Skip to content
DraconiticResearch
Search Sources API
203,234 studies31 sourcesUpdated 37 min ago
PreprintCC BY 4.0arXiv

Axion detection in the non-Markovian noise

Abstract

The detection of axion dark matter poses a significant challenge due to its exceptionally weak coupling to standard-model particles. Here we develop a noise-tolerant quantum-metrology scheme based on coupled 129Xe spin ensembles to search for such weakly interacting particles. Within an experimentally accessible parameter regime, our scheme achieves an ideal exclusion limit on the axion coupling constant that is several orders of magnitude more stringent than that of conventional detection methods. We further investigate the performance of our scheme under dissipative noise and find that its robustness is fundamentally governed by the energy-spectrum structure of the composite spin-environment system. Remarkably, when a bound state emerges in the spectrum, the exclusion limit asymptotically recovers its ideal value in the non-Markovian dynamics, whereas under the Markovian approximation the limit deteriorates significantly due to noise. Our results establish a universal mechanism for noise-resilient exploration of beyond-standard-model physics, which can be practically implemented by engineering bound-state formation via tuning the Larmor frequency of the spin ensembles.

Related

  1. From Axion Detection to Dark Matter Astronomy
    Jae Hyeok Chang, Stefano Profumo
    arXivPreprintCC BY 4.0Full textCosmologyHigh-energy & particle physicsarXiv
  2. Deep Learning Detection of Beyond-General-Relativity Deviations in Gravitational-Wave Signals: A Detection-Threshold Study with Real LIGO Noise
    Muhammad Adnan Shahzad
    arXivPreprintCC BY 4.0Full textInstrumentation & methodsGravitation & general relativityarXiv
  3. Optimal Strategies for Gravitational-Wave Memory Detection with Noise Marginalization in Pulsar Timing Arrays
    Rand Burnette, Xavier Siemens
    arXivPreprintCC BY-SA 4.0Full textInstrumentation & methodsGravitation & general relativityarXiv
  4. Fast and accurate false-alarm probabilities for linear detection statistics in Poisson noise
    Maayane T. Soumagnac, Eran O. Ofek, Shachar Israeli +1
    arXivPreprintarXiv licenceFull textInstrumentation & methodsarXiv
  5. The Quantum Noise Fraction and the addressable fraction in High-Frequency Gravitational Wave Detection
    Sergio Gaudio
    arXivPreprintarXiv licenceFull textInstrumentation & methodsGravitation & general relativityarXiv
BibTeX
@misc{dong2026axion,
  title = {{Axion detection in the non-Markovian noise}},
  author = {Jing Dong and Shuang-Quan Ma and Rong-Hang Chen and Bin-Kai Luo and Tao Liu and Qing Ai and Jun-Hong An},
  howpublished = {arXiv},
  year = {2026},
  month = oct,
  doi = {10.48550/arxiv.2610.27731},
  eprint = {2610.27731},
  archivePrefix = {arXiv},
  url = {https://arxiv.org/abs/2610.27731},
  note = {CC BY 4.0},
}
RIS
TY  - UNPB
TI  - Axion detection in the non-Markovian noise
AU  - Jing Dong
AU  - Shuang-Quan Ma
AU  - Rong-Hang Chen
AU  - Bin-Kai Luo
AU  - Tao Liu
AU  - Qing Ai
AU  - Jun-Hong An
PY  - 2026
DA  - 2026/10/20
PB  - arXiv
DO  - 10.48550/arxiv.2610.27731
UR  - https://arxiv.org/abs/2610.27731
AB  - The detection of axion dark matter poses a significant challenge due to its exceptionally weak coupling to standard-model particles. Here we develop a noise-tolerant quantum-metrology scheme based on coupled ^129Xe spin ensembles to search for such weakly interacting particles. Within an experimentally accessible parameter regime, our scheme achieves an ideal exclusion limit on the axion coupling constant that is several orders of magnitude more stringent than that of conventional detection methods. We further investigate the performance of our scheme under dissipative noise and find that its robustness is fundamentally governed by the energy-spectrum structure of the composite spin-environment system. Remarkably, when a bound state emerges in the spectrum, the exclusion limit asymptotically recovers its ideal value in the non-Markovian dynamics, whereas under the Markovian approximation the limit deteriorates significantly due to noise. Our results establish a universal mechanism for noise-resilient exploration of beyond-standard-model physics, which can be practically implemented by engineering bound-state formation via tuning the Larmor frequency of the spin ensembles.
ER  -