There are generally three main classes of gravimeters: (a) laser or atom interferometers using timed measurements, (b) cryogenic superconducting levitated masses, and (c) spring-type gravimeters.
Laser interferometers have been implemented commonly for precision metrology across many scales and allow absolute gravimetry measurements with 1 to 10 μGal accuracies. Typically, laser interferometers involve timed and multiple-sampled measurements with calibrated or stabilized lasers, including locked to atomic clocks, to measure the free-fall of a reflecting body. Recent advances, for example, have used cold atom interferometry to determine the gravitational redshift to an accuracy of 7×10−9, improved precision of the gravitational constant to 1×10−4, or the gravity to a sensitivity of 100 ng per shot. With the interferometric or timed measurements, however, significant isolation from the environment—be it laser stabilization or cooling—is often required, which might hinder portability or rugged field deployment realizations.
Superconducting gravimeters typically have low thermodynamical noise and low-drift, which can be due to the inherent stability of persistent currents in the superconductor, stability of the mechanical proof mass (e.g., a few grams), and insensitivity to ambient perturbations. Superconducting gravimeters, however, typically operate at cryogenic temperatures at ˜4.2K or lower the even in a closed-cycle cryostat requires ˜1 kW power for helium liquefaction, bringing challenges outside the laboratory environment.
The third class of gravimeters provides the spring-type approach for relative inertial force measurements. This approach is generally the most deployed. Prior work in the bulk involved simply an inclined spring to a cantilever beam (e.g., 10 cm spring) that gives a ˜100 nm displacement for a ˜10 ng relative gravity difference. This displacement can be sensed optically. The ensuing linearity about the zero-displacement point can provide a large measurement range; the use of quartz beams can alleviate concerns such as, e.g., hysteresis and fatigue in the sensor. This baseline design has been continuously modified and updated by, for example, Scintrex and sister company Micro-g La Coste, encompassing applications such as, e.g., mapping the deep ocean seafloor morphologies. In one particular implementation, the recent gPhone can achieve, for example, 100 nGal resolution, 1 μGal precision with a system noise of 3 μGal/Hz1/2, 7 Gal range and 1.5 mGal/month drift. This bulk unit can also include a rubidium clock to synchronize the global positioning system. A compact chip-scale gravimeter, however, till date only has a few initial recent suggestions, involving, for example, gravimeters with capacitative readout.
The purpose and advantages of the disclosed subject matter will be set forth in and apparent from the description that follows, as well as will be learned by practice of the disclosed subject matter. Additional advantages of the disclosed subject matter will be realized and attained by the methods and devices particularly pointed out in the written description and claims thereof, as well as from the appended drawings.
Accordingly, some example embodiments may enable the provision of a chip-scale high-performance gravimeter through cavity optomechanics and methods for using the same. Exemplary embodiments of the present disclosure may provide, for example, a compact and array-scalable optical readout gravimeter, with, for example, 10 μGal/Hz1/2 (or ˜10 ng/Hz1/2) noise levels at 20 mHz sampling rates, and methods for using the same. The cavity optomechanical measurement sensitivity (up to ˜5×10-17 m/Hz1/2) can benefit, for example, from the low amplitude and phase noise of coherent laser sources. This exemplary approach can extend, for example, prior work on cavity optomechanics, such as, e.g., photonic crystal based slot-cavities for laser cooling of mesoscopic states, and nonclassical phase control of phonon states through coupled cavity optomechanical modes.
In one example embodiment, a method of determining a gravitational force is provided. The method may include providing at least one first radiation to at least one optomechanical oscillator where the at least one optomechanical oscillator is structured to deform under the gravitational force to cause a shift in resonance associated with the at least one optomechanical oscillator. The method may further include receiving at least one second radiation from the at least one optomechanical oscillator where the at least one second radiation is associated with the shift in the resonance. The method may further include determining the shift in the resonance based on the first and second radiations.
In another example embodiment, a non-transitory computer readable medium for determining a shift in a resonance associated with at least one optomechanical oscillator is provided. The computer readable medium may include instructions stored therein and may be accessible by a hardware processing arrangement. When the processing arrangement executes the instructions, the processing arrangement may be configured to perform at least one procedure that may include directing at least one first radiation to at least one optomechanical oscillator where the at least one optomechanical oscillator is structured to deform under the gravitational force to cause a shift in resonance associated with the at least one optomechanical oscillator. The at least one procedure may further include receiving at least one second radiation from the at least one optomechanical oscillator where the at least one second radiation is associated with the shift in the resonance. The at least one procedure may further include determining the shift in the resonance based on the first and second radiations.
