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First IRENA-IANNA Workshop

Jun 9 – 11, 2024
Notre Dame
America/Indiana/Indianapolis timezone

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Session

Session 1

1
Jun 10, 2024, 9:00 AM
Notre Dame

Notre Dame

Embassy Suites by Hilton South Bend at Notre Dame, US 1140 E Angela Blvd, South Bend, IN 46617, US

Description

Chair: L. Acosta

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  1. 37. Welcome
    James deBoer (University of Notre Dame)
    6/10/24, 9:00 AM
    Welcome

    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.

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  2. 46. Welcome 2
    Luis Armando Acosta Sanchez (Universidad Nacional Autonoma (MX))
    6/10/24, 9:08 AM

    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. For the opening of the conferences, we will have short explanations about IRENA (James deBoer) and IANNA (Luis...

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  3. 48. Nuclear Astrophysics Landscape in Portugal
    Daniel Galaviz Redondo (Laboratory of Instrumentation and Experimental Particle Physics (PT))
    6/10/24, 9:15 AM

    This year, Portugal celebrates the 50$^{th}$ anniversary of the democratic revolution and the pacific start of democracy. Ever since, the Portuguese science landscape has evolved enormously, with many high quality scientists educated outside the Portuguese borders establishing their research groups in universities and research centers, and bringing Portugal into the international scientific...

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  4. 34. 58Ni(3He,t)58Cu Measurements to Constrain the Astrophysical Rate of 57Ni(p,γ)
    Patrick O'Malley (University of Notre Dame)
    6/10/24, 9:45 AM

    The 57Ni(p,γ)58Cu reaction rate significantly impacts nucleosynthesis in a variety of astrophysical sites. In core-collapse supernovae (CCSNe) this reaction impacts the production of 44Ti, a radioisotope whose observed gamma-ray emissions offer an important probe into CCSNe, providing a test of nucleosynthesis models. Furthermore, the 57Ni(p,γ)58Cu reaction rate has been shown to significantly...

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  5. 52. Experiments at the FRIB ReAccelerator
    Ana Henriques
    6/10/24, 10:15 AM

    The Facility for Rare Isotope Beams (FRIB) is a scientific user facility funded by the US Department of Energy Office of Science (DOE-SC) located at the Michigan State University. FRIB started operations in May 2022 and is ramping towards its designed 400 kW of driver beam power.

    Within the FRIB laboratory, the ReAccelerator (ReA) is a superconducting LINAC aimed to reaccelerate stopped...

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  6. 28. Systematic optical potentials for cluster-structured nuclei reactions
    Lucas Garrido
    6/10/24, 10:45 AM

    Within the IANNA framework, we propose new instruments for nuclear reactions measurements, systematical data and theoretical analyses. In Seville (Spain), we have the National Accelerator Centre (CNA), where a permanent experimental setup is coupled to the 3MV tandem accelerator. Such a setup is based on MARS (Modular Apparatus for nuclear Reactions Spectrometry). With MARS, first exploratory...

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