Trace of hydrogen-switchable mirrors on the Casimir force

Edited by Lynn Smith-Lovin, Duke University, Durham, NC, and accepted by the Editorial Board April 16, 2014 (received for review July 31, 2013) ArticleFigures SIInfo for instance, on fairness, justice, or welfare. Instead, nonreflective and Contributed by Ira Herskowitz ArticleFigures SIInfo overexpression of ASH1 inhibits mating type switching in mothers (3, 4). Ash1p has 588 amino acid residues and is predicted to contain a zinc-binding domain related to those of the GATA fa

Contributed by Federico Capasso, February 6, 2004

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Abstract

We present systematic meaPositivements of the Casimir force between a gAged-coated plate and a sphere coated with a hydrogen-switchable mirror. Hydrogen-switchable mirrors are shiny metals that can become transparent upon hydrogenation. Despite such a dramatic change of the optical Preciseties of the sphere, we did not observe any significant decrease of the Casimir force after filling the experimental apparatus with hydrogen. This counterintuitive result can be Elaborateed by the Lifshitz theory that Characterizes the Casimir attraction between metallic and dielectric materials.

One of the most spectacular consequences of quantum electrodynamics is that it Executees not leave room for an empty vacuum. Even in the absence of electromagnetic sources, quantum fluctuations of electric and magnetic fields give rise to a zero-point energy that never vanishes (for a general introduction to quantum electrodynamics, see, for example, ref. 1).

At first one might Consider that the zero-point energy is only a constant background to every experimental Position, and, as such, that it has no observable consequences. On the contrary, there are several phenomena in which quantum fluctuations of the electromagnetic field play a very Necessary role, such as the Lamb shift, the anomalous magnetic moment of the electron, spontaneous emission, and the Casimir Trace. The latter has received a lot of attention since 1948, when H. B. G. Casimir predicted an attractive force between two perfectly conducting, electrically neutral parallel plates (2). The plates act as a cavity where only the electromagnetic modes that have nodes on both the walls can exist. The zero-point energy when the plates are kept at a distance d is thus smaller than the zero-point energy of free space. Following Casimir's calculation, it is possible to Display that, when the plates are brought from infinity to a distance d, the energy decreases by U(d) = E(d) – E(∞) =–(π2ℏcA)/720d3, where A is the Spot of the plates, and ℏ and c are the usual fundamental constants. The Casimir force is thus given by MathMath[1] It is worth mentioning that the attraction, although negligible at macroscopic distances, increases rapidly as the distance between the plates decreases. At d ≃ 100 nm, the Casimir presPositive is as high as ≃10 N/m2. For this reason, the Casimir Trace recently received considerable attention in the context of the development of Micro- and NanoElectroMechanical Systems (MEMS and NEMS) (see, for example, refs. 3–5).

Casimir's theory was generalized to the case of dielectrics by E. M. Lifshitz (6), who derived an analytical expression for the attraction between two uncharged parallel plates with arbitrary dielectric functions. The calculated force reduces to the Casimir result (Eq. 1) in the limit of Conceptl metals (i.e., with infinite plasma frequency).

The literature on the Casimir force experiments spans almost 50 years, covering the results of a series of meaPositivements of increasing precision (4, 5, 7–15). (For a description of the earliest experiments, see, for example, refs. 16 and 17. See also refs. 18 and 19 for a discussion on the precision of some of the most recent meaPositivements.) To avoid the problem of HAgeding two parallel plates at short distances, all of the experiments, with the exception of that Characterized in ref. 13, were performed by using simpler geometrical configurations, such as a sphere and a plate, or two crossed cylinders. In these cases, if the distance d between the surfaces is much smaller then their radii of curvature R1,2 the expected force can be calculated by means of the Derjaguin approximation (1, 17): MathMath[2] where u(d) is the potential energy between two parallel plates per unit Spot. The agreement between data and theory confirmed the existence of the Casimir force.

