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Nanomechanical Sensing

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Volume 2012 |Article ID 617386 |

Rohit Mishra, Wilfried Grange, Martin Hegner, "Rapid and Reliable Calibration of Laser Beam Deflection System for Microcantilever-Based Sensor Setups", Journal of Sensors, vol. 2012, Article ID 617386, 6 pages, 2012.

Rapid and Reliable Calibration of Laser Beam Deflection System for Microcantilever-Based Sensor Setups

Academic Editor: Sangmin Jeon
Received14 Jun 2011
Accepted05 Aug 2011
Published19 Oct 2011


Cantilever array-based sensor devices widely utilise the laser-based optical deflection method for measuring static cantilever deflections mostly with home-built devices with individual geometries. In contrast to scanning probe microscopes, cantilever array devices have no additional positioning device like a piezo stage. As the cantilevers are used in more and more sensitive measurements, it is important to have a simple, rapid, and reliable calibration relating the deflection of the cantilever to the change in position measured by the position-sensitive detector. We present here a simple method for calibrating such systems utilising commercially available AFM cantilevers and the equipartition theorem.

1. Introduction

Cantilever-based sensor devices have extensively developed from the atomic force microscope (AFM) operating in the static mode [13] (surface stress based; qualitative method) and the dynamic mode [46] (frequency based; quantitative method) depending on the application. The most frequently used method of signal transduction where cantilevers are employed is change in surface stress being converted into mechanical signal through cantilever bending [7]. This deflection is an indication of the chemical [8], physical [9], or biophysical [10] process that occurs on the cantilever interface.

The laser beam-based deflection system [11] has been used most widely to measure the cantilever bending in the static mode because of the ease of use, robustness of the readout technique, and availability of high-sensitivity position-sensitive detectors (PSDs) which allow subangstrom resolution [12, 13]. Subsequently, several studies have been made to determine the limitations of this technique along with its resolution and sensitivity [1417]. One also comes across various techniques for determining the relation between the cantilever bending and the change in spot position observed by the PSD [1821]. The simple geometric calculation of this factor safely presumes that the bending of the cantilever is very small such that it can be assumed to be half that of the deflection angle of the laser beam [20]. Most other methods are tedious and require specialised methods [18] for determining this factor and may additionally require precise measurement of the angles [22] (azimuthal and incidence), distance between the cantilever surface and the PSD, and so forth, which gets more complicated for beam directing methods with complex geometries using mirrors. We present here a simple plug and measure system for determining this deflection factor (𝐺) using commercially available AFM cantilevers and applying the equipartition theorem for small cantilever deflections.

The displacement of the laser spot on the PSD (Δ𝑑) can be related to the cantilever bending (Δ𝑥) (Figure 1) using geometrical methods as [20] Δ𝑥=Δ𝑑𝐿4𝑠,(1) where 𝑠 is the distance from cantilever to the PSD, and 𝐿 is the length of the cantilever. Hence, the value of Δ𝑥 can be calculated based on the geometry of the setup. The absolute relationship used for relating Δ𝑥(nm) using a PSD, however, needs to include the geometrical factor needed for a particular setup which when incorporated gives the relationship as below:𝐼Δ𝑥=𝐺1𝐼2𝐼1+𝐼2𝑙psd2,(2) where 𝐼1𝐼2 is the difference signal, and 𝐼1+𝐼2 is the sum signal obtained from the PSD, and 𝑙psd is the active PSD length in mm. It is important to note that Δ𝑑(nm) for a PSD is generally defined as (when 𝑙psd is defined in mm)𝐼Δ𝑑=1𝐼2𝐼1+𝐼2𝑙psd2106.(3) Equation (1) gives purely a geometrically calculated value with the aforesaid assumption that if the deflection angle of the laser is Θ, the cantilever bending angle is Θ/2; it includes errors arising from differences in design and actual geometry such as the position and angle of the laser, the angle of the cantilever holder and the reflecting mirror, and the placement of the PSD. A more rigorous approach is needed to take into account not just the theoretical factors but also practical constraints of the setup.

The equipartition theorem relates the thermal energy of a system to its temperature in classical thermodynamics. Thermal noise of a cantilever can be quantified using this theorem [23, 24]. The equipartition theorem states that if a system is in thermal equilibrium, every independent quadratic term in its total energy has a mean value equal to 1/2𝑘𝐵𝑇, where 𝑘𝐵 is the Boltzmann constant and 𝑇 is the absolute temperature. The equipartition theorem relates this total energy to the potential energy of a rectangular cantilever with a mean square deflection of the cantilever caused by thermal vibrations as follows [25]:12𝜅𝑥2=12𝑘𝐵𝑥𝑇,2=𝑘𝐵𝑇/𝜅,(4) where 𝜅 is the spring constant of a rectangular cantilever with finite thickness and length provided that the bending is small. From (4), one can determine the thermal displacement of a cantilever provided that the spring constant is known. The deflection factor can hence be calculated if this thermal displacement can be related to the deflection obtained on a PSD.

