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Nuclear Theory·nucl-th

Wednesday·June 17, 2015

6 papers—3 primary·3 cross-listed

All6Primary3Cross-lists3
  1. 04

    [Submitted on 15 Jun 2015] (cross-list from hep-ph)

    Search for the critical point of strongly interacting matter at the CERN SPS NA61/SHINE experiment

    L. Turko🇵🇱

    The NA61/SHINE experiment performs a detailed study of the onset of deconfinement and search for critical point of hadronic matter by colliding nuclei of different sizes at various beam momenta from 13A to 158A GeV/c. Experimental setup and results on the theoretically expected signatures are discussed.

    Comments:
    6 pages, 8 figures, Talk presented at the International Workshop: Discovery Physics at the LHC -- Kruger 2014, RPA, December 1-6, 2014}, to appear in Journal of Physics: Conference Series (JPCS)
    Subjects:
    High Energy Physics — Phenomenology (hep-ph); Nuclear Theory (nucl-th)
    arXiv:
    1506.04794 [pdf]
    J.Phys.Conf.Ser.(2015)·1 citation
  2. 05

    [Submitted on 16 Jun 2015] (cross-list from cond-mat.quant-gas)

    Four-boson bound states from a functional renormalisation group

    Benjamin Jaramillo Avila · Michael C. Birse (University of Manchester)

    We use the functional renormalisation group to study the spectrum of three- and four-body states in bosonic systems around the unitary limit. Our effective action includes all energy-independent contact interactions in the four-atom sector and we introduce a running trimer field to eliminate couplings that involve the atom-atom-dimer channel. The results show qualitatively similar behaviour to those from exact approaches. The truncated action we use leads to overbinding of the two four-body states seen in those treatments. It also generates a third state, although only for a very narrow range of two-body scattering lengths.

    Comments:
    4 pages, 2 figures
    Subjects:
    Quantum Gases (cond-mat.quant-gas); Nuclear Theory (nucl-th); physics.atm-clus (physics.atm-clus)
    arXiv:
    1506.04949 [pdf]
    PRA(2015)·7 citations
  3. 06

    [Submitted on 16 Jun 2015] (cross-list from astro-ph.SR)

    Neutrino-driven winds in the aftermath of a neutron star merger: nucleosynthesis and electromagnetic transients

    Dirk Martin🇩🇪 · Albino Perego🇩🇪 · Almudena Arcones🇩🇪 · Friedrich-Karl Thielemann🇨🇭 · Oleg Korobkin🇸🇪 · Stephan Rosswog🇸🇪

    We present a comprehensive nucleosynthesis study of the neutrino-driven wind in the aftermath of a binary neutron star merger. Our focus is the initial remnant phase when a massive central neutron star is present. Using tracers from a recent hydrodynamical simulation, we determine total masses and integrated abundances to characterize the composition of unbound matter. We find that the nucleosynthetic yields depend sensitively on both the life time of the massive neutron star and the polar angle. Matter in excess of up to becomes unbound until . Due to electron fractions of mainly nuclei with mass numbers are synthesized, complementing the yields from the earlier dynamic ejecta. Mixing scenarios with these two types of ejecta can explain the abundance pattern in r-process enriched metal-poor stars. Additionally, we calculate heating rates for the decay of the freshly produced radioactive isotopes. The resulting light curve peaks in the blue band after about . Furthermore, high opacities due to heavy r-process nuclei in the dynamic ejecta lead to a second peak in the infrared after .

    Comments:
    15 pages, 18 figures, 2 tables, accepted by ApJ
    Subjects:
    Solar and Stellar Astrophysics (astro-ph.SR); High Energy Astrophysical Phenomena (astro-ph.HE); Nuclear Theory (nucl-th)
    arXiv:
    1506.05048 [pdf]
    ApJ(2015)·246 citations

Affiliations

first authorsco-authorsvia INSPIRE