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STAR focus: Observation of the Antimatter Hypernucleus $^4_{\bar{\Lambda}}\overline{\hbox{H}}$
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Matter-antimatter asymmetry is a research topic of fundamental interest, as it is the basis for the observed dominance of matter over antimatter in the universe. High energy nuclear collisions create conditions similar to the Universe microseconds after the Big Bang, with comparable amounts of matter and antimatter. Much of the antimatter created escapes the rapidly expanding fireball without annihilation, making such collisions an effective experimental tool to create heavy antimatter nuclear objects and study their properties.
In this work, we report the first observation of the antimatter hypernucleus $^4_{\bar{\Lambda}}\overline{\hbox{H}}$, composed of a Λ, an antiproton and two antineutrons. This discovery was made through its two-body decay channel $^4_{\bar{\Lambda}}\overline{\hbox{H}} {\rightarrow}^4\overline{\hbox{He}}+\pi^+$ in the STAR experiment at the Relativistic Heavy Ion Collider.
We use Kalman Filter algorithm to analyse the data totaling 6.6 billion collision events in the Au+Au, Ru+Ru, and Zr+Zr collisions with the collision energy $\sqrt{s_{NN}}=200$GeV, as well as U+U collisions with the collision energy of $\sqrt{s_{NN}}=193$GeV. We obtained 15.6 signal candidates for the antimatter hypernucleus ${}^{4}_{\bar{\Lambda}}\overline{\hbox{H}}$, with the estimated background counts 6.4 and significance of 4.7.
We also obtained 941 ${}^{3}_{\Lambda}\hbox{H}$ signal candidates, 637 ${}^{3}_{\bar{\Lambda}}\overline{\hbox{H}}$ signal candidates and 24.4 $^4_\Lambda\hbox{H}$ signal candidates using the same method.
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Figure: Invariant-mass distributions of $^3\hbox{He}+\pi^-$ (A), $^3\overline{\hbox{He}}+\pi^+$ (B), $^4\hbox{He}+\pi^-$ (C) and $^4\overline{\hbox{He}}+\pi^+$ (D).} The solid bands mark the signal invariant-mass regions. The obtained signal count ($N_{\rm Sig}$), background count ($N_{\rm Bg}$), and signal significances ($Z_{\rm count}$ and $Z_{\rm shape}$) are listed in each panel.
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Comparing lifetimes between a particle and its corrsponding antiparticle is an important experimental way to test the $CPT$ symmetry and to search for new mechanisms that cause this matter and antimatter asymmetry. In this work, we measured the lifetimes of ${}^{3}_{\Lambda}\hbox{H}$, ${}^{3}_{\bar{\Lambda}}\overline{\hbox{H}}$, ${}^{4}_{\Lambda}\hbox{H}$, and ${}^{4}_{\bar{\Lambda}}\overline{\hbox{H}}$. The lifetime difference between the hypernuclei and antihypernuclei was compared and we haven't found the CPT symmetry broken within the measurement uncertainty.
Various production yield ratios among (anti)hypernuclei and (anti)nuclei are measured. We found $\left(^3\overline{\hbox{He}}/^3\hbox{He}\right)\times\left(\bar{p}/p\right)\approx ^4\overline{\hbox{He}}/^4\hbox{He}$ and $\left(^3_{\bar{\Lambda}}\overline{\hbox{H}}/^3_{\Lambda}\hbox{H}\right)\times\left(\bar{p}/p\right) \approx ^4_{\bar{\Lambda}}\overline{\hbox{H}}/^4_{\Lambda}\hbox{H}$, these agree with the thermal model and coalescence picture predictions. And $^4_{\Lambda}\hbox{H}/^4\hbox{He}$ and $^4_{\bar{\Lambda}}\overline{\hbox{H}}/^4\overline{\hbox{He}}$ is expected to be about 4 times higher than $^3_{\Lambda}\hbox{H}/^3\hbox{He}$ and $^3_{\bar{\Lambda}}\overline{\hbox{H}}/^3\overline{\hbox{He}}$, respectively, hinting that $^4_{\Lambda}\hbox{H}$ has an excited state with spin 1. These measurements shed light on their production mechanism.
