Titlebook: Neutrino Mass, Dark Matter, Gravitational Waves, Monopole Condensation, and Light Cone Quantization; Behram N. Kursunoglu,Stephan L. Mintz

江湖骗子

Ultrahigh-Energy Neutrino Interactions and Neutrino Telescope Event Rates the PeV range due to neutrino-electron interactions. We show that future neutrino detectors, such as AMANDA, BAIKAL, DUMAND and NESTOR have a very good chance of detecting neutrinos which originate in the Active Galactic Nuclei.

妈妈不开心

大猩猩

COM

使人入神

irreparable

A Scale Invariant Superstring Theory With Dimensionless Coupling To Supersymmetric Gauge Theoriescted symmetries. The coupling is expressed in terms of chiral currents and superfields in superspace. The natural coupling to the superstring gives rise to a new observable that is “stringy” in nature and has no analogue in non-supersymmetric gauge theories. We compute the expectation value of this

Defraud

故意钓到白杨

爱管闲事

Interferometry for Gravity Wave Detectione metric very difficult if not impossible, but here on earth the gravitational fields are always weak enough so that they can be described by the so-called linearized theory. In this weak field limit, the metric can be approximated as .. ≈ η. + .., ǀ..ǀ « 1. The Weak-field Einstein equations in vacu

ungainly

LSND Neutrino Oscillation Resultsrms into a neutrino of another type (say .). For this phenomenon to occur, neutrinos must be massive and the apparent conservation law of lepton families must be violated. In 1995 the LSND experiment published data showing candidate events that are consistent with . oscillations.. Additional data ar