AMPM survey detects one microlensing candidate in LMC data and constrains up to 30% of Galactic primordial black hole dark matter at 95% C.L. in the asteroid-to-planetary mass range, with peak sensitivity shifted to lunar masses by second-order effects.
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Superposition of neutrino helicity states creates azimuthal asymmetry in recoil momenta for scattering on electrons, protons, and nuclei, offering a way to observe spin oscillations with directional detection.
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AMPM I. A Targeted Search for Asteroid Mass Primordial Black Hole Microlenses
AMPM survey detects one microlensing candidate in LMC data and constrains up to 30% of Galactic primordial black hole dark matter at 95% C.L. in the asteroid-to-planetary mass range, with peak sensitivity shifted to lunar masses by second-order effects.
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The potential of directional neutrino detection to observe neutrino spin oscillations
Superposition of neutrino helicity states creates azimuthal asymmetry in recoil momenta for scattering on electrons, protons, and nuclei, offering a way to observe spin oscillations with directional detection.