Compare Papers
Paper 1
Modular quantum computation in a trapped ion system.
Zhang K, Thompson J, Zhang X, Shen Y, Lu Y, Zhang S, Ma J, Vedral V, Gu M, Kim K.
- Year
- 2019
- Journal
- Nat Commun
- DOI
- 10.1038/s41467-019-12643-2
- arXiv
- -
No abstract.
Open paperPaper 2
Quantum Noise Fraction and the Thermal Frontier in High-Frequency Gravitational Wave Detection
Sergio Gaudio
- Year
- 2026
- Journal
- arXiv preprint
- DOI
- arXiv:2605.00053
- arXiv
- 2605.00053
We introduce a diagnostic -- the quantum noise fraction $β$ -- that determines the maximum sensitivity improvement achievable through quantum enhancement for any gravitational wave detector. Applied to the landscape of proposed high-frequency (kHz-GHz) detectors, this diagnostic reveals that resonant mass detectors operating through tidal coupling are thermally dominated ($β\approx 0$) at all frequencies below ~230 MHz at dilution temperatures, rendering squeezing and entanglement limited in effectiveness. Only above this thermal frontier, defined by $\hbar ω= k_B T \ln 3$, does the quantum regime become accessible. We identify a single concrete realization: a bulk acoustic wave resonator at 1 GHz and 10 mK ($β= 0.98$), and propose a gravitational wave detector employing squeezed phononic states via circuit QED readout. An array of $10^4$ such resonators with 10 dB mechanical squeezing reaches $\sqrt{S_h} = 7.6 \times 10^{-26}/\sqrt{\rm Hz}$ -- still a factor ~$10^9$ above the BBN bound on stochastic backgrounds at 1 GHz, indicating that the sensitivity gap remains predominantly classical in origin and that concurrent advances in classical detector parameters will be required.
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