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Register a new userPredictions for production of $rm{^3_Lambda H}$ and $rm{{^3_{overline Lambda}overline H}}$ in isobaric $^{96}_{44}$Ru+$^{96}_{44}$Ru and $^{96}_{40}$Zr+$^{96}_{40}$Zr collisions at $sqrt{s_{rm{NN}}}$ = 200 GeV
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The production of $rm{^3_Lambda H}$ and $rm{{^3_{overline Lambda}overline H}}$, as well as $rm{^3H}$, $rm{{^3overline H}}$, $rm{^3He}$, and $rm{{^3overline {He}}}$ are studied in central collisions of isobars $^{96}_{44}$Ru+$^{96}_{44}$Ru and $^{96}_{40}$Zr+$^{96}_{40}$Zr at $sqrt{s_{rm{NN}}}=200$ GeV, using the dynamically constrained phase-space coalescence model and the {footnotesize PACIAE} model with chiral magnetic effect. The yield, yield ratio, coalescence parameters, and strangeness population factor of (anti-)hypertriton and (anti-)nuclei produced in isobaric $^{96}_{44}$Ru+$^{96}_{44}$Ru and $^{96}_{40}$Zr+$^{96}_{40}$Zr collisions are predicted. The (anti-)hypertriton and (anti-)nuclei production is found to be insensitive to the chiral magnetic effects. Experimental data of Cu+Cu, Au+Au and Pb+Pb collisions from RHIC, LHC, and the results of {footnotesize PACIAE+DCPC} model are presented in the results for comparison.
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In the hydrodynamic model description of heavy ion collisions, the elliptic flow $v_2$ and triangular flow $v_3$ are sensitive to the quadrupole deformation $beta_2$ and octupole deformation $beta_3$ of the colliding nuclei. The relations between $v_n$ and $beta_n$ have recently been clarified and were found to follow a simple parametric form. The STAR Collaboration have just published precision $v_n$ data from isobaric $^{96}$Ru+$^{96}$Ru and $^{96}$Zr+$^{96}$Zr collisions, where they observe large differences in central collisions $v_{2,mathrm{Ru}}>v_{2,mathrm{Zr}}$ and $v_{3,mathrm{Ru}}<v_{3,mathrm{Zr}}$. Using a transport model simulation, we show that these orderings are a natural consequence of $beta_{2,mathrm{Ru}}ggbeta_{2,mathrm{Zr}}$ and $beta_{3,mathrm{Ru}}llbeta_{3,mathrm{Zr}}$. We are able to reproduce the centrality dependence of the $v_2$ ratio qualitatively and $v_3$ ratio quantitatively, and extract values of $beta_2$ and $beta_3$ that are consistent with those measured at low energy nuclear structure experiments. STAR data provide the first direct evidence of strong octupole correlations in the ground state of $^{96}$Zr in heavy ion collisions. Our analysis demonstrates that flow measurements in high-energy heavy ion collisions, especially using isobaric systems, are a new precision tool to study nuclear structure physics.
Anomalous Viscous Fluid Dynamics (AVFD) model calculations for $mathrm{^{96}_{44}Ru +, ^{96}_{44}Ru}$ and $mathrm{^{96}_{40}Zr +, ^{96}_{40}Zr}$ collisions ($sqrt{s_{rm NN}} = 200$ GeV) are used in concert with a charge-sensitive correlator, to test its ability to detect and characterize the charge separation difference expected from the Chiral Magnetic Effect (CME) in these isobaric collisions. The tests indicate a larger charge separation for $mathrm{^{96}_{44}Ru +, ^{96}_{44}Ru}$ than for $mathrm{^{96}_{40}Zr +, ^{96}_{40}Zr}$ collisions, and a discernible CME-driven difference of $sim 10$% in the presence of realistic non-CME backgrounds. They also indicate a strategy for evaluating the relative influence of the background correlations, present for each isobar. These results suggest that charge separation measurements for these isobaric species could serve to further constrain unambiguous identification and characterization of the CME in upcoming measurements at RHIC.
Fusion data for $^{40}$Ca+$^{96}$Zr are analyzed by coupled-channels calculations that are based on a standard Woods-Saxon potential and include couplings to multiphonon excitations and transfer channels. The couplings to multiphonon excitations are the same as used in a previous work. The transfer couplings are calibrated to reproduce the measured neutron transfer data. This type of calculation gives a poor fit to the fusion data. However, by multiplying the transfer couplings with a $sqrt{2}$ one obtains an excellent fit. The scaling of the transfer strengths is supposed to simulate the combined effect of neutron and proton transfer, and the calculated one- and two-nucleon transfer cross sections are indeed in reasonable agreement with the measured cross sections.
The isobaric collisions of $^{96}_{44}$Ru + $^{96}_{44}$Ru and $^{96}_{40}$Zr + $^{96}_{40}$Zr have recently been proposed to discern the charge separation signal of the chiral magnetic effect (CME). In this article, we employ the string melting version of a multiphase transport model to predict various charged-particle observables, including $dN/deta$, $p_T$ spectra, elliptic flow ($v_2$), and particularly possible CME signals in Ru + Ru and Zr + Zr collisions at $sqrt{s_{_{rm NN}}}$ = 200 GeV. Two sets of the nuclear structure parametrization have been explored, and the difference between the two isobaric collisions appears to be small, in terms of $dN/deta$, $p_T$ spectra, and $v_2$ for charged particles. We mimic the CME by introducing an initial charge separation that is proportional to the magnetic field produced in the collision, and study how the final-state interactions affect the CME observables. The relative difference in the CME signal between the two isobaric collisions is found to be robust, insensitive to the final-state interactions.
The nature of $J^{pi}=1^-$ levels of $^{96}$Zr below the $beta$-decay $Q_{beta}$ value of $^{96}$Y has been investigated in high-resolution $gamma$-ray spectroscopy following the $beta$ decay as well as in a campaign of inelastic photon scattering experiments. Branching ratios extracted from $beta$ decay allow the absolute $E1$ excitation strength to be determined for levels populated in both reactions. The combined data represents a comprehensive approach to the wavefunction of $1^-$ levels below the $Q_{beta}$ value, which are investigated in the theoretical approach of the Quasiparticle Phonon Model. This study clarifies the nuclear structure properties associated with the enhanced population of high-lying levels in the $^{96}$Y$_{gs}$ $beta$ decay, one of the three most important contributors to the high-energy reactor antineutrino spectrum.
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