A cavity containing an array of charged quantum harmonic oscillators pumped with low-frequency photons can detect single gravitons through correlated photon emissions or absorptions, circumventing Dyson's non-detectability argument.
Quantum Me- chanics of Gravitational Waves
3 Pith papers cite this work. Polarity classification is still indexing.
3
Pith papers citing it
years
2026 3verdicts
UNVERDICTED 3representative citing papers
Charged Weber bars in a cavity QED setup emit photons under gravitational-wave strain via a semi-classical Gertsenshtein analogue, enabling resonant GW detection.
Proposes graviton population inversion and lasing in ultra-cold squeezed bosons via prior interaction Hamiltonian, with growth tied to boson number and squeezing, yielding an experimental proposal for a graviton laser.
citing papers explorer
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`Seeing' the quantum ripples of spacetime
A cavity containing an array of charged quantum harmonic oscillators pumped with low-frequency photons can detect single gravitons through correlated photon emissions or absorptions, circumventing Dyson's non-detectability argument.
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Detecting gravitational waves by emission of photons from charged Weber bars
Charged Weber bars in a cavity QED setup emit photons under gravitational-wave strain via a semi-classical Gertsenshtein analogue, enabling resonant GW detection.
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Towards graviton lasing from squeezed ultra-cold systems
Proposes graviton population inversion and lasing in ultra-cold squeezed bosons via prior interaction Hamiltonian, with growth tied to boson number and squeezing, yielding an experimental proposal for a graviton laser.