81 research outputs found

    Magnetic field--induced modification of selection rules for Rb D2_2 line monitored by selective reflection from a vapor nanocell

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    Magnetic field-induced giant modification of the probabilities of five transitions of 5S1/2,Fg=2→5P3/2,Fe=45S_{1/2}, F_g=2 \rightarrow 5P_{3/2}, F_e=4 of 85^{85}Rb and three transitions of 5S1/2,Fg=1→5P3/2,Fe=35S_{1/2}, F_g=1 \rightarrow 5P_{3/2}, F_e=3 of 87^{87}Rb forbidden by selection rules for zero magnetic field has been observed experimentally and described theoretically for the first time. For the case of excitation with circularly-polarized (σ+\sigma^+) laser radiation, the probability of Fg=2, mF=−2→Fe=4, mF=−1F_g=2, ~m_F=-2 \rightarrow F_e=4, ~m_F=-1 transition becomes the largest among the seventeen transitions of 85^{85}Rb Fg=2→Fe=1,2,3,4F_g=2 \rightarrow F_e=1,2,3,4 group, and the probability of Fg=1, mF=−1→Fe=3, mF=0F_g=1,~m_F=-1 \rightarrow F_e=3,~m_F=0 transition becomes the largest among the nine transitions of 87^{87}Rb Fg=1→Fe=0,1,2,3F_g=1 \rightarrow F_e=0,1,2,3 group, in a wide range of magnetic field 200 -- 1000 G. Complete frequency separation of individual Zeeman components was obtained by implementation of derivative selective reflection technique with a 300 nm-thick nanocell filled with Rb, allowing formation of narrow optical resonances. Possible applications are addressed. The theoretical model is perfectly consistent with the experimental results.Comment: 6 pages, 5 figure

    Observation of magnetically-induced transition intensity redistribution in the onset of the hyperfine Paschen-Back regime

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    The Zeeman effect is an important topic in atomic spectroscopy. The induced change in transition frequencies and amplitudes finds applications in the Earth-field-range magnetometry. At intermediate magnetic field amplitude B∼B0=Ahfs/μBB\sim B_0 = A_\text{hfs}/\mu_B, where AhfsA_\text{hfs} is the magnetic dipole constant of the ground state, and μB\mu_B is the Bohr magneton (B0≈1.7B_0\approx 1.7 kG for Cs), the rigorous rule ΔF=0,±1\Delta F = 0, \pm1 is affected by the coupling between magnetic sub-levels induced by the field. Transitions satisfying ΔF=±2\Delta F = \pm2, referred to as magnetically-induced transitions, can be observed. Here, we show that a significant redistribution of the Cs 6S1/2→6P3/26\text{S}_{1/2}\rightarrow 6\text{P}_{3/2} magnetically-induced transition intensities occurs with increasing magnetic field. We observe that the strongest transition in the group Fg=3→Fe=5F_g=3\rightarrow F_e=5 (σ+\sigma^+ polarization) for B<B0B<B_0 cease to be the strongest for B>3B0B>3 B_0. On the other hand, the strongest transition in the group Fg=2→Fe=4F_g=2\rightarrow F_e=4 (σ−\sigma^- polarization) remains so for all our measurements with magnetic fields up to 9 kG. These results are in agreement with a theoretical model. The model predicts that similar observations can be made for all alkali metals, including Na, K and Rb atoms. Our findings are important for magnetometers utilizing the Zeeman effect above Earth field, following the rapid development of micro-machined vapor-cell-based sensors

    Sub-Doppler spectroscopy of the near-UV Cs atom 6S1/2_{1/2}-7P1/2_{1/2} transition in a microfabricated vapor cell

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    We report on the characterization of sub-Doppler resonances detected by probing the 6S1/2_{1/2}-7P1/2_{1/2} transition of Cs atom at 459 nm in a microfabricated vapor cell. The dependence of the sub-Doppler resonance (linewidth, amplitude) on some key experimental parameters, including the laser intensity and the cell temperature, is investigated. These narrow atomic resonances are of interest for high-resolution spectroscopy, instrumentation, and may constitute the basis of a near-UV microcell optical standard

    Remote Detection Optical Magnetometry

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    Sensitive magnetometers have been applied in a wide range of research fields, including geophysical exploration, bio-magnetic field detection, ultralow-field nuclear magnetic resonance, etc. Commonly, magnetometers are directly placed at the position where the magnetic field is to be measured. However, in some situations, for example in near space or harsh environments, near nuclear reactors or particle accelerators, it is hard to place a magnetometer directly there. If the magnetic field can be detected remotely, i.e., via stand-off detection, this problem can be solved. As optical magnetometers are based on optical readout, they are naturally promising for stand-off detection. We review various approaches to optical stand-off magnetometry proposed and developed over the years, culminating in recent results on measuring magnetic fields in the mesosphere using laser guide stars, magnetometry with mirrorless-lasing readout, and proposals for satellite-assisted interrogation of atmospheric sodium.Comment: 68 pages, 19 figure

    Mirrorless lasing: a theoretical perspective

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    Mirrorless lasing has been a topic of particular interest for about a decade due to promising new horizons for quantum science and applications. In this work, we review first-principles theory that describes this phenomenon, and discuss degenerate mirrorless lasing in a vapor of Rb atoms, the mechanisms of amplification of light generated in the medium with population inversion between magnetic sublevels within the D2D_2 line, and challenges associated with experimental realization

    Universal determination of comagnetometer response to spin couplings

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    We propose and demonstrate a general method to calibrate the frequency-dependent response of self-compensating noble-gas-alkali-metal comagnetometers to arbitrary spin perturbations. This includes magnetic and nonmagnetic perturbations like rotations and exotic spin interactions. The method is based on a fit of the magnetic field response to an analytical model. The frequency-dependent response of the comagnetometer to arbitrary spin perturbations can be inferred using the fit parameters. We demonstrate the effectiveness of this method by comparing the inferred rotation response to an experimental measurement of the rotation response. Our results show that experiments relying on zero-frequency calibration of the comagnetometer response can over- or under-estimate the comagnetometer sensitivity by orders of magnitude over a wide frequency range. Moreover, this discrepancy accumulates over time as operational parameters tend to drift during comagnetometer operation. The demonstrated calibration protocol enables accurate prediction and control of comagnetometer sensitivity to, for example, ultralight bosonic dark-matter fields coupling to electron or nuclear spins as well as accurate monitoring and control of the relevant system parameters
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