The Flavor of Neutrinos Could Determine How a Large Star Dies

Astrophysicists are investigating how the 'flavor' of neutrinos produced during a star's core collapse influences whether the star ends in a supernova explosion or a direct collapse into a black hole. Understanding these subatomic particles could resolve long-standing mysteries about stellar evolution.
Why it matters
Advances fundamental knowledge in astrophysics and the life cycles of massive stars.
A core-collapse supernova occurs when a massive star reaches the end of its life. After running out of hydrogen and other light elements to burn, the star makes a last ditch effort to counter gravity, fusing ever heavier elements at an ever faster pace. Eventually it reaches the point where heavy fusion extracts energy from the core rather than adds it. The core rapidly contracts, then recoils. The resulting explosion rips the star apart and briefly outshines an entire galaxy. But not all giant stars end with a bang. Some of them experience a core collapse so quick and dense that the core squeezes itself into a black hole. These stars end with a whimper rather than a bang.
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