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STAR focus: STAR uses weak bosons to probe the spin structure of the proton
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The STAR Collaboration has recently published,
“Measurement of the longitudinal spin asymmetries
for weak boson production in proton-proton
collisions at √s = 510 GeV,”
in
Physical Review D 99, 051102(R).
This paper reports on measurements of the
parity-violating asymmetry in the production of
positrons and electrons from decays of weak bosons
from collisions with one of the proton beams
polarized longitudinally. In 510 GeV center-of-mass
proton-proton collisions at RHIC, W+ bosons are
produced primarily in the interactions of up quarks
and down antiquarks, whereas W- bosons originate
from down quarks and up antiquarks. The
spin-asymmetry measurements of the decay positrons
thus provide sensitivity to the up quark and down
antiquark helicities in the proton, whereas the
decay electrons do so for the down quark and up
antiquark helicities. Combined, they make it
possible to delineate the light quark and antiquark
polarizations in the proton by flavor.
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Left: Longitudinal single-spin
asymmetries, AL,
for W± production as a
function of the positron or electron
pseudorapidity, ηe, for the
combined STAR 2011, 2012 and 2013 data samples for 25
< ET < 50GeV (points) in
comparison to theory expectations (curves and
bands). Right: The difference of the light
sea-quark polarizations as a function of x at a
scale of Q2 =
10(GeV/c)2. The green band shows the
NNPDFpol1.1 results and the blue hatched band shows
the corresponding distribution after the STAR 2013
W± data are included by reweighting.
These measurements provided one of the two initial
motivations for the spin-physics program at RHIC and
the data, shown in the left panel of the figure above,
are the final data from STAR on this topic. Shown are
the results from previously published data obtained in
2011 and 2012 combined with new results from the
dedicated RHIC run in 2013. As seen from the right
panel, the data have now reached a level of precision
that makes it possible, for the first time, to
conclude that the polarization of up antiquarks is
larger than that of the down antiquarks.
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Posted March 27, 2019
BNL News
Previous STAR Focus Features
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STAR focus: Polarization of Λ (Λ) hyperons along the beam
direction in Au+Au collisions at $\sqrt{s_{\rm{NN}}}$ = 200 GeV
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The STAR Collaboration has recently published
“Polarization of Λ (Λ) hyperons along the beam direction
in Au+Au collisions at collisions at $\sqrt{s_{\rm{NN}}}$ = 200 GeV”
in
Physical Review Letter 123, 132301.
This paper reports on the first ever measurements of the Λ hyperon polarization
along the beam direction in heavy-ion collisions.
In a non-central heavy-ion collision, the system expands stronger
in the reaction plane direction compared to that in the out-of-plane direction, a phenomenon known as elliptic flow.
Such nontrivial velocity fields lead to a non-zero vorticity component along the beam direction
dependent on the azimuthal angle of fluid elements relative to the reaction plane (see left figure), and therefore to particle spin polarization.
Spin polarization can be experimentally measured via hyperons parity-violating weak decay.
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Left:
A sketch illustrating the system created in a non-central heavy-ion collision
viewed in the transverse plane (x-y), showing stronger in-plane expansion (solid arrows)
and expected vorticities (open arrows). In this figure the colliding beams are
oriented along the z-axis and the x-z plane defines the reaction plane.
Right:
The second Fourier sine coefficient of the polarization of Λ and Λ along
the beam direction as
a function of centrality in Au+Au collisions at 200 GeV.
Results using Λ hyperons at 200 GeV exhibit Λ's emission angle dependence of the polarization
along the beam direction, as expected from elliptic flow, indicating a quadrupole pattern of
the vorticity z-component. Right figure presents a sine modulation of the polarization relative
to the reaction plane angle as a function of collision centrality. The observed phase of the sine modulation
is opposite to some theoretical predictions, e.g. a multi-phase transport model (AMPT) and viscous hydrodynamic model.