In another example embodiment, an apparatus is provided for measuring gravitational force including at least one optomechanical oscillator, the at least one optomechanical oscillator having an initial resonance, and a second resonance when displaced by gravitational force; and at least one photonic crystal having at least one cavity coupling optical and mechanical degrees of freedom of the oscillator.
It is to be understood that both the foregoing general description and the following detailed description are exemplary and are intended to provide further explanation of the disclosed subject matter claimed.
The accompanying drawings, which are incorporated in and constitute part of this specification, are included to illustrate and provide a further understanding of the method and device of the disclosed subject matter. Together with the description, the drawings serve to explain the principles of the disclosed subject matter.
a-f illustrate exemplary optical cavity modes of mode-gap air-slot cavity from finite-difference time domain and band structure calculations.
Reference will now be made in detail to various embodiments of the disclosed subject matter, an example of which is illustrated in the accompanying drawings. The method and corresponding steps of the disclosed subject matter will be described in conjunction with the detailed description of the device.
Some example embodiments may enable the provision of a chip-scale high-performance gravimeter that may be small and portable, while still providing a relatively high degree of sensitivity. Some embodiments may provide a mass attached to an optomechanical cavity. The impact of gravity on the mass may cause properties of the optomechanical cavity to be altered. For example, if gravity increases, the mass may sag more and cause the width of the cavity to increase. As the cavity dimensions change, the properties of the cavity relative to modulation of a laser passed therethrough may also change. By monitoring changes in the modulation, a determination may be made as to the corresponding change in gravity that caused the change in modulation. Furthermore, example embodiments may couple a non-linear response to the optical field coupled with the small mode volume to provide noise cancellation that increases sensitivity.
The provision of an accurate and sensitive gravimeter that is also portable may enable the gravimeter to be advantageously employed in a number of environments outside of the laboratory. For example, some example embodiments may be useful in connection with conducting large-scale surveys regarding changes in gravitational fields underground, which may be used in connection with oil and gas exploration. Some embodiments may also be useful in connection with performing earth observations relating to geophysics research. Example embodiments may also be employed to perform tunnel detection and underground structure surveys. Such surveys may be useful for national or homeland security applications as well as the mining industry for assessment of the stability of underground structures. In some cases, example embodiments may be used in marine navigation to obtain precise gravity data for global navigation. Many other uses are also possible, and thus the examples above should not be seen as limiting relative to the scope of example embodiments.
Some example embodiments can provide, for example, a compact and array scalable optical readout gravimeter, with, for example, 10 μGal/Hz1/2 (or ˜10 ng/Hz1/2) noise levels at 20 mHz sampling rates, and methods for using the same. The cavity optomechanical measurement sensitivity (up to ˜5×10−17 m/Hz1/2) can benefit, for example, from the low amplitude and phase noise of coherent laser sources. This exemplary approach can extend, for example, prior work on cavity optomechanics, such as, e.g., photonic crystal based slot-cavities for laser cooling of mesoscopic states, and nonclassical phase control of photon states through coupled cavity optomechanical nodes.
Some example embodiments are illustrated in
Under the principle of transduction, the intensity of the light transmitted by the waveguide may vary as the beam is displaced by different amounts. Changing gravitational forces may alter the amount one of the beams deflects (and its resonant frequency.) The transmission of the waveguide can be measured. An example device can have multiple modes so a second mode can probe the device to detect the resonance shift.
As illustrated in
An optomechanical oscillator 116, which can be a photonic crystal or similar crystal waveguide in one example, is fabricated in the chip 10. The optomechanical oscillator 116 can be fabricated in at least two components, as seen more clearly in
As shown in
The resonance characteristics of the slot 114 can be dependent upon the width of the slot 114. Thus, as a mass 110 that may be attached to the optical oscillator assembly is affected by gravity to make the mass sag, the width of the slot 114 may be altered. The alteration of the width of the slot 114 may then be detected as a change in resonance characteristics of the cavity. For example, the response of the mass 110 to the gravitational field may cause a change in the width of the slot 114. In this regard, the optomechanical oscillator 116 can be configured to deform under the gravitational field (whether by construction using the slot 114 as described or similar constructions).
As the slot 114 flexes in response to the impact of the gravitational field on the mass, a change in the amplitude and phase of laser energy transmitted through the slot 114 may be detected. The change in amplitude and phase of the laser energy may be indicative of the modulation of the laser energy as caused by a change in the gravitational field. In addition, the change can be detected by monitoring and comparing radiation associated with the modulation as transmitted and as received.
