This disclosure relates generally to an optical system for splitting light. More particularly, embodiments herein relate to an achromatic optical system for splitting light using a waveguide with a high V number in one dimension and a low V number in another dimension.
Generally, optical systems may employ multiple light sources for use in everyday devices. Although the systems may have multiple light outputs, there may be more light outputs than light sources as the light may be de-multiplexed or split. The optical systems may use light splitting systems that split light emitted by the light sources and may include different components such as de-multiplexers, diffraction gratings, optical splitters. These splitting components may vary from one another in different ways, such as size, optical efficiency, energy efficiency, wavelength dependence or independence, and so forth. In some examples, cascading light splitting systems may be used, but the size of the optical system may increase to an unreasonable size as the systems tend to increase in scale with the number of cascading light splitting stages. In other examples, star splitters may be used, but the free propagation region through which light propagates may cause large optical losses between the input waveguide and the output waveguides. Even though the star splitter may be size appropriate, the optical power loss may be too great to use in certain optical systems and thus a compact, low optical loss optical system may be desirable. In other examples, the light splitting systems may not perform consistently over broad wavelength ranges of light.
Embodiments of the systems, devices, methods, and apparatuses described in the present disclosure are directed to an optical device for splitting or combining light. Also described are systems, devices, methods, and apparatuses directed to splitting light using an optical device based on a star splitter. In some examples, the optical splitter may function as a one by N splitter, insofar as light may be input on an input waveguide and light may be output on any number of output waveguides. The optical splitter may include an input waveguide, a free propagation region, and an array of output waveguides. In some examples, a narrow input waveguide may provide light to the free propagation region, where the input waveguide is narrow enough that the diffraction in the free propagation region may provide for similar optical intensities at far field angles across a wide wavelength range, such as spanning approximately one micron. The input waveguide may have a mode size that is proportional to the wavelength, which may provide for uniform diffraction angles. When most or all of the wavelengths diffract at similar or the same angle, once the light reaches the output waveguides, the light may have similar or the same optical power at each of the output waveguides.
In some examples, the present disclosure describes an optical splitter. The optical splitter may include an input waveguide configured to input a wavelength range of light to a free propagation region, the input waveguide configured to achieve a proportional relationship between mode size and wavelength across the wavelength range of light at an input edge of the free propagation region, the free propagation region having the input edge and an output edge, optically coupled to the input waveguide on the input edge, and configured to receive the wavelength range of light from the input waveguide, and an array of output waveguides optically coupled to the output edge of the free propagation region, wherein each waveguide of the array of output waveguides is positioned at a predetermined angle (e.g., approximately normal) to a local phase front of light received by each waveguide from the free propagation region. In some examples, the input waveguide has a high V number in a first dimension and a low V number in a second dimension, a center channel output waveguide of the array of output waveguides has a narrower width than an outer channel output waveguide of the array of output waveguides, the input waveguide causes light to diffract at a same diffraction across the wavelength range of light, and multiple output waveguides of the array of output waveguides are uniformly spaced. Additionally, at least two of the array of output waveguides have different widths and at least some of the array of output waveguides have non-uniformly spacing between one another.
In some examples, the input waveguide weakly confines light in a diffraction direction of the free propagation region. In some examples, a width of at least one of the array of output waveguides depends, at least in part, on an intensity of diffracted light in the free propagation region. In some examples, a first dimension of the input waveguide depends, at least in part, on a first V number of the input waveguide, a second dimension of the input waveguide depends, at least in part, on a second V number of the input waveguide, and the first V number is greater than the second V number. In some examples, an input waveguide mode, as measured in a first dimension, matches a waveguide mode of the free propagation region, thereby reducing optical loss. In some examples, light coupled into each of the array of output waveguides has a same power for each waveguide across the wavelength range of light. Additionally, the input waveguide is a first input waveguide, the optical splitter may include a second input waveguide positioned adjacent to the first input waveguide and optically coupled to the free propagation region, and the first and second input waveguides are symmetrically positioned to input light to the free propagation region.
In some examples, the present disclosure describes an optical splitter. The optical splitter may include an input waveguide having a high V number in a first dimension, a low V number in a second dimension and configured to input a wavelength range of light, a slab waveguide with an input edge and an output edge, the slab waveguide optically coupled to the input waveguide and configured to receive light from the input waveguide, and an array of output waveguides positioned across the output edge of the slab waveguide such that some of the output waveguides are center channel output waveguides and others of the output waveguides are outer channel output waveguides, wherein each of the array of output waveguides are arranged to receive light having approximately a same optical power. In some examples, the input waveguide has a high V number in a vertical dimension and a low V number in a horizontal dimension, a mode size of the input waveguide is proportional to a wavelength in the wavelength range of light, in the slab waveguide, a diffraction angle is the same across the wavelength range of light, and a center channel spacing is uniform for center channel output waveguides of the array of output waveguides and an outer channel spacing is half as large as the uniform spacing for outer channel output waveguides. In some examples, the input waveguide may be a strip waveguide and the array of output waveguides are strip waveguides. In some examples, multiple waveguides of the array of output waveguides have non-uniform widths and at least one waveguide width is related to a local phase front at the output waveguide of the array of output waveguides.
In some examples, the array of output waveguides are uniformly spaced apart from one another and a center channel output waveguide width is narrower than a width of an outside channel output waveguide, thereby equalizing an amount of optical power received by each output waveguide of the array of output waveguides. In some examples, the wavelength range of light is one micron. In some examples, an optical power incident upon the slab waveguide is higher in the center channels of the array of output waveguides and decreases in optical power in the outer channels of the array of output waveguides, multiple center channel output waveguides of the array of waveguides are narrower than outer channel output waveguides, thereby receiving uniform optical power across the array of output waveguides, and the multiple center channel output waveguides are spaced apart from one another by a same distance. In some examples, an outer channel output waveguide of the array of output waveguides is half a width of an adjacent channel output waveguide width and an outer channel spacing between the outer channel output waveguides is half the channel spacing of the adjacent channel output waveguides.
