120762028
Present status of inelastic and elastic hadronic weak neutral currents
Since the first observations of weak neutral currents in the reactions ..nu../sub ..mu../(anti ..nu../sub ..mu../) + nucleon ..-->.. ..nu../sub ..mu../(anti ..nu../sub ..mu../) + hadrons in 1973, there have been a number of additional measurements of those reactions, and also of the elastic reactions ..nu../sub ..mu../(anti ..nu../sub ..mu../) + p ..-->.. ..nu../sub ..mu../(anti ..nu../sub ..mu../ + p. The methods utilized are briefly compared and the results obtained are summarized. Inferences are drawn from these results concerning the space-time structure and scale invariance of the hadronic weak neutral current. 23 references.
121246612
Scaling-variable distributions in high-energy inelastic neutrino interactions
123899161
NEUTRINOS AND MUONS IN AREA 1.
118712243
Comments on the letter «Limits on the electromagnetic production of heavy leptons»
38997255
Prototype detector for ultrahigh energy neutrino detection
Abstract Necessary technical experience is being gained from successful construction and deployment of current prototype detectors to search for UHE neutrinos in Antarctica, Lake Baikal in Russia, and the Mediterranean. The prototype detectors have also the important central purpose of determining whether or not UHE neutrinos do in fact exist in nature by observation of at least a few UHE neutrino-induced leptons with properties that are not consistent with expected backgrounds. We discuss here the criteria for a prototype detector to accomplish that purpose in a convincing way even if the UHE neutrino flux is substantially lower than predicted at present.
118973535
Some Recent Advances in Neutrino Physics
One answer to questions concerning the subject matter of elementary particle physics and its position within the physical sciences is that particle physics is the study of creation. To justify this idea, at least in part, consider the “big bang” model of creation of the universe. In that model the primeval fireball involved very high temperatures, estimated to be greater than 1011 degrees Kelvin (°K), which is to be compared with the interior temperature of the sun at about 107 degrees Kelvin. We believe the sun to be a nuclear furnace, generating its energy by individual nuclear interactions in the million electron volt (MeV) energy range. In the “big bang” the energies involved in the individual particle interactions would have been more than 104 times larger than in the sun, and thus in the tens of giga-electron volts (GeV). This is precisely the energy region of present-day high energy or elementary particle physics laboratory experiments. In this sense, then, laboratory experiments that study, even indirectly, lepton-lepton scattering or quark-quark interactions are revisiting creation.
122239911
Maximumvs. Critical temperature in a superfluid approach to strong interactions
53454093
Phase-space formulation of quantum mechanics and quantum-state reconstruction for physical systems with Lie-group symmetries
We present a detailed discussion of a general theory of phase-space distributions, introduced recently by the authors @J. Phys. A 31 ,L 9 ~1998!#. This theory provides a unified phase-space formulation of quantum mechanics for physical systems possessing Lie-group symmetries. The concept of generalized coherent states and the method of harmonic analysis are used to construct explicitly a family of phase-space functions which are postulated to satisfy the Stratonovich-Weyl correspondence with a generalized tracing condition. The symbol calculus for the phase-space functions is given by means of the generalized twisted product. The phase-space formalism is used to study the problem of the reconstruction of quantum states. In particular, we consider the reconstruction method based on measurements of displaced projectors, which comprises a number of recently proposed quantum-optical schemes and is also related to the standard methods of signal processing. A general group-theoretic description of this method is developed using the technique of harmonic expansions on the phase space. @S1050-2947~99!00702-7#
122704344
Mesonic structure in the nucleon
8618294
Development of a high-rate GEM-based TPC for PANDA
An ungated GEM-based TPC with continuous readout is considered as the central tracker of the PANDA experiment. Particles from up to 2ldr107 p macrp annih./s have to be tracked over a wide momentum range (0.1-8 GeV/c). Simulations demonstrate a space charge accumulation of up to 55 fC/cm3, leading to correctable track distortions of up to 6 mm. Ion backflow studies in triple-GEM structures have been performed. A spatial resolution of down to 140 mum has been achieved with a GEM-TPC test chamber, operated with an Ar/CO2 gas mixture and without magnetic field, recording the signals of cosmic muons.
123581677
LINEARIZED VERSION OF THE HARTREE--FOCK METHOD.