7,750 research outputs found
Shadowing and Absorption Effects on J/psi Production in dA Collisions
We study medium modifications of J/psi production in cold nuclear media in
deuterium-nucleus collisions. We discuss several parameterizations of the
modifications of the parton densities in the nucleus, known as shadowing, an
initial-state effect. We also include absorption of the produced J/psi by
nucleons, a final-state effect. Both spatially homogeneous and inhomogeneous
shadowing and absorption are considered. We use the number of binary
nucleon-nucleon collisions as a centrality measure. Results are presented for
d+Au collisions at sqrt{S_{NN}} = 200 GeV and for d+Pb collisions at
sqrt{S_{NN}} = 6.2 TeV. To contrast the centrality dependence in pA and dA
collisions, we also present pPb results at sqrt{S_{NN}} = 8.8 TeV.Comment: 22 pages, 11 figures, uses revte
Optical SETI: A Spectroscopic Search for Laser Emission from Nearby Stars
We have searched for nonastrophysical emission lines in the optical spectra
of 577 nearby F, G, K, and M main-sequence stars. Emission lines of
astrophysical origin would also have been detected, such as from a
time--variable chromosphere or infalling comets. We examined ~20 spectra per
star obtained during four years with the Keck/HIRES spectrometer at a
resolution of 5 km/s, with a detection threshold 3% of the continuum flux
level. We searched each spectrum from 4000-5000 angstroms for emission lines
having widths too narrow to be natural from the host star, as well as for lines
broadened by astrophysical mechanisms. We would have detected lasers that emit
a power, P>60 kW, for a typical beam width of ~0.01 arcsec (diffraction-limit
from a 10-m aperture) if directed toward Earth from the star. No lines
consisstent with laser emission were found.Comment: 27 pages, 11 figures, uses aastex.st
Bose-Einstein condensation of alkaline earth atoms: {Ca}
We have achieved Bose-Einstein condensation of Ca, the first for an
alkaline earth element. The influence of elastic and inelastic collisions
associated with the large ground state s-wave scattering length of Ca
was measured. From these findings, an optimized loading and cooling scheme was
developed that allowed us to condense about atoms after laser
cooling in a two-stage magneto-optical trap and subsequent forced evaporation
in a crossed dipole trap within less than 3 s. The condensation of an alkaline
earth element opens novel opportunities for precision measurements on the
narrow intercombination lines as well as investigations of molecular states at
the S--P asymptotes
New Models of General Relativistic Static Thick Disks
New families of exact general relativistic thick disks are constructed using
the ``displace, cut, fill and reflect'' method. A class of functions used to
``fill'' the disks is derived imposing conditions on the first and second
derivatives to generate physically acceptable disks. The analysis of the
function's curvature further restrict the ranges of the free parameters that
allow phisically acceptable disks. Then this class of functions together with
the Schwarzschild metric is employed to construct thick disks in isotropic,
Weyl and Schwarzschild canonical coordinates. In these last coordinates an
additional function must be added to one of the metric coefficients to generate
exact disks. Disks in isotropic and Weyl coordinates satisfy all energy
conditions, but those in Schwarzschild canonical coordinates do not satisfy the
dominant energy condition.Comment: 27 pages, 14 figure
Dissociation rates of J/psi's with comoving mesons - thermal vs. nonequilibrium scenario
We study J/psi dissociation processes in hadronic environments. The validity
of a thermal meson gas ansatz is tested by confronting it with an alternative,
nonequilibrium scenario. Heavy ion collisions are simulated in the framework of
the microscopic transport model UrQMD, taking into account the production of
charmonium states through hard parton-parton interactions and subsequent
rescattering with hadrons. The thermal gas and microscopic transport scenarios
are shown to be very dissimilar. Estimates of J/psi survival probabilities
based on thermal models of comover interactions in heavy ion collisions are
therefore not reliable.Comment: 12 pages, 6 figure
Shadowing Effects on the Nuclear Suppression Factor, R_dAu, in d+Au Interactions
We explore how nuclear modifications to the nucleon parton distributions
affect production of high transverse momentum hadrons in deuteron-nucleus
collisions. We calculate the charged hadron spectra to leading order using
standard fragmentation functions and shadowing parameterizations. We obtain the
d+Au to pp ratio both in minimum bias collisions and as a function of
centrality. The minimum bias results agree reasonably well with the BRAHMS data
while the calculated centrality dependence underestimates the data and is a
stronger function of p_T than the data indicate.Comment: 18 pages, 3 figures, final version, Phys. Rev. C in pres
Investigation of Normalization Methods using Plasma Parameters for Laser Induced Breakdown Spectroscopy (LIBS) under simulated Martian Conditions
Laser Induced Breakdown Spectroscopy data need to be normalized, especially in the field of planetary exploration We investigated plasma parameters as temperature and electron density for this purpose
The effect of bedrest on various parameters of physiological function. part xiv- effect of bedrest on plasma levels and urinary excretion of 17-hydroxycorticosteroids
Bed rest effect on plasma levels and urinary excretion of hydroxycorticosteroid
Impact parameter dependence of the nuclear modification of J/psi production in d+Au collisions at sqrt(S_NN) = 200 GeV
The centrality dependence of sqrt(s_NN)= 200 GeV d+Au {J/\psi} data, measured
in 12 rapidity bins that span -2.2 < y < 2.4, has been fitted using a model
containing an effective absorption cross section combined with EPS09 NLO
shadowing. The centrality dependence of the shadowing contribution was allowed
to vary nonlinearly, employing a variety of assumptions, in an effort to
explore the limits of what can be determined from the data. The impact
parameter dependencies of the effective absorption cross section and the
shadowing parameterization are sufficiently distinct to be determined
separately. It is found that the onset of shadowing is a highly nonlinear
function of impact parameter. The mid and backward rapidity absorption cross
sections are compared with lower energy data and, for times of 0.05 fm/c or
greater, data over a broad range of collision energies and rapidities are well
described by a model in which the absorption cross section depends only on time
spent in the nucleus.Comment: 11 pages, 11 figures. Expanded discussion of methods, and added
extensive comparison of effective absorption cross sections with lower energy
data, and with theory. Corrected minor typos in table 1, corrected typos in
best fit parameters for Fig.
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