In some examples, the present disclosure describes an optical splitter. The optical splitter may include a strip waveguide for inputting light across a wavelength range of light, a slab waveguide configured to receive the wavelength range of light from the strip waveguide, and an array of output waveguides positioned to receive the wavelength range of light from the slab waveguide and a same amount of optical power of light is received by each output waveguide of the array of output waveguides; where a strip waveguide mode size is proportional to a wavelength in the wavelength of light and a diffraction angle of light in the slab waveguide is similar across the wavelength range of light. In some examples, a spacing between a first output waveguide and an adjacent second output waveguide of the array of output waveguides is non-uniform and depends on the optical power received by the first output waveguide and the adjacent second output waveguide, a phase front of light of the slab waveguide has a cylindrical phase front, each waveguide of the array of output waveguides is positioned normal to a local phase front of light in the slab waveguide, and the array of output waveguides are strip waveguides. In some examples, the strip waveguide has a high V number in a first dimension and a low V number in a second dimension and a strip waveguide mode in the first dimension matches a waveguide mode of the slab waveguide, thereby reducing optical loss. Additionally, a non-uniform spacing between each of the output waveguides of the array of output waveguides is based on the optical power received by each of the output waveguides such that each output waveguide receives a uniform optical power of light across the wavelength range of light spanning one micron. Further, the array of output waveguides have varying waveguide widths, thereby equalizing an optical power received from the slab waveguide.
In addition to the example aspects and embodiments described above, further aspects and embodiments will become apparent by reference to the drawings and by study of the following description.
The use of cross-hatching or shading in the accompanying figures is generally provided to clarify the boundaries between adjacent elements and also to facilitate legibility of the figures. Accordingly, neither the presence nor the absence of cross-hatching or shading conveys or indicates any preference or requirement for particular materials, material properties, element proportions, element dimensions, commonalities of similarly illustrated elements, or any other characteristic, attribute, or property for any element illustrated in the accompanying figures.
It should be understood that the proportions and dimensions (either relative or absolute) of the various features and elements (and collections and groupings thereof) and the boundaries, separations, and positional relationships presented between them, are provided in the accompanying figures merely to facilitate an understanding of the various embodiments described herein and, accordingly, may not necessarily be presented or illustrated to scale, and are not intended to indicate any preference or requirement for an illustrated embodiment to the exclusion of embodiments described with reference thereto.
Reference will now be made in detail to representative embodiments illustrated in the accompanying drawings. It should be understood that the following description is not intended to limit the embodiments to one preferred embodiment. To the contrary, it is intended to cover alternatives, modifications, and equivalents as can be included within the spirit and scope of the described embodiments as defined by the appended claims.
Directional terminology, such as “top”, “bottom”, “upper”, “lower”, “above”, “below”, “beneath”, “front”, “back”, “over”, “under”, “left”, “right”, and so forth, is used with reference to the orientation of some of the components in some of the figures described below. Because components in various embodiments can be positioned in a number of different orientations, directional terminology is used for purposes of illustration only and is in no way limiting. The directional terminology is intended to be construed broadly, and therefore should not be interpreted to preclude components being oriented in different ways.
As used herein, the term “abutting” means that two elements share a common boundary or otherwise contact one another, while the term “adjacent” means that two elements are near one another and may (or may not) contact one another. Thus, elements that are abutting are also adjacent, although the reverse is not necessarily true. Two elements that are “coupled to” one another may be permanently or removably physically coupled to one another and/or operationally or functionally coupled to one another. Additionally, two elements that are “optically coupled” to one another may allow light to pass from one element to the other element.
In the following description of examples, reference is made to the accompanying drawings in which it is shown by way of illustration specific examples that can be practiced. It is to be understood that other examples can be used and structural changes can be made without departing from the scope of the various examples.
Generally, optical systems may employ multiple light sources emitting light that may be split, so that the number of output ports may be greater than the number of light sources. Various light splitting systems may be used to split light emitted by light sources and may include different components such as de-multiplexers, diffraction gratings, optical splitters, and so forth, and may vary from one another in different ways, such as size, optical efficiency, energy efficiency, wavelength dependence or independence, any combination thereof and so forth.
In some examples, multi-wavelength light may be split using cascading stages in a light splitting system and the light splitting system size may increase with the number of cascading light splitting stages. That is, the more light splitting stages that are used, the larger the light splitting system becomes. Because the number of cascading light splitters scale with the number of output ports, these light splitting systems may become unreasonably large and may not be easily incorporated into the overall optical system. Further, the cascading light splitters may introduce undesirable optical beating into the overall optical system.
In some examples, light may be split using a multi-mode interferometer. Generally, multi-mode interferometers may be smaller than cascading splitters and may perform consistently over small wavelength ranges, such as 10 nanometers to 50 nanometers, but may not be suitable for consistent performance over broadband wavelength ranges that may span approximately one micron.
In other examples, a star splitter may be used to split light in combination with an input waveguide, a free propagation region, and output waveguides. The input waveguide typically ends at the free propagation region where there is little confinement in the plane of the propagation region. The size of the star splitter may not scale with the number of output ports as another output waveguide may be added without causing a significant an increase in the footprint. However, the free propagation region through which light propagates may cause large optical losses between the input waveguide and the output waveguides. Even though the star splitter may be size appropriate, the optical power loss may be too great to use in certain optical systems and thus a compact, low optical loss optical system may be desirable. Additionally, star splitters may exhibit wavelength dependent performance and also may not be suitable for consistent performance over broadband wavelength ranges that may span approximately one micron.
