



02029nas a2200205   4500008004100000245009100041210006900132490000900201520141200210100001901622700002001641700001801661700001701679700002001696700002001716700001601736700001701752700001701769856003701786       2018                        eng d00aA spinor Bose-Einstein condensate phase-sensitive amplifier for SU(1,1) interferometry0 aspinor BoseEinstein condensate phasesensitive amplifier for SU110 vA 983 a<p>The SU(1,1) interferometer was originally conceived as a Mach-Zehnder interferometer with the beam-splitters replaced by parametric amplifiers. The parametric amplifiers produce states with correlations that result in enhanced phase sensitivity. F=1 spinor Bose-Einstein condensates (BECs) can serve as the parametric amplifiers for an atomic version of such an interferometer by collisionally producing entangled pairs of &lang;F=1,m=&plusmn;1| atoms. We simulate the effect of single and double-sided seeding of the inputs to the amplifier using the truncated-Wigner approximation. We find that single-sided seeding degrades the performance of the interferometer exactly at the phase the unseeded interferometer should operate the best. Double-sided seeding results in a phase-sensitive amplifier, where the maximal sensitivity is a function of the phase relationship between the input states of the amplifier. In both single and double-sided seeding we find there exists an optimal phase shift that achieves sensitivity beyond the standard quantum limit. Experimentally, we demonstrate a spinor phase-sensitive amplifier using a BEC of 23Na in an optical dipole trap. This configuration could be used as an input to such an interferometer. We are able to control the initial phase of the double-seeded amplifier, and demonstrate sensitivity to initial population fractions as small as 0.1\%.&nbsp;</p>1 aWrubel, J., P.1 aSchwettmann, A.1 aFahey, D., P.1 aGlassman, Z.1 aPechkis, H., K.1 aGriffin, P., F.1 aBarnett, R.1 aTiesinga, E.1 aLett, P., D.  uhttps://arxiv.org/abs/1807.06676