Posters

EPS Best Poster Prize:

• Jenny Feige (University of Vienna, Faculty of Physics)
  Supernova-produced 26Al and 60Fe in deep-sea sediments from the Indian Ocean
• Meng-Ru Wu (Institute for Nuclear Physics, Technical University Darmstadt)
  Neutrinos and nucleosynthesis of heavy elements
• Konrad Schmidt (Helmholtz-Zentrum Dresden-Rossendorf)
  The 40Ca(α,γ)44Ti reaction studied by in-beam γ-spectroscopy and activation

EPL Best Poster Prize:

• Kevin Ebinger (University of Basel, Department of Physics)
  Parametrized spherically symmetric core collapse supernova simulations: Push
• Andreas Best (INFN - Laboratori Nazionali del Gran Sasso)
  Low energy neutron background in deep underground laboratories
• Rosanna Depalo (Dipartimento di Fisica e Astronomia, Università degli studi di Padova and INFN Padova)
  Low-energy resonances in the 22Ne(p,gamma)23Na reaction directly observed at LUNA

List of accepted posters

• C. Abia, Spain
  On the existence of the LEPP mechanism
• A. Algora, Spain
  Total absorption measurements as a benchmark for nuclear models
• A. Arzhanov, Germany
  Large-scale Gogny-HFB calculation for r-process nucleosynthesis: Towards a fully-converged microscopic mass table
• A. Ayala-Gomez, Spain
  Stellar constraints to axions-like particles and the need of precise He-burning reaction rates
• C. Battistini, Sweden
  Exploring the origin and evolution of the odd iron-peak elements in the Milky Way stellar disk
• P. Benazzo, Sweden
  Type IA supernovae as empirical evidence for a curved, static and spatially closed cosmos
• A. Best, Italy
  Low energy neutron background in deep underground laboratories
• J. Bliss, Germany
  Nucleosynthesis of Mo in neutrino-driven winds
• M. Bouhelal, Algeria
  Shell-model studies of 22Mg and 30S at excitations of interest for the thermonuclear radiative capture reactions
• M. Buckner, United States
  Thermonuclear reaction rate of 17O(p,γ)18F—a high-current, low-energy study at sea level
• M. Busso, Italy
  MHD as a driver for mixing in AGB stars
• A. Caciolli, Italy
  Measurement of the 25Mg(α,n)28Si reaction cross section at LNL
• A. Caciolli, Italy
  17O hydrogen burning at the energies of classical nova at LUNA
• D-R. Constantin, Romania
  Gravitational redshift in the post-newtonian potential field:
  The schwarzschild problem
• S. Cristallo, Italy
  FRUITY upgrades on AGB nucleosynthesis
• M. Cruz, Brazil
  Nucleosynthesis in extremely metal-poor intermediate-mass stars
• A. Davis, United States
  The 13C-pockets in AGB stars and their fingerprints in mainstream SiC
  grains
• F. de Oliveira, France
  Nuclear astrophysics with radioactive beams at GANIL
• A. Deibel, United States
  How unique is the crust of an accreting neutron star? A multicomponent
  study
• P. Denisenkov, Canada
  CANFAR software-as-a-service for NuGrid data exploration
• R. Depalo, Italy
  Low-energy resonances in the 22Ne(p,gamma)23Na reaction directly observed at LUNA
• R. Depalo, Italy
  First direct measurement of the 2H(α,γ)6Li cross section at Big Bang energies at LUNA
• R. Diehl, Germany
  Nucleosynthesis ejecta in the galaxy
• C.L. Doherty, Australia
  New simulations of neutron captures in-between the S and the R process
• K. Ebinger, Switzerland
  Parametrized spherically symmetric core collapse supernova simulations: Push
• Z. Elekes, Hungary
  Fast neutron detection by resistive plate chambers
• J. Feige, Austria
  Supernova-produced 26Al AND 60Fe in deep-sea sediments from the Indian Ocean
• F. Ferraro, Italy
  Measurement of the strengths of the resonances at 417, 611, and 632 keV in the 22Ne(p,gamma)23Na reaction
• S. Fujimoto, Japan
  R-process nucleosynthesis in jets from collapsars and magnetars
• S.A. Giuliani, Germany
  Fission properties of neutron rich uranium isotopes
• J. Glorius, Germany
  Reaction studies using stored ions
• S. Goriely, Belgium
  Charge exchange nuclear excitations and beta decay within the self consistent deformed QRPA
• C. Griffin, United Kingdom
  β-decay studies of R-process nuclei using the advanced implantation detector array
• R. Güray, Turkey
  Experimental cross sections of proton-induced reactions on Gd-152 for the astrophysical p-process
• J. Harris, United States
  Advancing nucleosynthesis in self-consistent, multidimensional models of core-collapse supernovae
• Á. Horváth, Hungary
  Determination of the 8Li neutron capture via the inverse reaction
• C. Ishizuka, Japan
  How do neutron star radii depend on their core-crust EoS?
• M. Jadhav, United States
  Evidence for neutron capture at high neutron density in presolar grains
• P. Jimenez Bonilla, Spain
  Measurement of the 197Au(n,g) stellar cross section by activation
• O. Just, Germany
  Comprehensive nucleosynthesis analysis for ejecta of compact binary mergers
• H. Kadi, Algeria
  Heat capacity of the tin neutron-rich isotopes, including quantal and statistical fluctuations
• T. Kajino, Japan
  Asymmetric neutrino emission process and rapid spin-deceleration of magnetized  proto-neutron stars
• A. Kankainen, United Kingdom
  26Al/30P(d,n) reactions for key astrophysical resonances in explosive hydrogen burning
• M. Katsuma, Japan
  Theoretical reaction rates of the 12C(α,γ)16O reaction from the potential model
• S. Kawagoe, Japan
  Effects of collective oscillation and MSW matter effect on 3D hydrodynamics core-collapse supernova models
• T. Kibedi, Australia
  The radiative width of the hoyle state from cascading gamma-ray measurements
• Y. Kikuchi, Japan
  Effects of triple-alpha reactions on the supernova nucleosynthesis