In some examples, by starting with a narrower input waveguide than is typically used in a star splitter, the light provided to the free propagation region may then expand or spread out. In some examples, the narrower the input waveguide, the faster the light may diffract in the free propagation region. The diffraction in the free propagation region may yield similar optical intensities at far field angles across a wide wavelength range, such as spanning approximately one micron. When most or all of the wavelengths diffract at similar angles or the same angle, once the light reaches the output waveguides, the light may have similar optical power at most or all of the wavelengths at each of the output waveguides. It may be understood that when the term “same” is used herein (e.g., same angle, same optical power, same diffraction, same diffraction angle, and so forth, that the term “same” may mean in addition to being the same: similar enough to not significantly affect performance, and/or the same within standard measurement tolerances. Further, it may be understood that when the term “approximately” is used herein, this term may include a five to ten percent variation as reasonably allowed within the determined specification.
Disclosed herein is an optical splitter that includes an input waveguide, a free propagation region, and an array of output waveguides. The input waveguide may achieve a proportional relationship between mode size and a wavelength of light in the wavelength range of light and is optically coupled to the free propagation region. The free propagation region may have an input and output edge and may receive the wavelength range of light from the input waveguide; the input waveguide may be optically coupled to the input edge of the free propagation region. The input waveguide may be narrow enough that the diffraction angle is the same across the broad wavelength range of light. Each of the waveguides may be optically coupled to an output edge of the free propagation region and positioned across the output edge of the free propagation region, where each of the multiple output waveguides is positioned at a predetermined angle (e.g., approximately normal or any other suitable angle) to a local phase front of light of the wavelength range of light. The phase front is the phase of a propagating wave front. In some embodiments, the proportional relationship between the mode size and wavelength need not be exactly proportional. The relationship between mode size and wavelength may be plus or minus ten percent relative to a proportional relationship. As used herein, the term “proportional” encompasses not only a relationship where one object, element, or attribute (collectively, “object”) varies directly with another or according to a particular mathematical function, but also includes instances where an object change is primarily dependent on another. Put another way, one object is proportional to another when its variance is within 10% of a direct or mathematical variance with respect to the other object.
In some examples, the input waveguide may have a high V number in a vertical dimension and a low V number in a horizontal dimension to match the waveguide mode of the free propagation region of the optical splitter. Generally, the high V number (e.g., vertical dimension) may result in low optical loss, whereas the low V number (e.g., horizontal dimension) may result in wavelength independence. A high V number in a vertical dimension and a low V number in a horizontal dimension to match the waveguide mode of the free propagation region of the optical splitter may reduce optical loss. In some examples, the width and spacing may vary (e.g, be non-uniform) between the output waveguides in the array in order to provide uniform optical power coupling and to reduce a total optical loss of the system. Additionally, the center channel output waveguides may be narrower in width than the outer channel output waveguides. Further, spacing between the output waveguides may be uniform or may vary based on the optical power of the light coupled to the output waveguides.
These and other embodiments are discussed below with reference to
The input 102 may be an input waveguide that provides input light to the one by four splitter 104. The input light may be provided by a light source, which may be connected to or otherwise integrated into a photonics device. In some examples, the photonics device may include more than one light source, such as lasers, light emitting diodes, semiconductor lasers, coherent light sources, semi-coherent light sources, any combination thereof, and so forth. In some examples, the photonics device is a device with photonics and/or optical functionality and components. The photonics device may include the optical splitters.
In the first splitting stage, the one by four splitter 104 may equally split and output light among the four intermediate light paths 106a-106d. In some examples, there may be optical loss associated with each splitting stage. In some examples, the intermediate light paths 106a-106d may be waveguides optically coupled to, and receiving light from, the one by four splitter 104. The intermediate light paths 106a-106d also may be optically coupled to the one by two splitters 108a-108d and may provide light to the one by two splitters 108a-108d. Each of the one by two splitters 108a-108d may provide light outputs 112a-112d. The one by two splitter 108a may provide two light outputs 112a, the one by two splitter 108b may provide two light outputs 112b, and so forth. As shown in
Also, the one by eight splitter 100 may increase in size with each additional splitting stage. For example, instead of a one by four splitter 104 being used, the input 102 may be provided to a one by two splitter, and then for each of those two outputs, another set of one by two splitters may be used to achieve the four intermediate outputs. Because an additional splitting stage is added in this described example, this example system may be larger than the system illustrated in
The input waveguide 200 may generate a mode size that achieves a proportional relationship to the wavelength by weakly confining the input waveguide 200 in the plane of a substrate or in the horizontal dimension. As illustrated in
The physical dimensions of the input waveguide 200 may be configured based on the first and second target V numbers and the wavelength(s) of light transmitted by the input waveguide. The V numbers and the wavelengths of light are used to generate a mode size, as discussed herein. In some examples, the input waveguide 200 may have a propagation region that is approximately two to five microns in a first dimension (e.g., a vertical dimension) and less than a micron in a second dimension (e.g., a horizontal dimension). In one example, the input waveguide may be three microns in the vertical dimension and 0.6 microns in the horizontal dimension. These dimensions may be used for an input waveguide of rectangular cross-section that transmits light having wavelengths from 1.4 microns to 2.4 microns, for example.