Combining (2) and (4), 𝐺𝐼1𝐼2𝐼1+𝐼2𝑙psd22=𝑘𝐵𝑇𝜅.(5) Hence, deflection factor2𝐺=𝑙psd𝑘𝐵𝑇𝜅𝐼1𝐼2𝐼1+𝐼22.(6) The term ((𝐼1𝐼2)/(𝐼1+𝐼2))2 in the above equation is obtained from the PSD signals, using a power spectral analysis program (Virtual instrument, Labview, National Instruments) normalized to the sum signal of the PSD and is the area under the first resonance peak of a cantilever beam of known spring constant. The program essentially obtains the power spectrum which is a computation of the single-sided, scaled spectrum of the time domain signal from the PSD into the frequency domain. For a signal 𝑥(𝑡), the complex spectrum is obtained by a fast Fourier transform (FFT) defined as (in the frequency domain)𝑋(𝑓)𝑥(𝑡)𝑒2𝜋𝑓𝑡𝑑𝑡.(7) This gives, furthermore, the definition of the one sided power spectrum (in Sq. Amplitude/Hz) which is defined as||||Powerspectrum,𝜙(𝑓)𝑋(𝑓)2𝑛2||||||||𝑋(𝑓)𝑋(𝑓)𝑛2,(8) where 𝑛 is the number of points in the signal, and * denotes the complex conjugate. The integral of the power spectrum (area under the curve) provides the final value according to the Parseval's theorem which states that the area under the energy spectral density curve is equal to the total energy.

It is important to note that only the area under the first resonance peak is considered in further measurements, neglecting the higher modes since their contribution was seen to be minor (modelled as a simple harmonic oscillator with one degree of freedom). The spring constant of the calibration cantilevers hence needs to be measured as well. There are several methods available to perform such calibration to obtain spring constants [2632] including the most frequently used thermal noise method. We chose the thermal calibration module in the Asylum MFP-3D AFM [33, 34] (Asylum research, USA) which has been shown to measure the values with relatively good accuracy and reproducibility [34]. The method records the change in PSD position as a function of cantilever angular bending when pressed against a hard surface using a closed loop piezo actuator and then converts it into values for cantilever spring constant using a predetermined sensitivity factor called inverse optical lever sensitivity. With the rest of the terms known in the equation, the calibration factor can be calculated.

2. Materials and Methods

Different sets of commercially available AFM cantilevers were used namely Mikromasch CSC38/AIBS “B” (Mikromasch, Estonia) and NTMDT CSCS12 “E” (NT-MDT, Russia) cantilevers for the measurement of the thermal noise spectrum and final calibration. The cantilevers were calibrated using the Asylum MFP-3D AFM to get individual values for their spring constants 𝜅. Table 1 enlists manufacturer specifications for these AFM cantilevers.

SpecificationsMikromasch CSC38/AIBS “B”NTMDT CSCS12 “E”

Length (l) μm350350
Width (w) μm3535
Thickness, μm0.
Resonant frequency (kHz)7101481012
Force constant (N/m)

The power spectrum of the thermal noise was obtained using a 150 kHz band pass position-sensitive detector (SiTek, Sweden). This detector is a modified version of the low-pass 5 Hz sensor which is used for performing static mode biological experiments. A Labview program was used to obtain the averaged power spectrum from the differential and sum signals from the PSD. The parameters for obtaining the power spectrum had to be chosen so as to eliminate effects like aliasing which leads to truncated or artificially small resonance peaks and also electronic noise. Also it was necessary to choose the number of samples and the sampling frequency such that it avoided overloading the system and the data acquisition card (DAQ, National instruments). Keeping in mind all these details and following the Nyquist theorem (signal must be sampled at a rate at least greater than twice the highest frequency component of the signal) the parameters which were chosen for the power spectral analysis were as follows: sampling frequency: 100 kHz, number of samples: 10,000, and number of averages: 5000. The area under the first resonance peak was obtained using a Lorentzian fit in origin graphical software (OriginLab Corporation, USA). The area hence calculated along with the spring constant values was then used to determine the value of 𝐺 for a particular setup. Two different cantilevers were used for the calibration of each setup with three trials on each cantilever, and the values were finally averaged. Between each trial, the cantilever was taken out of the holder chamber and reinserted. The laser power and the temperature of the chamber were kept constant for all trial measurements.

3. Results

3.1. Geometric Method for Calibration Factor

For our present instrumental scheme, the geometrical calculation for both the setups is the same as derived below. For: 𝑠=61mm (for instrument 1 and 2) and 𝐿=500𝜇m.

