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May 9, 20260 citationsOpen Access

High-Frequency Gravitational Wave Detection via Tri-Axial Microwave Interferometry

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MRManuel Rebellón

Key Points

  • The aim is to develop a resonant detector for high-frequency gravitational waves in the GHz range with improved sensitivity.
  • Utilized a microwave bridge interferometer topology with a tri-axial superconducting cavity arrangement.
  • Employed a cryogenic sapphire oscillator to enhance performance.
  • Performed a noise budget analysis to assess thermal and phase noise impacts.
  • Achieved strain sensitivities of h ∼ 10−22 / Hz with Q ∼ 10^10.
  • Demonstrated capability to overcome thermal and phase noise floors.
  • Indicated potential for detecting primordial cosmological sources.

Abstract

We propose a resonant detector architecture for High-Frequency Gravitational Waves (HFGW) in the GHz band, utilizing a microwave bridge interferometer topology. Unlike prior proposals relying on the inverse Gertsenshtein effect (photon conversion), which scales quadratically with strain (P ∝ h2 ), the “Rebellon Bridge” exploits the geometric modulation of the cavity boundary conditions to achieve linear sensitivity (V ∝ h). The system employs a tri-axial superconducting cavity arrangement fed by a cryogenic sapphire oscillator. A passing gravitational wave induces a quadrupole deformation of the cavity geometry, disrupting the destructive interference condition atthe readout port. We present a noise budget analysis demonstrating that with a cavity Quality Factor of Q ∼ 1010 and millikelvin cooling, the √ system can overcome thermal and phase noise floors to reach strain sensitivities of h ∼ 10−22 / Hz, potentially opening the window to primordial cosmological sources.

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Cite This Study

Manuel Rebellón (2026) studied this question.

synapsesocial.com/papers/69fed17eb9154b0b82878d09https://doi.org/10.5281/zenodo.20073346
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