Proposes entangled vibrational qubits in linear Paul traps for detecting high-frequency gravitational waves via graviton-photon conversion or relative motion, with N-squared sensitivity enhancement.
Broadband Limits on Stochastic Length Fluctuations from a Pair of Table-Top Interferometers
4 Pith papers cite this work. Polarity classification is still indexing.
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A hemilithic OPA squeezed light source demonstrates up to 6.8 dB squeezing maintained at least 3 dB across 100 MHz bandwidth, with 8.6 dB inferred after dark noise correction, and 138 MHz linewidth claimed as broadest for long-term use.
Deformed alpha-attractor T-models with a Gaussian feature near the minimum yield more smaller shorter-lived oscillons during self-resonance preheating, suppressing energy in oscillons and altering the high-frequency gravitational wave tail while leaving low frequencies unchanged.
Computes UV-finite noise spectra in interferometers from graviton fluctuations in vacuum/thermal/squeezed states and from massless scalar vacuum stress-energy, all Planck-suppressed.
citing papers explorer
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Probing high-frequency gravitational waves with entangled vibrational qubits in linear Paul traps
Proposes entangled vibrational qubits in linear Paul traps for detecting high-frequency gravitational waves via graviton-photon conversion or relative motion, with N-squared sensitivity enhancement.
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A Broadband Squeezed Light Source for Table-Top Interferometry
A hemilithic OPA squeezed light source demonstrates up to 6.8 dB squeezing maintained at least 3 dB across 100 MHz bandwidth, with 8.6 dB inferred after dark noise correction, and 138 MHz linewidth claimed as broadest for long-term use.
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Self-resonance preheating in deformed attractor models: oscillon formation and evolution
Deformed alpha-attractor T-models with a Gaussian feature near the minimum yield more smaller shorter-lived oscillons during self-resonance preheating, suppressing energy in oscillons and altering the high-frequency gravitational wave tail while leaving low frequencies unchanged.
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Geometric noise spectrum in interferometers
Computes UV-finite noise spectra in interferometers from graviton fluctuations in vacuum/thermal/squeezed states and from massless scalar vacuum stress-energy, all Planck-suppressed.