M. Zurek’s research while affiliated with Argonne National Laboratory and other places

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Publications (257)


Erratum: Measurement of the Sixth-Order Cumulant of Net-Proton Multiplicity Distributions in Au + Au Collisions at s NN = 27 , 54.4, and 200 GeV at RHIC [Phys. Rev. Lett. 127 , 262301 (2021)]
  • Article

April 2025

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6 Reads

Physical Review Letters

M. S. Abdallah

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J. Adam

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L. Adamczyk

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[...]

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M. Zyzak






Fig. 2. Centrality dependence of the mid-rapidity correlation functions for í µí±-í µí±‘, (top panel) and í µí±‘-í µí±‘, (bottom panel) displayed as a function of the relative momenta. Statistical and systematic uncertainties from the measurements are shown as bars and boxes, respectively. The results of the Lednický-Lyuboshits (LL) fits are shown as the red-lines. Orange bands represent the calculations from the SMASH model with coalescence procedure for the formation of deuterons plus CRAB afterburner while gray bands show the model calculation with directly produced deuterons plus CRAB. Blue dashed lines are the results with Coulomb interactions only. and singular (í µí°º 0 ) s-wave Coulomb functions. The scattering amplitude í µí±“ í µí±† í µí± (í µí±˜ * ), which includes Coulomb interaction, is given by:
Fig. 3. Collision centrality dependence of the source radius parameter extracted from í µí±-í µí±‘, (circles) and í µí±‘-í µí±‘, (squares) correlation functions in √ í µí± NN = 3 GeV Au + Au collisions. Statistical and systematic uncertainties are all smaller than the size of the symbols. The values of the Gaussian source radius from SMASH model are shown as green and blue bands, for í µí±-í µí±‘ and í µí±‘-í µí±‘ pairs, respectively. The shadow bands represent the RMS values calculated from SMASH model.
Fig. 4. (a) Spin-averaged final state strong interaction parameters: í µí±“ 0 scattering length, and í µí±‘ 0 , effective range, extracted from í µí±-í µí±‘ (filled circle) and í µí±‘-í µí±‘ (filled square) correlation functions. The statistical uncertainties are smaller than the marker size. Open boxes represent the systematic uncertainties. Data of ̄ í µí±-̄ í µí± correlation function in 200 GeV Au + Au collisions [6] are shown as the solid black point. The interaction parameters from í µí±›-í µí±›, í µí±-í µí±, í µí±›-í µí± singlet (í µí± ), í µí±›-í µí± triplet (í µí±¡) states [68,69] and í µí±-í µí±‘ [70-74] are shown as open symbols and hatched area. The 1-3í µí¼Ž fitting contours are shown in the right plots (b,c).
The extracted source size í µí± í µí°º parameters in í µí±-í µí±‘ and í µí±‘-í µí±‘ pairs with individ- ual fit and simultaneous fit. The errors represent statistical uncertainites from fitting.
Light Nuclei Femtoscopy and Baryon Interactions in 3 GeV Au+Au Collisions at RHIC
  • Article
  • Full-text available

March 2025

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12 Reads

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1 Citation

Physics Letters B

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FIG. 1. Kinematics of the γ p → K 0 + reaction.
FIG. 4. Missing mass (π + , π − ) for one cos θ c.m. K 0 and E γ bin. The dashed vertical line shows the PDG mass of the + .
FIG. 5. Example of a so-called corner plot, showing the posterior distributions of the observables evaluated at W = 1.786 GeV and cos θ c.m. K 0 = −0.28, together with the correlation plots.
FIG. 7. Real (upper row) and imaginary parts (lower row) of the E 1+ (left) and M 1+ (right) multipoles for the reaction γ p → K 0 + from the Jülich-Bonn dynamical coupled channels model. Brown lines: JuBo2022 solution. Blue lines: JuBo2023-1 solution that includes the data of this work in the fits.
Photoproduction of the Σ + hyperon using linearly polarized photons with CLAS

