PaperPanorama

Nuclear Theory·nucl-th

Friday·September 18, 2015

13 papers7 primary·6 cross-listed

  1. 01

    Direct Urca processes involving singlet proton superfluidity in neutron star cooling

    Yan Xu · Xiu Lin Huang · Xiao Jun Zhang · Tmurbagan Bao · Lin Xiao · Cun Bo Fan · Cheng Zhi Liu

    A detailed description of the baryon direct Urca processes A: , B: , C: related to the neutron star cooling is given in the relativistic mean field approximation.The contributions of the reactions B and C on the neutrino luminosity are calculated by means of the relativistic expressions of the neutrino energy losses.Our results show that the total neutrino luminosities of the reactions A, B, C within the mass range 1.603-2.067 (1.515-1.840 for TM1 model) for GM1 model are larger than the corresponding values for neutron stars in npe matter. Although the hyperon direct Urca processes B and C reduce the neutrino emissivity of the reaction A, it illustrates the reactions B and C still make the total neutrino luminosity enhancement in the above mentioned areas.Furthermore, when we only consider the proton superfluidity in neutron star cooling, we find that although the neutrino emissivity of the reactions A and B is suppressed with the appearance of proton superfluidity, the total contribution of the reactions A, B, C can still quicken a massive neutron star cooling.These results could be used to help prove appearing hyperons in PSR J1614-2230 and J0348+0432 from neutron star cooling perspective.

    nucl-thCommun.Theor.Phys.(2018)·5 citations
  2. 02

    Deconfinement Phase Transition with External Magnetic Field in Friedberg-Lee Model

    Shijun Mao🇨🇳

    The deconfinement phase transition with external magnetic field is investigated in the Friedberg-Lee model. In the frame of functional renormalization group, we extend the often used potential expansion method for continuous phase transitions to the first-order phase transition in the model. By solving the flow equations we find that, the magnetic field displays a catalysis effect and it becomes more difficult to break through the confinement in hot and dense medium.

    nucl-thChin.Phys.Lett.(2016)·2 citations
  3. 03

    Phase space factors and half-life predictions for Majoron emitting decay

    J. Kotila🇫🇮 · J. Barea🇨🇱 · F. Iachello🇺🇸

    A complete calculation of phase space factors (PSF) for Majoron emitting decay modes is presented. The calculation makes use of exact Dirac wave functions with finite nuclear size and electron screening and includes life-times, single electron spectra, summed electron spectra, and angular electron correlations. Combining these results with recent interacting boson nuclear matrix elements (NME) we make half-life predictions for the the ordinary Majoron decay (spectral index =1). Furthermore, comparing theoretical predictions with the obtained experimental lower bounds for this decay mode we are able to set limits on the effective Majoron-neutrino coupling constant .

    nucl-thPRC(2015)·51 citations
  4. 04

    Neutrinoless double positron decay and positron emitting electron capture in the interacting boson model

    J. Barea🇨🇱 · J. Kotila🇺🇸 · F. Iachello🇺🇸

    Neutrinoless double- decay is of fundamental importance for determining the neutrino mass. Although double electron () decay is the most promising mode, in very recent years interest in double positron () decay, positron emitting electron capture (), and double electron capture () has been renewed. We present here results of a calculation of nuclear matrix elements for neutrinoless double- decay and positron emitting electron capture within the framework of the microscopic interacting boson model (IBM-2) for Ni, Zn, Kr, Ru, Cd, Xe, Ba, and Ce decay. By combining these with a calculation of phase space factors we calculate expected half-lives.

    nucl-thPRC(2013)·35 citations
  5. 05

    Production of antimatter Li nuclei in central Au+Au collisions at GeV

    Kai-Jia Sun🇨🇳 · Lie-Wen Chen🇨🇳

    Combining the covariant coalescence model and a blast-wave-like analytical parametrization for (anti-)nucleon phase-space freezeout configuration, we explore light (anti-)nucleus production in central Au+Au collisions at GeV. Using the nucleon freezeout configuration (denoted by FO1) determined from the measured spectra of protons (p), deutrons (d) and He, we find the predicted yield of He is significantly smaller than the experimental data. We show this disagreement can be removed by using a nucleon freezeout configuration (denoted by FO2) in which the nucleons are assumed to freeze out earlier than those in FO1 to effectively consider the effect of large binding energy value of He. Assuming the binding energy effect also exists for the production of , , and due to their similar binding energy values as He, we find the yields of these heavier (anti-)nuclei can be enhanced by a factor of about one order, implying that although the stable (anti-)Li nucleus is unlikely to be observed, the unstable (anti-)Li nucleus could be produced in observable abundance in Au+Au collisions at GeV where it may be identified through the p- (-) invariant mass spectrum. The future experimental measurement on (anti-) would be very useful to understand the production mechanism of heavier antimatter.

    nucl-thastro-ph.COhep-phnucl-exPLB(2015)·40 citations
  6. 06

    Reference calculations for subthreshold production

    Boris Tomasik🇨🇿 · Evgeni E Kolomeitsev🇸🇰

    We present a minimal statistical model designed for the description of rare-hadron multiplicities in nucleus-nucleus collisions at energies below the threshold of the particle production in binary elementary collisions. Differences to more conventional canonical statistical model are explained. The minimal statistical model is applied to the description of multiplicity ratios involving hyperons, which are measured by the HADES collaboration at GSI-SIS. It is argued that the HADES data cannot be reproduced by the model based on the statistical equilibrium and the strangeness conservation. The data remain underpredicted even when in-medium potentials acting on hadrons are taken into account. This hints to non-equilibrium production of the hyperons and their continuous freeze-out.

    nucl-thhep-phJ.Phys.Conf.Ser.(2016)·0 citations

Affiliations

first authorsco-authorsvia INSPIRE