Heterotic string theory implies the QCD axion mass is bounded below by 0.5 neV and typically falls in [0.5, 0.8] neV across most compactifications.
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Superradiant clouds around Kerr black holes amplify stochastic gravitational-wave backgrounds via stimulated emission, with rate depending on boson mass and potentially enhancing signals by orders of magnitude.
LILA can detect IMBH binaries at redshifts 20-30, IMRIs, and provide months-to-years early warnings with high-SNR events for gravity tests.
citing papers explorer
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Heterotic String Theory Suggests a QCD Axion Near 0.5 neV
Heterotic string theory implies the QCD axion mass is bounded below by 0.5 neV and typically falls in [0.5, 0.8] neV across most compactifications.
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Stimulated Emission from Boson Clouds
Superradiant clouds around Kerr black holes amplify stochastic gravitational-wave backgrounds via stimulated emission, with rate depending on boson mass and potentially enhancing signals by orders of magnitude.
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Black Hole Binary Detection Landscape for the Laser Interferometer Lunar Antenna (LILA): Signal-to-Noise Calculations & Science Cases
LILA can detect IMBH binaries at redshifts 20-30, IMRIs, and provide months-to-years early warnings with high-SNR events for gravity tests.