7–13 Sept 2024
Asia/Shanghai timezone
The third circular has been released.

Neutrino and Heavy-element Nucleosynthesis in Supernovae

10 Sept 2024, 10:15
25m
Invited Talk Explosive Stellar Objects and Nuclear Physics Explosive Stellar Objects and Nuclear Physics

Speaker

Xilu WANG (Institute of High Energy Physics, Chinese Academy of Sciences)

Description

Neutrinos can play an important role in the synthesis of nuclides in high energy astrophysical processes involving compact objects, such as core-collapse supernovae or binary neutron star mergers, where neutrinos can experience collective flavor oscillations driven by neutrino-neutrino interactions. Here, we seek to explore the possible influences of neutrino interactions on the heavy-element nucleosynthesis including νp-process and r-process in supernova environments with different astrophysical conditions and neutrino inputs. We find that the potential impact is particularly strong in high-entropy, proton-rich conditions, where neutrino interactions can nudge an initial νp process neutron rich, introducing a new neutrino-induced neutron capture process "νi process".

Primary author

Xilu WANG (Institute of High Energy Physics, Chinese Academy of Sciences)

Co-authors

Baha BALANTEKIN (University of Wisconsin, Madison) Michael CERVIA Amol PATWARDHAN Rebecca SURMAN (University of Notre Dame)

Presentation materials

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