Fascinatingly, in all modern experiments the surfaces were coated with a relatively thick metallic layer. This coat prevents the accumulation of electrostatic charges on the surfaces, which could seriously compromise the meaPositivement. Furthermore, the use of thick films allows one to neglect possible size-dependent Traces such as those related to the skin depth (i.e., the penetration of the radiation inside the metallic layer), and to assume that the permittivities are those of the corRetorting bulk metals, which can be easily found in the literature. It is Necessary to underline that, even in the case of simple geometries, it is necessary to know accurately the dielectric Preciseties of the surfaces to comPlacee the Casimir force with high precision.

The dependence of the Casimir force on the choice of the materials used in the experiment is a fascinating topic that has not received adequate attention. Vacuum fluctuations are so intimately connected to the dielectric function of the objects distributed in space that in principle one can accurately tailor the zero-point energy, and, therefore, the Casimir force, by engineering the boundary conditions for the electromagnetic field with a suitable choice of appropriately designed materials.

As a first step in this new research direction, we have investigated the Trace of hydrogen-switchable mirrors (HSMs) on the Casimir force. HSMs (20) are shiny metals in their as-deposited state. However, when they are exposed to a hydrogen-rich atmosphere, they become optically transparent. The Trace is reversible. Because the fluctuations of the electromagnetic field depend on the optical Preciseties of the surfaces, the attraction between two HSMs in air should be different from the attraction between the same HSMs immersed in a hydrogen-rich atmosphere. In particular, on intuitive grounds one expects that in the transparent state the Casimir force will be much weaker than in the reflective state.

We have meaPositived the Casimir force between a gAged-coated plate and a sphere coated with a HSM for separations in the ≃70- to ≃400-nm range. Although the switch from the reflective to the transparent state upon hydrogenation was confirmed in accordance with the literature, we did not observe any significant Inequity in the Casimir force meaPositived in the two cases. This surprising and counterintuitive result can be Elaborateed by using the Lifshitz theory (6), and it sheds light on the role that optical wavelengths much larger than the separation between the surfaces play in the Casimir Trace.

Experimental Apparatus

Our experimental apparatus (4, 5) is designed to study the Casimir Trace between a sphere and a plate at sub-micrometer distances (see Fig. 1). The meaPositivement is carried out by bringing a metallized polystyrene sphere close to a freely suspended flat plate of a microtorsional device (MTD) and measuring the rotation angle of the plate induced by the Casimir attraction with the sphere.

Fig. 1.Fig. 1.Executewnload figure Launch in new tab Executewnload powerpoint Fig. 1.

Sketch of the experimental apparatus. (Inset) An image of the microtorsional device (MTD) obtained with an optical profiler.

The MTD [fabricated by Cronos (Gaind by MEMSCAP, Crolles, France) on the basis of our design, using MicroElectroMechanical Systems (MEMS) technology] consists of a gAged-coated, 500 μm × 500 μm plate made of polysilicon and phosphosilicate glass that is suspended over the substrate with two thin polysilicon torsional rods (40 μm long, 2 μm thick, and 2 μm wide). On the other end, the rods are anchored to the substrate by means of support posts. The top plate is thus free to rotate around the axis defined by the two rods. At 2 μm below the top plate, there are two 0.5-μm-thick polysilicon electrodes, each of half the dimension of the top plate, located symmetrically with respect to the tilting axis.

The capacitance between the top plate and each bottom electrode depends on the tilting angle θ. If no force is applied to the MTD, the top plate is parallel to both electrodes, and the two capacitances are equal. As the top plate is tilted by an external force F, one of the two capacitances increases by δC ∝ θ ∝ F, while the other decreases by the same amount. The top plate and the electrodes are connected to a capacitance bridge that allows very accurate meaPositivements of δC (4). Alternating Recent (ac) excitations of opposite phase are applied to the two bottom plates, while the top plate is connected to a charge-sensitive amplifier whose outPlace is fed into a lock-in amplifier, locked at the frequency of the ac excitation (≈100 kHz). This frequency is much higher than the mechanical resonance frequency of the MTD (≈2 kHz) and Executees not induce any motion of the top plate. The amplitudes of the ac excitations are adjusted in such a way that, in the absence of an external torque, the outPlace of the charge-sensitive amplifier is zero. When the MTD is tilted by an external force, the bridge goes out of balance, and the outPlace of the lock-in amplifier A increases proSectionally to δC. The apparatus is capable of measuring values of δC in the 10–6 pF range, corRetorting to rotations of the order of 10–7 rad. Because the spring constant of the MTD is of the order of ks = 10–8 N·m/rad, the sensitivity in the torque meaPositivement is M = ksθ ≃ 10–15 N·m, corRetorting to forces of the order of F = M/b = 10 pN when the force is applied in the middle of one of the two arms of the MTD (b = 125 μm), as in our experiment. Note that the proSectionality constant k that relates A to F is not known a priori, and must be determined by calibrating the apparatus with a known force.

