Abstract:We study the hyperfine spectrum of atoms of 87 Rb dressed by a radio-frequency field, and present experimental results in three different situations: freely falling atoms, atoms trapped in an optical dipole trap and atoms in an adiabatic radio-frequency dressed shell trap. In all cases, we observe several resonant side bands spaced (in frequency) at intervals equal to the dressing frequency, corresponding to transitions enabled by the dressing field. We theoretically explain the main features of the microwave … Show more
“…To do this, we load the bi-chromatic shell trap for several pairs of ω 1 and ω 2 and then we fit Lorentzian curves to the number of atoms transferred to the upper state as we scan the microwave frequency ω MW /2π. By finding the combination of ω 1 and ω 2 that gives the minimum line-width, we can thus match the two traps (see figure 2(a)), at which point we observe a reduction in line-width by of the order of ×10 with respect to the mono-chromatic shell (measured elsewhere [29]).…”
Section: Microwave Spectroscopy Of the Bi-chromatic Rf-dressed Shell mentioning
confidence: 68%
“…The solution of this Hamiltonian for a weak MW-field that acts as a probe on the RF-dressed energy levels leads to inter-manifold transitions [28][29][30] on a spectrum of 7 groups (spaced by the RF-dressing frequency) of 5 transitions (spaced by the RF-dressing Rabi frequency), when the initial state is [29] for a detailed study). Concretely, the transition with n=0, k=0 is coincident with the hyperfine splitting [29]. In practice, this transition is shifted both by the nonlinear dependence of the eigenenergies on the magnetic field and on the difference in magnitude of g 1 and g 2 .…”
Section: Microwave Spectroscopy Of the Bi-chromatic Rf-dressed Shell mentioning
confidence: 99%
“…We explain these multi-photon transitions with a semi-classical two-level toy model in appendix C. An analysis on the complete microwave spectrum between rfdressed ultra-cold Rubidium 87 Zeeman sub-levels can be found in [29]. In this work, we focus only on the transition from -ñ 1, 1 | to ñ 2, 1 | .…”
Section: Microwave Spectroscopy Of the Bi-chromatic Rf-dressed Shell mentioning
Free space atom-interferometry traditionally suffers from the large distances that atoms have to fall in order to achieve long interaction times. Trapped atom interferometry is emerging as a powerful way of achieving long interaction times in a reduced experimental volume. Here, we demonstrate bi-chromatic adiabatic magnetic shell traps as a novel tool for matterwave interferometry. We dress the magnetic hyperfine states of the F=1 and F=2 Rubidium 87 Bose-Einstein Condensates thus creating two independently controllable shell traps of which we use the = =-ñ F m 1, 1Using microwave pulses, we put atoms originally loaded into one of the two shell-traps into a superposition between the two shell traps. Since the two traps can be manipulated independently, their position and vertical curvature can be matched, thus creating a good starting point for an atom interferometer. This interferometer can be sensitive to spatially varying electric or magnetic fields, which could be DC or RF magnetic fields or microwaves. We demonstrate that the trap-matching afforded by the independent control of the shell traps allows for a tenfold increase in coherence times when compared to adiabatic potentials created by a single RF-frequency. For large-radius shells the atoms are confined to a 2D surface enabling highly sensitive imaging matterwave interferometers.Atom interferometry is a rapidly maturing quantum technology both for fundamental experiments and for applications. It has been successfully used to measure the Newtonian constant [1], and to put atominterferometric constraints on dark energy [2]. Which path and delayed choice experiments have been carried out using atom interferometry [3,4]. Atom interferometry may be used to test forces on atoms from small source masses in tests for small forces [5] and in the search for Ultralight Scalar Field Dark Matter [6,7]. Simple tests of the weak equivalence principle have been performed using atom interferometry [8] and there are proposals for space based extreme accuracy tests at the 10 −15 level [9] with some projections reaching 10 −19 [7,10]. On the applied side, atom interferometers have been used in absolute gravimetry on a ship [11] and in space [12]. Most precision interferometers still operate in the free-fall-regime, where, e.g.in the case of acceleration, the precision scales with the square of the interaction time. As a consequence, the most precise interferometers tend to become very tall, in some cases reaching ten or even one hundred meters in height [13]. Even larger interaction times are only possible in zero gravity on parabolic flights or in space [14]. Large sensitivity typically requires long interaction times and thus a large free-fall distance, which in turn makes the apparatus rather large.There have been numerous attempts to miniaturize such systems, e.g.using shaken lattices [15], partially trapped atoms interferometry with Sr [16] and coherent accelerations performed by the Bloch oscillations technique [17]. Even though some progress has been achieved...