This work has been published by NATURE in August 2024.
Posted Aug 26, 2024
Previous STAR Focus Features
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STAR focus: Hyperon polarization along the beam direction relative to the second and third harmonics event planes in isobar collisions at √sNN = 200 GeV
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Polarization phenomena in heavy-ion collisions has drawn great attention since the observation of hyperon global polarization,
the non-zero average spin polarization of produced particles along the orbital angular momentum of colliding nuclei.
The STAR Collaboration measurement of the polarization along the beam direction relative to the second harmonic event plane,
indicated the local vorticity due to the elliptic flow (stronger collective expansion in in-plane than in out-of-plane directions).
These experimental results being in contradiction to the hydrodynamical and transport model predictions based on thermal vorticity,
posed the "spin sign puzzle" in heavy-ion collisions. The contribution from thermal shear is recently found to be important
to explain the data but the intense discussion is still ongoing to solve the puzzle.
Recently, the STAR Collaboration published a paper entitled "Hyperon polarization along the beam direction
relative to the second and third harmonics event planes in isobar collisions
at √sNN = 200 GeV"
in Physical Review Letter131, 202301 (2023).
Our new study extended the polarization measurements due to vorticity originating in the triangular flow, thus providing new independent information.
As shown in the figure below, Λ polarization along the beam direction relative to the triangluar flow plane (third harmonic event plane)
is found to be similar in phase to the result with the second harmonic event plane, with magnitude exhibiting increasing trend towards peripheral collisions.
These results indicate that complex vortical structures are created in heavy-ion collisions. Our results are compared with hydrodynamic model calculations
with two different implementations of the thermal shear leading to the opposite sign of polarization and require further investigation.
Our new data provide important inputs for resolving the spin puzzle and better understanding of the spin dynamics.
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Figure:
Centrality dependence of Λ hyperon polarization along the beam direction relative to the second and third harmonic
event planes in isobar Ru+Ru and Zr+Zr collisions at 200 GeV.
Solid bands show hydrodynamic model calculations with contribution from the shear-induced-polarization
in two different implementations (SIPBBP and SIPLY).
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Posted Jan 7, 2024
Previous STAR Focus Features
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STAR focus: Reaction plane correlated triangular flow in Au + Au Collisions at $\sqrt{s_{\mathrm{NN}}}$ = 3 GeV
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One of the primary objectives of the Beam Energy Scan II (BES II), undertaken by the STAR collaboration, is to identify and study the transition from hadronic matter to the Quark Gluon Plasma (QGP). A critical aspect of this research is to discern how nuclear matter transforms from a state of high baryon density nucleons in low-energy heavy ion collisions to a QGP in higher energy collisions. BES II allows us to study this transition by measuring anisotropic flow at various collision energies and observing how the expansion of the medium produced by the collisions changes. Anisotropic flow describes the shape and direction of expansion of the medium produced in heavy-ion collisions, and triangular flow ($v_{3}$) describes the strength of a triangular component during that expansion. In past reports from energies above $\sqrt{s_{\mathrm{NN}}}=27$ GeV, $v_3$ was determined to arise from a random triangular arrangement during some collisions. This description implies that $v_3$ will have no correlation to the reaction plane of collisions as the orientation of the triangle fluctuates with no preferred angle.
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Figure: Measurement of triangular flow as a function of center of mass rapidity for protons in 3 GeV Au+Au collisions at RHIC. The solid markers show the measurements from data in three centrality bins and the open markers are a mirror image of the measrements to showcase the likely behavior in a larger rapidity range. The solid lines show predictions from an identical measurement using the JAM simulation when including a baryon density dependent potential in the equation of state.
