For KAGRA's post-O5 upgrade, a filter-cavity frequency-dependent squeezing scheme yields the best binary neutron star range, beating frequency-independent squeezing by at least 23% in detection rate, while EPR squeezing is best for heavy binaries.
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Quantum noise reduction schemes for KAGRA post-O5 upgrade
For KAGRA's post-O5 upgrade, a filter-cavity frequency-dependent squeezing scheme yields the best binary neutron star range, beating frequency-independent squeezing by at least 23% in detection rate, while EPR squeezing is best for heavy binaries.