1,972 research outputs found
The two-pseudoscalar-meson decay of with twist-3 corrections
The decays of are discussed
within the standard and modified hard scattering approach when including the
contributions from twist-3 distribution amplitudes and wave functions of the
light pseudoscalar meson. A model for twist-2 and twist-3 distribution
amplitudes and wave functions of the pion and kaon with BHL prescription are
proposed as the solution to the end-point singularities. The results show that
the contributions from twist-3 parts are actually not power suppressed
comparing with the leading-twist contribution. After including the effects from
the transverse momentum of light meson valence-quark state and Sudakov factors,
the decay widths of the into pions or kaons are comparable with the
their experimental data.Comment: 31 pages, 5 figures, 3 table
Realistic Expanding Source Model for Invariant One-Particle Multiplicity Distributions and Two-Particle Correlations in Relativistic Heavy-Ion Collisions
We present a realistic expanding source model with nine parameters that are
necessary and sufficient to describe the main physics occuring during
hydrodynamical freezeout of the excited hadronic matter produced in
relativistic heavy-ion collisions. As a first test of the model, we compare it
to data from central Si + Au collisions at p_lab/A = 14.6 GeV/c measured in
experiment E-802 at the AGS. An overall chi-square per degree of freedom of
1.055 is achieved for a fit to 1416 data points involving invariant pi^+, pi^-,
K^+, and K^- one-particle multiplicity distributions and pi^+ and K^+
two-particle correlations. The 99-percent-confidence region of parameter space
is identified, leading to one-dimensional error estimates on the nine fitted
parameters and other calculated physical quantities. Three of the most
important results are the freezeout temperature, longitudinal proper time, and
baryon density along the symmetry axis. For these we find values of 92.9 +/-
4.4 MeV, 8.2 +/- 2.2 fm/c, and 0.0222 + 0.0096 / - 0.0069 fm^-3, respectively.Comment: 37 pages and 12 figures. RevTeX 3.0. Submitted to Physical Review C.
Complete preprint, including device-independent (dvi), PostScript, and LaTeX
versions of the text, plus PostScript files of all figures, are available at
http://t2.lanl.gov/publications/publications.html or at
ftp://t2.lanl.gov/publications/res
Gravitino perturbations in Schwarzschild black holes
We consider the time evolution of massless gravitino perturbations in
Schwarzschild black holes, and show that as in the case of fields of other
values of spin, the evolution comes in three stages, after an initial outburst
as a first stage, we observe the damped oscillations characteristic of the
quasinormal ringing stage, followed by long time tails. Using the sixth order
WKB method and Prony fitting of time domain data we determine the quasinormal
frequencies. There is a good correspondence between the results obtained by the
above two methods, and we obtain a considerable improvement with respect to the
previously obtained third order WKB results. We also show that the response of
a black hole depends crucially on the spin class of the perturbing field: the
quality factor becomes a decreasing function of the spin for boson
perturbations, whereas the opposite situation appears for fermion ones
HELAS and MadGraph with spin-3/2 particles
Fortran subroutines to calculate helicity amplitudes with massive spin-3/2
particles, such as massive gravitinos, which couple to the standard model and
supersymmetric particles via the supercurrent, are added to the HELAS (HELicity
Amplitude Subroutines) library. They are coded in such a way that arbitrary
amplitudes with external gravitinos can be generated automatically by MadGraph,
after slight modifications. All the codes have been tested carefully by making
use of the gauge invariance of the helicity amplitudes.Comment: 12 pages, 4 figures; sections rearranged, typos corrected, version to
appear in EPJ
Space-time extensions from space-time densities and Bose-Einstein correlations
Using a (3+1)-dimensional solution of the relativistic Euler-equations for
at 160 , space-time extensions of kaon emission zones are
calculated from space-time densities and compared to the inverse widths of
two-kaon Bose-Einstein correlation functions. The comparison shows a
satisfactory agreement and it is concluded that because of the Gaussian shape
of the kaon correlation functions, the space-time parameters of the kaon source
can be calculated directly from space-time densities. In the case of intensity
