The present invention relates to optical-thin-film structures and methods for making them.
As is relevant for this specification, an “optical thin film” is a layer of material(s) having a thickness that is on the order of the coherence length of the light with which it interacts. Such optical thin films typically have a thickness within the range of a fraction of a nanometer to many micrometers.
Structures comprising plural optical thin films, and having appropriate characteristics, are useful for optical applications. A few examples of such optical-thin-film structures include mirrors, wavelength filters, anti-reflection coatings, and windows.
Optical-thin-film structures often comprise multiple layers of dielectric materials, typically alternating between those comprising materials having a relatively high refractive index and those having a relatively low refractive index. In the context of infrared (IR) wavelengths in the range between about 1.5 to about 20 microns (“mid-IR”), “low-index” materials/layers are those having a refractive index less than about 1.7, and “high-index” materials/layers are those having a refractive index of about 1.7 and greater.
The optical thin films composing such structures should be robust to temperature changes, mechanical shock, humidity, and other environmental factors. Moreover, the optical thin films of optical reflectors, filters, and windows must absorb no more than a minimal amount of light over a broad range of wavelengths.
For mid-IR applications, Silicon (Si), Germanium (Ge), ZnSe or ZnS often serve as the high-index material, meeting the various requirements referenced above.
In the past, Thorium Fluoride (ThF4) was the preferred low-index material, but its radioactivity has limited its practical uses. Some other fluoride compounds that have low refractive index and exhibit relatively low absorption losses in the IR spectrum (e.g., AlF3, BaF2, SrF2, NaF, LiF, MgF2 and CaF2, etc.) have been used as the low-index layer for certain optical applications.
Problems can arise, however, when attempting to produce high-quality, smooth, optical thin films. The most common problems limiting the use of certain fluoride compounds are: (a) environmental deterioration in humid environments and (b) the tendency to form crystalline layers having rough surfaces/interfaces, which result in losses due to light scattering.
Manufacturers have continued to struggle to produce optical-thin-film multilayer structures that include low-index materials for optical applications, especially for mid-IR wavelengths.
The present invention provides optical-thin-film structures consisting essentially of fluorides as a low-index material, and methods for making such structures. In optical-thin-film structures in accordance with the illustrative embodiment, at least one low-index thin film consists essentially of a major amount (i.e., >50 weight percent) of Barium Fluoride (BaF2) and a minor amount of one or more secondary fluoride compounds.
The secondary fluoride compounds suitable for use in conjunction with embodiments of the invention include those that: (1) reduce the average crystal size of a low-index optical thin film (relative to that of a low-index optical thin film consisting solely of Barium Fluoride), (2) have suitable optical properties for the particular optical application (e.g., refractive index, absorption losses, etc.), and (3) have suitable chemical stability. Fluoride compounds that satisfy requirements (1) through (3) above for a variety of optical applications include, without limitation: CaF2, AlF3, YF3, YbF3, CeF3, ThF4, NaF, LiF, KF, SrF2, and MgF2.
The amount of the secondary fluoride compound—which may include one or more suitable fluoride compounds—is typically in the range of about 1 to about 25 weight percent, as a function of: (1) the particular secondary fluoride compound used, (2) substrate temperature and the temperature of the deposited thin films, and (3) required film thickness, among any other parameters. More typically, the amount of the secondary fluoride will be in the range of about 1 to about 15 weight percent.
Optical-thin-film structures consistent with the present teachings are particularly well-suited for operation at infrared wavelengths in the range of about 1.5 to about 20 microns, and may be configured as an antireflection coating, a high-reflection coating, a long-wavelength-pass filter, a short-wavelength-pass filter, a wide-bandpass filter, and a narrow-bandpass filter, among any other optical devices.
Some embodiments in accordance with the present teachings provide an article comprising an optical-thin-film structure, wherein the optical-thin-film structure comprises alternating thin films of low-index material and high index material, the low-index material having a refractive index less than about 1.7, and the high-index material having a refractive index of at least about 1.7, wherein at least one of the thin films of low-index material consists essentially of a mixture of:
Some other embodiments in accordance with the present teachings provide a method comprising forming a low-index optical thin film by co-evaporating Barium fluoride and a secondary fluoride compound on to a first surface; and forming a high-index optical thin film on the low-index optical thin film.