Further exemplary specifications of the gravimeters 100 are provided in Table 1 and Table 2:
In some embodiments, the gravimeter is a chip-scale gravimeter that can be based on, for example, the high-Q/V air-slot photonic crystal mode gap cavity examined for cavity optomechanics. As illustrated in
a-f illustrate exemplary optical cavity modes of a mode-gap air-slot cavity from finite-difference time-domain and band structure calculations according to example embodiments.
The mechanical oscillator displacement sensitivity in high-Q/V systems such as the disclosed subject matter can be remarkable, with an experimentally-observed minimal photoreceiver-noise-limited sensitivity of, for example, ˜5×10−17 m/Hz1/2, or about four times the standard quantum limit. In a homodyne detection, the theoretical shot-noise-limited displacement sensitivity of the cavity optomechanical system can be described by the following equation:
For the exemplary cavity Q of ˜40,000, P at 1 μW and scaling coefficient η of 0.5, the displacement sensitivity can reach ˜8×10−19 m/Hz1/2 theoretically, which can be even feasible for zero-point motion detection with a 1 kHz resolution bandwidth, if the readout laser has quantum limited amplitude and phase noise.
The practical noise contributions can arise, for example, from thermal Brownian noise, photoreceiver (detector) noise, optical shot noise, and quantum backaction noise from optical gradient force fluctuations.
The thermal Brownian motion can be represented as follows:
The optical shot noise comes from noise in the light field at the output. The noise spectrum contains all the information on the mechanical displacement spectrum, but also a background term that is due to the quantum noise. This background constitutes the imprecision of the measurement. The optical shot noise is represented as follows:
The detector noise can be represented as follows:
The measurement of the oscillator's position disturbs. In the case of an optomechanical system, this is due to the fluctuation of intracavity radiation pressure. The force noise is referred to as quantum backaction noise, and is represented as follows:
Balanced homodyne phase-sensitivity measurement is described. Displacement sensitivity for the exemplary gravimeter design is illustrated in
Since the device and systems described herein detect the transmission of light, the RF spectrum shows us the noise power-spectral-density (PSD) directly, which arise from the contribution of the thermal Brownian noise, photoreceiver (detector) noise, optical shot noise, and quantum backaction noise. With
Exemplary embodiments of the present disclosure can also facilitate Pound-Drever-Hall locking and detection—this phase sensitive detection technique can allow a direct measurement of nanomechanical position (see example measurement setup in
In any case, measurement of nanomechanical position can facilitate the characterization of the displacement noise spectrum and the thermal Brownian motion [given, e.g., as 2 kBTsense/meffΩmΓm where Tsense can be the effective temperature of the sensing (e.g., fundamental) mechanical mode, meff can be the effective mass of the mechanical mode, Ωm can be the resonance frequency, and Γm can be the mode decay rate] of the chip-scale optomechanical gravimeter.
Exemplary Resonant detection: It is likely that a resonantly-driven measurement provide a better signal-to-noise to achieve the 10−8 sensitivities desired for the gravimeter. In the present case, the optical gradient force can drive the exemplary system on its RF mechanical resonance Ωm. The optical gradient force can arise from, for example, the evanescent optical fields and can be calculated through the Maxwell stress tensor and first-order perturbation theory. The optical force can give rise to an optical stiffening of the RF resonance, a resonance shift (Ω′m−Ωm) that can depend on the gravity-induced slot displacement as described by
where the optical interaction rate gom can be dependent on the gravity-induced slot displacement δx, |ao|2 can be the time-averaged Δ′o the laser-cavity detuning, and Δ2≡Δ′o2+(Γ0/2)2 with Γ0 the optical cavity photon decay rate. For a fixed laser-optical resonance detuning, the input laser power can be swept; the resulting characteristic slope of the mechanical frequency optical stiffening can differ for varying gravitational forces.
The high transduction sensitivity can benefit from the low amplitude and phase noise of coherent laser sources, in addition to the resonant driving approach. Further, resonant nanomechanical oscillators—by going to higher frequencies—can facilitate mass sensing in the range of attograms to zeptograms (10−21 grams), equivalent to the inertia force of several xenon atoms or an individual kDa molecule. The frequency shift can be read out electrically. This differential inertia force sensitivity can range ˜from 1 part in 105 to 1 part in 1012, very promising to reach 10−8 sensitivities desired in this gravimeter implementation. With the two-available optical cavity modes and wavelength-division multiplexing, a combined drive-and-sense protocol can also be implemented in the chip-scale optical gravimeter for compactness, noise normalization and robustness.