interferometry of identical pions this simplification is not recommended when
applying Gaussian fits because of the present strong effects of resonance
decays. The whole discussion is based on the assumption that hadron emission in
ultra-relativistic heavy-ion collisions is purely chaotic or that coherence is
at least negligible.Comment: 11 pages, 2 figures (distributed on 3 Postscript files
Diffractive vector meson electroproduction at small Bjorken within GPD approach
We study light vector meson electroproduction at small within the
generalized parton distributions (GPDs) model. The modified perturbative
approach is used, where the quark transverse degrees of freedom in the vector
meson wave function and hard subprocess are considered. Our results on the
cross section and spin observables are in good agreement with experimentComment: 6 pages, 5 figures, presented at Symmetries and Spin meeting, Prague,
8- 14 July, 200
Равновесие и динамика адсорбции паров воды на металлорганическом каркасе MOF-801
В работе представлены результаты исследования равновесия и динамики адсорбции паров воды на металлоорганическом каркасе MOF-801 с целью оценки потенциала его применения в системах адсорбционного охлаждения. Показано, что адсорбция воды на MOF-801 характеризуется S-образными изобарами IV типа по классификации ИЮПАК. В условиях типичного рабочего цикла адсорбционного холодильника (АХ) MOF-801 обменивает 0,21 г/г и может быть регенерирован при 80-85°С, что позволяет использовать источники низкотемпературной теплоты (солнечная энергия). Динамика адсорбции на гранулах MOF-801 в условиях рабочего цикла АХ происходит в режиме, при котором скорость процесса определяется отношением S/m площади поверхности теплопереноса S к массе адсорбента m. Эффективность и удельная мощность АХ с использованием пары "MOF-801-вода" достигают 0,67 и 2 кВт/кг соответственно, что представляет большой практический интерес
Hydrodynamical analysis of symmetric nucleus-nucleus collisions at CERN/SPS energies
We present a coherent theoretical study of ultrarelativistic heavy-ion data
obtained at the CERN/SPS by the NA35/NA49 Collaborations using 3+1-dimensional
relativistic hydrodynamics. We find excellent agreement with the rapidity
spectra of negative hadrons and protons and with the correlation measurements
in two experiments: at 200 and at 160 (preliminary
results). Within our model this implies that for () a
quark-gluon-plasma of initial volume 174 (24 ) with a lifetime 3.4
(1.5 ) was formed. It is found that the Bose-Einstein correlation
measurements do not determine the maximal effective radii of the hadron sources
because of the large contributions from resonance decay at small momenta. Also
within this study we present an NA49 acceptance corrected two-pion
Bose-Einstein correlation function in the invariant variable, .Comment: 21 pages, 11 Postscript figures (1 File, 775654 Bytes, has to be
requested for submission via e.mail from [email protected]
Various Models for Pion Probability Distributions from Heavy-Ion Collisions
Various models for pion multiplicity distributions produced in relativistic
heavy ion collisions are discussed. The models include a relativistic
hydrodynamic model, a thermodynamic description, an emitting source pion laser
model, and a description which generates a negative binomial description. The
approach developed can be used to discuss other cases which will be mentioned.
The pion probability distributions for these various cases are compared.
Comparison of the pion laser model and Bose-Einstein condensation in a laser
trap and with the thermal model are made. The thermal model and hydrodynamic
model are also used to illustrate why the number of pions never diverges and
why the Bose-Einstein correction effects are relatively small. The pion
emission strength of a Poisson emitter and a critical density
are connected in a thermal model by , and this fact
reduces any Bose-Einstein correction effects in the number and number
fluctuation of pions. Fluctuations can be much larger than Poisson in the pion
laser model and for a negative binomial description. The clan representation of
the negative binomial distribution due to Van Hove and Giovannini is discussed
using the present description. Applications to CERN/NA44 and CERN/NA49 data are
discussed in terms of the relativistic hydrodynamic model.Comment: 12 pages, incl. 3 figures and 4 tables. You can also download a
PostScript file of the manuscript from
http://p2hp2.lanl.gov/people/schlei/eprint.htm
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