Layer 102 is a low-index optical thin film consisting essentially of a mixture of Barium Fluoride and one or more other “secondary” fluoride compounds. Layer 104 is a high-index optical thin film, which typically consists of one of Ge, Si, ZnS, or ZnSe.
It is notable that the refractive index of Barium fluoride at 10 microns is about 1.41, and is 1.352 at 14 microns. Moreover, Barium fluoride exhibits low absorption losses over a wide spectral range up to 15 microns (extinction coefficient k=0.0004 at 10 um and k=0.001277 at 14 um). In addition, Barium fluoride is physically hard, and does not easily absorb moisture from the air compared to other fluoride compounds. These properties make Barium fluoride particularly attractive as a candidate for use as the low-index material in optical-thin-film structures for mid-IR applications.
Thin-film deposition of Barium fluoride can be accomplished, for example, by thermal evaporation, electron-beam (E-beam) evaporation, or by using a sputter deposition process in which ions are accelerated onto a Barium fluoride target. When thermal evaporation is used, fluoride deposition rates of over 2 nm/sec can be achieved, and the thin films of multi-layer mirrors can be deposited accurately if a quartz crystal oscillator monitor is used to measure the thickness of the films.
However, a problem arises when depositing Barium fluoride for use in an optical-thin-film structure. In particular, the surface of the deposited Barium fluoride film becomes increasingly rough with (increasing) film thickness, which results in light-scattering losses in the resulting optical structures. This is a consequence of the crystal structure of Barium fluoride, the growth of which generates this roughness.
The present inventors discovered that co-depositing (such as by co-evaporating) one or more secondary fluoride compounds with the Barium fluoride results in a smoother optical thin film. The co-deposition of the secondary fluoride compound reduces the average crystal size in the resulting optical thin film (relative to what it would have been had the optical thin film consisted of 100 percent Barium fluoride). Importantly, the co-deposition can be performed without substantially compromising the refractive index or adhesion properties of the resulting thin film.
In addition to reducing the average crystal size in the deposited thin-film, it is believed that co-deposition of Barium fluoride with other fluoride compounds reduces the grain size of the Barium fluoride. This is because during co-deposition, defects in the crystal structure of Barium fluoride arise due to a difference in crystal shape or a mismatch of lattice constants between Barium fluoride and the secondary fluoride.
As to crystal shape, YF3, for example, has an orthorhombic Pnma space group that is different from that of Barium fluoride. And regarding lattice mismatch, the BaF2 crystal has a lattice constant of 0.62 nm, whereas the CaF2 crystal has a lattice constant of 0.54 nm. In fact, since all other fluorides compounds have a different crystal structure and/or lattice constant than BaF2, they are all suitable for causing defects in the crystal structure of BaF2 and are expected to result in an optical thin film having a smoother surface than BaF2 alone. Expectations aside, surface smoothness is readily determined by simple experimentation.
As a consequence, the usefulness of such secondary fluoride compounds as co-deposition partners for Barium fluoride may ultimately be a function of suitability of the optical properties of such compounds for the optical application of interest (e.g., IR absorption losses in the wavelength region of interest, etc.) Additionally, the secondary fluorides must possess adequate chemical stability. And of course, even if a particular fluoride compound is otherwise suitable based on the aforementioned characteristics, its cost, availability, and/or difficulty of synthesis may remove it from consideration.
Optical thin films have been formed in which Barium fluoride was co-deposited via co-evaporation with (on an individual basis): YF3, YbF3, AlF3, CeF3, CaF2, and ThF4. The resulting optical thin films demonstrated significantly smoother interfaces than pure Barium fluoride films. The results of such experimentation are discussed below for CaF2, AlF3, YF3, and YbF3.
