Can neutron star mergers alone explain the r-process enrichment of the Milky Way?

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  SRP72: SRP-Onderzoekszwaartepunt: High-energy physics (HEP@VUB).

  Craps, B. (Administrative Promotor), D'Hondt, J. (Administrative Promotor), D'Hondt, J. (CoI (Co-Promotor)), Buitink, S. (Co-Promotor), Craps, B. (Co-Promotor), De Vries, K. (Co-Promotor), Lowette, S. (Co-Promotor), Mariotti, A. (CoI (Co-Promotor)), Tytgat, M. (CoI (Co-Promotor)), Uhlemann, C. (CoI (Co-Promotor)), Sevrin, A. (CoI (Co-Promotor)) & Van Eijndhoven, N. (CoI (Co-Promotor))

  1/11/22 → 31/10/29

  Project: Fundamental

  • Detectors 100%
  • Standard Model 73%
  • Lepton 72%
  • Muon 61%
  • Higgs Boson 58%