Final answer:
The collapse and explosion of a high-mass star involve the formation of heavier elements through fusion, core collapse beyond the Chandrasekhar limit, creation of neutrons, a rebound shock wave, and the outward propagation of the shock wave leading to a supernova.
Step-by-step explanation:
The steps of a high-mass star's core collapse and explosion event, also known as a supernova, are as follows:
- Nuclear fusion of heavier and heavier elements until an iron core is formed.
- The core exceeds the Chandrasekhar limit and begins to collapse, forming a neutron star.
- Electrons are absorbed by protons, creating neutrons and neutrinos.
- The collapse of the core is abruptly halted by degenerate neutrons, causing a rebound.
- A shock wave propagates outward from the core due to the rebound.
This process leads to the explosion of the star, dispersing elements into space and possibly leaving behind a neutron star, or in some cases, a pulsar. The shock wave that blows apart the star is aided by the neutrinos interacting with the surrounding matter, reversing the infall of the star's layers and causing the explosion.