PaperPanorama

Nuclear Theory·nucl-th

Wednesday·September 1, 2021

14 papers8 primary·6 cross-listed

  1. 09

    Lightweight self-conjugate nucleus Zr

    A. Hamaker (1,2,3)🇺🇸 · E. Leistenschneider (1,2,6)🇺🇸 · R. Jain (1,2,3)🇺🇸 · G. Bollen (1,2,3)🇺🇸 · S.A. Giuliani (1,4,5)🇺🇸 · K. Lund (1,2)🇺🇸 · W. Nazarewicz (1,3)🇺🇸 · L. Neufcourt (1)🇺🇸 · C. Nicoloff (1,2,3)🇺🇸 · D. Puentes (1,2,3)🇺🇸 · R. Ringle (1,2)🇺🇸 · C.S. Sumithrarachchi (1,2)🇺🇸 · I.T. Yandow (1,2,3) ((1) Facility for Rare Isotope Beams, Michigan State University, East Lansing, Michigan, USA, (2) National Superconducting Cyclotron Laboratory, Michigan State University, East Lansing, Michigan, USA, (3) Department of Physics and Astronomy, Michigan State University, East Lansing, Michigan, USA, (4) European Centre for Theoretical Studies in Nuclear Physics and Related Areas (ECT*-FBK), Trento, Italy, (5) Department of Physics, Faculty of Engineering and Physical Sciences, University of Surrey, Guildford, Surrey, United Kingdom, (6) CERN, Geneva, Switzerland)

    Protons and neutrons in the atomic nucleus move in shells analogous to the electronic shell structures of atoms. Nuclear shell structure varies across the nuclear landscape due to changes of the nuclear mean field with the number of neutrons and protons . These variations can be probed with mass differences. The self-conjugate nucleus Zr is of particular interest as its proton and neutron shell structures are expected to be very similar, and its ground state is highly deformed. In this work, we provide evidence for the existence of a deformed double shell closure in Zr through high precision Penning trap mass measurements of Zr. Our new mass values show that Zr is significantly lighter, and thus more bound than previously determined. This can be attributed to the deformed shell closure at and the large Wigner energy. Our statistical Bayesian model mixing analysis employing several global nuclear mass models demonstrates difficulties with reproducing the observed mass anomaly using current theory.

    nucl-exnucl-thNat.Phys.(2021)·38 citations
  2. 10

    Ratios of jet and hadron spectra at LHC energies: measuring high- suppression without a reference

    Jasmine Brewer🇨🇭 · Alexander Huss🇨🇭 · Aleksas Mazeliauskas🇨🇭 · Wilke van der Schee🇨🇭

    We analyze the reliability of several techniques for computing jet and hadron spectra at different collision energies. This is relevant for discovering energy loss in the upcoming oxygen-oxygen (OO) run at the LHC, for which a reference pp run is currently not planned. For hadrons and jets we compute the ratio of spectra between different pp collision energies in perturbative QCD, which can be used to construct a reference spectrum. Alternatively, it can be interpolated from measured spectra at nearby energies. We estimate the precision of both strategies for the spectra ratio relevant to the oxygen run, and conclude that the central values agree to 4% accuracy for hadrons and 2% accuracy for jets. Finally we propose taking the ratio of OO and pp spectra at different collision energies, which cleanly separates the experimental measurement and theoretical computation.

    hep-phnucl-exnucl-thPRD(2022)·16 citations
  3. 11

    Heavy-quark effects on cold quark matter and self-bound stars

    José C. Jiménez🇧🇷 · Eduardo S. Fraga🇧🇷

    Heavy-quark effects on the equation of state for cold and dense quark matter are obtained from perturbative QCD, yielding observables parametrized only by the renormalization scale. In particular, we investigate the thermodynamics of charm quark matter under the constraints of equilibrium and electric charge neutrality in a region of densities where perturbative QCD is, in principle, much more reliable. Finally, we analyze the stability of charm stars, a possible new branch of ultradense, self-bound compact stars, and find that they are unstable under radial oscillations.

