wave detector (Zhou et al., 2015). Using this system as the negative dispersion medium (NDM) in the WLC-SR, we get an enhancement in the quantum noise (QN) limited sensitivity-bandwidth product by a factor of ∼18. Here, we show how to realize this GEIT system in a realistic platform, using non-degenerate Zeeman sublevels in cold Rb atoms, employing anomalous dispersion at 795 nm. Using the Caves model for a phase insensitive linear amplifier, we show that an enhancement of the sensitivity-bandwidth product by a factor of ∼17 is possible for potentially realizable experimental parameters. While the current LIGO apparatus uses light at 1064 nm, a future embodiment thereof may operate at a wavelength that is consistent with the wavelength considered here.
AB - Previously, we had proposed an optically-pumped five-level Gain EIT (GEIT) system, which has a transparency dip superimposed on a gain profile and exhibits a negative dispersion suitable for the white-light-cavity signal-recycling (WLC-SR) scheme of the interferometric gravitational wave detector (Zhou et al., 2015). Using this system as the negative dispersion medium (NDM) in the WLC-SR, we get an enhancement in the quantum noise (QN) limited sensitivity-bandwidth product by a factor of ∼18. Here, we show how to realize this GEIT system in a realistic platform, using non-degenerate Zeeman sublevels in cold Rb atoms, employing anomalous dispersion at 795 nm. Using the Caves model for a phase insensitive linear amplifier, we show that an enhancement of the sensitivity-bandwidth product by a factor of ∼17 is possible for potentially realizable experimental parameters. While the current LIGO apparatus uses light at 1064 nm, a future embodiment thereof may operate at a wavelength that is consistent with the wavelength considered here.
KW - Gain with electromagnetically induced transparency
KW - Gravitational wave detection
KW - Negative dispersion
KW - Quantum noise
KW - Zeeman sublevels
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U2 - 10.1016/j.optcom.2017.06.036
DO - 10.1016/j.optcom.2017.06.036
M3 - Article
AN - SCOPUS:85021149346
SN - 0030-4018
VL - 402
SP - 382
EP - 388
JO - Optics Communications
JF - Optics Communications
ER -