1,084 research outputs found

    Non-linear amplification of small spin precession using long range dipolar interactions

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    In measurements of small signals using spin precession the precession angle usually grows linearly in time. We show that non-linear interactions between particles can lead to an exponentially growing spin precession angle, resulting in an amplification of small signals and raising them above the noise level of a detection system. We demonstrate amplification by a factor of greater than 8 of a spin precession signal due to a small magnetic field gradient in a spherical cell filled with hyperpolarized liquid 129^{129}Xe. This technique can improve the sensitivity in many measurements that are limited by the noise of the detection system, rather then the fundamental spin-projection noise.Comment: 4 pages, 4 figure

    Cancellation of nonlinear Zeeman shifts with light shifts

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    Nonlinear Zeeman (NLZ) shifts arising from magnetic-field mixing of the two hyperfine ground-states in alkali atoms lead to splitting of magnetic-resonance lines. This is a major source of sensitivity degradation and the so-called "heading errors" of alkali-vapor atomic magnetometers operating in the geophysical field range (B approx. 0.2-0.7 G). Here, it is shown theoretically and experimentally that NLZ shifts can be effectively canceled by light shifts caused by a laser field of appropriate intensity, polarization and frequency, a technique that can be readily applied in practical situations.Comment: 5 pages, 5 figures, to be published in PR

    Temperature dependence of the nitrogen-vacancy magnetic resonance in diamond

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    The temperature dependence of the magnetic resonance spectra of nitrogen-vacancy (NV-) ensembles in the range of 280-330 K was studied. Four samples prepared under different conditions were studied with NV- concentrations ranging from 10 ppb to 15 ppm. For all of these samples, the axial zero-field splitting (ZFS) parameter, D, was found to vary significantly with temperature, T, as dD/dT = -74.2(7) kHz/K. The transverse ZFS parameter, E, was non-zero (between 4 and 11 MHz) in all samples, and exhibited a temperature dependence of dE/(EdT) = -1.4(3) x 10^(-4) K^(-1). The results might be accounted for by considering local thermal expansion. The observation of the temperature dependence of the ZFS parameters presents a significant challenge for room-temperature diamond magnetometers and may ultimately limit their bandwidth and sensitivity.Comment: 5 pages, 2 figures, 1 tabl

    How do you know if you ran through a wall?

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    Stable topological defects of light (pseudo)scalar fields can contribute to the Universe's dark energy and dark matter. Currently the combination of gravitational and cosmological constraints provides the best limits on such a possibility. We take an example of domain walls generated by an axion-like field with a coupling to the spins of standard-model particles, and show that if the galactic environment contains a network of such walls, terrestrial experiments aimed at detection of wall-crossing events are realistic. In particular, a geographically separated but time-synchronized network of sensitive atomic magnetometers can detect a wall crossing and probe a range of model parameters currently unconstrained by astrophysical observations and gravitational experiments.Comment: 5 pages, 2 figure; to appear in the PR

    Spin-exchange relaxation free magnetometry with Cs vapor

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    We describe a Cs atomic magnetometer operating in the spin-exchange relaxation-free (SERF) regime. With a vapor cell temperature of 103∘C103^\circ\rm{C} we achieve intrinsic magnetic resonance widths ΔB=17μG\Delta B=17 {\rm \mu G} corresponding to an electron spin-relaxation rate of 300s−1300 {\rm s^{-1}} when the spin-exchange rate is ΓSE=14000s−1\Gamma_{SE}=14000 {\rm s^{-1}}. We also observe an interesting narrowing effect due to diffusion. Signal-to-noise measurements yield a sensitivity of about 400 pG/Hz400\thinspace{\rm pG/\sqrt{Hz}}. Based on photon shot noise, we project a sensitivity of 40pG/Hz40 {\rm pG/\sqrt{Hz}}. A theoretical optimization of the magnetometer indicates sensitivities on the order of 2pG/Hz2 {\rm pG/\sqrt{Hz}} should be achievable in a 1cm31 {\rm cm^3} volume. Because Cs has a higher saturated vapor pressure than other alkali metals, SERF magnetometers using Cs atoms are particularly attractive in applications requiring lower temperatures.Comment: 8 pages, 6 figures. submitted to PR

