2,423 research outputs found
HR Analytics: Talent Acquisition
[Excerpt] HR Analytics is becoming increasingly important as new technologies, software and new methods of data collection are revolutionizing the HR function. One area in which analytics tools are particularly flourishing is the talent acquisition space. With an increasingly competitive talent market, talent acquisition presents itself as an area in which analytics tools can greatly supplement decision making for these 3 reasons: here are many measurable, verifiable metrics to measure in terms of sources of talent, candidate qualifications, and the efficacy of the recruitment process here is an abundance of sources from which to collect data (Online sources, interviews, etc.) With the increased importance of sourcing the correct talent, the opportunity to use analytics tools to make better decisions is quite compelling
Given these reasons, talent acquisition presents itself as an opportunity for organizations to build their analytics capabilities while driving measurable business outcomes and improvements to their organization. As evidenced in the above graphic, many organizations are already undertaking these changes or considering changes in the near future
Recent results of the STAR high-energy polarized proton-proton program at RHIC at BNL
The STAR experiment at the Relativistic Heavy-Ion Collider (RHIC) at
Brookhaven National Laboratory (BNL) is carrying out a spin physics program
colliding transverse or longitudinal polarized proton beams at
GeV to gain a deeper insight into the spin structure and
dynamics of the proton. These studies provide fundamental tests of Quantum
Chromodynamics (QCD).
One of the main objectives of the STAR spin physics program is the
determination of the polarized gluon distribution function through a
measurement of the longitudinal double-spin asymmetry, , for various
processes. Recent results will be shown on the measurement of for
inclusive jet production, neutral pion production and charged pion production
at GeV. In addition to these measurements involving longitudinal
polarized proton beams, the STAR collaboration has performed several important
measurements employing transverse polarized proton beams. New results on the
measurement of the transverse single-spin asymmetry, , for forward
neutral pion production and the first measurement of for mid-rapidity
di-jet production will be discussed.Comment: 8 pages, 5 figures, Invited talk given at the 17th International Spin
Physics Symposium (SPIN 2006), October 2006, Kyoto, Japa
Selected results on Strong and Coulomb-induced correlations from the STAR experiment
Using recent high-statistics STAR data from Au+Au and Cu+Cu collisions at
full RHIC energy I discuss strong and Coulomb-induced final state interaction
effects on identical () and non-identical () particle
correlations. Analysis of correlations reveals the strong and
Coulomb-induced FSI effects allowing for the first time to estimate space
extension of and sources and average shift between them. Source
imaging technique providing clean separation of these effects from effects due
to the source function itself is applied to one-dimensional relative momentum
correlation function of identical pions. For low momentum pions and/or
non-central collisions large departure from a single-Gaussian shape is
observed
Longitudinal Spin Asymmetry and Cross Section of Inclusive pi0 Production in Polarized p+p Collisions at RHIC
We present the first measurement of the cross section and the double
longitudinal spin asymmetry of inclusive pi0 production in polarized p+p
collisions at Sqrt(s) = 200 GeV at mid-rapidity with the STAR detector, using
the barrel electromagnetic calorimeter. The measured cross section is compared
to NLO pQCD calculations and can provide constraints on the pion fragmentation
functions. Fragmentation is studied directly by measuring the momentum fraction
of pi0 in jets, a quantity that is affected by the fragmentation process and
jet reconstruction effects. The double longitudinal spin asymmetry is compared
to NLO pQCD calculations based on different assumptions for the gluon
polarization in the nucleon to provide constraints on delta g/g. At the present
level of statistics the measured asymmetry disfavors a large positive gluon
polarization, but can not yet distinguish between other scenarios.Comment: 4 pages, 2 figures, submitted to the proceedings of the 17th
International Spin Physics Symposium (SPIN2006), Kyoto, Japan, October 2 to
7, 200
Measurements of Transverse Spin Effects with the Forward Pion Detector of STAR
Measurements by the STAR collaboration of neutral pion production at large
Feynman x (x_F) in the first polarized proton collisions at GeV
were reported previously. Cross sections measured at , 3.8 and 4.0
are found to be consistent with next-to-leading order perturbative QCD
calculations. The analyzing power is consistent with zero at negative x_F and
at positive x_F up to ~0.3, then grows more positive with increasing x_F. This
behavior can be described by phenomenological models including the Sivers
effect, the Collins effect or higher twist contributions in the initial and
final states. Forward calorimetry at STAR has been extended, and there are
plans for further expansion. An integrated luminosity of 6.8 pb^ with
average beam polarization of 60% from online polarimetry measurements was
sampled with the upgraded FPD in the 2006 RHIC run. This data sample will allow
for a detailed map of the \pi^0 analyzing power over kinematic variables
bounded by 0.3 < x_F < 0.6 and 1.2 < p_T < 5.0 GeV/c at GeV. The
expanded FPD has observed multi-photon final states expected to have "jet-like"
characteristics. The transverse spin dependence of jet-like events can
discriminate between the Collins and Sivers effects and lead to further
progress in understanding the origin of single spin asymmetries in forward
particle production. Data were also obtained at GeV for x_F ->
1 to test predictions based on phenomenological fits to earlier STAR results.