The V number is a normalized frequency and determines the number of modes a fiber can carry. As used herein “high V” and “low V” are relative terms. Specifically, a high V number is one that supports multiple modes of light, whereas a low V number is one that supports a single mode of light. Because the devices described here are configured to work across a range of wavelengths, it should be appreciated that high and low V numbers in these contexts are intended to apply to single or multi-mode light across this range of wavelengths. Accordingly, the actual values for a given waveguide are dependent on the target wavelength range. Further, given these wavelengths of light and the aforementioned dimensions of the input waveguide, the first (or “high”) V number is 3 or greater and the second (or “low”) V number is less than 3. Many embodiments may use this same cutoff even if their dimensions differ, e.g., a high V number is 3 or greater while a low V number is less than 3. In other embodiments, 3 may be a low V number rather than a high V number. Generally for many embodiments, the cutoff between a high V number and a low V number occurs where the light transitions from single mode light to multimode light, and may vary with the wavelengths of light propagating through the waveguide, as well as the dimension of the waveguide. Thus, the input waveguide may have a low V number with respect to a first axis and a high V number with respect to a second axis, for example where the dimension of the waveguide is smaller along the first axis but larger along the second axis.
Because the waveguide may be smaller than the wavelength of light along a short axis of the plane of the wafer (e.g., the horizontal dimension, as shown in
The input waveguide 200 geometry, as depicted, has a high V number in a first dimension, (here, a vertical dimension) and a low V number in a second dimension, (here, a horizontal dimension). Because the input waveguide 200 has a high V number in the vertical dimension and the low V number in the horizontal dimension, the input waveguide mode of light may match the waveguide mode of the free propagation region of the optical splitting device, which may reduce optical loss. The low V number results in achieving a proportional relationship between the mode size and the wavelength and for an input waveguide that obeys the high index approximation, the high V number dimension (e.g., vertical dimension) defines a common mode size in a single axis for all wavelengths with a high V number.
The specific examples used herein are provided for explanatory purposes only. The optical splitter 300 may produce approximately uniform power over all the output waveguides and across a wavelength range of light spanning approximately one micron, all while maintaining a relatively small form factor. Additionally, in
The optical splitter 300 may include an input waveguide 305, a free propagation region 310, and multiple output waveguides 315a-315h. The free propagation region 310 may be formed from similar materials as the input waveguide 305 and multiple output waveguides 315a-315h. In some examples, the free propagation region 310 as well as the input waveguide 305 and the output waveguides 315a-315h may be surrounded by a cladding region 320, which may be an oxide material, such as silicon dioxide, or any other dielectric material that provides the same optical confining functionality. The cladding region 320 may extend beyond the depicted boundaries in
In some examples, the input waveguide 305 may be optically coupled to the free propagation region 310, may provide light to the free propagation region 310, and may terminate at the free propagation region 310. The light propagating through the input waveguide may be a broad wavelength range of light that may span approximately one micron. The free propagation region 310 may be configured to receive the wavelength range of light from the input waveguide 305; this light may freely propagate and diffract in the free propagation region 310. Generally, the narrower the input waveguide 305, the faster the light may diffract or spread out in the free propagation region 310. As previously mentioned with reference to
In some examples, the input waveguide 305 may be a strip waveguide and the output waveguides 315a-315h may be strip waveguides as well. In some examples, the output waveguides 315a-315h may instead be rib waveguides or some combination of strip and rib waveguides. Additionally, the free propagation region 310 may be a slab waveguide. It may be understood that all of the waveguides may be surrounded by a low-index cladding region to confine light to the waveguides. Generally, the waveguides described herein may include a core or propagation region, with cladding layers on both sides of the propagation region. Further, the propagation region of a waveguide is distinct from the free propagation region of the optical splitter as the free propagation region is a region where light may diffract and spread out.
Once the light passes from the input waveguide 305 to the free propagation region 310, it may diffract at about the same angle and form an approximately Gaussian diffraction wave front that may be reproduced similarly at all wavelengths. The diffracting light in the free propagation region 310 may propagate to form approximately the same (or the same) far field angle across the broad wavelength range. When the different wavelengths of light of the wavelength range diffract at approximately the same angle and once the light reaches the output waveguides, each of the waveguides may output light having approximately the same or the same optical power. By providing a mode size that may be proportional to the wavelength, the far field angle may become independent of the wavelength. In some examples, the input waveguide mode in a vertical dimension may approximately match the waveguide mode of the free propagation region 310, thereby reducing optical loss.
In some examples, the light may diffract at the same angle for all constituent wavelengths by producing a waveguide mode size that depends on and that is proportional to the wavelength, thus providing far field angles that may be independent of the wavelength of light. It may be understood that a waveguide mode size is a mode size that results from light passing through the waveguide. In some examples, by using an input waveguide 305 with a high V number in a vertical dimension and a low V number in a horizontal dimension (or vice versa depending on an orientation of the waveguide), the far field angles may be independent of wavelength as described with reference to
In some examples, the free propagation region 310 may include an input edge 380 and an output edge 381, where the input waveguide may be optically coupled to the input edge 380. The output waveguides 315a-315h of the optical splitter 300 may be coupled to the output edge 381 of the free propagation region 310. Additionally, the multiple output waveguides 315a-315h may be each positioned at a respective predetermined angle (e.g., approximately normal or any other suitable angle) to a local phase front of light. In the variation of free propagation region 310 shown in
The position, width, and angle of a given output waveguide collectively impact the amount of light coupled into the output waveguide, and as such each may be selected to achieve a given light coupling to a particular output waveguide. For example, each waveguide may preferably be positioned normal to the local phase front to increase the amount of light and optical power coupling into the output waveguide, although it should be appreciated that other angles may be albeit with increased loss for an otherwise identical waveguide. In some examples, the array of waveguides 315a-315h may preferably be positioned along a circular curve (e.g., centered on where the input waveguide meets the free propagation region), such that each waveguide is positioned along the same phase front. It should be appreciated that the array of waveguides 315a-315h may be positioned along other curves, provided that losses associated with these other curves are acceptable and within the overall system specifications. As depicted in
As shown in
In some examples, the total system efficiency may be approximately the same across all the wavelengths of light, and the output waveguides have the same power or approximately the same power across all the wavelengths of light.
