PaperPanorama

Nuclear Theory·nucl-th

Tuesday·May 19, 2015

10 papers4 primary·6 cross-listed

  1. 01

    Heavy flavor suppression predictions at 5.1 TeV Pb+Pb collisions at LHC

    Magdalena Djordjevic🇷🇸 · Marko Djordjevic🇷🇸

    High momentum hadron suppression is considered to be an excellent probe of jet-medium interactions in QCD matter created in ultra-relativistic heavy ion collisions. We previously showed that our dynamical energy loss formalism can accurately explain suppression measurements at 200 GeV Au+Au collisions at RHIC and 2.76 TeV Pb+Pb collisions at the LHC. With the upcoming LHC measurements at notably higher collision energies, there is a question of what differences, with respect to the current (2.76 TeV) measurements, can be expected. In this paper we concentrate on heavy flavor suppression at the upcoming 5.1 TeV Pb+Pb collisions energy at the LHC. Naively, one would expect a notably () larger suppression at 5.1 TeV collision energy, due to estimated (significant) energy loss increase when transitioning from 2.76 to 5.1 TeV. Surprisingly, more detailed calculations predict nearly the same suppression results at these two energies. We show that this unexpected result is due to an interplay of the following two effects, which essentially cancel each other: i) flattening of the initial distributions with increasing collision energies, and ii) significantly slower than naively expected increase in the energy loss. Therefore, the obtained nearly the same suppression provides a clear (qualitative and quantitative) test of our energy loss formalism.

    nucl-thhep-phPRC(2015)·86 citations
  2. 02

    Rapidity window dependences of higher order cumulants and diffusion master equation

    Masakiyo Kitazawa🇯🇵

    We study the rapidity window dependences of higher order cumulants of conserved charges observed in relativistic heavy ion collisions. The time evolution and the rapidity window dependence of the non-Gaussian fluctuations are described by the diffusion master equation. Analytic formulas for the time evolution of cumulants in a rapidity window are obtained for arbitrary initial conditions. We discuss that the rapidity window dependences of the non-Gaussian cumulants have characteristic structures reflecting the non-equilibrium property of fluctuations, which can be observed in relativistic heavy ion collisions with the present detectors. It is argued that various information on the thermal and transport properties of the hot medium can be revealed experimentally by the study of the rapidity window dependences, especially by the combined use, of the higher order cumulants. Formulas of higher order cumulants for a probability distribution composed of sub-probabilities, which are useful for various studies of non-Gaussian cumulants, are also presented.

    nucl-thhep-phnucl-exNPA(2015)·24 citations
  3. 03

    Origin of Low-Lying Enhanced E1 Strength in Rare-Earth Nuclei

    M. Spieker · S. Pascu · A. Zilges · F. Iachello

    The experimental strength distribution below 4 MeV in rare-earth nuclei suggests a local breaking of isospin symmetry. In addition to the octupole states, additional states with enhanced E1 strength have been observed in rare-earth nuclei by means of () experiments. By reproducing the experimental results, the spdf interacting boson model calculations provide further evidence for the formation of an cluster in medium-mass nuclei and might provide a new understanding of the origin of low-lying E1 strength.

    nucl-thPRL(2015)·49 citations
  4. 04

    Neutron skin and halo in medium and heavy nuclei within the extended Thomas-Fermi theory

    S.V. Lukyanov · A.I. Sanzhur

    The neutron skin and halo distributions in medium and heavy nuclei are calculated within the extended Thomas-Fermi approximation. Calculations are carried out for the effective Skyrme-like forces using the direct variational method. The analytical expression for the isovector shift of the rms radii as a sum of skin- and halo-like terms is obtained. The contribution of halo and skin terms to are found to be approximately equal.

    nucl-thNucl.Phys.Atom.Energy(2016)·4 citations

Affiliations

first authorsco-authorsvia INSPIRE