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Resonant nonlinear magneto-optical effects in atoms∗ - The Budker ...

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B. Polarimetry<br />

For a 1-mW visible-light beam and χ ≃ 0.5, this corresponds<br />

to ∼2 × 10 −8 rad Hz −1/2 . Similar shot-noiselimited<br />

sensitivity can be achieved with a balanced po-<br />

Successful application of the NMOE-based experimental<br />

methods (Sec. XII) depends on one’s ability to perform<br />

precision polarimetry or, more specifically, laser Various modifications of the spectropolarimetry techlarimeter<br />

(Birich et al., 1994).<br />

spectropolarimetry.<br />

niques have been developed to meet specific experimental<br />

In a “balanced polarimeter” (Huard, 1997), a sample is requirements, with the common challenge of realiz<strong>in</strong>g the<br />

placed between a polarizer and a polariz<strong>in</strong>g beam splitter<br />

(analyzer) whose transmission axes are oriented at and polarimetry of condensed matter was given by Za-<br />

shot-noise limit of Eq. (31). A review of <strong>magneto</strong>-optics<br />

45 ◦ to one another. <strong>The</strong> <strong>optical</strong> rotation ϕ due to the passkii and Feofilov (1975). Birich et al. (1994) considered<br />

<strong>in</strong> detail experimental approaches to measurement<br />

<strong>optical</strong> activity of the sample can be found from a simple<br />

expression valid for ϕ ≪ 1<br />

of small <strong>optical</strong> rotation and their limit<strong>in</strong>g factors.<br />

ϕ = I 1 − I 2<br />

2(I 1 + I 2 ) , (29)<br />

C. Nonl<strong>in</strong>ear <strong>magneto</strong>-<strong>optical</strong> rotation with<br />

where I 1 and I 1 are the light <strong>in</strong>tensities detected <strong>in</strong> the<br />

frequency-modulated light<br />

two output channels of the analyzer. In order to measure<br />

the ellipticity ɛ of the transmitted light, a λ/4-plate is<br />

placed <strong>in</strong> front of the analyzer, oriented at 45 ◦ <strong>Budker</strong> et al. (2000b) showed that NMOR can be used<br />

to its<br />

for measurements of sub-microgauss magnetic fields with<br />

axis, to form a circular analyzer (Huard, 1997, see also<br />

sensitivity potentially exceed<strong>in</strong>g 10 −11 G Hz −1/2 (Sec.<br />

Sec. XI.E).<br />

VIII.E). However, for many applications (such as geophysics,<br />

magnetic prospect<strong>in</strong>g, and navigation), it is nec-<br />

Another method of polarimetry employs a crossed polarizer<br />

and analyzer (Fig. I and Sec. II.B) and polarization<br />

modulation. A polarization modulator us<strong>in</strong>g a<br />

essary to have a <strong>magneto</strong>meter with dynamic range ∼1<br />

G. <strong>Budker</strong> et al. (2002b) recently demonstrated that if<br />

Faraday-glass element is shown <strong>in</strong> Fig. XI.A. <strong>The</strong> signal<br />

frequency-modulated light is used to <strong>in</strong>duce and detect<br />

<strong>in</strong> the “dark” (crossed) channel of the analyzer is given<br />

<strong>nonl<strong>in</strong>ear</strong> <strong>magneto</strong>-<strong>optical</strong> rotation (FM NMOR), the ultranarrow<br />

features <strong>in</strong> the magnetic-field dependence of<br />

by<br />

(<br />

I s (t) ≃ χI 0 r e + 1 )<br />

2 α2 m+ ϕ 2 <strong>optical</strong> rotation normally centered at B = 0 can be translated<br />