“…To do this, we load the bi-chromatic shell trap for several pairs of ω 1 and ω 2 and then we fit Lorentzian curves to the number of atoms transferred to the upper state as we scan the microwave frequency ω MW /2π. By finding the combination of ω 1 and ω 2 that gives the minimum line-width, we can thus match the two traps (see figure 2(a)), at which point we observe a reduction in line-width by of the order of ×10 with respect to the mono-chromatic shell (measured elsewhere [29]).…”
Section: Microwave Spectroscopy Of the Bi-chromatic Rf-dressed Shell mentioning
confidence: 68%
“…The solution of this Hamiltonian for a weak MW-field that acts as a probe on the RF-dressed energy levels leads to inter-manifold transitions [28][29][30] on a spectrum of 7 groups (spaced by the RF-dressing frequency) of 5 transitions (spaced by the RF-dressing Rabi frequency), when the initial state is [29] for a detailed study). Concretely, the transition with n=0, k=0 is coincident with the hyperfine splitting [29]. In practice, this transition is shifted both by the nonlinear dependence of the eigenenergies on the magnetic field and on the difference in magnitude of g 1 and g 2 .…”
Section: Microwave Spectroscopy Of the Bi-chromatic Rf-dressed Shell mentioning
confidence: 99%
“…We explain these multi-photon transitions with a semi-classical two-level toy model in appendix C. An analysis on the complete microwave spectrum between rfdressed ultra-cold Rubidium 87 Zeeman sub-levels can be found in [29]. In this work, we focus only on the transition from -ñ 1, 1 | to ñ 2, 1 | .…”
Section: Microwave Spectroscopy Of the Bi-chromatic Rf-dressed Shell mentioning
Free space atom-interferometry traditionally suffers from the large distances that atoms have to fall in order to achieve long interaction times. Trapped atom interferometry is emerging as a powerful way of achieving long interaction times in a reduced experimental volume. Here, we demonstrate bi-chromatic adiabatic magnetic shell traps as a novel tool for matterwave interferometry. We dress the magnetic hyperfine states of the F=1 and F=2 Rubidium 87 Bose-Einstein Condensates thus creating two independently controllable shell traps of which we use the = =-ñ F m 1, 1Using microwave pulses, we put atoms originally loaded into one of the two shell-traps into a superposition between the two shell traps. Since the two traps can be manipulated independently, their position and vertical curvature can be matched, thus creating a good starting point for an atom interferometer. This interferometer can be sensitive to spatially varying electric or magnetic fields, which could be DC or RF magnetic fields or microwaves. We demonstrate that the trap-matching afforded by the independent control of the shell traps allows for a tenfold increase in coherence times when compared to adiabatic potentials created by a single RF-frequency. For large-radius shells the atoms are confined to a 2D surface enabling highly sensitive imaging matterwave interferometers.Atom interferometry is a rapidly maturing quantum technology both for fundamental experiments and for applications. It has been successfully used to measure the Newtonian constant [1], and to put atominterferometric constraints on dark energy [2]. Which path and delayed choice experiments have been carried out using atom interferometry [3,4]. Atom interferometry may be used to test forces on atoms from small source masses in tests for small forces [5] and in the search for Ultralight Scalar Field Dark Matter [6,7]. Simple tests of the weak equivalence principle have been performed using atom interferometry [8] and there are proposals for space based extreme accuracy tests at the 10 −15 level [9] with some projections reaching 10 −19 [7,10]. On the applied side, atom interferometers have been used in absolute gravimetry on a ship [11] and in space [12]. Most precision interferometers still operate in the free-fall-regime, where, e.g.in the case of acceleration, the precision scales with the square of the interaction time. As a consequence, the most precise interferometers tend to become very tall, in some cases reaching ten or even one hundred meters in height [13]. Even larger interaction times are only possible in zero gravity on parabolic flights or in space [14]. Large sensitivity typically requires long interaction times and thus a large free-fall distance, which in turn makes the apparatus rather large.There have been numerous attempts to miniaturize such systems, e.g.using shaken lattices [15], partially trapped atoms interferometry with Sr [16] and coherent accelerations performed by the Bloch oscillations technique [17]. Even though some progress has been achieved...
“…Another consequence is the emergence of groups of transitions to quasienergy levels that are separated by multiples of the RF-dressing frequency, ω RF . 21 Each group occurs near one of the seven possible bare transition frequencies, and these reflect the standard selection rules for microwave polarisation. Even numbered groups n = 0, ±2 may be addressed with π-polarised MW, and odd numbered groups n = ±1, ±3 with σ-polarisation.…”
“…Additional aspects include the possibility of low-noise dispersive detection, 20 and also a complex spectrum of hyperfine multi-photon transitions that combine RF-photons from the dressing fields with additional microwave driving. 21 The principle of RF-dressed potentials 22 is to combine static B DC with time-dependent B RF (t) magnetic fields that drive atomic spin-flips. Neglecting the internal structure of an atom and within the weak field regime, the Hamiltonian for an atom with total spin F interacting with a static and single-frequency RF-field of arbitrary polarisation is given by…”
We describe our progress in the development of an atom based rotation sensor, which employs state-dependent trapping potentials to transport ultracold atoms along a closed path and perform Sagnac interferometry. Whilst guided atom interferometers are sought after to build miniaturized devices that overcome size restrictions from free-falling atoms, fully trapped interferometers also remove free-propagation along an atomic waveguide. This provides additional control of motion, e.g. removing wave-packet dispersion and enabling operation that remains independent of external acceleration. Our experimental scheme relies on radio-frequency and microwave-fields, which are partly generated via atom-chip technology, providing a step towards implementing a small, robust, and eventually portable atomic-gyroscope.
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