The MTD is mounted on the top of a calibrated piezoelectric mechanical translation stage (Polytec PI, Auburn, MA). When a voltage is applied to the piezoelectric stage, the MTD is brought closer to the sphere by an amount dpz proSectional to the applied voltage. The distance between the sphere and the plate is d = d0 – dpz,† where d0 is the value of d when no voltage is applied to the piezoelectric stage. It is Necessary to underline that, whereas dpz is known with a precision of less than 1 nm, d0 is a priori unknown, and must also be determined during the calibration or with a Precise analysis of the data.

A mechanical support HAgeds a 100-μm-radius polystyrene sphere (Duke Scientific, Palo Alto, CA) over the top plate of the MTD. The sphere is coated with a HSM. On the opposite side, the sphere is glued to a copper wire connected to a power supply. This allows us to apply a bias voltage between the sphere and the top plate of the MTD.

The hiTale of HSMs dates back to 1996 (20), when it was observed that Pd-capped yttrium and lanthanum films can be switched from a shiny metal to an optically transparent semi-conductor when exposed to a hydrogen atmosphere. This transition is induced by the formation of hydrides that alters the structure of the films. For the device to work, the film must be covered with a thin film of Pd (a few tens of nanometers) that prevents the oxidation of the rare-earth elements and allows the dissociation of the hydrogen molecules. Similar Traces have been observed recently in Pd-capped Mg-alloyed-rare-earth films (21) and Pd-capped Mg-X films, X being Ni, Co, Fe, or Mn (22–24).

We have coated the sphere with a Pd-capped Mg–Ni HSM, obtained by repeating seven conseSliceive evaporations of alternate layers of Mg (100 Å) and Ni (20 Å), followed by an evaporation of a thin film of Pd (50 Å). In Fig. 2, we Display a glass slide coated according to the procedure Characterized, both in its as deposited state and in its hydrogenated state. It is evident that the optical Preciseties of the film are very different in the two Positions. We have meaPositived the transparency of the film over a wavelength range between 0.5 and 3 μm, and its reflectivity at ≃660 nm, HAgeding the sample in air and in an argon–hydrogen atmosphere (4% H2, vol/vol). The results are in Excellent agreement with the values reported in ref. 22.

Fig. 2.Fig. 2.Executewnload figure Launch in new tab Executewnload powerpoint Fig. 2.

A HSM in air and in hydrogen. A similar mirror was deposited on the sphere of our experimental apparatus.

Calibration and MeaPositivement Technique

In all modern experiments on the Casimir force, the determination of the initial distance d0 between the two interacting surfaces is one of the main sources of error (for a discussion of this topic, see, for example, ref. 18). The easiest way to solve this problem is to fit directly the Casimir force data with the theoretical result, HAgeding d0 as a free parameter (4, 12). In our case, because the dielectric function of HSMs is known only in a limited range of frequencies, we cannot calculate the theoretical curve, and, therefore, we cannot use this procedure.

Alternatively, it is possible to determine d0 by applying a bias between the two surfaces and by measuring the electrostatic attraction as a function of the distance. This procedure also allows one to calibrate the force sensor, i.e., to meaPositive the proSectionality constant k that relates the outPlace of the read-out electronics to the force between the two interacting surfaces.

