We discuss a model of dark matter consisting of high energy anti-electronneutrinos with leptonic force, which is produced by the conserved leptonic charge g ℓ associated with Lee-Yang's U1 gauge symmetry. Based on particle-cosmology for early universe, the high energy neutrino (HEN) model of dark matter assumes that the neutron decay processes, n → p + + e − + νe, dominate the epoch after the creation, collision and confinement processes of quarks and antiquarks in the beginning. The HEN model implies the following results: There are almost equal numbers of electrons, protons and anti-electron-neutrinos dominated the matter cosmos. There are unobservable and ubiquitous anti-electron-neutrinos νe with leptonic charge g ℓ in the universe. Although the total mass of anti-electronneutrino dark matter is negligible in the universe, its enhanced gravitational and leptonic forces could lead to the observed flat rotation curves due to relativistic νe, whose static force involves a factor Eν/mν ≈ 10 6 . We estimate the leptonic charge to be g ℓ ≈ 7 × 10 −21 . The model predicts that the anti-electronneutrino dark matter can interact with cosmic-ray protons to produce positrons, i.e. νe + p + → e + + n, through weak interaction of the unified electroweak theory. The anti-electron-neutrino dark matter sheds light on the Alpha Magnetic Spectrometer (AMS) experiment, which has detected the intriguing excess of cosmic-ray positrons over what is expected. The HEN model of dark matter suggests an experimental test of the new Lee-Yang force between electrons by using modern precision Cavendish experiment.