In contrast, the blast-wave model calculations representing the kinematic vorticity reproduce the modulation phase better.
These results together with the results of the global polarization
(Nature 548, 62 (2017),
PRC98, 014910 (2018))
may provide information on the relaxation time needed to convert the vorticity to particle polarization.
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Posted October 24, 2019
Previous STAR Focus Features
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STAR focus:
Measurements of inclusive $J/\psi$ suppression in Au+Au collisions at $\sqrt{s_{\rm{NN}}}$ = 200 GeV through the dimuon channel
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The STAR Collaboration has recently published "Measurements of inclusive $J/\psi$ suppression
in Au+Au collisions at $\sqrt{s_{\rm{NN}}}$ = 200 GeV through the dimuon channel at STAR"
in Phys. Lett. B 797 (2019) 134917.
This publication reports the first measurement of inclusive $J/\psi$ suppression at mid-rapidity
through the dimuon decay channel in Au+Au collisions at $\sqrt{s_{\rm{NN}}}$ = 200 GeV. It is made possible
thanks to the Muon Telescope Detector upgrade completed in 2014 at STAR. Among the various probes
used to study the existence and properties of the Quark Gluon Plasma (QGP) created in relativistic heavy-ion
collisions, quarkonia are considered a unique one. A fundamental feature of the QGP is that partons, instead
of hadrons, are the relevant degrees of freedom of the system. Quarkonia are expected to exist as hadrons
in the QGP until the Debye radius, which is inversely proportional to the medium temperature, becomes smaller
than the quarkonium size. Under such conditions, the color-screening effect would lead to dissociation of
the quarkonia in the medium. This can be observed experimentally through measurements of $J/\psi$ suppression in
heavy-ion collisions with respect to that in p+p collisions. Such a suppression is believed to be unambiguous
evidence of the QGP formation.
The figure below shows the $J/\psi$ RAA, used to quantify the suppression level, as a function of
centrality for pT > 0.15 GeV/c and pT > 5 GeV/c in Au+Au collisions
at $\sqrt{s_{\rm{NN}}}$ = 200 GeV. At both low and high pT, the $J/\psi$ RAA is seen to
decrease from peripheral to central collisions, consistent with increasing hot medium effects.
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Figure: $J/\psi$ RAA as a function of centrality above 0.15 (left) and 5 (right) GeV/c in Au+Au
collisions at $\sqrt{s_{\rm{NN}}}$ = 200 GeV, compared to those for Pb+Pb collisions at $\sqrt{s_{\rm{NN}}}$ = 2.76 TeV.
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For high-pT $J/\psi$, where the cold nuclear matter effects and the regeneration contribution are
expected to be minimal, the $J/\psi$ production in 0-10% central collisions is suppressed by a factor of 3.1, providing strong
evidence for the color-screening effect in a deconfined medium. Compared to similar measurements carried out for Pb+Pb collisions
at $\sqrt{s_{\rm{NN}}}$ = 2.76 TeV, the low-pT $J/\psi$'s are much more suppressed in central and semi-central collisions
at RHIC than at the LHC, likely due to the smaller charm quark production cross-section and thus smaller regeneration contribution at
RHIC. On the Other hand, there is a hint that the high-pT $J/\psi$ RAA is systematically higher at
RHIC for semi-central bins. This could be because the temperature of the medium created at the LHC is higher than that at RHIC,
leading to a higher dissociation rate. The new results presented in this publication could help constrain model calculations and
deepen our understanding of the QGP properties.
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Posted October 24, 2019
Previous STAR Focus Features
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STAR focus:
Precise Measurement of the Mass Difference and the Binding Energy of the Hypertriton and Antihypertriton at STAR
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In March 2020, the STAR Collaboration published "Measurement of the mass difference and the binding energy of the
hypertriton and antihypertriton" in
Nature Physics.
