High-energy neutrino flux from SN2024ggi: constraints from semi-analytic modeling of its post-explosive emission

Documenti analoghi

• Long-rising Type II supernovae resembling supernova 1987A -- II. A new analytical model to describe these events
  di: Pumo, M. L., et al.
  Pubblicazione: (2025)
• High-Energy Neutrinos by Hydrogen-rich Supernovae interacting with low-massive Circumstellar Medium: The Case of SN 2023ixf
  di: Cosentino, S. P., et al.
  Pubblicazione: (2025)
• Constraints on the progenitor and explosion of SN 2024ggi in harmony with pre-explosion detection and hydrodynamic simulations
  di: Aryan, Amar, et al.
  Pubblicazione: (2025)
• Physical properties of long-rising type II supernovae -- Bayesian analytic modeling and spectrophotometric correlations
  di: Cosentino, S. P., et al.
  Pubblicazione: (2025)
• The compact circumstellar material of SN 2024ggi: Another supernova with a pre-explosion effervescent zone and jet-driven explosion
  di: Soker, Noam
  Pubblicazione: (2024)