    Gyroscopes based on nitrogen-vacancy centers in diamond

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    We propose solid-state gyroscopes based on ensembles of negatively charged nitrogen-vacancy (NV−{\rm NV^-}) centers in diamond. In one scheme, rotation of the nitrogen-vacancy symmetry axis will induce Berry phase shifts in the NV−{\rm NV^{-}} electronic ground-state coherences proportional to the solid angle subtended by the symmetry axis. We estimate sensitivity in the range of 5×10−3rad/s/Hz5\times10^{-3} {\rm rad/s/\sqrt{Hz}} in a 1 mm3{\rm mm^3} sensor volume using a simple Ramsey sequence. Incorporating dynamical decoupling to suppress dipolar relaxation may yield sensitivity at the level of 10−5rad/s/Hz10^{-5} {\rm rad/s/\sqrt{Hz}}. With a modified Ramsey scheme, Berry phase shifts in the 14N{\rm ^{14}N} hyperfine sublevels would be employed. The projected sensitivity is in the range of 10−5rad/s/Hz10^{-5} {\rm rad/s/\sqrt{Hz}}, however the smaller gyromagnetic ratio reduces sensitivity to magnetic-field noise by several orders of magnitude. Reaching 10−5rad/s/Hz10^{-5} {\rm rad/s/\sqrt{Hz}} would represent an order of magnitude improvement over other compact, solid-state gyroscope technologies.Comment: 3 figures, 5 page

    Production and detection of atomic hexadecapole at Earth's magnetic field

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    Anisotropy of atomic states is characterized by population differences and coherences between Zeeman sublevels. It can be efficiently created and probed via resonant interactions with light, the technique which is at the heart of modern atomic clocks and magnetometers. Recently, nonlinear magneto-optical techniques have been developed for selective production and detection of higher polarization moments, hexadecapole and hexacontatetrapole, in the ground states of the alkali atoms. Extension of these techniques into the range of geomagnetic fields is important for practical applications. This is because hexadecapole polarization corresponding to the ΔM=4\Delta M=4 Zeeman coherence, with maximum possible ΔM\Delta M for electronic angular momentum J=1/2J=1/2 and nuclear spin I=3/2I=3/2, is insensitive to the nonlinear Zeeman effect (NLZ). This is of particular interest because NLZ normally leads to resonance splitting and systematic errors in atomic magnetometers. However, optical signals due to the hexadecapole moment decline sharply as a function of magnetic field. We report a novel method that allows selective creation of a macroscopic long-lived ground-state hexadecapole polarization. The immunity of the hexadecapole signal to NLZ is demonstrated with F=2 87^{87}Rb atoms at Earth's field.Comment: 4 pages, 5 figure

    Constraints on short-range spin-dependent interactions from scalar spin-spin coupling in deuterated molecular hydrogen

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    A comparison between existing measurements and calculations of the scalar spin-spin interaction (J-coupling) in deuterated molecular hydrogen (HD) yields stringent constraints on anomalous spin-dependent potentials between nucleons at the atomic scale (∼1A˚{\rm \sim 1 \AA}). The dimensionless coupling constant gPpgPN/4πg_P^pg_P^{N}/4\pi associated with exchange of pseudoscalar (axion-like) bosons between nucleons is constrained to be less than 5×10−75\times 10^{-7} for boson masses in the range of 5keV5 {\rm keV}. This represents improvement by a factor of about 100 over constraints placed by measurements of the dipole-dipole interaction in molecular H2{\rm H_2}. The dimensionless coupling constant gApgAN/4πg_A^pg_A^N/4 \pi associated with exchange of a heretofore undiscovered axial-vector boson between nucleons is constrained to be gApgAN/4π<2×10−19g_A^pg_A^N/4 \pi < 2 \times 10^{-19} for bosons of mass ≲1000eV\lesssim 1000 {\rm eV}, improving constraints at this distance scale by a factor of 100 for proton-proton couplings and more than 8 orders of magnitude for neutron-proton couplings. This limit is also a factor of 100 more stringent than recent constraints obtained for axial-vector couplings between electrons and nucleons obtained from comparison of measurements and calculations of hyperfine structure.Comment: 4 pages 2 figure
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