STAR has recently published measurements of $v_3$ from Au+Au collisions at the lowest STAR energy of $\sqrt{s_{\mathrm{NN}}}=3.0$ GeV. It was found that protons exhibit a non-zero $v_3$ signal that is correlated to the reaction plane, revealing a stark difference between $v_3$ at low and high energies. This report also includes comparisons to predictions of $v_3$ by the JAM simulation in order to explain the source of this signal. A new triangular arrangement was found at this low energy, and it was discovered that there is a strong connection between this low energy $v_3$ and the equation of state for the medium produced in collisions. This new form of $v_3$ could be a useful tool for studying the equation of state and the transition between hadronic matter and the QGP.
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Posted April 22, 2024
Previous STAR Focus Features
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STAR focus: Cross Section and Transverse Single Spin Asymmetry of Z Boson from 510 GeV p+p Collisions
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Nuclear science focuses on the origin and structure of the nucleus and the nucleons within it, which
account for essentially all the mass of the visible universe. Half a century of investigations has revealed
that nucleons themselves are composed of quarks, bound together by gluons, and have led to the
development of the fundamental theory of Quantum Chromo-Dynamics (QCD). Recent-generation
colliders have precisely measured the collinear parton distributions (1 dimension) inside the nucleon
along the longitudinal direction, while the investigation of nucleon structure in transverse momentum and
space has been limited. From transverse momentum dependent parton distributions (TMDs) we can obtain
an “image” of the proton structure in transverse as well as in longitudinal momentum space (2+1
dimensions).
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Figure:Differential cross section of the Z boson as a function of its transverse momentum (left) and
transverse single spin asymmetry of the Z boson (right).
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The STAR Collaboration has recently published “Measurements of the Z boson cross section and
transverse single spin asymmetry in 510 GeV p+p collisions” in Phys. Lett. B 854 (2024) 138715 . In this
Letter, we report the first measurement of the Z boson differential cross section as a function of its
transverse momentum in p+p collisions at a center-of-mass energy of 510 GeV, shown in the left panel of
the above figure. It provides important constraints on the evolution of the TMDs in phase space. We also
report the precision measurement of the Z boson transverse single spin asymmetry (TSSA) in transversely
polarized p+p collisions at 510 GeV, shown in the right panel of the above figure. The TSSA of the Z
boson is sensitive to one of the polarized TMDs, the Sivers function, which is predicted to have the
opposite sign in p+p → W/Z + X compared to that which enters in semi-inclusive deep inelastic
scattering. This non-universality of the Sivers function is a fundamental prediction from the gauge
invariance of QCD. The experimental verification of this sign change hypothesis is a crucial measurement
in hadronic physics and provides an important test of QCD factorization. So far, the STAR result cannot
conclusively verify the prediction with the current statistics (340 $pb^{-1}$ ). The precision of the TSSA
measurement will be improved using an additional 400 $pb^{−1}$ sample of p+p data at 508 GeV that STAR
collected in 2022.
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Posted May 24, 2024
Previous STAR Focus Features
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recent news
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September 5, 2024
Please join us in congratulating Dr. Xiaofeng Wang, from Shandong
University, who recently successfully defended her Ph.D. thesis, called
"The study of γγ → e+e− process in peripheral
Au+Au collisions at RHIC”.
Her co-advisors were Profs. Zhangbu Xu, Chi Yang, and Daniel Brandenburg.
Xiaofeng will continue as a postdoc at OSU.
Congratulations, Dr. Wang, and many thanks, Zhangbu, Chi, and Daniel for
your continued support in mentoring the next generation of physicists!
August 12, 2024
We are happy to announce the debut of the STAR Early Career Awards. With
these awards, the Collaboration wants to recognize and honor our
hardworking students and postdocs for their outstanding work and dedication
to service tasks.
Renee Fatemi has kindly agreed to be the inaugural chair of the STAR Early
Career Awards Committee. Once per year, the committee will call for
nominations and select awardees. We will honor them at a dedicated Award
Ceremony during the Fall/Winter Collaboration Meeting.
We want to thank Renee and the committee members Helen Caines, JH Lee, and
Jerome Lauret for serving on this committee and look forward to recognizing
the important work that many do for our collaboration!
