Measurement of Mirror Birefringence at the Sub-Ppm Level: Proposed Application to a Test of QED

Measurement of Mirror Birefringence at the Sub-Ppm Level: Proposed Application to a Test of QED

PHYSICAL REVIEW A, VOLUME 62, 013815 Measurement of mirror birefringence at the sub-ppm level: Proposed application to a test of QED John L. Hall,* Jun Ye,* and Long-Sheng Ma† JILA, National Institute of Standards and Technology and University of Colorado, Boulder, Colorado 80309-0440 ͑Received 6 January 2000; published 15 June 2000͒ We present detailed considerations on the achievable sensitivity in the measurement of birefringence using a high finesse optical cavity, emphasizing techniques based on frequency metrology. Alternative approaches of laser locking and cavity measurement techniques are discussed and demonstrated. High-precision measure- ments of the cavity mirror birefringence have led to the interesting observations of photorefractive activities on mirror surfaces. PACS number͑s͒: 42.50.Ϫp, 42.79.Ϫe, 42.81.Ϫi, 12.20.Ϫm In the last decade, progress in the preparation and under- distance below 10Ϫ2 Åϭ10Ϫ10 cm. When we now feed this standing of mirrors of exceedingly low reflection losses has interferometer with a mW of technically quiet coherent light, been spectacular, leading to a feasible cavity finesse ap- in a one second averaging time—if all goes well and we have proaching 106. Measurements of optical phase anisotropy only shot noise as the limitation—these fringes can be effec- across the mirror surface can thus be enhanced by a similar tively subdivided into about ten million parts. The resulting factor. Shot-noise-limited measurement of the cavity reso- distance resolution is 10Ϫ17 cm. Sensitivity to these incred- nance frequency with orthogonal polarizations can poten- ibly small distance changes has attracted wide attention be- tially resolve birefringence effects another factor of 106 cause of their many potential applications, including the pos- smaller, limited by one’s ability to split the cavity linewidth. sibility of building interferometric antennas for gravitational Such measurement capability will open up interesting mea- wave radiation ͓4͔, and several groups worldwide are now surements regarding intrinsic mirror properties and their designing and building such major facilities ͓5͔. The three modification by light beams: the Cotton-Mouton effect in purposes of this paper are ͑i͒ to consider other attractive various gases ͓1͔, the influence of parity-nonconserving ef- physical measurements as enabled by this mirror and laser- fects in chiral molecules, and an interesting test of QED locking technology, namely, measurements based on bire- based on magnetically induced birefringence of the vacuum, fringence interferometry, ͑ii͒ to document our present status the so-called ‘‘light-by-light’’–scattering Feynman diagram of precisely measuring mirror birefringence, and ͑iii͒ to dis- ͓2͔. With the intracavity light beam of a high finesse cavity cuss the considerations that govern the achievable sensitivity threaded through a string of strong dipole magnets, the shot- in the measurement of birefringence. noise-limited measurement sensitivity of the cavity reso- We begin with a discussion of the operational interfero- nance would allow for the detection ͑and measurement͒ of metric experience using high grade mirrors: All such ‘‘gyro- the predicted ⌬n ͑birefringence͒ due to QED vacuum polar- quality’’ mirrors are observed to have a different reflection Ϫ ization (1.4ϫ10 22). Furthermore, such an experiment phase shift ͑or effective plane of reflection͒ depending upon would allow for a search for light scalar and pseudoscalar the state of polarization of the incident light. Perhaps during particles ͑such as the axion͒, which can couple by a two- polishing some microscopic stress fields were written into photon vertex. The limit for the axion–two-photon coupling the substrate and not fully erased by the randomizing process constant measured by this technique should be comparable to of the slow spindle rotation. Perhaps during the coating pro- the bound set from astrophysical arguments. cess the flying molecules were incident at some inclined Several industrial organizations have independently in- angle to the surface, leading to some small level of preferred- vested adequate efforts to develop the art of ‘‘superpolish- direction effects in the coating’s otherwise glassy, isotropic, ing’’ substrates to angstrom-level surface roughness, aug- and nearly structureless coated layers. In any event, it is a mented by the art of depositing 40–50 alternating layers of fact of experience that all mirrors tested show some level of high and low index dielectric materials, leading to the com- birefringent behavior that can be as small as a 0.1-␮rad dif- mercial availability of mirrors with losses guaranteed to be ferential phase shift/bounce. Indeed, it is extremely difficult below five parts in 106. Losses of ϳ1 ppm have been docu- to robustly mount fused silica mirrors without inducing mented over selected submillimeter areas ͓3͔. The resulting stress-related birefringence. A cavity formed with birefrin- sharpness of the associated Fabry-Perot fringes is breathtak- gent mirrors will