• G. Kiss, Hungary
  Alpha induced thick target yield measurement on iridium isotopes
• M. Kiss, Hungary
  Rate analysis or a possible interpretation of abundances
• C. Kobayashi, United Kingdom
  Faint population III supernova as the origin of the most iron-poor stars
• A. Kontos, United States
  Gas-jet targets for reaction studies in nuclear astrophysics
• H. Leeb, Austria
  Microscopic approach to alpha-nucleus optical potentials for nucleosynthesis
• A. Lepine-Szily, Brazil
  Spectroscopy of 9BE close to the proton threshold using 8Li(p,p), 8Li(p,d) and 8Li(p,α) reactions
• C. Liu, Sweden
  Finding the lost siblings of the sun
• W. Liu, China
  Measurement of astrophysical 13C(α,n)16O reaction and ßeta decay of nuclei in rp-process
• R. Longland, United States
  New techniques for integrating nuclear reaction networks
• M. Martin, Germany
  Nucleosynthesis in the ejecta of neutron star mergers
• V. Maslyuk, Ukraine
  Atomic nuclei formation as a result of the nuclear matter disintegration
• Z. Meisel, United States
  Time-of-flight mass measurement of neturon-rich nuclei
• H. Möller, Germany
  Impact of nuclear reactions at high densities on the fate of intermediate-mass stars
• A. Murphy, United Kingdom
  Study of the 44Ti(α,p)47V reaction and implications for core collapse supernovae
• N. Nishimura, United Kingdom
  A large scale Monte Carlo study of nucleosynthesis based on nuclear physics uncertainties
• N. Nishimura, United Kingdom
  Global simulations of magneto-rotational supernova with MRI for an origin of R-process nucleosynthesis
• L. Oláh, Hungary
  Portable tracking detector for cosmic background measurements
• W.J. Ong, United States
  Resonance energy measurements along the rp-process path with GRETINA
• A. Ornelas, Hungary
  α-scattering experiment on 64ZN and the low energy α-nucleus optical potential
• U. Ott, Hungary
  Ruthenium isotope composition of allende refractory metal nuggets
• N. Özkan, Türkey
  Charged particle induced reaction cross sections on p-isotopes of erbium for the astrophysical γ-process
• A. Palumbo, USA
  Nuclear reaction rates for astrophysical nucleosynthesis
• M. Patial, Sweden
  A novel approach for odd-odd nuclei applied to proton emitters
• M. Paul, Israel
  44Ti half-life (continued)
• G. Perdikakis, United States
  Using (p,n) reactions to experimentally access reaction rates relevant to the νp-process
• R. Pozhath, India
  Chemical tagging of stellar streams: Origin scenarios
• T. Prodanovic, Serbia
  Galactic interactions: New source of lithium?
• S. Quinn, United States
  Measurement of the 58Ni(a,g)62Zn reaction and its astrophysical impact
• T. Rauscher, United Kingdom
  Production of 146SM and 92NB in the g-process
• J. Refsgaard, Denmark
  Characterisation of the 12C(α,γ)16O-reaction through study of the β-delayed α-decay from 16N
• T. Reinhardt, Germany
  S-factor measurement of the 12C(p,gamma)13N reaction in inverse kinematics
• C. Ritter, Canada
  THE GCE SYGMA (Stellar Yields for Galaxy Modeling Applications) module
• C. Ritter, Canada
  I process and CEMP-s+r stars
• P. Roy Chowdhury, India
  The possibility of existence of massive pulsars with quark core
• P. Roy Chowdhury, India
  From nuclear reactions to stellar matter: A unified approach
• K. Sagara, Japan
  Measurement of 4He (12C, 16O)  total cross section down to Ecm = 1.0 MeV at KUTL
• M. Sancho Miranda, United Kingdom
  The distribution of metals in the thick disc
• V. Schaffenroth, Austria
  Observation of the extreme runaway HD 271791: Nucleosynthesis in a core collapse supernova
• K. Schmidt, Germany
  The 40Ca(α,γ) 44Ti reaction studied by in-beam γ-spectroscopy and activation
• P. Scholz, Germany
  Experimental approaches for charged-particle induced reaction studies relevant for the p process
• S. Sengupta, Germany
  The BONNFIRES scheme for population studies of CEMP stars
• S. Shibagaki, Japan
  R-process nucleosynthesis in neutron star merger with new fission model
• A. Sieverding, Germany
  Neutrino nucleosynthesis in the outer layers of supernovae
• C. Siqueira Mello, Brazil
  High-resolution abundance analysis of very metal-poor R-I stars
• Y. Skakun, Ukraine
  Cross sections of the 76Se(p,γ)77m,gBr, 77Se(p,n)77m,gBr and 80Se(p,n)80m,gBr reactions for the astrophysical γ-process
• K. Smith, United States
  β-decay studies of very neutron-rich Pd and Ag isotopes
• T. Suda, Japan
  Formation and evolution of carbon-enhanced metal-poor stars
• C. Sullivan, United States
  Understanding the sensitivity of core-collapse supernovae simulations to weak interaction rates
• T. Szalai, Hungary
  The chemical composition of the ejecta of the rare type IIb supernova 2013df
• T. Szücs, Hungary
  Determination of level widths in 15N using nuclear resonance fluorescence
• T. Szücs, Hungary
  Background intercomparison with an active shielded HPGE detector extended to Freiberg mine in Germany
• M. Takács, Germany
  The 3He(alpha, gamma)7Be reaction rate, solar 7Be and 8B neutrino fluxes, and the production of 7Li during the Big Bang
• N. Targosz-Sleczka, Poland
  New experimental constraints on the electron screening effect in astrophysical plasma
• O. Tesileanu, Romania
  Astrophysics studies at the future ELI-NP European Research Center
• B. Thomas, Germany
  The Production of‭ ‬91NB for a measurement‭ ‬of the‭ ‬91NB(p,g‭) ‬reaction‭ ‬at Franz
• H. Togashi, Japan
  Nuclear equation of state for core-collapse supernovae with realistic nuclear forces
• C. Travaglio, Italy
  GCE and solar S-process abundances: Dependence on the 13C-pocket structure
  