In some instances, the output waveguides 415a-415g may be configured so that the light received by the outcouplers 430a-430g may have different phases. That is, the output waveguides 415a-415g may provide light with different phases 425a-425g to outcouplers 430a-430g. Put another way, the output waveguides 415a-415g may provide light with different group delays. The outcouplers 430a-430g are used for explanatory purposes only, as the light from the output waveguides 430a-430g may be provided to any type of optical element, such as a prism, a mirror, a lens, a collimator, any combination thereof, and so forth. In some examples, the output waveguides 430a-430g may provide light for measurement of a sample or to a reference detector for monitoring light. In some examples, the waveguides may be divided into groups so that the light from multiple output waveguides may be received by one outcoupler. In this example, the grouped output waveguides may positioned closer to one another within the group than to the corresponding outcoupler(s). By grouping the output waveguides, this may create the effect of a “single output” for each waveguide group. In still other embodiments, some of the output waveguides may provide different phases from one another, however the output waveguides within the grouped output waveguides may provide light of the same phase to the corresponding outcoupler(s).
When the output waveguides are discussed above as being positioned normal to the local phase front, it should be appreciated that the waveguide is positioned formal to the local phase front at one point in space (since it is not possible for the waveguide to be normal to multiple points on a curve simultaneously). This point may be selected to help minimize loss (e.g., by positioning the waveguide to be normal to an average tilt of the local phase front encompassed by the waveguide), but may not be able to address all the losses caused by local phase front curvature. This is magnified as the output waveguide grows, and thus may disproportionally impact the outer waveguides. For example, in the output waveguides shown in
The optical splitter 450 may mitigate issues described with reference to
The outer channel output waveguide 455a1 may output light along light path 465a1 to outcoupler 470a1, and the outer channel output waveguide 455a2 may output light along light path 456a2 to outcoupler 470a2. The outcouplers 470a1, 470a2 may be positioned closer to one another than outcouplers 470c, 470d that receive light from inner channel output waveguides. The outer channel outcouplers 470a1, 470a2 may be positioned close enough that the two portions of launched light may function as a single portion of light from a single inner channel outcoupler, such as outcoupler 470d. Due to the size and spacing of the outer channel output waveguides 455a1, 455a2, light from these waveguides may be launched by the two outcouplers 470a1 and 470a2 as though it is unitary. The smaller outer channel output waveguides 455a1, 455a2 may launch light having the same (or nearly same) phase close to one another, via the outer channel outcouplers. Thus, the optical power of the launched light may combine and so be the same as, or similar to, optical power of light launched by the single outer channel output waveguide 415a of
Although the optical splitter 400 of
In some examples, the spacing between the output waveguides 455a1-455g1 of FIG. 4B may have uniform spacing or half uniform spacing. In some examples, the center channel spacing between the center channel output waveguides and the outer channel output waveguides may be different from one another to mitigate the non-uniform optical power distribution of the phase front of light. The center channel output waveguides may have uniform center channel spacing as the phase front may be close to that of a plane wave, whereas the outer channel spacing between the outer channel output waveguides 455a1 and 455a2 and between 455b1 and 455b2 may be half the uniform spacing of the center channel output waveguides. The spacing of the outer channel output waveguides may be half the uniform spacing because the outer channel output waveguides 455a1 and 455a2 may be half the size of the center channel output waveguide 455d. Further, because the output waveguides 455a1 and 455a2 may be treated as a single channel output, the spacing may be smaller and may be half the uniform spacing because the output waveguides are half the size and the two output waveguides are used in the same spacing as a single channel.
In some embodiments, the outer channel output waveguides 455a1 and 455a2 may be half the width of the adjacent outer channel output waveguides 455b1 and 455b2. Similarly, the outer channel waveguides 455g1 and 455g2 may be half the width of the adjacent outer channel waveguides 455f1 and 455f2. Additionally, the summed power received by the outer channel output waveguides 455a1 and 455a2 may receive a similar amount of optical power as the power received by other single waveguides (such as adjacent outer channel output waveguides 455b1 and 455b2) due to the width variation between the outer channel output waveguides 455a1 and 455a2 and the adjacent outer channel output waveguides 455b1 and 455b2.
In some embodiments, the grouped outer channel output waveguides 455a1 and 455a2 also may collect the same amount of light as one of the adjacent outer channel output waveguides 455b1, 455b2. Further, the grouped outer channel output waveguides 455a1 and 455a2 may collect the same amount of light (e.g., optical power) as other grouped outer channel output waveguides. The light provided by each of the grouped outer channel output waveguides 455a1, 455a2 may or may not be evenly distributed between the outer channel output waveguides 455a1, 455a2. Similarly, in any group of output waveguides, the light (e.g., optical power) provided by each of the output waveguides in the group of output waveguides may or may not be evenly distributed between each of the output waveguides in the group. Additionally, each output waveguide in the grouped outer channel output waveguides 455a1, 455a2 may be positioned to collect light of the same phase. Generally, each output waveguide within a group of output waveguides may be positioned with respect to the free propagation region so that the collected light may be the same phase as other output waveguides within the group.
In
In
In some examples, the first and second input waveguides 605a and 605b may have similar waveguide parameters as one another, and may not differ from the single input waveguides as described with reference to
The first input waveguide 605a may be positioned as close to the second input waveguide 605b as fabrication processes allow to reduce any optical loss associated with the addition of the second input waveguide. Generally, the first and second input waveguides 605a and 605b may be positioned adjacent to one another and symmetrically about the position where a single input waveguide may be positioned in a single input waveguide optical splitter. In other examples, the first and second input waveguides 605a, 605 may not be symmetrically positioned to where the single input waveguide may be typically positioned.
