The limit beyond which the stars suffer internal collapse is referred to as the Chandrashekhar limit.
Explanation:
The Chandrashekhar limit is the maximum mass of a stable white dwarf star, beyond which it cannot sustain itself against gravitational collapse.
It is approximately 1.4 times the mass of the Sun, and exceeding this limit leads to the collapse of the star, potentially resulting in a supernova or the formation of a neutron star or black hole.
Other Options:
Raman Effect: A physical phenomenon related to the scattering of photons, discovered by Sir C.V. Raman.
Aurora Borealis: Also known as the Northern Lights, a display of natural light in the Earth's sky, predominantly seen in high-latitude regions.