Table I shows the composition of the low-index layer for
For
The smoothness of the low-index optical thin film is also a function of the amount of the secondary fluoride compound(s) that is co-deposited with the Barium fluoride. This can be seen, for example, by comparing
Temperature also plays a role in controlling the roughness of an optical thin film. Cooling of the deposited optical thin films (and the substrate upon which they are deposited) may reduce grain size, thereby improving the smoothness of the deposited optical thin films. Conversely, heating typically generates larger grains and more roughness. When depositing “thin” optical thin films (<0.5 microns) on to substrates at room temperature, it is typically not necessary to control temperature. However, depositing “thick” optical thin films (≥0.5 microns), such as for infrared mirrors and filters, increases the substrate temperature due to radiative heating from the hot evaporation source. This necessitates temperature control, either via active cooling of the substrate during deposition, or by pausing growth during the optical-thin-film deposition process, thereby enabling the materials to cool passively. The substrate temperature should be limited to no more than 100° C. Preferably, the substrate temperature is maintained at less than 50° C., and more preferably at 25° C. or less. Either form (active or passive) of temperature control is important reducing surface roughness as well as strain in an optical-thin-film structure.
To compensate for relatively higher temperatures during deposition, the concentration of the secondary fluoride can be increased. But because many of the secondary fluorides have higher IR absorption than Barium fluoride at wavelengths of interest, it is generally preferable to keep their concentration relatively low, such as 15 weight percent or less, notwithstanding the prospect of further improvements in the smoothness of the optical thin films at higher concentrations.
A further consideration when depositing fluoride optical thin films, particularly in relatively thick multi-layer structures having high-index optical thin films consisting of Germanium or Silicon, is poor adhesion of the (dissimilar) optical thin films to one another due to stress. This stress increases with increasing thickness of the optical thin film, often resulting from the differing coefficients of thermal expansion of the constituents of the multi-layer structure. To mitigate the stress build-up and poor interface adhesion, adhesion-assisting layers have traditionally been included between the high-index and low-index optical thin films. Such a layer is depicted in optical-thin-film optical structure 100′ of
In summary, secondary fluoride compounds suitable for use in conjunction with embodiments of the invention include those that: (1) reduce the average crystal size of a low-index optical thin film (relative to that of a low-index optical thin film consisting solely of Barium Fluoride), (2) have suitable optical properties for the particular optical application, and (3) have suitable chemical stability. Fluoride compounds that satisfy requirements (1) through (3) above for a variety of optical applications include, without limitation: CaF2, AlF3, YF3, YbF3, CeF3, ThF4, NaF, LiF, KF, SrF2, and MgF2.
In accordance with the present teachings, stress mitigation and interface adhesion may be improved via the following techniques.
In some embodiments, a surface treatment, such as ion bombardment or the like is used to improve the adhesion between optical thin films of a multi-layer optical-thin-film structure. In particular, at each interface between hi-index and low-index optical thin films, the surface is cleaned with Argon via ion beam, DC glow discharge, or RF glow discharge. Such bombardment cleans the surface of a deposited optical thin film to: (a) remove any contamination that might accumulate during the transition from one deposition step to the next, and (b) promote covalent bonding between the high-index material (e.g., Ge, Si, etc.) and the low-index fluoride-containing thin films. Using this technique, the thickness of any adhesion-assisting layers may be reduced below 5 nanometers, or these layers may be completely eliminated. Ion bombardment has been shown to prevent delamination of the optical thin films and result in a more robust and durable optical-thin-film structure. In some embodiments, a different surface treatment (e.g., laser ablation, desorption, etc.) is used to improve the adhesion between at least two of the optical thin films of a multi-layer optical-thin-film structure.
Exemplary Optical-Thin-Film Structures.
Optical-thin-film structures 400A, 400B, and 400C in accordance with the present teachings, which are depicted in respective
Optical-thin-film structure 400A includes first Bragg mirror 4081A and second Bragg mirror 4082A separated by optically resonant cavity 410A. Bragg mirror 4081A includes five optical thin films: low-index optical thin films (1021, 1022, and 1023) and high-index optical thin films (1041 and 1042), alternating as previously disclosed. Bragg mirror 4082A includes four optical thin films: low-index optical thin films (1024 and 1025) and high-index optical thin films (1043 and 1044), alternating as previously disclosed. The low-index optical thin films consist of a co-deposited mixture of Barium Fluoride and AlF3. The high-index optical thin films are Germanium. Optically resonant cavity 410A can be comprise any one of a number of high-index materials, such as fused silica, germanium, silicon, zinc selenide, yttrium aluminum garnet (YAG), etc. In some other embodiments, the optically resonant cavity can be other than a solid material, such as a liquid or gas, the latter of which may be under partial vacuum.
