In stars below about 2.2 solar masses, what condition makes the onset of helium fusion an explosive "Helium Flash"?

Answer

The core is degenerate, meaning pressure does not immediately increase with temperature

In a degenerate core, the pressure is independent of temperature. When helium finally begins fusing via the triple-alpha process, the energy release accelerates without corresponding pressure relief to stop it, causing a runaway reaction.

In stars below about 2.2 solar masses, what condition makes the onset of helium fusion an explosive "Helium Flash"?
evolutionhydrogenCorestarFusion