1,295 research outputs found
On the forward-backward charge asymmetry in e+e- -annihilation into hadrons at high energies
The forward-backward asymmetry in e+ e- annihilation into a quark-antiquark
pair is considered in the double-logarithmic approximation at energies much
higher than the masses of the weak bosons. It is shown that after accounting to
all orders for the exchange of virtual photons and W, Z -bosons one is lead to
the following effect (asymmetry): quarks with positive electric charge (e.g. u,
\bar{d}) tend to move in the e+ - direction whereas quarks with negative
charges (e.g. d, \bar{u}) tend to move in the e- - direction. The value of the
asymmetry grows with increasing energy when the produced quarks are within a
cone with opening angle, in the cmf, \theta_0\sim 2M_Z/\sqrt{s} around the e+e-
-beam. Outside this cone, at \theta_0 << \theta << 1, the asymmetry is
inversely proportional to \theta .Comment: 17 Pages, 2 Tables, 4 Figures. Hadronization effects to the asymmetry
are considered with more detail
Scintillation reduction for combined Gaussian-vortex beam propagating through turbulent atmosphere
We numerically examine the spatial evolution of the structure of coherent and
partially coherent laser beams (PCBs), including the optical vortices,
propagating in turbulent atmospheres. The influence of beam fragmentation and
wandering relative to the axis of propagation (z-axis) on the value of the
scintillation index (SI) of the signal at the detector is analyzed. A method
for significantly reducing the SI, by averaging the signal at the detector over
a set of PCBs, is described. This novel method is to generate the PCBs by
combining two laser beams - Gaussian and vortex beams, with different
frequencies (the difference between these two frequencies being significantly
smaller than the frequencies themselves). In this case, the SI is effectively
suppressed without any high-frequency modulators.Comment: 13 pages, 8 figure
Photon storage in Lambda-type optically dense atomic media. I. Cavity model
In a recent paper [Gorshkov et al., Phys. Rev. Lett. 98, 123601 (2007)], we
used a universal physical picture to optimize and demonstrate equivalence
between a wide range of techniques for storage and retrieval of photon wave
packets in Lambda-type atomic media in free space, including the adiabatic
reduction of the photon group velocity, pulse-propagation control via
off-resonant Raman techniques, and photon-echo-based techniques. In the present
paper, we perform the same analysis for the cavity model. In particular, we
show that the retrieval efficiency is equal to C/(1+C) independent of the
retrieval technique, where C is the cooperativity parameter. We also derive the
optimal strategy for storage and, in particular, demonstrate that at any
detuning one can store, with the optimal efficiency of C/(1+C), any smooth
input mode satisfying T C gamma >> 1 and a certain class of resonant input
modes satisfying T C gamma ~ 1, where T is the duration of the input mode and 2
gamma is the transition linewidth. In the two subsequent papers of the series,
we present the full analysis of the free-space model and discuss the effects of
inhomogeneous broadening on photon storage.Comment: 16 pages, 2 figures. V2: significant changes in presentation, new
references, higher resolution of figure
Faddeev-type calculations of few-body nuclear reactions including Coulomb interaction
The method of screening and renormalization is used to include the Coulomb
interaction between the charged particles in the description of few-body
nuclear reactions. Calculations are done in the framework of Faddeev-type
equations in momentum-space. The reliability of the method is demonstrated. The
Coulomb effect on observables is discussed.Comment: Proceedings of the 4th Asia-Pacific Conference on Few-Body Problems
in Physics (APFB08), Depok, Indonesia, August 19 - 23, 2008, to be published
in Mod. Phys. Lett.