accumulate the differential phase shift in- ing to contemplate: one full fringe width is represented by a curred per mirror bounce and magnify it by a factor of (2ϫfinesse/␲) at the cavity transmission. This mirror- related cavity birefringence presents an adversity to many *Also at the Quantum Physics Division, National Institute of high-precision measurements using a high finesse cavity. For Standards and Technology, Boulder, CO. example, in the measurement of parity nonconservation in Cs †Permanent address: Laboratory for Quantum Optics, East China atoms, a small systematic error is introduced when the two Normal University, Shanghai, China. counterpropagating waves inside the cavity have slightly dif- 1050-2947/2000/62͑1͒/013815͑8͒/$15.0062 013815-1 ©2000 The American Physical Society JOHN L. HALL, JUN YE, AND LONG-SHENG MA PHYSICAL REVIEW A 62 013815 ferent polarizations, which result from the existence of cavity realized in several different ways. For example, in the pro- birefringence ͓6͔. In the experiment involving optical cavity posed QED birefringence experiment, two polarization states QED, cavity birefringence prevents the realization of the full of light are resonantly interacting with mirrors with small potential of strong coupling between an atom and the cavity polarization phase shifts. Theoretically, one finds that good mode ͓7͔. However, one could also take advantage of this performance and sensitivity can be obtained by measuring intrinsic birefringence to boost the useful signal level. With the differences in the apparent transmission when it is tuned an appropriate polarimetric setup, this dc bias can be gain- near the high slope regions around the half height of the fully employed to convert a quadratic signal of interest to a resonance line shape. A simpler method would be to illumi- linearized one, with a scaling factor equal to the magnitude nate the cavity with light polarized at ϩ45° to the birefrin- of cavity birefringence ͓8͔. Accurately measuring the mirror gence axes, and analyze the transmitted light with a crossed birefringence could also lead to useful information on sur- polarizer ͓9,10͔. Another technique is to add some external face science. As for scale, a reasonable contemporary gyro- ellipticity modulation to the beam in order to again linearize quality mirror may show about 10Ϫ6 waves of phase differ- the signal ͓11͔. Because of the cavity resonance effect, a very ence at normal incidence for light polarized in two small birefringence will detune the two-cavity polarization perpendicular linear polarizations. Exceptional mirrors may modes by a significant part of a linewidth. A compensating be threefold or even tenfold less. The residual circular bire- phase plate in the exit beam can delay the faster component fringence for almost all mirrors is at least an order smaller so that the dark fringe condition can be reestablished in the than the birefringence observed with linearly polarized light. polarizer-transmitted light. The birefringence is then the Realizing that the high signal-to-noise ratio enabled by a measured phase, divided by the cavity finesse F. One sees an cavity configuration ͑splitting of the linewidth͒ offers us ac- inconvenience for this method also: What happens if our cess to another factor of ϳ107 in terms of sensitivity en- birefringence phase could be larger than ␲/F? Now we can- hancement, it seems likely that some interesting things can not excite both modes of the cavity simultaneously, so a be turned up. lower finesse—broader cavity resonance—must be used. How can we precisely measure these subtle optical phase However, it is clear we prefer to use a very high finesse— shifts? Ideally, we will be able to measure them sufficiently this directly increases the sensitivity. We want to use a fre- accurately so that two measurements taken with some time quency based scheme to provide the large dynamic range. separation can be found to agree at some attractive level of For the locking, one also prefers to use some appropriate precision. Then we will be ready to jump into our applica- modulation method so that the desired antisymmetric reso- tions. But first, operationally, how can we measure the effect nance curve is produced by synchronous detection at the cen- accurately? What are the possible tools? It is instantly clear tral tuning condition. A particularly attractive modulation/ from the numbers quoted above that it is only with detection scheme was described in 1983 by Drever et al. ͓12͔ frequency-based metrology that we can hope to have the ac- for producing this ‘‘discriminator’’ line shape using laser curacy necessary to deal with an effect that can range from light reflected from the cavity. They showed that it was de- ϳ1toϳ10Ϫ13 waves as the dynamic range. The possibility sirable to use a modulation frequency well above the cavity for the two polarizations to coexist between the cavity mir- resonance response width so that the modulation sidebands rors and then be separated externally with a polarizing prism would be nonresonant and would therefore be essentially re- is very attractive since it enables the measurement of the flected from the cavity input mirror.

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