• 专利附录
  • 专利说明
  • 权利要求
  • 类似技术
  • 同族专利
  • 引用文献
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  • 优先权
    • 专利摘要:
    Integrated photonic device. In this document, a photonic device is described that allows performing both separation and combination of wavelength bands in optical signals. For this the device described here presents a star coupler, a set of input optical waveguides connected to the input of the star coupler, a formation of waveguides connected to the output of the star coupler, and a set of reflectors and phase shifters connected to said waveguide array. (Machine-translation by Google Translate, not legally binding)
    公开号:ES2540378A1
    申请号:ES201331792
    申请日:2013-12-05
    公开日:2015-07-09
    发明作者:Pascual Muñoz Muñoz；Bernardo GARGALLO JAQUOTOT；Javier Antonio SANCHEZ FANDIÑO；José Capmany Francoy
    申请人:Universidad Politecnica de Valencia；
    IPC主号:
    专利说明:

    DESCRIPTION

    INTEGRATED PHOTONIC DEVICE

    The present invention relates to a photonic device, more specifically to a reflective Arrayed Waveguide Grating (AWG) device with reflectors based on a Sagnac reflector loop (SLR).
    STATE OF THE TECHNIQUE
     10
    Conventional AWGs photonic devices, R-AWGs based on reflectors formed with the facet or reflectors with grating are known in the state of the art, in fact US5002350 documents describing the original Dragone AWG device are known, or the document of the same company US5450511 that details an R-AWG where the input and output guides are interspersed with reflectors in the output guides 15.

    There is also evidence of US539650 describing an adjustable laser where the reflector is formed using one of the faces of the chip. Similarly, document US 2003007728 A1 is known which describes an AWG and its manufacturing method, with a substantially flat response in a wavelength band. The device described in this document consists of a substrate, an optical input waveguide for receiving a wavelength multiplexed signal, a set of optical output waveguides parallel to the input and connected together with it to a star coupler, a first group of waveguides connected to the output of the star coupler with a difference L between consecutive guide lengths and a Fabry-Perot resonator formed by a second group of guides connected to the output of the guide guides the first grouping with a 2L difference between consecutive guide lengths, an 11% metallic reflectance film on the face in contact with the first array and a 100% reflectance metallic film on the opposite face. 30

    Document XP006039590 presents a multi-wavelength laser consisting of a grouping of Fabry-Perot cavities constructed between two Sagnac loop reflectors, an AWG frequency selector and semiconductor optical amplifiers (SOA) of half amplifier. 35

    In view of these and other documents, it is understood that different ways of implementing reflectors for R-AWG can be found in the literature, many using reflective material on chip faces or photonic crystals, but also external reflectors. Many of them resort to non-integrated structures and / or additional manufacturing processes. 5

    None of the aforementioned devices allows modifying the spectral response of the AWG through the SLR reflectors and they also have very large sizes that condition their applications, manufacturing and use.
     10 DESCRIPTION OF THE INVENTION


    This document describes an integrated Arrayed Waveguide Grating (AWG) reflective photonic device that can be used to process (multiplex / demultiplex) 15 wavelength bands, a device that has reflectors based on a Sagnac reflector loop (SLR) and the coupling constant of the reflector loop coupler, preferred but not restricted, set to 0.5. In more detail and in response to one of the above-mentioned problems related to size, an R-AWG is treated in which the reflectors are obtained in the same lithographic process as the AWG. twenty

    As indicated above the invention object of this report is a reflective AWG allows multiplexing / demultiplexing (combining / separating) bands of wavelengths, the device described here also allows obtaining a flat response forcing a “sync” type distribution of the signal in training by modifying the amplitude with the SLRs and the phase with broadband phase shifters (PS).

    The present invention presents an AWG device configuration which is an integrated photonic device (PIC) which is used for the separation / combination of wavelength bands. 30

    An AWG device is composed of:
     A set of optical input waveguides, connected to the input of a first star coupler known as Dragone coupler for being the developer of the same. 35
     A formation of waveguides (grouping) connected to the output of the first star coupler and the input of the second star coupler.
     A set of output waveguides connected to the output of the second star coupler.
     5
    In the AWG device, a light signal connected to the input waveguide is spatially separated between the outputs depending on the wavelengths of which the signal is composed (separate, demultiplex). Contrary to this, when several signals are introduced by several outputs, they can be combined into one input (combine, multiplex). The device is passive and reciprocal. 10

    The field at the input of the first star coupler is diffracted towards the output (far field) of the coupler. This far field is collected in the grouping. For waveguides typically used in PIC technologies, the far field is a widened version of the field in the input guide, that is, it has the same shape (typically, 15 but not necessarily, Gaussian form) but widens over a longer angle or length. The mathematical relationship between the field in the input guide and the coupler output is the Fresnel diffraction integral, which can be approximated by the Fourier transform in most AWG design cases. Therefore, the waveguide formation guide that is in the center picks up the maximum amplitude 20 of the field, while the amplitude collected by the rest of the guides will be smaller, and related to the guide of the training center or formation by the far field form (typically, but not necessarily, Gaussian).