Optical-thin-film structure 400B comprises first Bragg mirror 4081B and second Bragg mirror 4082B, which are separated by optically resonant cavity 410B. Bragg mirror 4081B includes four optical thin films: low-index optical thin films (1021 and 1022) and high-index optical thin films (1041 and 1042), alternating as previously disclosed. Bragg mirror 4082B includes four optical thin films: low-index optical thin films (1023 and 1024) and high-index optical thin films (1043 and 1044), alternating as previously disclosed. The low-index optical thin films consist of a co-deposited mixture of Barium Fluoride and AlF3. The high-index optical thin films are Germanium.
In structure 400B, the length of cavity 410B varies in a transverse direction, wherein, in
As in optical-thin-film structure 400B, the length of cavity 410C varies in a transverse direction, wherein, in
In the embodiments depicted in
First optical-thin-film structure 5081 has four optical thin films: low-index optical thin films (1021 and 1022) and high-index optical thin films (1041 and 1042), alternating as previously disclosed. Second optical thin film structure 5082 includes eight optical thin-films: low-index optical thin films (1023, 1024, 1025, and 1026) and high-index optical thin films (1043, 1044, 1045, and 1046), alternating as previously disclosed. In the illustrative embodiment, both first and second optical-thin-film structures 5081 and 5082 include at least some low-index optical thin films consisting essentially of Barium fluoride and AlF3. And the substrate is Silicon, and the high-index optical thin film is Germanium.
As mentioned in conjunction with the discussion of Bragg reflectors, the various high-index and low-index optical thin films are nominally quarter-wave layers, except that in optical assembly 500, the fifth optical thin film 1045 of structure 5082 is a half-wave layer (i.e., thickness=λ/2n). Optical assembly 500 functions as an optical filter of moderate quality factor Q and resolution.
In step S606, query if more optical thin films are to be deposited. If “yes,” then optionally perform steps S607 (ion bombardment) and S608 (deposit adhesion-assisting layer), and then loop back to step S601 to co-deposit a low-index optical thin film on to the just-deposited high-index optical thin film (or adhesion-assisting layer). As appropriate, in some alternative embodiments, the process can begin by depositing a high-index optical thin film, followed by the deposition of a low-index optical thin film.
In summary, an optical-thin-film structure, as depicted and described, comprises at least one low-index optical thin film consisting essentially of Barium fluoride and at least one secondary fluoride compound that reduces the average crystal size of a low-index thin film (relative to that of a low-index optical thin film consisting solely of Barium Fluoride), and at least one high-index optical thin film. Embodiments of an optical-thin-film optical structure in accordance with the present invention may further comprise at least one of the following features, in any (non-conflicting) combination, among other features disclosed herein:
Other than in the examples, or where otherwise indicated, all numbers expressing, for example, quantities of ingredients used in the specification and in the claims are to be understood as being modified in all instances by the term “about.” Accordingly, unless indicated to the contrary, the numerical parameters set forth in the following specification and attached claims are understood to be approximations that may vary depending upon the desired properties to be obtained in ways that will be understood by those skilled in the art. Generally, this means a variation of at least +/−15%.
Also, it should be understood that any numerical range recited herein is intended to include all sub-ranges encompassed therein. For example, a range of “1 to 10” is intended to include all sub-ranges between (and including) the recited minimum value of about 1 and the recited maximum value of about 10, that is, having a minimum value equal to or greater than about 1 and a maximum value of equal to or less than about 10.
It is to be understood that the disclosure describes a few embodiments and that many variations of the invention can easily be devised by those skilled in the art after reading this disclosure and that the scope of the present invention is to be determined by the following claims.
This specification claims priority of U.S. Pat. App. 63/309,098, filed Feb. 11, 2022 and which is incorporated by reference herein.
Number | Date | Country | |
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63309098 | Feb 2022 | US |