Inverse-designed tapers to improve throughput of on-chip astrophotonic spectrographs

@misc{seenivasan2026inversedesigned,
  title = {{Inverse-designed tapers to improve throughput of on-chip astrophotonic spectrographs}},
  author = {Vikram Seenivasan and Pradip Gatkine},
  howpublished = {arXiv},
  year = {2026},
  month = oct,
  doi = {10.48550/arxiv.2610.24699},
  eprint = {2610.24699},
  archivePrefix = {arXiv},
  url = {https://arxiv.org/abs/2610.24699},
  note = {CC BY 4.0},
}

TY  - UNPB
TI  - Inverse-designed tapers to improve throughput of on-chip astrophotonic spectrographs
AU  - Vikram Seenivasan
AU  - Pradip Gatkine
PY  - 2026
DA  - 2026/10/17
PB  - arXiv
DO  - 10.48550/arxiv.2610.24699
UR  - https://arxiv.org/abs/2610.24699
AB  - Astrophotonics offers a pathway towards compact and stable spectrographs for future large telescopes. The size of these spectrographs does not scale with the diameter of the telescope aperture; thus, they offer a cost-effective way to achieve astronomy science requirements compared to traditional optical spectrographs. A major limitation of current on-chip astrophotonic spectrographs is the significant loss incurred at interfaces between distinct components, particularly at the input and output fiber interfaces, limiting overall throughput. In this work, we investigate inverse-designed architectures to optimize transitions between these components to improve throughput. Inverse design formulates device design as an optimization problem, enabling non-intuitive geometries that can achieve high performance. We focus on optimizing coupling between an arrayed waveguide grating (AWG) spectrograph and an input single-mode fiber. Our approach explores two classes of fabrication-constrained inverse design. The first is shape optimization, which optimizes the geometry of the boundary of a coupling taper. The second is topology optimization, which optimizes the material distribution in a design region to gradually transform the optical mode between components. Both methods are implemented using the Tidy3D package from Flexcompute. We use germanium-doped silica for the core of the photonic components and silica as the cladding, and we use an SMF-28 fiber as input. This work demonstrates a pathway to improve astrophotonic spectrographs through computational inverse-design methods. Leveraging higher throughput, we can improve signal-to-noise ratios offered by photonic devices and position ourselves to design high-performance, cost-effective instrumentation for the next generation of telescopes, both on the ground and in space.
ER  -