Question

What are the processes that reverse the in fall of matter during a type II supernova explosion and blast material out of the star?

Short answer

Neutrino heating revitalizes the shock wave that ejects the star's outer layers in a type II supernova.

Step-by-step solution

Core Collapse

In a type II supernova explosion, the core of the massive star has exhausted its nuclear fuel, causing it to collapse under gravity. The collapse is halted by neutron degeneracy pressure, forming a neutron star at the center of the core.

Shock Wave Formation

As the core collapses, it releases a tremendous amount of energy in the form of neutrinos. This energy generates a shock wave that propagates outward, attempting to reverse the infall of matter from the outer layers of the star.

Neutrino Heating

The shock wave initially loses energy as it pushes against the infalling material. Neutrinos, which carry away most of the core's gravitational binding energy, deposit energy behind the shock wave, revitalizing it through a process called neutrino heating.

Shock Wave Propagation

The energy transferred by neutrino heating re-energizes the shock wave, allowing it to overcome the gravitational pull of the star's outer layers and push them outward, converting the implosion into an explosion.

Ejection of Stellar Material

The revitalized shock wave, now carrying sufficient energy, blasts the outer layers of the star into space, creating the supernova explosion and leaving behind a neutron star or, in some cases, a black hole.

Key concepts

Core Collapse

At the heart of a type II supernova explosion lies the dramatic core collapse. This process begins when a massive star exhausts its nuclear fuel. Without this fuel, the core cannot generate the pressure needed to counteract gravity. As a result, gravity wins, and the core rapidly collapses.
This collapse continues until it is halted by a phenomenon known as "neutron degeneracy pressure." Imagine the core densely packed with neutrons, a state where further compression is strongly resisted. Here, the core transforms into a neutron star.
Understanding core collapse is key to grasping how a massive star begins its journey to becoming a spectacular supernova.

Neutrino Heating

As the core collapses and becomes a neutron star, it releases an immense amount of energy in the form of neutrinos. These are nearly massless particles that travel almost at the speed of light.
Neutrinos play a crucial role by transporting energy away from the core, a process known as "neutrino heating." These elusive particles deposit enough energy behind the initial shock wave to reinvigorate it.

• Neutrinos carry away gravitational binding energy.
• They rejuvenate the shock wave by depositing energy behind it.

Without this rejuvenation, the shock wave would peter out quickly, unable to overturn the star's gravitational pull.

Shock Wave Propagation

The shock wave propagation in a supernova marks the turning point where the implosion transforms into an explosion. Initially, as the shock wave moves outward from the core, it loses energy battling against the infalling outer layers of the star.
Thanks to neutrino heating, the shock wave receives a much-needed energy boost. This revitalized shock wave can now overcome the gravitational forces of the outer star layers.

• The shock wave earns a fresh burst of energy from neutrino heating.
• It then spreads, reversing the doom-bound collapse into a triumphant breakout.

The energy and momentum imparted during shock wave propagation are pivotal for the eventual supernova explosion.

Nuclear Fuel Exhaustion

Nuclear fuel exhaustion is the silent precursor to a star's monumental collapse and explosion. During its life, a star fuses lighter elements like hydrogen and helium into heavier ones in its core, a process that slashes the star's lifespan.
Once the star depletes its nuclear fuel reserves, specifically its ability to fuse iron, the star can no longer support itself against its own gravity.

• Nuclear fusion processes are halted.
• The core's energy production dissipates.

This exhaustion sets the stage for the core collapse, ultimately leading to the chain reaction that causes the type II supernova. Understanding fuel exhaustion is essential to comprehending why these dramatic events occur.