1997
DOI: 10.1080/014423597230316
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The Cotton-Mouton effect in gases: Experiment and theory

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Cited by 124 publications
(118 citation statements)
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“…The integration time was T = 4 hours. Given that F = 6.7 × 10 5 , λ = 1064 nm, B 2 dl = 10.25 T 2 m, from the amplitude of the He peak at 32 µbar, the value of ∆n u for helium results ∆n (He,PVLAS) u = (2.2 ± 0.1) × 10 −16 T −2 atm −1 , in perfect agreement with other published values [6,28,29]. It must be noted that this value is obtained from a single low pressure point.…”
Section: Calibrationsupporting
confidence: 78%
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“…The integration time was T = 4 hours. Given that F = 6.7 × 10 5 , λ = 1064 nm, B 2 dl = 10.25 T 2 m, from the amplitude of the He peak at 32 µbar, the value of ∆n u for helium results ∆n (He,PVLAS) u = (2.2 ± 0.1) × 10 −16 T −2 atm −1 , in perfect agreement with other published values [6,28,29]. It must be noted that this value is obtained from a single low pressure point.…”
Section: Calibrationsupporting
confidence: 78%
“…The magnetic birefringence of gases also depends linearly on pressure. In Table V the equivalent partial pressures P eq which would mimic a vacuum magnetic birefringence for various gases [6,[28][29][30] are reported. The vacuum system must maintain these species well below their vacuum equivalent pressures.…”
Section: Polarizersmentioning
confidence: 99%
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“…At low temperatures these vapours will act in many ways like a gas phase analogue of ferrofluids. We predict in particular that the Cotton-Mouton effect (the dependence of index of refraction on direction with respect to an external magnetic field) which is proportional 24 to the product of polarizability anisotropy and magnetic susceptibility anisotropy, will be exceptionally strong. The dimer anisotropy energy can be extracted from the temperature dependence of the Cotton-Mouton effect which is sensitive to suppressed magnetic response perpendicular to the molecular axis when the anisotropy is strong.…”
mentioning
confidence: 99%
“…[1][2][3] Effects depending on the square of the flux density B of the applied field should be observable for the nuclear spin-spin coupling constants, 4 and for the molecular magnetizabilities, 5 which, for a diamagnetic molecule, are given by [6][7][8] ␣␤ ͑B͒ = ␣␤ + 1 2 X ␣␤␥␦ B ␥ B ␦ +¯. ͑1͒…”
Section: Introductionmentioning
confidence: 99%