In this paper, we present two measurements from gold-gold collisions at a center-of-mass energy per nucleon pair of
$\sqrt{s_{NN}} = 200$ GeV: the relative mass difference between $\rm^3_\Lambda H$ (the hypertriton) and $\rm^3_{\bar{\Lambda}}\overline{H}$
(the antihypertriton) (see Fig. 1), as well as the $\Lambda$ hyperon binding energy for $\rm^3_\Lambda H$ and $\rm^3_{\bar{\Lambda}}\overline{H}$
(see Fig. 2). The hypernucleus $\rm^3_{\Lambda}H$ is reconstructed through its mesonic decay channels
$\rm^3_{\Lambda}H \rightarrow {^3}He + \pi^-$ (2-body decay) and $\rm^3_{\Lambda}H \rightarrow$ $ d + p + \pi^-$ (3-body decay).
The significance $S/ \sqrt{S+B}$, where $S$ is signal counts and $B$ is background counts in the invariant mass window
$2.986 - 2.996$ GeV$/c^{2}$, is 11.4 for $^3_\Lambda$H and 6.4 for $\rm^3_{\bar{\Lambda}}\overline{H}$.
The signal counts from 2-body/3-body decay channels are about 121/35 for $^3_\Lambda$H and 36/21 for $\rm^3_{\bar{\Lambda}}\overline{H}$,
respectively.
According to the CPT theorem, which states that the combined operation of charge conjugation, parity transformation and time reversal must be
conserved, particles and their antiparticles should have the same mass and lifetime but opposite charge and magnetic moment. Here, we test CPT
symmetry in a nucleus containing a strange quark, more specifically in the hypertriton. A comparison of the masses of the hypertriton and the
antihypertriton allows us to test CPT symmetry in a nucleus with strangeness for the first time, and we observe no deviation from the expected
exact symmetry with precision of 10$^{-4}$.
This hypernucleus is the lightest one yet discovered and consists of a proton, a neutron, and a $\Lambda$ hyperon. We measure the
$\Lambda$ hyperon binding energy $B_{\Lambda}$ for the hypertriton, and find that it differs from the widely used value and from
predictions, where the hypertriton is treated as a weakly bound system. Our results place stringent constraints on the hyperon-nucleon
interaction, and have implications for understanding neutron star interiors, where strange matter may be present.
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Fig 1: Measurements of the relative mass-to-charge ratio differences between nuclei and antinuclei. The current measurement of the
relative mass difference ${\Delta m}/m$ between $^3_\Lambda$H and $\rm^3_{\bar{\Lambda}}\overline{H}$ constrained
by the existing experimental limits for decay daughters is shown by the red star marker. The green point is the new $^{3}$He result after
applying the constraint provided by the present $^{3}_{\Lambda}$H result. The differences between $d$ and $\bar{d}$ and
between $^3$He and $\rm^3\overline{He}$ measured by the ALICE collaboration are also shown. The two $^3$He - $\rm^3\overline{He}$ points
are staggered vertically for visibility. The dotted vertical line at zero is the expectation from CPT invariance. The horizontal error bars
represent the sum in quadrature of statistical and systematic uncertainties.
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Posted March 10, 2020
Read More
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code of conduct
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The STAR Collaboration
believes that our scientific
mission is best achieved by
building a culture of
inclusion...
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Incoming events
STAR Collaboration Meeting Mar. 11-15, 2020, Berkeley, UC Clark Kerr Campus
Past events
STAR Pre-QM Meeting Oct. 29 - Nov. 1, 2019, Qingdao
STAR Collaboration Meeting Aug. 19, 2019, Cracow
STAR Collaboration Meeting Mar. 29 - Apr 2, 2019, BNL
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ALICE-STAR Indian Meeting Sep. 17-21, 2018, NISER
STAR Regional Meeting Oct. 31 - Nov. 2, 2018, USTC
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STAR Collaboration Meeting July 16-21, 2018, Lehigh University
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