1965
DOI: 10.1103/physrev.137.a1062
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Theory of Spin Exchange between Optically Pumped Rubidium and Foreign Gas Nuclei

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Cited by 78 publications
(29 citation statements)
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“…We obtain 0.45 ml s À 1 W À 1 for our device, again comparable to this quantity in large-scale polarizers 23 (see Supplementary Table 1). In this work, we employ the 87 Rb atoms as in situ detectors 13,18,19 of the 129 Xe magnetization and take advantage of the Fermi-contact interaction 13,[18][19][20][21] to enhance the detection sensitivity to 129 Xe by a factor of B500. This approach represents an important feature of our device that can be used to detect or monitor the 129 Xe polarization with high sensitivity at low magnetic fields in cases where the polarized gas can be cleanly extracted from the sample region.…”
Section: Discussionmentioning
confidence: 99%
“…We obtain 0.45 ml s À 1 W À 1 for our device, again comparable to this quantity in large-scale polarizers 23 (see Supplementary Table 1). In this work, we employ the 87 Rb atoms as in situ detectors 13,18,19 of the 129 Xe magnetization and take advantage of the Fermi-contact interaction 13,[18][19][20][21] to enhance the detection sensitivity to 129 Xe by a factor of B500. This approach represents an important feature of our device that can be used to detect or monitor the 129 Xe polarization with high sensitivity at low magnetic fields in cases where the polarized gas can be cleanly extracted from the sample region.…”
Section: Discussionmentioning
confidence: 99%
“…• It is thought that this term is particularly large for xenon due to polarization of the xenon core electron shells during a collision [97,98]. The polarization not transferred to the xenon is lost to the rotational angular momentum of the complex, N, which is subsequently dissipated as translational energy when the complex is broken up in another collision.…”
Section: Microscopic Picturementioning
confidence: 99%
“…As shown by Herman [27], the Fermi contact interaction is enhanced in the rubidium-xenon complex due to the electron exchange interaction between the rubidium5s electron and the core s orbitals of xenon. The enhancement is on the order \ of 10 3 which can be derived by writing a Slater determinant for the rubidium valence electron with the xenon Is orbitals:…”
Section: (J) + [(!) :::} 8u) + [(J)mentioning
confidence: 99%
“…They considered the xenon-NO and xenon-02 collision pairs and determined that the Fermi-contact interaction was responsible in both cases for the unusually iarge resonance shifts observed in mixtures of these gases. Just as in the case of Rb-Xe [27], the valence electrons of the paramagnetic species have a large spin density at the xenon nucleus due to the enhancement by the Pauli exclusion principle.…”
Section: Xenon With Other Gasesmentioning
confidence: 99%