June 20, 2024
Please join us in congratulating Dr. Ziyang Li and Dr. Kaifeng Shen,
both from USTC, who recently successfully defended their Ph.D. theses.
- Dr. Ziyang Li’s thesis was titled "Study of very low pT
J/psi production in Au+Au collisions at 200 GeV with STAR experiment”
- Dr. Kaifeng Shen’s thesis was titled "Measurements of e+e- and J/psi
production in heavy-ion collisions at RHIC”
Their co-advisors were Prof. Zebo Tang, Prof. Wangmei Zha, and Dr. Rongrong
Ma.
We wish them both all the best in their future careers!
Congratulations, Dr. Li and Dr. Shen, and many thanks, Zebo, Wangmei, and
Rongrong, for your continued support in mentoring the next generation of
physicists.
May 28, 2024
Please join us in congratulating Dr. YingYing Shi, Dr. Yike Xu, and Dr. Yi
Yu from Shandong University, who have all successfully defended their
Ph.D. theses on May 22, 2024:
- YingYing Shi’s PhD thesis is titled "R&D of Forward sTGC Tracker at
RHIC-STAR” and was supervised by Prof. Chi Yang;
- Yike Xu’s PhD thesis is titled "Measurement of Transverse Single Spin
Asymmetry of Hardron and Transverse Polarization Transfer of in Proton
Proton Collisions at RHIC-STAR” and was supervised by Prof. Qinghua Xu;
- Yi Yu’s PhD thesis is titled "Measurements of Longitudinal Double Spin
Asymmetry and Spin Transfer in Polarized Proton-Proton Collisions at
RHIC-STAR” and was supervised by Prof. Qinghua Xu.
All three are looking for jobs in multiple fields, including a postdoc
position (Yi Yu).
Congratulations, Dr. Shi, Dr. Xu, and Dr. Yu!
Many thanks, Chi and Qinghua, for your continued support in mentoring the
next generation of physicists.
May 18, 2024
Please join us in congratulating Dr. Hui Liu from CCNU, who, on May 18,
successfully defended her Ph.D. thesis, "Production of Protons and Light
Nuclei in Au+Au Collisions at 3 GeV with the STAR Detector at RHIC.” Her
supervisors were Profs. Xiaofeng Luo, Norbert Herrmann, and Nu Xu. Hui will
continue her career in physics research as a faculty member at Huzhou
University. We wish her all the best in her future career.
Congratulations, Dr. Liu, and many thanks, Xiaofeng, for your continued
support in mentoring the next generation of physicists.
March 13, 2024
Please join us in congratulating Dr. Jagbir Singh from Panjab University in
Chandigarh, who, on February 16, 2024, successfully defended his Ph.D.
thesis, "Investigation Of Elliptic Flow And Chiral Magnetic Effect With The
Star Detector.” His supervisors were Drs. M.M. Aggarwal and A.K. Bhati.
Jabgbir plans on continuing in academia, and we wish him all the best.
Congratulations, and many thanks to Dr. M.M. Aggarwal and Dr. A.K. Bhati.
for their continued contribution to educating the next generation of
physicists.
March 13, 2024
Please join us in congratulating Dr. Yiding Han from Rice University
(Houston, TX), who, on March 5, 2024, successfully defended his Ph.D.
thesis, "Thermal dielectron measurements in Au+Au collisions at sqrt(sNN) =
14.6, and 19.6 GeV with the STAR experiment." His supervisor was Prof.
Frank Geurts (Rice University). Yiding will continue his career in medical
physics at Baylor College of Medicine. We wish him all the best in his
future career.
March 4, 2024
Please join us in congratulating Dr. Lukas Kramarik from Czech Technical
University in Prague, who, on February 28, 2024, successfully defended his
Ph.D. thesis, "Open Charm Production at STAR." His supervisor was Prof.
Jaroslav Bielcik and co-advisor Xin Dong (LBNL). Congratulations, and many
thanks to Prof. Bielcik and Dr. Dong for their continued contribution to
educating the next generation of physicists. Lukas will continue his
career in the private sector. We wish him all the best in his future
career.
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