Production of a pion in association with a high-Q2 dilepton pair in antiproton-proton annihilation at GSI-FAIR
We evaluate the cross section for anti-p p -> l+ l- pi0 in the forward
direction and for large lepton pair invariant mass. In this kinematical region,
the leading-twist amplitude factorises into a short-distance matrix element,
long-distance dominated antiproton Distribution Amplitudes and proton to pion
Transition Distribution Amplitudes (TDA). Using a modelling inspired from the
chiral limit for these TDAs, we obtain a first estimate of this cross section,
thus demonstrating that this process can be measured at GSI-FAIR.Comment: Latex, 5 pages, 3 figure
Photon storage in Lambda-type optically dense atomic media. III. Effects of inhomogeneous broadening
In a recent paper [Gorshkov et al., Phys. Rev. Lett. 98, 123601 (2007)] and
in the two preceding papers [Gorshkov et al., Phys. Rev. A 76, 033804 (2007);
76, 033805 (2007)], we used a universal physical picture to optimize and
demonstrate equivalence between a wide range of techniques for storage and
retrieval of photon wave packets in homogeneously broadened Lambda-type atomic
media, including the adiabatic reduction of the photon group velocity,
pulse-propagation control via off-resonant Raman techniques, and
photon-echo-based techniques. In the present paper, we generalize this
treatment to include inhomogeneous broadening. In particular, we consider the
case of Doppler-broadened atoms and assume that there is a negligible
difference between the Doppler shifts of the two optical transitions. In this
situation, we show that, at high enough optical depth, all atoms contribute
coherently to the storage process as if the medium were homogeneously
broadened. We also discuss the effects of inhomogeneous broadening in solid
state samples. In this context, we discuss the advantages and limitations of
reversing the inhomogeneous broadening during the storage time, as well as
suggest a way for achieving high efficiencies with a nonreversible
inhomogeneous profile.Comment: 15 pages, 8 figures. V2: minor changes in presentation, new
references, higher resolution of figure
Photon storage in Lambda-type optically dense atomic media. II. Free-space model
In a recent paper [Gorshkov et al., Phys. Rev. Lett. 98, 123601 (2007)], we
presented a universal physical picture for describing a wide range of
techniques for storage and retrieval of photon wave packets in Lambda-type
atomic media in free space, including the adiabatic reduction of the photon
group velocity, pulse-propagation control via off-resonant Raman techniques,
and photon-echo based techniques. This universal picture produced an optimal
control strategy for photon storage and retrieval applicable to all approaches
and yielded identical maximum efficiencies for all of them. In the present
paper, we present the full details of this analysis as well some of its
extensions, including the discussion of the effects of non-degeneracy of the
two lower levels of the Lambda system. The analysis in the present paper is
based on the intuition obtained from the study of photon storage in the cavity
model in the preceding paper [Gorshkov et al., Phys. Rev. A 76, 033804 (2007)].Comment: 26 pages, 8 figures. V2: significant changes in presentation, new
references, higher resolution of figure
Interpolation of equation-of-state data
Aims. We use Hermite splines to interpolate pressure and its derivatives
simultaneously, thereby preserving mathematical relations between the
derivatives. The method therefore guarantees that thermodynamic identities are
obeyed even between mesh points. In addition, our method enables an estimation
of the precision of the interpolation by comparing the Hermite-spline results
with those of frequent cubic (B-) spline interpolation.
Methods. We have interpolated pressure as a function of temperature and
density with quintic Hermite 2D-splines. The Hermite interpolation requires
knowledge of pressure and its first and second derivatives at every mesh point.
To obtain the partial derivatives at the mesh points, we used tabulated values
if given or else thermodynamic equalities, or, if not available, values
obtained by differentiating B-splines.
Results. The results were obtained with the grid of the SAHA-S
equation-of-state (EOS) tables. The maximum difference lies in the range
from to , and difference varies from to
. Specifically, for the points of a solar model, the maximum
differences are one order of magnitude smaller than the aforementioned values.
The poorest precision is found in the dissociation and ionization regions,
occurring at K. The best precision is achieved at
higher temperatures, K. To discuss the significance of the
interpolation errors we compare them with the corresponding difference between
two different equation-of-state formalisms, SAHA-S and OPAL 2005. We find that
the interpolation errors of the pressure are a few orders of magnitude less
than the differences from between the physical formalisms, which is
particularly true for the solar-model points.Comment: Accepted for publication in A&
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