Batalin-Tyutin Quantization of the Chiral Schwinger Model
We quantize the chiral Schwinger Model by using the Batalin-Tyutin formalism. We show that one can systematically construct the first
16 indexed results
We quantize the chiral Schwinger Model by using the Batalin-Tyutin formalism. We show that one can systematically construct the first
We have investigated the correlation functions of interacting bosons at the generic superfluid-insulator transition, a prototypical quantum phase transition, in
We research the entropy of a black hole in curved space-times by 't Hooft`s approach, so-called the brick wall method.
Coherent misfitting precipitates in elastically stressed media such as $γ\prime$ particles in nickel-based super-alloys show various splitting patterns such as
We study the zero-temperature phase transitions of a two-dimensional disordered boson Hubbard model at incommensurate boson densities. Via matrix diagonalization
We obtained optical and infrared spectra of Cha Ha 5/cc 1, a faint possibly sub-stellar companion candidate next to the
Two dense dark cloud cores representing different stages of dynamical evolution were observed in a number of molecular spectral lines.
We report the results of VLT and Keck adaptive optics surveys of known members of the Eta Chamaeleontis, MBM 12,
We present high-spatial resolution HST and adaptive optics observations, and high-sensitivity ISO (ISOCAM & ISOPHOT) observations of a sample of
Given their proximity and age differences, nearby groups of young stars are valuable laboratories for investigations of disk evolution and
V2051 Oph is an eclipsing dwarf novae with an orbital period of 90 min. This system belongs to a small
Based on an improved SU(2) slave-boson approach showing coupling between the cha rge and spin degrees of freedom, we derive
We study the kinematics of T Tauri stars (TTS) located in the cores of the Chamaeleon clouds as well as
An overview is given of all the magnetic CVs found in the UCT CCD CV Survey (Woudt & Warner 2001,
According to the Kosterlitz-Thouless-Theory two-dimensional solid films melt by the unbinding of dislocation pairs. A model including quenched random impurities
The eta Chamaeleontis star cluster is one of the most important nearby groupings of pre-main sequence (PMS) stars. With accurately