Data
First IANNA-IReNA Workshop on New Reaction Rates for Nuclear Astrophysics (Opens in a new window)
The first IANNA-IReNA workshop on new reaction rates for Nuclear Astrophysics is being organized as a collaboration between IANNA (Ibero American Network of Nuclear Astrophysics) and IReNA (International Research Network for Nuclear Astrophysics), with main co-sponsorship from IReNA.
2024 CeNAM Frontiers in Nuclear Astrophysics Meeting (Opens in a new window)
Hosted by the University of Notre Dame
The 2024 CeNAM Frontiers in Nuclear Astrophysics Meeting continues the series of former JINA and JINA-CEE Frontiers meetings with the goal to bring together the participants, collaborators, and other interested researchers in nuclear physics, astronomy, astrophysics, and other relevant fields to discuss progress and future directions in the understanding of the origin of the elements and the physics of neutron stars in the multi-messenger era.
Probing Dense Matter in Neutron Stars featuring Juergen Schaffner-Bielich (Goethe University Frankfurt) (Opens in a new window)
*Please note that this seminar will take place at 10am Eastern Time
Hosted by Melissa Mendes Silva (TU Darmstadt)
First Light And Reionisation Epoch featuring Aswin Vijayan (University of Sussex) (Opens in a new window)
Hosted by: Rob Yates (University of Surrey)
Nucleosynthesis with multi-dimensional supernova simulations featuring Andre Sieverding (LLNL) (Opens in a new window)
Hosted by: Avrajit Bandyopadhyay
The Other Side of Physics: Understanding, Awareness, and Support of Mental Health featuring Rachel Younger (MSU) (Opens in a new window)
Hosted by: Melissa Mendes (TU Darmstadt)
19th Russbach School on Nuclear Astrophysics (Opens in a new window)
The 19th Russbach School on Nuclear Astrophysics will take place in the village of Rußbach am Paß Gschütt, southeast of Salzburg, Austria. The school dates will be from March 03 (arrival and registration) to March 09 (departure) 2024.
Measurement of the 235U(n,f) cross section relative to n-p scattering up to 500 MeV at the n_TOF facility at CERN featuring Alice Manna (CERN) (Opens in a new window)
Hosted by: Denise Piatti (University of Padova)
Nuclear Reaction Rates for the s-process (Opens in a new window)
The slow neutron capture process (s-process) is one of the main mechanisms for the production of heavy elements in stars. In the recent years great effort was devoted on improving our knowledge on the nuclear reactions primarily responsible for s-process, i.e.13C(a,n)16O and 22Ne(a,n)25Mg.
Scalar and Vector Dark Matter Admixed in Neutron Stars featuring Cédric Jockel (Max Planck Institute for Gravitational Physics - Potsdam) (Opens in a new window)
Hosted by: Melissa Mendes Silva (TU Darmstadt)
The abundances of the elements in stars: 3D non-LTE modelling featuring Anish Amarsi (Uppsala University, Sweden) (Opens in a new window)
Hosted by: Thibaut Dumont (CNRS Strasbourg)
LUNA: Present and Future of Nuclear Astrophysics at LNGS featuring Federico Ferraro (LNGS) (Opens in a new window)
Hosted by: Denise Piatti (University of Padova)
The LUNA (Laboratory for Underground Nuclear Astrophysics) experiment is located at the LNGS (Laboratori Nazionali del Gran Sasso) in Italy. LUNA is aimed at studying the nuclear reactions that are responsible for the synthesis of the elements and shape the life of stars in the universe. The reduction of the cosmic-rays induced background provided by the 1400 m thick rock overburden at LNGS allows the direct measurement of the cross section in the energy range relevant to astrophysics.
Delving into the Chemical Diversity of the Metal-Poor Milky Way featuring Nicole Buckley (University of Surrey) (Opens in a new window)
Hosted by: Rob Yates (University of Hertfordshire)
Pulsational pair-instability supernovae in gravitational-wave and electromagnetic transients featuring David Hendriks (University of Surrey) (Opens in a new window)
Hosted by: Rob Yates (University of Hertfordshire)
Spectroscopic observations as tracers of stellar nucleosynthesis featuring Shreeya Shetye (KU Leuven) (Opens in a new window)
Hosted by: Thibaut Dumont (CNRS Strasbourg)
The groundwork for stellar nucleosynthesis was established over 70 years ago, marking the beginning of a fascinating journey. Since then, substantial progress has unfolded on both theoretical and observational fronts. On the theoretical side, intricate models of stellar evolution and nucleosynthesis have evolved, utilising increasingly precise nuclear data. Simultaneously, the observational realm has witnessed a significant rise in the number of stars analysed.
POSTPONED: Pulsational pair-instability supernovae in gravitational-wave and electromagnetic transients featuring David Hendriks (University of Surrey) (Opens in a new window)
*THIS SEMINAR HAS BEEN POSTPONED TO FRIDAY, DECEMBER 8th AT 2PM EASTERN TIME*
Hosted by: Rob Yates (University of Hertfordshire)
Atomic masses for nuclear structure and astrophysics: The new ion catcher and mass spectrograph at RIKEN's RIBF facility featuring Marco Rosenbusch (RIKEN) (Opens in a new window)
*Please note that this seminar will take place at 10am Eastern Time*
Hosted by: Shun Iimura (Rikkyo University)
Neutron-capture in the wild: finding r-process enhanced metal-poor stars in the Milky Way and beyond featuring Vinicius Placco (NSF NOIRLab) (Opens in a new window)
Hosted by: Avrajit Bandyopadhyay (University of Florida)
CANCELED: Measurement of the 235U(n,f) cross section relative to n-p scattering up to 500 MeV at the n_TOF facility at CERN featuring Alice Manna (CERN) (Opens in a new window)
*Due to unforeseen circumstances, this seminar is canceled*
Hosted by: Denise Piatti (University of Padova)