to much larger magnetic fields. In this setup, light<br />

+ 2χI 0 α m ϕ s<strong>in</strong> ω m t − 1 (30)<br />

polarization modulation (Fig. XI.A) is replaced by frequency<br />

modulation of the laser, and the time-dependent<br />

2 χI 0αmcos 2 2ω m t.<br />

<strong>optical</strong> rotation is measured at a harmonic of the light<br />

Here χ is the coefficient def<strong>in</strong>ed by absorption and scatter<strong>in</strong>g<br />

of light by the atomic vapor cell, I 0 is the <strong>in</strong>tenfects<br />

both <strong>optical</strong> pump<strong>in</strong>g and prob<strong>in</strong>g of atomic polar-<br />

modulation frequency Ω m . <strong>The</strong> frequency modulation afsity<br />

of the l<strong>in</strong>early polarized light (<strong>in</strong> photons per unit ization. This technique should enable the dynamic range<br />

time) transmitted through the polarizer, r e is polarizer of an NMOR-based <strong>magneto</strong>meter to extend beyond the<br />

(analyzer) ext<strong>in</strong>ction ratio, and α m and ω m are polarization<br />

modulation amplitude and frequency, respectively.<br />

Earth-field range.<br />

For sufficiently low light <strong>in</strong>tensities (so that the <strong>optical</strong><br />

<strong>The</strong> amplitude of the first harmonic of the signal Eq.<br />

pump<strong>in</strong>g saturation parameter does not exceed unity),<br />

(30) is a measure of the polarization rotation caused by<br />

FM NMOR can be understood as a three-stage (pump,<br />

the sample. <strong>The</strong> first-harmonic amplitude is also proportional<br />

to the modulation amplitude α m . Typically, with<br />

precession, probe) process (Sec. V.B). Due to the frequency<br />

modulation of the laser light, the <strong>optical</strong> pump<strong>in</strong>g<br />

a Faraday modulator with a high-Verdet-constant glass<br />

(such as Hoya FR-5), the modulation α m is ∼10 −2 and prob<strong>in</strong>g acquire a periodic time dependence. When<br />

rad<br />

the pump<strong>in</strong>g rate is synchronized with the precession of<br />

(Wolfenden et al., 1990, 1991) at modulation frequencies<br />

atomic polarization, a resonance occurs and the atomic<br />

∼1 kHz. (High frequency modulation is often limited<br />

medium is pumped <strong>in</strong>to an aligned state whose axis rotates<br />

at the Larmor frequency Ω L . <strong>The</strong> <strong>optical</strong> proper-<br />

by the <strong>in</strong>ductance of the Faraday modulator solenoid.)<br />

<strong>Resonant</strong> photoelastic modulators can also be used for<br />

ties of the medium are modulated at 2Ω L , due to the<br />

polarimetry (as <strong>in</strong> the work of, for example, Oakberg,<br />

symmetry of atomic alignment. This periodic change of<br />

1995; Wang and Oakberg, 1999), allow<strong>in</strong>g for larger polarization<br />

modulation and higher modulation frequencies<br />

the <strong>optical</strong> properties of the atomic vapor modulates the<br />

angle of the light polarization, lead<strong>in</strong>g to the high-field<br />

(several tens of kilohertz).<br />

FM NMOR resonances. If the time-dependent <strong>optical</strong><br />

From Eq. (30), one can obta<strong>in</strong> the sensitivity of the polarimeter<br />

with data accumulation time T for shot-noise-<br />

rotation is measured at the first harmonic of Ω m , a resonance<br />

occurs when Ω m co<strong>in</strong>cides with 2Ω L . Additional<br />

limited detection of the first-harmonic signal <strong>in</strong> the case<br />

of an “ideal polarimeter” (αm 2 ≫ r e + ϕ 2 resonances can be observed at higher harmonics.<br />

):<br />

It should be noted that this technique is closely related<br />

to the work of Bell and Bloom (1961), <strong>in</strong> which the<br />

1<br />

δϕ s ≃<br />

2 √ χI 0 T . (31) <strong>in</strong>tensity of pump light was modulated <strong>in</strong> order to op-<br />

34

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