17th Rußbach School on Nuclear Astrophysics

Speaker List

• David Aguado (Università degli Studi di Firenze, Italy)
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    Hunting the Descendants of the Very Massive First Stars

• Filippo Angelini (Università degli Studi di Padova, Italy)
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    Study of the interplay between nuclear charge and energy loss in the FALSTAFF spectrometer

• Axel Boeltzig (HZDR)
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    Nuclear Astrophysics in Underground Laboratories

• François de Oliveira Santos (GANIL, France)
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    A textbook case in experimental nuclear astrophysics: The 18F(a,p)15O reaction

• Dijana Đeorđić ( Jožef Stefan International Postgraduate School)
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    Electron Screening in Nuclear Reactions

• Roland Diehl (Max Planck Institute for Extraterrestrial Physics, Germany)
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    Cosmic Gamma-Rays in the Multi-Messenger Era

• Hoa Dinh Thi (Laboratoire de Physique Corpusculaire, France)
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    The nuclear matter density functional under the nucleonic hypothesis

• Jérôme Guilet (CEA Saclay, France)
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    The physics of core collapse supernovae (part 1)

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    The physics of core collapse supernovae (part 2)

• János Kodolányi (Max Planck Institute for Chemistry, Germany)
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    Presolar grains - a general introduction

• Dominik Koll (Helmholtz-Zentrum Dresden-Rossendorf, Germany)
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    Combined search for live stellar Fe-60 and r-process synthesized Pu-244 in terrestrial archives

• Sándor Kovács (University of Debrecen)
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    Measuring the half-life values for exotic rare-earth isotopes

• Karl-Ludwig Kratz ( Johannes-Gutenberg-Universität zu Mainz)
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    The classical r-process revisited: what’s left over — what’s new?

• Karl-Ludwig Kratz (ohannes Gutenberg-Universität Mainz, Germany)
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    From the classical r-process to the multimessenger era

• Pavel Kroupa (Rheinische Friedrich-Wilhelms-Universität Bonn, Germany, and Univerzita Karlova, Czech Republic)
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    The initial mass function of stars

• Pavel Kroupa
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    The formation of super-massive black holes and on the (probable?) very rapid initial metal & r-process enrichment

• Marco Salvatore La Cognata (IFIN-LNS)
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    Recent results in nuclear astrophysics with indirect methods

• Gerrit Leck (TU Darmstadt and GSI)
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    Simulating kilonova spectra with detailed atomic opacities

• Matej Lipoglavšek (Jožef Stefan Institute, Ljubljana, Slovenia)
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    Nuclear reactions in normal versus inverse kinematics

• Laura Magrini (INAF Osservatorio Astrofisico di Arcetri)
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    GAIA-ESO survey: origin and evolution of neutron capture elements

• Maria Markova (Universitetet i Oslo, Norway)
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    Comprehensive test of the brink-axel hypothesis in the energy region of the pygmy dipole resonance

• Sébastien Martinet (Université de Genève, Switzerland)
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    Short-lived nuclei in very massive stars

• Marta Molero (Università degli Studi di Trieste, Italy)
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    Evolution of neutron capture elements in dwarf galaxies

• Chiranjib Mondal (Laboratoire de Physique Corpusculaire, Caen, France)
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    Can we decipher the composition of the core of a neutron star?

• Jean Nippert (Université de Strasbourg and IPHC, France)
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    12C fusion at deep sub-barrier energies with STELLA

• Sara Palmerini (INFN and University of Perugia)
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    AGB stars and s-process

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    Introduction to stellar evolution

• Wanja Paulsen (Universitetet i Oslo, Norway)
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    Reassessment of the radiative ɣ-decay branch of the Hoyle state

• Francesco Pogliano (University of Oslo)
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    i process and the neutron-capture rate of Sb-126

• Georg Rugel (Helmholtz-Zentrum Dresden-Rossendorf, Germany)
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    Nuclear astrophysics with Accelerator Mass Spectrometry (AMS)

• Georg Rugel (Helmholtz-Zentrum Dresden-Rossendorf, Germany)
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    In Memory of Shawn Bishop

• Konrad Schmidt (HZDR)
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    Closing Remarks

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    Nuclear Astrophysics Schools partnering with ChETEC INFRA

• Ása Skúladóttir (University of Florence and INAF)
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    Dwarf galaxies' view of the heavy elements

• Tibor Norbert Szegedi (University of Debrecen)
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    Cross section measurement of the 92,94Mo(α,n) and 92Mo(α,p) reactions by γ-spectroscopy

• Aurora Tumino (Università Kore di Enna and INFN-LNS)
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    Resonant 12C+12C fusion at astrophysical energies

• Louis Wagner (TRIUMF, Canada)
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    Direct measurement of 56Ni(α,p)59Cu to improve X-ray burst models

• Kaitlin Webber (Texas A&M University, USA)
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    Abundance analysis of the Cetus II dwarf galaxy

• Tyler Wheeler (Michigan State University, USA)
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    The 15O(α,γ)19Ne reaction in type I X-ray bursts

• Erin White (Michigan State University, USA)
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    Progress towards a single atom microscope for nuclear astrophysics

• Henriette Wirth (Charles University of Prague)
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    How many explosions does one need? - Quantifying supernovae in globular clusters from iron abundace spreads