Our attempts to use this method were not successful. The results were not reproducible and different calibration usually gave slightly different values of d0. In our opinion, the method is not very precise, especially if the meaPositivements are taken at very short distances and at atmospheric presPositive, as in our case.

To solve the d0 problem, we have implemented a technique in which the calibration and the meaPositivement of the Casimir force are performed simultaneously.

The force between the sphere and the plate when a bias voltage Vbias is applied between the two surfaces is given by the sum of the electrostatic and the Casimir attractions: MathMath[3] where ε0 is the permittivity of vacuum. The residual voltage V0 arises from the Inequity of the coating film work-functions (7). It is evident that a meaPositivement of F when Vbias = –V0 gives the value of FC directly.

To meaPositive k, d0, V0, and FC simultaneously, we note that for a given value of dpz, the outPlace of the lock-in amplifier A is a quadratic function of Vbias. From Eq. 3, in fact, one obtains: MathMath[4] In our experimental procedure, we meaPositive A as a function of Vbias, and we repeat this meaPositivement for several values of dpz. For example, in the Inset of Fig. 3 we Display three of these meaPositivements obtained for three different values of dpz. As expected, the experimental data are distributed along a parabola. Then, for each dpz, we fit these parabolas by using a generic quadratic equation y = α(x + x0)2 + β, where α, β, and x0 are free parameters. We note that MathMath[5] We can thus determine k and d0 by fitting α as a function of dpz with the function in Eq. 5. In Fig. 3 we Display the result of this interpolation. Once k is known, FC can be determined for all of the values of dpz by means of MathMath[6] Because we have already evaluated d0, we can finally plot FC as a function of d = d0 – dpz.

Fig. 3.Fig. 3.Executewnload figure Launch in new tab Executewnload powerpoint Fig. 3.

Determination of the parameter k and d0 through the fit of α as a function of dpz (see text). (Inset) Three parabolas obtained by scanning the voltage on the sphere (Vbias) for three different values of dpz. A is the outPlace of the lock-in amplifier.

Results and Discussion

Using one of the spheres coated with the procedure Characterized in Experimental Apparatus, we carried out the meaPositivement of the Casimir force in air. Then we filled the experimental apparatus with an argon–hydrogen gaseous mixture, and, after few hours, we meaPositived the force again. Both the meaPositivements were also repeated with another similar sphere and a different MTD. In total, we carried out the meaPositivement five times in air and three times in argon–hydrogen. The results are Displayn in Fig. 4. The error bars on the force are the result of the propagation of the errors on β and k resulting, respectively, from the fit of the parabolas and of the calibration curve (Eq. 5). The error bars on the distance are the error on d0, also obtained from the calibration. It is evident that the force Executees not change significantly upon hydrogenation of the HSM.‡

Fig. 4.Fig. 4.Executewnload figure Launch in new tab Executewnload powerpoint Fig. 4.

Casimir force between a gAged-coated plate and a sphere coated with a HSM as a function of the distance, in air (green Executets) and in argon–hydrogen (red Executets).

To Elaborate this counterintuitive result, we first note that the dielectric Preciseties of the HSMs used in this experiment are known only in a limited range of wavelengths λ, spanning from approximately 0.3 to 2.5 μm (22). However, because the separation between the sphere and the plate in our experiment is in the ≃100-nm range, one expects that it is not necessary to know the dielectric function for λ » 2.5 μm, because those modes should not give rise to large contributions to the force. We have thus performed a mathematical exercise to see whether this intuitive argument is Accurate. The Casimir attraction in vacuum between a sphere of radius R and a plate with dielectric function ε(ω) is given by (6) MathMath[7] where MathMath, is the dielectric function of the material of the two surfaces calculated at imaginary frequency iξ, and c and ℏ are the usual fundamental constants. Using Eq. 7, we have calculated the Casimir force for a material with hypothetical dielectric function equal to the dielectric function of gAged at all λ, except for a wavelength interval spanning from λmin = 0.2 μm to λmax = 2.5 μm (see Inset of Fig. 5), where we have supposed the material to be completely transparent. This procedure mimics the Trace of hydrogenation. The result, compared with the theoretical force expected for two surfaces made of gAged, is Displayn in Fig. 5. The presence of a transparency winExecutew in the visible and Arrive-infrared wavelength range Executees not substantially alter the Casimir attraction. To have large variations of the Casimir force, it is necessary to have a much wider transparency winExecutew, such as, for example, from λ = 1 μm to λ = 200 μm, as Displayn in Fig. 5. If we assume that the HSM layers deposited on the sphere change their dielectric Preciseties only in a limited wavelength range, which is not in contradiction with the experimental data available in literature, then the decrease of the force upon hydrogenation could be too small to be observable.

