Important dates
1 February 2014
Start of registration
15 February 2014
Abstract submission open
6 April 2014
Abstract submission closed
22 April 2014 !!!
Early bird reg. fee payment
Conference program announced
30 June 2014
Regular reg. fee payment
7 July 2014
Start of conference
News
11 June 2014
Detailed scientific
program launched
30 May 2014
Poster abstracts
published
10 May 2014
Oral lectures' abstracts
& Invited speakers
CVs published
30 April 2014
Speakers list announced
10 April 2014
Early bird registration
extended to 22 April
4 April 2014
Confirmed invited
speakers announced
1 April 2014
Abstract submision
deadline extended
to 6 April
10 March 2014
Social events & optional
tours menu launched
4 March 2014
Accommodation
information launched
3 March 2014
Information on the
"Classical Novae in
the Cosmos" workshop
26 February 2014
Information on the
Budapest-Debrecen
organised transfer
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