    hep-phastro-ph.HEnucl-thEPJ Web Conf.(2022)·0 citations
  4. 12

    Charm and beauty in the deconfined plasma from quenched lattice QCD

    Heng-Tong Ding🇨🇳 · Olaf Kaczmarek🇨🇳 · Anna-Lena Lorenz🇩🇪 · Hiroshi Ohno🇯🇵 · Hauke Sandmeyer🇩🇪 · Hai-Tao Shu🇩🇪

    We present continuum extrapolated results of charmonium and bottomonium correlators in the vector channel at several temperatures below and above . The continuum extrapolation jointly performed with the interpolations to have physical values of and masses in the confined phase is based on calculations on several large quenched isotropic lattices using clover-improved Wilson valence fermions carrying different quark masses. The extrapolated lattice correlators are confronted with perturbation theory results incorporating resummed thermal effects around the threshold from pNRQCD and vacuum asymptotics above the threshold. An additional transport peak is modelled below the threshold allowing for an estimate of the diffusion coefficients for charm and bottom quarks. We find that charmonium correlators in the vector channel can be well reproduced by perturbative spectral functions above where no resonance peaks for are needed at and above 1.1 , while for bottomonium correlators a resonance peak for is still needed up to 1.5 . By analyzing the transport contribution to the correlators we find that the drag coefficient of a charm quark is larger than that of a bottom quark.

    hep-lathep-phnucl-exnucl-thPRD(2021)·16 citations
  5. 13

    Pionic depth of the hadron gas after a heavy-ion collision

    Guillermo Gómez Fonfría🇪🇸 · Felipe J. Llanes-Estrada🇪🇸 · Javier Suárez Sucunza🇪🇸 · Juan M. Torres-Rincon🇩🇪

    The final stage of a relativistic heavy-ion collision is a hadron gas. Final-state interactions therein distort the spectrum of particles coming from the phase transition upon cooling the quark-gluon plasma. Using recent state-of-the-art parametrizations of pion interactions we provide theoretical computations of the pionic depth of the gas: how likely is it that a given pion rescatters in it (we find a high probability around GeV at midrapidity, corresponding to the formation of the resonance), a comparison of the collision and Bjorken expansion rates, and how many pions make it through without interacting as a function of . This is in the range 10-24 and shown in this plot, the main result of the contribution.

    hep-phnucl-thPoS(2022)·1 citation
  6. 14

    Stellar Structure and Stability of Charged Interacting Quark Stars and Their Scaling Behaviour

    Chen Zhang🇨🇦 · Michael Gammon🇨🇦 · Robert B. Mann🇨🇦

    We explore the stellar structure and radial stability of charged quark stars composed of interacting quark matter (IQM) in three classes of commonly used charge models. We adopt a general parametrization of IQM equation of state that includes the corrections from perturbative QCD, color superconductivity, and the strange quark mass into one parameter , or one dimensionless parameter after being rescaled with the effective bag constant . We find that increasing charge tends to increase the mass and radius profiles, and enlarges the separation size in mass between the maximum mass point and the point where zero eigenfrequencies of the fundamental radial oscillation mode occur. The sign of the separation in central density depends on the charge model; this separation also has a dependence on such that increasing (which can occur for either large color superconductivity or small strange quark mass) tends to decrease this separation size for the first and third classes of charge models monotonically. Moreover, for the second and third classes of charge models, we manage to numerically and analytically identify a new kind of stellar structure with a zero central pressure but a finite radius and mass. All the calculations and analysis are performed in a general dimensionless rescaling approach so that the results are independent of explicit values of dimensional parameters.

    astro-ph.HEgr-qchep-phnucl-thPRD(2021)·21 citations

Affiliations

first authorsco-authorsvia INSPIRE