Implications of the chiral anomaly for quantum Hall-effect devices.
The anomaly equation ${\ensuremath{\partial}}_{\ensuremath{\mu}}$${J}_{5}$${}^{\ensuremath{\mu}}$=-(${e}^{2}$/8${\ensuremath{\pi}}^{2}$ ${\ensuremath{\Elzxh}}^{2}$c) (${F}_{\ensuremath{\lambda}\ensuremath{\sigma}}^{\mathrm{*}}$${F}^{\ensuremath{\lambda}\ensuremath{\sigma}}$) is used to derive a relationship between the filling factor (\ensuremath{\nu}) and the Hall conductance on the gate capacitor of a field-effect-transistor device. In addition, the chiral phase (\ensuremath{\theta}) states are shown to be related to those of the filling factor by \ensuremath{\Vert}\ensuremath{\theta}〉=\ensuremath{\Vert}2\ensuremath{\pi}\ensuremath{\nu}〉.

title: Two-time correlation functions:
stochastic and conventional quantum mechanics

abstract: An investigation of two-time correlation functions is reported
within the framework of (i) stochastic quantum mechanics and (ii)
conventional Heisenberg-Schrödinger quantum mechanics. The
spectral functions associated with the two-time electric dipole moment
correlation functions are worked out in detail for the case of the
hydrogen atom. While the single time averages are identical for
stochastic and conventional quantum mechanics, differences arise in
the two approaches for multiple time correlation functions.

title: Gravitational Wave Detection with Michelson Interferometers
abstract: Electromagnetic methods recently proposed for detecting gravitational waves modify the Michelson phase shift analysis (historically employed for special relativity). We suggest that a frequency modulation analysis is more suited to general relativity. An incident photon in the presence of a very long wavelength gravitational wave will have a finite probability of being returned as a final photon with a frequency shift whose magnitude is equal to the gravitational wave frequency. The effect is due to the non-linear coupling between electromagnetic and gravitational waves. The frequency modulation is derived directly from the Maxwell-Einstein equations.

title: Modeling Pion and Nucleon Total Cross-sections
abstract: With an eye towards proposed experiments at the LHC, an earlier eikonal mini‐jet model with soft gluons has now been extended to compute πp and ππ total cross‐sections.

title: Viscosity of high energy nuclear fluids
abstract: Relativistic high energy heavy ion collision cross sections have been interpreted in terms of almost ideal liquid droplets of nuclear matter. The experimental low viscosity of these nuclear fluids have been of considerable recent quantum chromodynamic interest. The viscosity is discussed here in terms of the string fragmentation models wherein the temperature dependence of the nuclear fluid viscosity obeys the Vogel–Fulcher–Tammann law.

title: Vacuum spin waves through the chiral anomaly
abstract: It is shown that the quantum electrodynamic chiral anomaly generates “spin waves” in the vacuum, when a low-energy electromagnetic field is applied. Such spin waves are (in principle) observable in a vacuum region with a condensed matter boundary surface which has a finite Hall conductance.

title: Fidelity of photon interferometry for recording the evolution of a nascent quark-gluon plasma.
abstract: The fidelity of two-photon intensity interferometry for reflecting the dynamics of a nascent quark-gluon plasma formed in a high energy nucleus-nucleus collision is examined. A (3+1)-dimensional expansion of the plasma as well as a (1+1)-dimensional expansion according to Bjorken hydrodynamics, both with a first order phase transition, are considered. The correlation of high transverse-momentum photons is shown to be a precision tool for the investigation of the space-time evolution of the high-density QCD plasma. In particular, the longitudinal correlation function, which depicts the time development of the system, is seen to have its origin in two sources: one corresponding to the early plasma phase and the second to the later stages. This aspect may help identify thermal photons according to their time of birth'' during evolution.