Broadband, Dead-Time-Free Spectrometer Using RFSoC for WISP Dark Matter Searches
Abstract Ultra-light dark matter candidates, such as axions and dark photons, particularly within the mass range of $\mu 10^{\rm V}$ to ${\rm meV}$, have garnered significant research interest. Detection approaches such as the dish-antenna method benefit from broadband spectrometers, allowing for efficient scanning across a broad dark matter mass range. This study presents a novel spectrometer solution based on an RFSoC. The spectrometer’s programmable logic implements an optimized fast Fourier transform (FFT) that minimizes memory usage, enabling an instantaneous bandwidth of $4 \,{\rm GHz}$ with a frequency resolution of $16 \,{\rm kHz}$. This configuration achieves more than 99.6% time efficiency, effectively doubling search efficiency, compared with traditional approaches. This paper provides a comprehensive description of the hardware architecture, FPGA firmware, and software implementation, with a focus on the resource-efficient pipelined FFT algorithm. Performance validation results are also presented, demonstrating the accuracy and time efficiency of the developed spectrometer, highlighting its potential for advancing dark matter search.
Authors
- O. Tajima (ORCID: https://orcid.org/0000-0003-2439-2611)
- S. Adachi (ORCID: https://orcid.org/0000-0002-0400-7555)
- J. Suzuki (ORCID: https://orcid.org/0000-0001-6816-8123)
- Hiroshi Takeuchi (ORCID: https://orcid.org/0009-0003-4022-7154)
Institutions
- Kyoto University (JP)
Publication Details
- Journal
- Progress of Theoretical and Experimental Physics
- Published
- 2025-04-29
- DOI
- https://doi.org/10.1093/ptep/ptaf065
- Primary Topic
- Dark Matter and Cosmic Phenomena
- Type
- article
- Field-Weighted Citation Impact
- 0.00
Funders
- Japan Society for the Promotion of Science
- Core Research for Evolutional Science and Technology