Equation (1) can be modified to obtain Δ𝑥=Δ𝑑488(9) Substituting Δ𝑑 from (3) 𝐼Δ𝑥=20491𝐼2𝐼1+𝐼2𝑙psd2.(10) Comparing (2) and (10) the deflection factor 𝐺 from geometric calculations is 2049 for the particular geometry and is the same for any instrument made to this scheme.

3.2. Calibration Factor 𝐺 Using Equipartition Theorem
3.2.1. Determination of Spring Constants for the Cantilevers Using Asylum AFM

The spring constants for the calibration cantilevers were determined as an average of three trials during which the cantilevers were removed and replaced in the AFM setup in order to average out errors. The averaged values of the cantilevers are summarized in Table 2.

Spring constantMicromasch B cantileversNTMDT cantilevers E

𝜅 ( p N / n m ) 69.66166.7432.6453.13

3.2.2. Thermal Noise Data Acquisition from the Instrumental Setups

Calibration factor, 𝐺 was calculated for two different deflection setups both identical with respect to geometrical design using the previously mentioned cantilever sets. The power spectrum was obtained when keeping the differential signal as close as possible to zero (centre of the PSD) and the sum signal as high as possible. Figure 2 shows a sample powers pectrum obtained for Cantilever E1 on the second trial. According to the power spectrum analysis, we relate the vibrational amplitude in ambient air to the spring constant using (4).

Table 3 summarizes the results for the calibration of the instruments using the above set of cantilevers and substituting the values of the spring constant and the area under the power spectrum into (6).

Area under curve 𝐺 Average 𝐺

Deflection factor 𝐺 setup 1
Cant B1 ( 𝜅 = 6 9 . 6 6 p N / n m ) Trial 1 5 . 2 0 𝐸 1 0 21282077.5
Trial 2 4 . 5 1 𝐸 1 0 2284
Trial 3 4 . 9 8 𝐸 1 0 2175
Cant B2 ( 𝜅 = 1 6 6 . 7 4 p N / n m ) Trial 1 2 . 4 9 𝐸 1 0 1986
Trial 2 2 . 5 0 𝐸 1 0 1982
Trial 3 2 . 7 0 𝐸 1 0 1910

Deflection factor 𝐺 setup 2
Cant E1 ( 𝜅 = 3 2 . 6 4 p N / n m ) Trial 1 7 . 9 3 𝐸 1 0 25172679.5
Trial 2 5 . 3 6 𝐸 1 0 3062
Trial 3 6 . 0 1 𝐸 1 0 2891
Cant E3 ( 𝜅 = 5 3 . 1 3 p N / n m ) Trial 1 3 . 9 2 𝐸 1 0 2807
Trial 2 5 . 5 0 𝐸 1 0 2368
Trial 3 5 . 2 2 𝐸 1 0 2432

From the above set of values of the 𝐺 factor, it can be seen that the two setups differ from the theoretical geometric value and also from each other. The difference between the two values (the value of 𝑠 differs by ~13.518 mm between the two when back calculated from the obtained calibration factors) indicates that the two setups despite having similar geometry have different travel lengths of the laser from the cantilever surface to the PSD. This could be attributed mainly to the change in position and tilt of the mirror, small differences in the setting up and machining of the home made systems and angles of the cantilever holders and hence the manner in which the lasers spot is reflected by the mirror onto the PSD. It is, hence, important to note that modifications of any kind to such laser deflection systems require a recalibration especially when the differential measurements are close ranged. When compared to results from the geometric method, it is clear that the method we propose shows the variation between individual deflection setups despite their similar geometric design within reasonable error margins (5–10%).

4. Conclusions

The importance of having sensitive measurements especially in systems involving a differential analysis is of foremost significance for ensuring the reliability of cantilever sensor systems. Establishing the occurrence of an event of interest on the cantilever surface using in situ reference cantilevers is absolutely essential to eliminate convoluted environmental signals. Hence, a reliable method to calibrate the deflection of the cantilever is mandatory.

We demonstrate here a simple and reliable method for rapid calibration of laser-based deflection systems. Using commercially available AFM cantilevers, we can show that the relationship between the spot movement on the PSD and the actual cantilever deflection can be determined although within the accuracy of the assumptions and the thermal calibration method (~5–10%) [35]. The method was used to calibrate comparable cantilever array systems with a mirror used for deflecting the laser onto the PSD because of space restrictions. This indicates the application of the method to more complex geometries without the need for accurate measurement of other physical parameters of the geometry.


The authors would like to thank the Science Foundation Ireland and F. Hoffman La Roche for their support through research Grants (SFI 00/PI.1/C02, 09IN.1B2623, and Roche 5AAF11).


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Copyright © 2012 Rohit Mishra et al. This is an open access article distributed under the Creative Commons Attribution License, which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.

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