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International Conference on Nuclear Astrophysics and Stellar Evolution

📅 7–8 Jun 2027 📍 Kobe, Japan 👤 Standard / Listener

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$185

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Conference session tracks

Key research areas covered across the sessions — tap a track to read more.

This track focuses on the fundamental nuclear processes that occur within stars, including fusion and fission reactions. Participants will discuss the implications of these reactions for stellar evolution and nucleosynthesis.

This session will explore advanced computational techniques used to model stellar interiors and evolution. Emphasis will be placed on the accuracy of simulations in predicting stellar behavior and nucleosynthesis outcomes.

This track will cover the latest observational techniques and findings related to supernovae, including their role in cosmic nucleosynthesis. Discussions will include the implications of supernova observations for our understanding of stellar evolution.

Participants will delve into the unique properties of neutron stars and their formation processes. The track will also address their role in the broader context of stellar evolution and nucleosynthesis.

This session will focus on the contributions of gamma-ray astronomy to our understanding of nucleosynthesis in the universe. Key topics will include the detection of gamma-ray emissions from various astrophysical sources.

This track will investigate the isotopic compositions produced in different stellar environments and their significance for understanding stellar evolution. Participants will discuss methods for measuring isotopic abundances and their implications for nucleosynthesis theories.

This session will explore the role of plasmas in stellar environments, including their impact on stellar dynamics and nucleosynthesis. Discussions will include the interaction of magnetic fields and plasma flows in stellar interiors.

This track will provide a comprehensive overview of the theoretical frameworks that underpin our understanding of stellar evolution. Participants will discuss recent advancements and future directions in stellar evolution theory.

This session will focus on the processes that lead to the formation of elements in stars and during explosive events like supernovae. Discussions will include the implications of these processes for the chemical evolution of galaxies.

This track will examine the importance of reaction rates in the context of stellar nucleosynthesis. Participants will discuss experimental and theoretical approaches to determining these rates and their implications for stellar models.

This session will explore the processes of star formation and how they influence subsequent stellar evolution. Discussions will include the interplay between initial conditions and the resulting stellar characteristics.