46 research outputs found

    Improved Limits on Spin-Mass Interactions

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    Very light particles with CP-violating couplings to ordinary matter, such as axions or axion-like particles, can mediate long-range forces between polarized and unpolarized fermions. We describe a new experimental search for such forces between unpolarized nucleons in two 250 kg Pb weights and polarized neutrons and electrons in a 3^3He-K co-magnetometer located about 15 cm away. We place improved constrains on the products of scalar and pseudoscalar coupling constants, gpngsN<4.2×1030g^n_p g^N_s < 4.2\times10^{-30} and gpegsN<1.7×1030g^e_p g^N_s < 1.7\times10^{-30} (95% CL) for axion-like particle masses less than 10610^{-6} eV, which represents an order of magnitude improvement over the best previous neutron laboratory limit

    New classes of systematic effects in gas spin co-magnetometers

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    Atomic co-magnetometers are widely used in precision measurements searching for spin interactions beyond the Standard Model. We describe a new 3^3He-129^{129}Xe co-magnetometer probed by Rb atoms and use it to identify two general classes of systematic effects in gas co-magnetometers, one associated with diffusion in second-order magnetic field gradients and another due to temperature gradients. We also develop a general and practical approach for calculating spin relaxation and frequency shifts due to arbitrary magnetic field gradients and confirm it experimentally.Comment: 5 pages, 4 figure

    Observation of optical chemical shift by precision nuclear spin optical rotation measurements and calculations

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    Nuclear spin optical rotation (NSOR) is a recently developed technique for detection of nuclear magnetic resonance via rotation of light polarization, instead of the usual long-range magnetic fields. NSOR signals depend on hyperfine interactions with virtual optical excitations, giving new information about the nuclear chemical environment. We use a multi-pass optical cell to perform first precision measurements of NSOR signals for a range of organic liquids and find clear distinction between proton signals for different compounds, in agreement with our earlier predictions. Detailed first principles quantum-mechanical NSOR calculations are found to be in good agreement with the measurements.Comment: 4 page

    Electric Dipole Moments as Probes of CPT Invariance

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    Electric dipole moments (EDMs) of elementary particles and atoms probe violations of T and P symmetries and consequently of CP if CPT is an exact symmetry. We point out that EDMs can also serve as sensitive probes of CPT-odd, CP-even interactions, that are not constrained by any other existing experiments. Analyzing models with spontaneously broken Lorentz invariance, we calculate EDMs in terms of the leading CPT-odd operators to show that experimental sensitivity probes the scale of CPT breaking as high as 10^{12}GeV.Comment: 4 pages, typos correcte

    New limits on Anomalous Spin-Spin Interactions

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    We report the results of a new search for long range spin-dependent interactions using a Rb -21^{21}Ne atomic comagnetometer and a rotatable electron spin source based on a SmCo5_{5} magnet with an iron flux return. By looking for signal correlations with the orientation of the spin source we set new constrains on the product of the pseudoscalar electron and neutron couplings gpegpn/c<1.7×1014g^e_p g^n_p/\hbar c<1.7\times10^{-14} and on the product of their axial couplings gAegAn/c<5×1042g^e_A g^n_A/\hbar c<5\times10^{-42} to a new particle with a mass of less than about 1 μ1~\mueV. Our measurements improve by about 2 orders of magnitude previous constraints on such spin-dependent interactions.Comment: 4 pages, 4 figure

    Nuclear-Spin Gyroscope Based on an Atomic Co-Magnetometer

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    An experimental nuclear-spin gyroscope is based on an alkali-metal/noblegas co-magnetometer, which automatically cancels the effects of magnetic fields. Whereas the performances of prior nuclear-spin gyroscopes are limited by sensitivity to magnetic fields, this gyroscope is insensitive to magnetic fields and to other external perturbations. In addition, relative to prior nuclear-spin gyroscopes, this one exhibits greater sensitivity to rotation. There is commercial interest in development of small, highly sensitive gyroscopes. The present experimental device could be a prototype for development of nuclear spin gyroscopes suitable for navigation. In comparison with fiber-optic gyroscopes, these gyroscopes would draw less power and would be smaller, lighter, more sensitive, and less costly

    Laboratory Constraints on the Neutron-Spin Coupling of feV-scale Axions

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    Ultralight axion-like particles can contribute to the dark matter near the Sun, leading to a distinct, stochastic signature in terrestrial experiments. We search for such particles through their neutron-spin coupling by re-analyzing approximately 40 days of data from a K-3^3He co-magnetometer with a new frequency-domain likelihood-based formalism that properly accounts for stochastic effects over all axion coherence times relative to the experimental time span. Assuming that axions make up all of the dark matter in the Sun's vicinity, we find a median 95% upper limit on the neutron-spin coupling of 2.4×10102.4 \times 10^{-10} GeV1^{{-1}} for axion masses from 0.4 to 4 feV, which is about five orders of magnitude more stringent than previous laboratory bounds in that mass range. Although several peaks in the experiment's magnetic power spectrum suggest the rejection of a white-noise null hypothesis, further analysis of their lineshapes yields no positive evidence for a dark matter axion.Comment: 23 pages, 15 figure

    Limits on isotropic Lorentz violation in QED from collider physics

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    We consider the possibility that Lorentz violation can generate differences between the limiting velocities of light and charged matter. Such effects would lead to efficient vacuum Cherenkov radiation or rapid photon decay. The absence of such effects for 104.5 GeV electrons at the Large Electron Positron collider and for 300 GeV photons at the Tevatron therefore constrains this type of Lorentz breakdown. Within the context of the standard-model extension, these ideas imply an experimental bound at the level of -5.8 x 10^{-12} <= \tilde{\kappa}_{tr}-(4/3)c_e^{00} <= 1.2 x 10^{-11} tightening existing laboratory measurements by 3-4 orders of magnitude. Prospects for further improvements with terrestrial and astrophysical methods are discussed.Comment: Replaced with final version published in PR
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