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Hirschegg 2025 - Nucleosynthesis of Heavy Elements: r-process

19.–25. Jan. 2025
Darmstädter Haus
Europe/Berlin Zeitzone

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Liste der Beiträge

43 von 43 angezeigt
  1. 49. Comprehensive modeling of Core Collapse Supernovae
    William Raphael Hix (Oak Ridge National Laboratory / University of Tennessee)
    20.01.25, 09:00
  2. 50. Magnetically-powered explosions in the multimessenger era
    Philipp Mösta (University of Amsterdam)
    20.01.25, 09:30
  3. 51. Nucleosynthesis in magnetorotational supernovae
    Martin Obergaulinger (Universitat de València)
    20.01.25, 10:00
  4. 52. Nucleosynthesis of QCD driven core-collapse supernovae as rare r-process site
    Tobias Fischer (University of Wroclaw)
    20.01.25, 11:00
  5. 53. Estimates for the nebular emission from r-process elements
    Giacomo Ricigliano (TU Darmstadt)
    20.01.25, 11:20
  6. 54. Equation of state constraints from helium in kilonovae
    Oliver Just (GSI Helmholtzzentrum für Schwerionenforschung)
    20.01.25, 11:40
  7. 55. TBD
    Daniel Siegel (University of Greifswald)
    20.01.25, 16:45
  8. 56. Chemical evolution of neutron-capture elements: a homogenous approach
    Marta Molero (TU Darmstadt)
    20.01.25, 17:15
  9. 57. Galactic Archaeology with neutron capture elements
    Gabriele Cescutti (Università degli studi di Trieste)
    20.01.25, 17:45
  10. 58. Galactic Chemical Evolution with r-process elements
    Benjamin Wehmeyer (University of Wroclaw)
    21.01.25, 09:00
  11. 59. r-process enrichment in simulations of galaxy formation
    Freeke van de Voort (Cardiff University)
    21.01.25, 09:30
  12. 60. Nuclear theory for the r -process: masses, fission and β decays
    Giuliani Samuel A. (Universidad Autónoma de Madrid)
    21.01.25, 10:00
  13. 61. Fast neutrino flavor conversions in QCD supernovae and potential effects on nucleosynthesis
    Zewei Xiong (GSI Helmholtzzentrum für Schwerionenforschung)
    21.01.25, 11:00
  14. 62. r-process nucleosynthesis and radioactively powered transients from magnetar giant flares
    Anirudh Patel (Department of Physics, Columbia University)
    21.01.25, 11:20
  15. 63. TBD
    Christine Collins (Trinity College Dublin)
    21.01.25, 11:40
  16. 64. Dwarf galaxies showing evidence of two r-process sources
    Ása Skúladóttir (Department of Physics and Astronomy, University of Florence)
    21.01.25, 16:45
  17. 65. Actinide Production in Galactic Mergers
    David Aguado (Instituto de Astrofísica de Canarias (IAC))
    21.01.25, 17:15
  18. 66. Complete and Calibrated Lanthanide Opacities
    Andreas Flörs (GSI Helmholtzzentrum für Schwerionenforschung)
    21.01.25, 17:45
  19. 67. TBD
    Ryan Foley (UC Santa Cruz)
    22.01.25, 09:00
  20. 68. Direct numerical modeling of binary neutron star mergres
    Kenta Kiuchi (Albert Einstein Institute)
    22.01.25, 09:30
  21. 69. Nebular Emission of Neutron Star Merger
    Kenta Hotokezaka (University of Tokyo)
    22.01.25, 10:00
  22. 70. An NLTE Analysis of Infra-Red Forbidden Emission Lines in Kilonovae
    Quentin Pognan (Albert Einstein Institute)
    22.01.25, 11:00
  23. 71. Directional Spectra from 3D Neutron Star Merger Simulations
    Dr. Luke Shingles (GSI Helmholtzzentrum für Schwerionenforschung)
    22.01.25, 11:20
  24. 72. Modelling realistic kilonova spectra at nebular phase
    Smaranika Banerjee (Stockholm University)
    22.01.25, 11:40
  25. 73. What we know about kilonovae from observations over the past seven years
    Darach Watson (Niels Bohr Institute, University of Copenhagen)
    22.01.25, 16:45
  26. 74. Mid-infrared emission by kilonovae, and opportunities with JWST
    Anders Jerkstrand (Stockholm University)
    22.01.25, 17:15
  27. 75. Modelling the spectra and light curves of binary neutron star mergers
    Stuart Sim (Queen's University Belfast)
    22.01.25, 17:45
  28. 76. Neutrinos in and from r-process sources
    Irene Tamborra (Niels Bohr Institute)
    23.01.25, 09:00
  29. 77. Precision mass measurements for the r process
    Anu Kankainen (University of Jyväskylä)
    23.01.25, 09:30
  30. 78. Nuclear astrophysics utilising highly charged ions
    Yury Litvinov (GSI Helmholtzzentrum für Schwerionenforschung)
    23.01.25, 10:00
  31. 79. High precision measurement of alpha-induced reactions for weak r-process nucleosynthesis
    Gabor Kiss (Atomki)
    23.01.25, 11:00
  32. 80. Ab initio calculations of beta-decay half-lives for N=50 neutron-rich nuclei
    Zhen Li (TU Darmstadt)
    23.01.25, 11:20
  33. 81. Neutron capture Rates and RIB experiments
    Dennis Muecher (Institute for Nuclear Physics, University of Cologne)
    23.01.25, 11:40
  34. 82. Constraining neutron-capture reactions for the r process
    Artemis Spyrou (Michigan State University)
    23.01.25, 16:45
  35. 83. Forging the Cosmos: Exploring Stellar Explosions, Neutron Star Mergers, and the R-Process
    Fernando Montes (Facility for Rare Isotope Beams at Michigan State University)
    23.01.25, 17:15
  36. 84. Solar r-process abundances and direct neutron capture measurements on radioactive isotopes
    César Domingo-Pardo (IFIC (CSIC-UV))
    23.01.25, 17:45
  37. 85. TBD
    Carla Frohlich (North Carolina State University)
    24.01.25, 09:00
  38. 86. Heavy element abundances from a universal primordial distribution
    Gerd Roepke (University of Rostock, Institute of Physics)
    24.01.25, 09:30
  39. 87. Beta-decay properties of neutron-rich lanthanides and the formation of the rare-earth peak
    Sándor Kovács (HUN-REN Institute for Nuclear Research)
    24.01.25, 09:50
  40. 88. Improving nuclear structure calculations through new measurements of beta-delayed neutron emitters.
    Max Pallàs Solís (Universitat Politènica de Catalunya (UPC))
    24.01.25, 10:10
  41. 89. Constraining the helium abundance in AT2017gfo
    Rasmus Damgaard (DAWN, NBI, Copenhagen University)
    24.01.25, 11:00
  42. 90. Structure and Production of Superheavy Nuclei and the Island of Stability
    Horst Lenske (U. Giessen)
    24.01.25, 11:20
  43. 91. 56Ni production in neutrino-driven winds from long-lived binary neutron star merger remnants
    Maximilian Jacobi (Friedrich-Schiller-Universität Jena)
    24.01.25, 11:40