February 2025

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36 Reads

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1 Citation

Physical Review C

Measurements of the polarization observables Σ , P , T , O x , O z for the reaction γ ⃗ p → K S 0 Σ + using a linearly polarized photon beam of energy 1.1 to 2.1 GeV are reported. The measured data provide information on a channel that has not been studied extensively, but is required for a full coupled-channel analysis in the nucleon resonance region. Observables have been simultaneously extracted using likelihood sampling with a Markov-Chain Monte Carlo process. Angular distributions in bins of photon energy E γ are produced for each polarization observable. T , O x , and O z are first time measurements of these observables in this reaction. The extraction of Σ extends the energy range beyond a previous measurement. The measurement of P , the recoil polarization, is consistent with previous measurements. The measured data are shown to be significant enough to affect the estimation of the nucleon resonance parameters when fitted within a coupled-channels model. Published by the American Physical Society 2025



FIG. 1. As an example, the initial spin vector ⃗ S(t = 0) points in vertical direction. An rf device providing a magnetic field ⃗ B rf (t) = ⃗ B0 cos(2πf rf t) with ⃗ B0 = B0 ⃗ m then rotates the spin vector by an angle χ(t) ∝ B rf (t) per pass around the axis ⃗ m ∥ ⃗ B0, see Eq. (2). In addition, the holding field ⃗ B of the accelerator causes the spin vector to precess with the frequency fs = νsfrev around the vertical axis. This only works if the resonance condition in Eq. (1) is satisfied.
FIG. 6. Upper Panel: Normalized asymmetry as a function of the spin-tune phase based on the assumed, fixed spin tune (here ν fixed s = 0.161 006 673 7) of data taken during a ∆t = 1 s period. The distribution is fitted according to Eq. (12). In this example the offset of the spin precession phase is φs = 1.12(8) rad. Lower Panels: Spin-tune phase offset and change of spin tune (according to Eq. (13), including uncertainties) as a function of time in the cycle. In this example, the change of the spin tune amounts to ∆νs ≈ 10 −8 during a 150 s interval.
FIG. 10. Out-of-plane angle α (top) and relative phase φ meas rel (bottom) as a function of time for two initial values of φ demand rel (left and right). The dashed line marks the time the Wien filter is switched on t on WF . The blue data points represent the signal bunch, the green ones the unaffected bunch used by the feedback system. The fit parameters are listed in Table IV.
Maintaining a Resonance Condition of an RF Spin Rotator Through a Feedback Loop in a Storage Ring

January 2025

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35 Reads

This paper presents the successful application of a phase-lock feedback system to maintain the resonance condition of a radio frequency (rf) spin rotator (specifically, an rf Wien filter) with respect to a 120 kHz spin precession in the Cooler Synchrotron (COSY) storage ring. Real-time monitoring of the spin precession and the rf Wien filter signal allows the relative phase between the two to be stabilized at an arbitrary setpoint. The feedback system compensates for deviations in the relative phase by adjusting the frequency and/or phase as needed. With this method, a variation in phase relative to the demand phase with a standard deviation of σΔφ0.2rad\sigma_{\Delta\varphi}\approx 0.2\mathrm{rad} could be achieved. The system was implemented in two runs aiming at a first direct measurement of the deuteron electric dipole moment in 2018 and 2021. In addition, the difference between a single-bunch beam affected by the spin rotator and a two-bunch system in which only one bunch is exposed to the spin rotator fields is discussed. Both methods have been used during these beam times. The ability to keep the spin precession and the rf fields synchronized is also crucial for future investigations of electric dipole moments of charged particles using storage rings.


Citations (71)


... Femtoscopy of nuclei has also become possible in which deuteron or more massive particles have been used. Recently, femtoscopy studies involving proton and deuteron pairs have been carried out in high-multiplicity p + p collisions at √ s = 13 TeV by the ALICE [28] experiment, in Au + Au collisions at √ s NN = 3 GeV measured by the STAR experiment [29], and in Ag + Ag collisions at √ s NN = 2.55 GeV by the HADES experiment [30]. ...

Reference:

Two-body femtoscopy approach to the proton-deuteron correlation function
Light Nuclei Femtoscopy and Baryon Interactions in 3 GeV Au+Au Collisions at RHIC

Physics Letters B

... The pseudodata tested here is based on polarisation observables of the γ + p → K 0 + Σ + reaction [10], whose angular-dependent parts are sums of Legendre polynomials. It was assumed for testing purposes that the energydependent part consists of Gaussians, which are dependent on the order of Legendre polynomial. ...