Further, although process steps or method steps can be described in a sequential order, such processes and methods can be configured to work in any suitable order. In other words, any sequence or order of steps that can be described in the disclosure does not, in and of itself, indicate a requirement that the steps be performed in that order. Further, some steps may be performed simultaneously despite being described or implied as occurring non-simultaneously (e.g., because one step is described after the other step). Moreover, the illustration of a process by its description in a drawing does not imply that the illustrated process is exclusive of other variations and modification thereto, does not imply that the illustrated process or any of its steps are necessary to one or more of the examples, and does not imply that the illustrated process is preferred.
Representative applications of methods and apparatuses according to the present disclosure are described in this section. These examples are being provided solely to add context and aid in the understanding of the described examples. It will thus be apparent to one skilled in the art that the described examples may be practiced without some or all of the specific details. Other applications are possible, such that the following examples should not be taken as limiting.
Although the disclosed examples have been fully described with reference to the accompanying drawings, it is to be noted that various changes and modifications will become apparent to those skilled in the art. Such changes and modifications are to be understood as being included within the scope of the disclosed examples as defined by the appended claims.
This application is a nonprovisional of, and claims the benefit under 35 U.S.C. 119(e) of, U.S. Provisional Patent Application No. 63/083,691, filed Sep. 25, 2020, the content of which are incorporated by reference as if fully disclosed herein.
Number | Name | Date | Kind |
---|---|---|---|
4934775 | Koai | Jun 1990 | A |
5287376 | Paoli | Feb 1994 | A |
5488678 | Taneya | Jan 1996 | A |
5524156 | Van Der Tol | Jun 1996 | A |
5544268 | Bischel | Aug 1996 | A |
5586206 | Brinkman | Dec 1996 | A |
5644667 | Tabuchi | Jul 1997 | A |
5647036 | Deacon | Jul 1997 | A |
5652817 | Brinkman | Jul 1997 | A |
5664032 | Bischel | Sep 1997 | A |
5708674 | Berrnink | Jan 1998 | A |
5718989 | Aoki | Feb 1998 | A |
5724463 | Deacon | Mar 1998 | A |
5742631 | Paoli | Apr 1998 | A |
5790720 | Marcuse | Aug 1998 | A |
5818989 | Nakamura | Oct 1998 | A |
5835458 | Bischel | Nov 1998 | A |
5850411 | Major, Jr. | Dec 1998 | A |
5911018 | Bischel | Jun 1999 | A |
5912997 | Bischel | Jun 1999 | A |
5915165 | Sun | Jun 1999 | A |
5978524 | Bischel | Nov 1999 | A |
6014390 | Joyner | Jan 2000 | A |
6078704 | Bischel | Jun 2000 | A |
6118908 | Bischel | Sep 2000 | A |
6122042 | Wunderman et al. | Sep 2000 | A |
6141465 | Bischel | Oct 2000 | A |
6167169 | Brinkman | Dec 2000 | A |
6330378 | Forrest | Dec 2001 | B1 |
6393185 | Deacon | May 2002 | B1 |
6415080 | Sappey et al. | Jul 2002 | B1 |
6522794 | Bischel | Feb 2003 | B1 |
6594409 | Dutt et al. | Jul 2003 | B2 |
6628686 | Sargent | Sep 2003 | B1 |
6657723 | Cohen | Dec 2003 | B2 |
6674949 | Allan et al. | Jan 2004 | B2 |
6795622 | Forrest | Sep 2004 | B2 |
6803604 | Takahashi et al. | Oct 2004 | B2 |
6842545 | Lackritz et al. | Jan 2005 | B2 |
6882758 | Betty | Apr 2005 | B2 |
6892449 | Brophy et al. | May 2005 | B1 |
6903820 | Wang | Jun 2005 | B2 |
6934447 | Kim | Aug 2005 | B2 |
6940182 | Hilton et al. | Sep 2005 | B2 |
6947639 | Singh | Sep 2005 | B2 |
6952504 | Bi | Oct 2005 | B2 |
6954568 | Liu | Oct 2005 | B2 |
6987906 | Nakama et al. | Jan 2006 | B2 |
7031568 | Laming et al. | Apr 2006 | B2 |
7054517 | Mossberg | May 2006 | B2 |
7058245 | Farahi | Jun 2006 | B2 |
7079715 | Kish | Jul 2006 | B2 |
7149387 | Balakrishnan et al. | Dec 2006 | B2 |
7151635 | Bidnyk et al. | Dec 2006 | B2 |
7189011 | Harker | Mar 2007 | B2 |
7203401 | Mossberg | Apr 2007 | B2 |
7203426 | Wu et al. | Apr 2007 | B2 |
7209611 | Joyner | Apr 2007 | B2 |
7245379 | Schwabe | Jul 2007 | B2 |
7263394 | Wang | Aug 2007 | B2 |
7283694 | Welch | Oct 2007 | B2 |
7314451 | Halperin et al. | Jan 2008 | B2 |