• E. Vangioni, France
  Standard Big-Bang nucleosynthesis after Planck
• E. Vangioni, France
  Cosmic star formation, gamma-ray burst rate at high redshift and cosmic chemical evolution
• L. Wagner, Germany
  The 14N(p,gamma)15O S factor at 0.4 – 1.5 MeV
• R. Werner, South Africa
  Shell-model studies of the astrophysical RP-reaction 30P(p,gamma)31S
• M. Wu, Germany
  Neutrinos and nucleosynthesis of heavy elements
• H. Yamaguchi, Japan
  Equipment to measure He(12C,16O)γ total cross section at Ecm = 1.0 MeV at KUTL
• Y. Yamamoto, Japan
  A systematic theoretical study of explosion energies in core collapse supernovae
• T. Yoshida, Japan
  Type IC core-collapse supernovae evolved from very massive stars

Not confirmed posters

• A. Chen, Canada
  Structure of 31S from (d,t) and (p,d) transfer reactions
• N.I. Costiris, Greece
  β—decay half-lives of nuclei in the crust of neutron stars: The ANN model
• D. Jain, India
  Role of spin dependent nuclear potential in the fusion of Se* isotopes
• H.M. Silva, Portugal
  Measurement of the 16O + 16O elastic scattering cross section below the coulomb barrier