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Chaperone-Mediated Regulation of Tau Phase Separation, Fibrillation, and Toxicity. [PDF]
J Am Chem SocMörman C +12 more
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Topological Fermiology of gate-tunable Rashba electron gases. [PDF]
Sci AdvHu J +10 more
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A High Statistics Search for Electron-Neutrino --> Tau-Neutrino Oscillations [PDF]
, 1998 Ccfr, D. Naples, A. Romosan
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Planetary Laser Interferometric Seismoacoustic Observatory. [PDF]
Sensors (Basel)Dolgikh G +4 more
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Thermodynamics of the Primordial Universe. [PDF]
Entropy (Basel)Pereira DS +3 more
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Non-KAM classical chaos topology for electrons in superlattice minibands determines the inter-well quantum transition rates. [PDF]
Sci RepWang F +3 more
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Philosophical Transactions of the Royal Society of London. Series A: Mathematical, Physical and Engineering Sciences, 2002
The wave theory of light, and in particular the principle of interference, was formulated by Thomas Young in 1801. In the 20th century, the principle of interference was extended to the quantum mechanical wave functions describing matter. The phenomenon of quantum mechanical interference of different neutrino states, neutrino oscillations, has provided
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The wave theory of light, and in particular the principle of interference, was formulated by Thomas Young in 1801. In the 20th century, the principle of interference was extended to the quantum mechanical wave functions describing matter. The phenomenon of quantum mechanical interference of different neutrino states, neutrino oscillations, has provided
openaire +2 more sources
Physical Review Letters, 1985
The theory of oscillations of solar neutrinos is developed as it applies to the electron-recoil spectrum in neutrino-electron scattering. The spectral information obtained by such measurements (as opposed to counting total event rates) is crucial for allowing observation of neutrino oscillations for masses down to 500 neV.
Lawrence M. Krauss, Frank Wilczek
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The theory of oscillations of solar neutrinos is developed as it applies to the electron-recoil spectrum in neutrino-electron scattering. The spectral information obtained by such measurements (as opposed to counting total event rates) is crucial for allowing observation of neutrino oscillations for masses down to 500 neV.
Lawrence M. Krauss, Frank Wilczek
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