7324195 | Packirisamy et al. | Jan 2008 | B2 |
7327918 | Yamazaki et al. | Feb 2008 | B2 |
7366364 | Singh | Apr 2008 | B2 |
7366421 | Cho et al. | Apr 2008 | B2 |
7447393 | Yan | Nov 2008 | B2 |
7460742 | Joyner | Dec 2008 | B2 |
7477384 | Schwabe | Jan 2009 | B2 |
7483599 | Dominic et al. | Jan 2009 | B2 |
7526007 | Chua et al. | Apr 2009 | B2 |
7558301 | Lin et al. | Jul 2009 | B2 |
7595879 | Wang | Sep 2009 | B2 |
7680364 | Nilsson | Mar 2010 | B2 |
7720328 | Yan | May 2010 | B2 |
7831298 | Wang | Nov 2010 | B1 |
7840108 | Miyadera | Nov 2010 | B2 |
7876983 | Doerr | Jan 2011 | B2 |
7885302 | Eberhard | Feb 2011 | B2 |
7885492 | Welch | Feb 2011 | B2 |
7970458 | Norris et al. | Jun 2011 | B2 |
7974504 | Nagarajan et al. | Jul 2011 | B2 |
7999938 | Wang | Aug 2011 | B2 |
8222084 | Dallesasse et al. | Jul 2012 | B2 |
8300994 | Welch et al. | Oct 2012 | B2 |
8411260 | Feng | Apr 2013 | B1 |
8498681 | Wang et al. | Jul 2013 | B2 |
8559775 | Babie et al. | Oct 2013 | B2 |
8564784 | Wang et al. | Oct 2013 | B2 |
8724100 | Asghari et al. | May 2014 | B1 |
8920332 | Hong et al. | Dec 2014 | B2 |
8983250 | Black et al. | Mar 2015 | B2 |
9020004 | Jeong | Apr 2015 | B2 |
9031412 | Nagarajan | May 2015 | B2 |
9052447 | Luo et al. | Jun 2015 | B2 |
9110259 | Black | Aug 2015 | B1 |
9135397 | Denyer et al. | Sep 2015 | B2 |
9176282 | Pottier | Nov 2015 | B2 |
9217669 | Wu et al. | Dec 2015 | B2 |
9348154 | Hayakawa | May 2016 | B2 |
9370689 | Guillama et al. | Jun 2016 | B2 |
9395494 | Krishnamurthi et al. | Jul 2016 | B2 |
9405066 | Mahgerefteh | Aug 2016 | B2 |
9543736 | Barwicz et al. | Jan 2017 | B1 |
9620931 | Tanaka | Apr 2017 | B2 |
9643181 | Chang | May 2017 | B1 |
9678012 | Rothberg et al. | Jun 2017 | B2 |
9759865 | Lin | Sep 2017 | B1 |
9766370 | Aloe et al. | Sep 2017 | B2 |
9784679 | Rothberg et al. | Oct 2017 | B2 |
9804027 | Fish et al. | Oct 2017 | B2 |
9817296 | Sharkawy et al. | Nov 2017 | B2 |
9829631 | Lambert | Nov 2017 | B2 |
9869816 | Ishikura et al. | Jan 2018 | B2 |
9880352 | Florjanczyk et al. | Jan 2018 | B2 |
9882073 | Krasulick et al. | Jan 2018 | B2 |
9943237 | Baker et al. | Apr 2018 | B2 |
9948063 | Caneau et al. | Apr 2018 | B2 |
10009668 | Liboiron-Ladouceur | Jun 2018 | B2 |
10126498 | Marcuse | Nov 2018 | B1 |
10132996 | Lambert | Nov 2018 | B2 |
10238351 | Halperin et al. | Mar 2019 | B2 |
10285898 | Douglas et al. | May 2019 | B2 |
10310196 | Hutchison | Jun 2019 | B2 |
10359571 | Horth | Jul 2019 | B2 |
10411433 | Weber | Sep 2019 | B2 |
10429597 | ten Have et al. | Oct 2019 | B2 |
10520672 | Ma et al. | Dec 2019 | B2 |
10529003 | Mazed | Jan 2020 | B2 |
10578806 | Lamponi et al. | Mar 2020 | B2 |
10687718 | Allec et al. | Jun 2020 | B2 |
10852492 | Vermeulen et al. | Dec 2020 | B1 |
10901148 | Ma et al. | Jan 2021 | B2 |
10935726 | Lee | Mar 2021 | B1 |
10976489 | Jou et al. | Apr 2021 | B2 |
11022522 | Piazza et al. | Jun 2021 | B2 |
11064592 | Bismuto et al. | Jul 2021 | B1 |
11079542 | Fertig et al. | Aug 2021 | B2 |
11079547 | Trita | Aug 2021 | B2 |
11131809 | Villafranca Velasco | Sep 2021 | B2 |
11231319 | Tu et al. | Jan 2022 | B1 |
11280960 | Qi et al. | Mar 2022 | B2 |
11320720 | Puckett et al. | May 2022 | B2 |
11480731 | Liu et al. | Oct 2022 | B2 |
11500154 | Tu et al. | Nov 2022 | B1 |
11506535 | Tu et al. | Nov 2022 | B1 |
11561346 | Tu | Jan 2023 | B2 |
11630262 | Shin et al. | Apr 2023 | B2 |
11644619 | Qi et al. | May 2023 | B2 |
20020114572 | Bouda | Aug 2002 | A1 |
20030091265 | Lin et al. | May 2003 | A1 |
20030133663 | Orignac et al. | Jul 2003 | A1 |
20040126117 | Lo et al. | Jul 2004 | A1 |
20040131313 | Van Weerden | Jul 2004 | A1 |
20050053112 | Shams-Zadeh-Amiri | Mar 2005 | A1 |
20050063431 | Gallup et al. | Mar 2005 | A1 |
20050196102 | Yamazaki | Sep 2005 | A1 |
20050207702 | Yamazaki | Sep 2005 | A1 |
20060002443 | Farber et al. | Jan 2006 | A1 |
20060188198 | Charters | Aug 2006 | A1 |
20080044128 | Kish et al. | Feb 2008 | A1 |
20080266639 | Melloni et al. | Oct 2008 | A1 |
20080310470 | Ooi et al. | Dec 2008 | A1 |
20120002924 | Okayama | Jan 2012 | A1 |
20140029943 | Mathai et al. | Jan 2014 | A1 |
20150104130 | Anderson et al. | Apr 2015 | A1 |
