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CGS17

17–21 Jul 2023
MAISON MINATEC
Europe/Paris timezone

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Session

Session 8

S8
19 Jul 2023, 09:00
Amphitheater (MAISON MINATEC)

Amphitheater

MAISON MINATEC

Centre de Congrès Maison MINATEC 3 parvis Louis Néel 38054 Grenoble Cedex 9

Conveners

Session 8

  • G. Lotay (University of Surrey, Guildford, UK)

Presentation materials

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  1. 161. The nuclear physics of r-process observables
    Rebecca Surman (University of Notre Dame, USA)
    19/07/2023, 09:00
    Nuclear Astrophysics
    Keynote

    Over five years ago the groundbreaking gravitational wave event GW170817 provided the first direct proof that neutron star mergers produce heavy elements via rapid neutron capture (r-process) nucleosynthesis. Still, the extent of the element synthesis in this environment and the role of neutron star mergers in contributing to the galactic tally of r-process elements have yet to be clarified....

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  2. 122. Underground nuclear astrophysics at LUNA and the Bellotti Ion Beam Facility of the INFN-LNGS
    Andreas Best
    19/07/2023, 09:45
    Nuclear Astrophysics
    Invited Oral

    Deep underground nuclear astrophysics with the LUNA experiment at the Gran Sasso National Laboratory by now has a 30-year history and a long track record of measuring crucial reactions for various nucleosynthesis scenarios, from the Big Bang to p-p and CNO reactions to the production of the heavy elements in the s process.
    With the recent installation of a 3.5 MV accelerator at the LNGS and...

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  3. 127. Cross section measurements for Nuclear Astrophysics using the Trojan horse method
    Aurora Tumino (UKE & INFN-LNS)
    Nuclear Astrophysics
    Invited Oral

    I discuss the basic concepts of the Trojan Horse Method in nuclear astrophysics and the opportunity it offers to determine the cross sections of various stellar burning reactions when it is difficult to perform the corresponding direct measurements. I will focus on recent results to investigate carbon burning and primordial nucleosynthesis.

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  4. 152. The nuclear physics of r-process observables
    Rebecca Surman (University of Notre Dame, USA)
    Nuclear Astrophysics
    Keynote

    Over five years ago the groundbreaking gravitational wave event GW170817 provided the first direct proof that neutron star mergers produce heavy elements via rapid neutron capture (r-process) nucleosynthesis. Still, the extent of the element synthesis in this environment and the role of neutron star mergers in contributing to the galactic tally of r-process elements have yet to be clarified....

    Go to contribution page
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