Recent results, the status of the analysis of 2006 run data and near-term plans
will be discussed.Comment: 4 pages, 3 figures, to be published in the proceedings of the 17th
International Spin Physics Symposium (SPIN2006), October 2-7, 2006, Kyoto,
Japa
Measurement of Sivers Asymmetries for Di-jets in \sqrt{s}=200 GeV pp Collisions at STAR
Measurement of the transverse spin dependence of the di-jet opening angle in
pp collisions at sqrt{s}=200 GeV has been performed by the STAR collaboration.
An analyzing power consistent with zero has been observed over a broad range in
pseudorapidity sum of the two jets with respect to the polarized beam
direction. A non-zero (Sivers) correlation between transverse momentum
direction of partons in the initial state and transverse spin orientation of
the parent proton has been previously observed in semi-inclusive deep inelastic
scattering (SIDIS).
The present measurements are much smaller than deduced from predictions made
for STAR di-jets based on non-zero quark Sivers functions deduced from SIDIS,
and furthermore indicate that gluon Sivers asymmetries are comparably small.Comment: 4 pages, 3 figures, talk presented at SPIN 2006, Kyoto, October 200
Longitudinal Double Spin Asymmetry in Inclusive Jet Production at STAR
This contribution reports on the first measurement of the longitudinal
double-spin asymmetry for the inclusive production of jets in
polarized proton-proton collisions at . The data
were collected with STAR at RHIC in the years 2003 and 2004, and correspond to
a sampled integrated luminosity of with beam
polarizations up to 45%. The results on cover jet transverse momenta
and agree with perturbative QCD evaluations
based on deep-inelastic scattering parametrizations for the gluon polarization
in the proton. The results disfavor large positive gluon polarization in the
polarized proton.Comment: 5 pages, 1 figur
New Challenges to Hydrodynamics from Azimuthal Anisotropy at RHIC
This paper presents ratio as a function of transverse
momentum (), pseudorapidity () and collision centrality in Au+Au
collisions at GeV using the STAR detector at the
Relativistic Heavy Ion Collider (RHIC). It is found that is
larger than Hydrodynamic calculations, the centrality and transverse dependence
of this ratio can not be fully described by Hydrodynamics, and the
pseudorapidity dependence is opposite to what one expects from Hydrodynamics.
The dependence of is also presented. It is found that
for changes sign, and two possible explanations of
the sign change are discussed.Comment: 4 pages, 3 figures. CIPANP 06 proceedin
An Integrated Tracker for STAR
The STAR experiment at the Relativistic Heavy Ion Collider RHIC studies the
new state of matter produced in relativistic heavy ion collisions and the spin
structure of the nucleon in collisions of polarized protons. In order to
improve the capabilities for heavy flavor measurements and the reconstruction
of charged vector bosons an upgrade of the tracking system both in the central
and the forward region is pursued. The integrated system providing high
resolution tracking and secondary vertex reconstruction capabilities will use
silicon pixel, strip and GEM technology.Comment: 4 pages, 2 figures, to be published in the Proceedings of the 9th
Conference on the Intersections of Particle and Nuclear Physics (CIPANP
2006), Rio Grande, Puerto Rico, May 30 - June 3, 200
Energy and system size dependence of elliptic flow: using rapidity gaps to suppress non-flow contribution
In this talk I present new STAR results on measurements of integrated
elliptic flow at midrapidity in Au+Au and Cu+Cu collisions at
200 and 62 GeV energies. These results have been obtained from
azimuthal correlations between particles in the main STAR TPC and two forward
TPCs, and are to a large extent free from so-called non-flow correlations.
These results along with the previously reported values of ``participant''
eccentricity taking into account eccentricity fluctuations are used for testing
the v_2/\eps scaling, which is found to hold relatively well.Comment: 4 pages. Talk at CIPANP 2006, 9th Conference on the Intersections of
Particle and Nuclear Physics, May 30-June 3, 2006, Rio Grande, Puerto Ric
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