20160224750 | Kethman et al. | Aug 2016 | A1 |
20170164878 | Connor | Jun 2017 | A1 |
20190052063 | Tolstikhin | Feb 2019 | A1 |
20190339468 | Evans | Nov 2019 | A1 |
20190342009 | Evans | Nov 2019 | A1 |
20200152615 | Krasulick et al. | May 2020 | A1 |
20200244045 | Bismuto et al. | Jul 2020 | A1 |
20200253547 | Harris et al. | Aug 2020 | A1 |
20200309593 | Bismuto et al. | Oct 2020 | A1 |
20210033805 | Bishop et al. | Feb 2021 | A1 |
20210191039 | Jou et al. | Jun 2021 | A1 |
20210199576 | Arbore et al. | Jul 2021 | A1 |
20210263216 | Bishop et al. | Aug 2021 | A1 |
20210270699 | Piazza et al. | Sep 2021 | A1 |
20220091338 | Tu et al. | Mar 2022 | A1 |
20230071329 | Wu et al. | Mar 2023 | A1 |
20230110382 | Wu et al. | Apr 2023 | A1 |
20230125733 | Thomas et al. | Apr 2023 | A1 |
Number | Date | Country |
---|---|---|
104614084 | May 2015 | CN |
109445026 | Dec 2020 | CN |
1403985 | Mar 2004 | EP |
1432045 | Jun 2004 | EP |
H04204508 | Jul 1992 | JP |
H06003709 | Jan 1994 | JP |
2006284791 | Oct 2006 | JP |
2007279240 | Oct 2007 | JP |
2008262118 | Oct 2008 | JP |
2010223991 | Oct 2010 | JP |
2015152729 | Aug 2015 | JP |
2016148810 | Aug 2016 | JP |
2018004692 | Jan 2018 | JP |
WO 01014929 | Mar 2001 | WO |
WO 04031824 | Apr 2004 | WO |
WO 05091036 | Sep 2005 | WO |
WO 11090274 | Jul 2011 | WO |
WO 17040431 | Mar 2017 | WO |
WO 17184420 | Oct 2017 | WO |
WO 17184423 | Oct 2017 | WO |
WO 19152990 | Aug 2019 | WO |
WO 20106974 | May 2020 | WO |
Entry |
---|
Gonzalez-Sanchez et al., “Capacitive Sensing for Non-Invasive Breathing and Heart Monitoring in Non-Restrained, Non-Sedated Laboratory Mice,” Sensors 2016, vol. 16, No. 1052, pp. 1-16. |
He et al., “Integrated Polarization Compensator for WDM Waveguide Demultiplexers,” IEEE Photonics Technology Letters vol. 11, No. 2, Feb. 1999, pp. 224-226. |
Kybartas et al., “Capacitive Sensor for Respiratory Monitoring,” Conference “Biomedical Engineering,” Nov. 2015, 6 pages. |
Lapedus, “Electroplating IC Packages—Tooling challenges increase as advanced packaging ramps up,” Semiconductor Engineering, https://semiengineering.com/electroplating-ic-packages, Apr. 10, 2017, 22 pages. |
Materials and Processes for Electronic Applications, Series Editor: James J. Licari, AvanTeco, Whittier, California, Elsevier Inc., 2009, 20 pages. |
Worhoff et al., “Flip-chip assembly for photonic circuits,” MESA+ Research Institute, University of Twente, Integrated Optical MicroSystems Group, The Netherlands, 12 pages. |
U.S. Appl. No. 17/725,418, filed Apr. 20, 2022, Wu et al. |
U.S. Appl. No. 17/851,252, filed Jun. 28, 2022, Wu. |
Dai et al., “10-Channel Mode (de)multiplexer with Dual Polarizations,” Laser & Photonics Reviews, vol. 12, No. 1, Nov. 17, 2017, 9 pages. |
Liu et al., “Silicon Multimode Waveguide Grating Filter at 2 μm,” Journal of Lightwave Technology, IEEE USA, vol. 37, No. 10, May 15, 2019, pp. 2217-2222. |
International Search Report and Written Opinion dated Dec. 22, 2021, PCT/US2021/051341, 14 pages. |
Krubhakar et al., “Design and fabrication of integrated optical 1x8 power splitter in SOI substrate using large cross-section single-mode waveguides,” Photonics 2010: Tenth International Conference on Fiber Optics and Photonics, Proceeding of SPIE, Bellingham, Washington, vol. 8173, No. 1, Dec. 29, 2010, pp. 1-6. |
Dai et al., “Compact silicon-on-insulator-based multimode interference coupler with bilevel taper structure,” Applied Optics, Optical Society of America, vol. 44, No. 24, 2005, pp. 5036-5041. |
Li et al., “Compact and low-loss silicon power splitter based on inverse tapers,” Optics Letters, Optical Society of America, vol. 38, No. 20, 2013, pp. 4220-4223. |
Rasigade et al., “Compact wavelength-insensitive fabrication-tolerant silicon-on-insulator beam splitter,” Optics Letters, Optical Society of America, vol. 35, No. 21, 2010, pp. 3700-3702. |
U.S. Appl. No. 17/903,875, filed Sep. 6, 2022, Pelc et al. |
U.S. Appl. No. 17/985,615, filed Nov. 11, 2022, Wu et al. |
U.S. Appl. No. 18/142,729, filed May 2023, Dezfouli et al. |
U.S. Appl. No. 18/430,275, filed Aug. 2023, Arbore et al. |
Number | Date | Country | |
---|---|---|---|
20220099889 A1 | Mar 2022 | US |
Number | Date | Country | |
---|---|---|---|
63083691 | Sep 2020 | US |