Photoproduction of the Σ + hyperon using linearly polarized photons with CLAS

Physical Review C

... Compared with protons, pions and kaons have smaller ∆(dv 1 /dy) magnitudes, which is understandable in view of factors such as mean p T and the formation time. A companion STAR analysis [66] assumes the coalescence sum rule using combinations of hadrons without transported quarks and concludes that the presence of the EM-field dominated by the Hall effect in mid-central events explains the observed v 1 splitting. The combined inference from Ref. [66] and the current work is that a competition between the Hall effect and the Faraday+Coulomb effect, its flavor and centrality dependence may lead to the observed v 1 splittings. ...

Electric-charge-dependent directed flow splitting of produced quarks in Au+Au collisions
  • Citing Article
  • March 2025

Physics Letters B

... This is the so-called standard event plane method [13]. The event plane method has been widely used in the collective flow analysis in the past decades [14][15][16][17][18][19][20] , but it is still crucial to optimize the method for the CEE experiment and to validate that the collective flow signal obtained from CEE spectrometer is reliable. ...

Measurement of directed flow in Au + Au collisions at s N N = 19.6 and 27 GeV with the STAR event plane detector
  • Citing Article
  • January 2025

Physical Review C

... This simple model has proven to be very successful in describing the measured yields of many different hadron species in heavy-ion collisions across a broad collision energy range [22,27,[36][37][38]. Figure 1 depicts various F-O points from different experiments, including STAR-BES [27], NA49 [25,[39][40][41], E-802 [25,42,43], and GSI-SIS [44]. To fill the gap at high μ B , we additionally performed fits to the recent data for 0-10 % central Au-Au collisions at √ s NN = 3 GeV from the STAR Collaboration [45,46] using Thermal-FIST and the Id-HRG model in the strangeness-canonical ensemble. Namely, we fitted the 4π yields of primordial protons, light nuclei (d, 3 H, 3 H, 4 H), 054903-2 N part , and the yields of , K 0 S , K − , φ, − normalized by N part . ...

Production of protons and light nuclei in Au + Au collisions at s N N = 3 GeV with the STAR detector
  • Citing Article
  • November 2024

Physical Review C

... However, most of the analytical work presented here will be useful for that case. Extending the study to a spin-1 target, such as the deuteron, would also be valuable since deuteron GPDs have very interesting new facets [52,53], and the DVCS and TCS processes on the deuteron should soon be experimentally accessible [54]. ...

First Measurement of Deeply Virtual Compton Scattering on the Neutron with Detection of the Active Neutron

Physical Review Letters

... All cited uncertainties are statistical only and should be interpreted accordingly. For the final analysis of the EDM data a more sophisticated and complete model incorporating these effects is used [21]. ...

Spin decoherence and off-resonance behavior of radio-frequency-driven spin rotations in storage rings

Physical Review Accelerators and Beams

... Moreover, subtle differences in background effects between Ru + Ru and Zr + Zr collisions arising from approximately defined nuclear structures can significantly influence the relative magnitudes of the CME observables. Furthermore, incorporating higher-order deformations, such as quadrupole β 2 and octupole β 3 deformations, into the WS equation could provide deeper insights into the event-by-event initial geometric configurations [39]. This would not only make the initial conditions more interesting but also lead to a more varied initial magnetic field, which could have significant implications for the observed CME signals. ...

Imaging shapes of atomic nuclei in high-energy nuclear collisions

Nature

... The combined UrQMD+SMM framework has recently demonstrated its capabilities to describe the light nuclei and hypernuclei multiplicities and spectra in Au+Au collisions at √ s NN = 3 GeV [37] and is therefore well suited for the present analysis of harmonic flow. [14,48]. The lower panel shows the ratio integrated over the midrapidity interval |y| ≤ 0.5 as a function of mass number A. ...

Strangeness production in sNN \sqrt{s_{\textrm{NN}}} = 3 GeV Au+Au collisions at RHIC

Journal of High Energy Physics