    The field collected on each path of the formation is subjected to a different lag or 25 path traveled. The AWG object of the invention has a configuration that allows the optical phase difference (ΔΦ) between consecutive paths in the cluster is an integer number of times (m) 2π, that is ΔΦ = m · 2π, each path being the group consisting of guide, phase shifter and reflector so that the difference in optical phases (ΔΦ) occurs between each and every one of these elements: the consecutive optical guides of the formation, as well as the phase shifters and reflectors to which they are respectively connected said consecutive optical guides of the formation. This generally implies a difference in lengths between consecutive waveguides ΔL = m · 0 / nw, where the operating wavelength is λ0, and where nw is the effective propagation index in the guide. The optical propagation constant in the guide is β = 2π · nw / λ, so that the phase difference between consecutive guides changes with the wavelength
    used (linearly with the optical frequency ν = c / λ, where c is the speed of light in a vacuum). This linear phase front, combined in the second star coupler (acting as a spatial Fourier transform), entails the aforementioned separation of the input wavelengths into bands at the AWG outputs (the focus point in the different positions Output depends on the wavelength / frequency 5 due to the different offset depending on the frequency that is introduced into the grouping).

    Another possible configuration for AWGs is the reflective AWG (R-AWG). In this case, the device has a configuration equal to half of the AWG device and optical reflectors are used in the middle of the cluster. In this way, the signal travels to the reflectors and is sent back to the input star coupler.

    The device described here consists of optical waveguides that are manufactured on different substrates by different techniques, such as lithography techniques. For the device of the present invention, and as indicated throughout this document, use is made of reflectors that are Sagnac interferometers. Since this interferometer is also formed by optical waveguides, it is possible to manufacture in the same process and substrate the device with its different parts as well as the reflector at the same time, without the need for additional manufacturing processes and / or steps.
     twenty
    Throughout the description and the claims the word "comprises" and its variants are not intended to exclude other technical characteristics, additives, components or steps. For those skilled in the art, other objects, advantages and features of the invention will be derived partly from the description and partly from the practice of the invention. The following examples and figures are provided by way of illustration, and are not intended to be limiting of the present invention.
    BRIEF DESCRIPTION OF THE FIGURES

    FIG. 1 Shows a schematic view of the device object of the invention in which the different components that comprise it as well as their arrangement are appreciated.
    EXAMPLES

    The invention will now be illustrated by tests carried out by the inventors, which demonstrates the effectiveness of the product of the invention.
    The present invention consists of an integrated photonic device (1) for processing AWG or R-AWG wavelength bands comprising at least one reflector (5) that is manufactured in the same lithographic process as the device (1), the which has an arrangement like the one seen in figure 1. The reflectors (5) are based on a Sagnac reflector loop (5) (SLR of the Sagnac Loop Reflector). The reflector device 5 (1) comprises a star coupler (2), which can have one or two input guides, and two output guides couplers 1x2 and 2x2, respectively. The two output guides are interconnected forming a loop, as shown in Fig. 1. When the coupling constant (K) of the star coupler (2) is 0.5, total reflection occurs in the reflector ( 5) SLR, that is, all the light introduced in one of the input guides is reflected 10 towards the same input. The coupler can be implemented in different ways: directional coupler (DC of the English directional coupler), wavelength insensitive coupler (WINC) or multimode interference coupler (MMI of English multimode interference coupler). For the present invention, a broadband coupler is required that maintains the same coupling for a wide range of wavelengths. Because of this, both the WINC coupler and the MMI can be used. MMIs are generally the smallest size once integrated into any of the integration technologies. When K is not 0.5, the amount of power reflected by the SLR towards the input is not 100%. In MMIs it is well known in the state of the art that can be designed to obtain the desired coupling constant. twenty

    The operating principle of the AWG requires that the difference between the optical phases (ΔΦ) of at least two consecutive guides in the formation of waveguides (3) has to be an integer number of times (m) 2π, that is ΔΦ = m2π. In any case, the phase difference depends on all those structures that the light goes through. 25

    The most general case of the present invention is shown on each path in waveguide formation (3) consists of: optical waveguide, phase shifting section (PS of the English phase shifting) and SLR reflector (5). The offset in guide number 'i' (i = 1..N) is: Φi = Φw, i + ΦPS, i + ΦSLR, i, where Φw, i is the optical offset in the guide that connects the star coupler 30 to the phase shifter, ΦPS, i is the optical offset in the phase shifter and ΦSLR, i is the optical offset in the Sagnac reflector (5).

    The SLR reflector (5) has a field transfer function (amplitude and phase) that depends on both the coupler and the guide that forms the loop. In the general case, every 35
    path may have a different SLR, so to maintain the phase relationship ΔΦ between consecutive guides (i.e. ΔΦ = Φi + 1 - Φi) it is necessary to use different PSs on each path.

    Like the star coupler (2), the PS needs to be broadband, that is, it needs to maintain the phase difference over a wide range of wavelengths. The 5-band PS can be implemented by using normal waveguides or by modifying the center of the waveguide.