Exemplary Measurement considerations: The physical measurements and device nanofabrication can be examined, along with approaches to suppress the primarily noise sources. For field deployment, commercially available vertical cavity surface emitting lasers with low relative intensity noise can be embedded. The exemplary chip gravimeter can be packaged in vacuum that can facilitate the resonant mass to be kept constant to avoid, for example, spurious frequency shifts, to attain a high quality factor mechanical resonance, and to avoid molecular dynamical noise. The exemplary sensor can also be placed in vibration-isolated mounts (such as, e.g., from Minus-K) so as to suppress seismic noise. With an exemplary sampling rate in the range of 20 mHz and the tens to hundreds kHz resonances, e.g., a large sampling to average down the noise fluctuations can be feasible, although long-term (e.g., in the period of days) drift corrections are preferably carefully considered. A referencing between two (or more) gravimeters on the same chip should normalize out much of the seismic noise, while facilitating more rapid data acquisition. Readout noise and resonant dynamic range can be examined, from nonlinear optical stiffening at the high end (e.g., to avoid nonlinear Duffing instability), to source and detector shot noise at the low end. Thermoelectric cooling of the chip can also be examined for possible noise reductions. For exemplary absolute measurements, the exemplary chip-scale gravimeter can also be calibrated at a known-gravity site or with a laser-interferometer absolute gravimeter, although calibration variability are preferably carefully examined. The chip-scale implementation can also provide arrayed capability, such as for tensor gradiometer and parallel multiple measurements for improved noise averaging and multi-modal functionality in the same compact package.
As shown in
Further, the exemplary processing arrangement 502 can be provided with or include an input/output arrangement 514, which can include, e.g., a wired network, a wireless network, the internet, an intranet, a data collection probe, a sensor, etc. As shown in
It should be understood that the exemplary procedures described herein can be stored on any computer accessible medium, including a hard drive, RAM, ROM, removable disks, CD-ROM, memory sticks, etc., and executed by a processing arrangement and/or computing arrangement which can be and/or include a hardware processors, microprocessor, mini, macro, mainframe, etc., including a plurality and/or combination thereof. In addition, certain terms used in the present disclosure, including the specification, drawings and claims thereof, can be used synonymously in certain instances, including, but not limited to, e.g., data and information. It should be understood that, while these words, and/or other words that can be synonymous to one another, can be used synonymously herein, that there can be instances when such words can be intended to not be used synonymously.
Accordingly, some example embodiments may be provided to employ a relatively small and potentially mobile assembly for conducting gravimetry measurements. In this regard, some example embodiments may provide a chip-scale gravimeter that is capable of measuring relatively small and/or slow changes in gravitational fields with a relatively high degree of sensitivity. Example embodiments may provide a small space for light to pass through with a strong non-linear interaction employed to couple optic and mechanical modes. The non-linear response to the optical field coupled with the small mode volume of example embodiments, which small mode volume may be provided as the volume between a slot and mirror-like holes formed on either side of the slot within a photonic crystal, may provide noise cancellation that provides superior sensitivity for example embodiments.
Many modifications and other embodiments of the example embodiments of the invention set forth herein will come to mind to one skilled in the art to which these embodiments pertain having the benefit of the teachings presented in the foregoing descriptions and the associated drawings. Therefore, it is to be understood that the invention is not to be limited to the specific embodiments disclosed and that modifications and other embodiments are intended to be included within the scope of the appended claims. Moreover, although the foregoing descriptions and the associated drawings describe exemplary embodiments in the context of certain exemplary combinations of elements and/or functions, it should be appreciated that different combinations of elements and/or functions may be provided by alternative embodiments without departing from the scope of the appended claims. In this regard, for example, different combinations of elements and/or functions than those explicitly described above are also contemplated as may be set forth in some of the appended claims. In cases where advantages, benefits or solutions to problems are described herein, it should be appreciated that such advantages, benefits and/or solutions may be applicable to some example embodiments, but not necessarily all example embodiments. Thus, any advantages, benefits or solutions described herein should not be thought of as being critical, required or essential to all embodiments or to that which is claimed herein. Although specific terms are employed herein, they are used in a generic and descriptive sense only and not for purposes of limitation.
This application is a continuation-in-part of co-pending U.S. patent application Ser. No. 13/587,689, entitled “APPARATUS FOR MEASURING GRAVITATIONAL FORCE AND METHODS OF USING THE SAME,” filed Aug. 16, 2012, and co-pending U.S. patent application Ser. No. 13/586,135, entitled “CHIP-SCALE OPTOMECHANICAL GRAVIMETER,” filed Aug. 15, 2012, each of which application claims priority to and the benefit of U.S. Provisional Application No. 61/524,055 filed on Aug. 16, 2011, the entireties of each of which are hereby incorporated by reference herein.
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20140060178 A1 | Mar 2014 | US |
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