Bidirectional internal squeezing using opposing optical parametric amplifiers saturates quantum noise lower bounds from internal dissipation and renders high-frequency signal-referred noise independent of arm and signal-extraction transmissivities.
arXiv:2603.24243
4 Pith papers cite this work. Polarity classification is still indexing.
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2026 4representative citing papers
Machine learning extracts core rotation and signal properties from CCSN gravitational waves, with next-generation detectors constraining rotation beyond 100 kpc for favorable orientations despite some uncertainties.
Linear analysis of protoneutron star oscillations identifies potential universal relations with supernova gravitational wave signals that are independent of model parameters.
Stellar evolution and atmosphere models predict black hole progenitors are predominantly hot and blue with a direct-collapse rate of ~0.4 per century in a 1 Msun/yr star-forming galaxy.
citing papers explorer
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Bidirectional Internal Squeezing for Gravitational-Wave Detectors
Bidirectional internal squeezing using opposing optical parametric amplifiers saturates quantum noise lower bounds from internal dissipation and renders high-frequency signal-referred noise independent of arm and signal-extraction transmissivities.
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Parameter Estimation Horizon of Core-Collapse Supernovae with Current and Next-Generation Gravitational-Wave Detectors
Machine learning extracts core rotation and signal properties from CCSN gravitational waves, with next-generation detectors constraining rotation beyond 100 kpc for favorable orientations despite some uncertainties.
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Understanding supernova gravitational waves with protoneutron star asteroseismology
Linear analysis of protoneutron star oscillations identifies potential universal relations with supernova gravitational wave signals that are independent of model parameters.
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Hot blue progenitors of stellar-mass black holes
Stellar evolution and atmosphere models predict black hole progenitors are predominantly hot and blue with a direct-collapse rate of ~0.4 per century in a 1 Msun/yr star-forming galaxy.