    Answer Gaussian SRAWG
    The simplest embodiment of the present invention makes use of identical reflectors (5) SLRs 10 are used in all paths (guide, phase shifter (4), reflector (5)) of waveguide formation (3). The reflector (5) SLR is comprised of a 1x2 coupler with a coupling constant K = 0.5. In this way, all the power entering the reflector (5) SLR is reflected towards the input. Because all SLR reflectors (5) are equal, ideally the incident field in SLR reflectors (5) will have the same variation in amplitude and phase in all paths of waveguide formation (3).

    Therefore, in this particular embodiment, the SLR reflector (5) acts only as a light reflector. When the amplitude in any path of the waveguide formation (3) is not altered by any structure, and the phase relationship between consecutive guides 20 is ΔΦ, the spectral bands have a Gaussian shape. The mode of operation and the spectral form in the passing bands of the device (1) acting as SRAWG are equivalent to those of the normal and reflective AWGs: the device (1) operates as a wavelength band multiplexer / demultiplexer, and the The shape of the spectral bands has the form of a Gaussian function. 25

    Spectral SRAWG Flat Response.
    There are different techniques to adjust the spectral response of the AWG, the least used being the modification of the amplitude and phase of the field distribution in waveguide formation (3). The far field in the star coupler (2) follows a Fourier transform ratio with respect to the field in the input guide. It is known in signal theory that the Fourier transform of a sinc function is a rectangular function.

    The operation of the R-AWG device (1) is as follows. The light injected by one of its 35 input guides is propagated by the star coupler (2) (known by its nomenclature
    Anglo-Saxon “slab coupler”) and feeds each of the waveguides of a waveguide formation (3) of waveguides (3), as previously described (also called Gaussian beams). For each waveguide, the light propagates first towards the Sagnac reflectors (5). When the light reaches the entrance of the Sagnac reflector (5), it is divided into two parts by the reflector coupler, which can be different depending on the coupling constant of said reflector coupler. Each of said parts travels through the reflector loop (5), in the opposite direction that it closes on the same reflector coupler (5). Thus, said parts interfere back in the input guide of the reflector coupler (5), with an amplitude and electric field phase ratio that is dependent on the coupling constant of said coupler. The light then travels 10 back, in the opposite direction to the star coupler (2). This happens for all waveguides of the waveguide formation (3) and their respective Sagnac reflectors (5). The star coupler (2) will combine the field of all of them and direct it towards the exit guides. The effect produced by the star coupler (2) in said combination will be a function of the phase relationship between the waveguides of the formation of 15 waveguides (3). In the case mentioned above, where the phase relationship between consecutive guides of waveguide formation (3) is an integer number of times (m) 2 , the effect is the separation (de-multiplexing) of the different wavelengths of the light present in the R-AWG input optical waveguide, between the different optical output waveguides. twenty
    权利要求:
    Claims (4)
    [1]

    1. Integrated photonic device (1) for processing wavelength bands comprising:
     at least one star coupler (2) and, 5
     at least one optical input guide, connected to at least one star coupler input (2),
     at least two optical output guides connected to at least one star coupler output (2) and interconnected forming a loop,
     a formation of waveguides (3) connected to at least one output of the star coupler 10 (2), and
     at least one phase shifter (4) located in each of the waveguides of the waveguide formation (3),
    device (1) characterized in that it comprises:
     located next to the phase shifter (4) and at an opposite end to that at the 15 that connects each waveguide of the waveguide formation (3) with the star coupler (2), at least one reflector (5) Optical based on a Sagnac reflector loop (5) (SLR) being this an optical coupler which in turn comprises at least one reflector input guide, and two reflector output guides where the two reflector output guides are they find interconnected 20 forming a loop, and
    - a difference in optical phases (ΔΦ) between two consecutive optical guides of waveguide formation (3), phase shifters (4) and reflectors (5) to which said consecutive optical guides of guide formation are respectively connected wave (3), where said difference is equal to an integer 25 times (m) 2π, that is ΔΦ = m · 2π.

    [2]
    2. Integrated photonic device (1) according to claim 1 characterized in that the coupling constant of the reflector loop coupler (5) is between 0 and 1. 30

    [3]
    3. Integrated photonic device (1) according to claim 2 characterized in that the coupling constant of the reflector loop coupler (5) is 0.5.

    [4]
    4. Integrated photonic device (1) according to claim 1 or 2 comprising more than one reflector (5) characterized in that each loop of each reflector (5) has different lengths.
    5
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    ES201331792A|ES2540378B1|2013-12-05|2013-12-05|INTEGRATED PHOTONIC DEVICE|ES201331792A| ES2540378B1|2013-12-05|2013-12-05|INTEGRATED PHOTONIC DEVICE|
    EP14868641.3A| EP3078997B1|2013-12-05|2014-10-16|Photonic integrated device|
    US15/101,469| US9588290B2|2013-12-05|2014-10-16|Photonic integrated device|
    PCT/ES2014/070782| WO2015082738A1|2013-12-05|2014-10-16|Photonic integrated device|
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