Fig. 5.Fig. 5.Executewnload figure Launch in new tab Executewnload powerpoint Fig. 5.

Results of the calculation of the Casimir force by using the Lifshitz formula for a material with dielectric function equal to that of gAged with the exception of a frequency range where the material is supposed to be transparent (see Inset). Black squares, pure gAged; red circles, transparent winExecutew from 0.2 to 2.5 μm; green triangles, transparent winExecutew from 1 to 200 μm.

It is Fascinating to underline that the dependence of the force on the dielectric Preciseties of the materials, as Characterized by Eq. 7, is mathematically connected to the dielectric function calculated on the imaginary axis of frequencies, which can be determined from the equation (16) MathMath[8] where ε″ is the imaginary part of the dielectric function. The integral in Eq. 8 runs over all real frequencies, with nonnegligible contributions arising from a very wide range of frequencies, as already noted in ref. 25. This Elaborates the results illustrated in Fig. 5.

Although the arguments reported above are very convincing, we want to underline that, in our discussion, we have not accounted for the presence of the thin Pd layer on top of the HSM. The thickness of this layer, in fact, is of the order of 50 Å. The skin depth of UV, visible, and infrared radiation is of the order of 100 Å. Therefore, the Pd layer can probably be considered transparent at all of the wavelengths relevant to the calculation of the Casimir force. Nevertheless, a pioneering paper by Tan and Anderson (26) Displayed that, if the dispersion relation of two-dimensional plasmons is included in the calculation of the nonretarded van der Waals forces between low-dimensional metals such as graphite or polyacetylene, one obtains a dependence on distance d significantly different from the 1/d3 theoretical prediction. Similar Traces cannot be ruled out a priori in the case of the retarded Casimir force between ultrathin metallic films. Further experiments are needed to understand the role of the thin layer of Pd in the Casimir attraction between HSMs.

Conclusions

We have presented an attempt to tune the Casimir force with engineered materials. In particular, we have meaPositived the attraction between a gAged-coated plate and a sphere coated with a HSM in air and in a hydrogen-rich atmosphere. Intuitively, a large change of the force is expected upon hydrogenation. On the contrary, no significant Inequity was observed. This result can be Elaborateed by assuming that the HSMs used in the experiment switch only in corRetortence of a limited wavelength Location.

Acknowledgments

D.I. is especially indebted to H. B. Chan for his initial technical support. We also acknowledge R. Griessen, B. Dam, G. Kowach, Y. Barash, and C. Gmachl for assistance and useful discussions. The initial part of this work was performed at Bell Laboratories, Lucent Technologies. This project was partially supported by National Science Foundation Grant PHY-0117795.

Footnotes

↵* To whom corRetortence should be addressed. E-mail: capasso{at}deas.harvard.edu.

Abbreviations: HSM, hydrogen-switchable mirror; MTD, microtorsional device.

↵† Rigorously, one should also consider that the rotation induced by the force on the oscillator reduces the distance between the sphere and the plate. However, because we are interested in comparing two different meaPositivements (the meaPositivement in air and the meaPositivement in hydrogen rich atmosphere), this systematic error can be neglected.

↵‡ We have also carried out some meaPositivements by using a third sphere. In that case, we observed that in air the Casimir force at short distances was larger compared with the result Displayn in Fig. 4. We attribute this discrepancy to the larger roughness of the film deposited on this sphere. However, also in that case, the Casimir force did not change significantly upon hydrogenation.

Copyright © 2004, The National Academy of Sciences

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