In The Final Dying Moments
When you're interest extends to astronomy, you quickly realise that in almost every area, we have learned so much, yet are still so far off from certainties.
One area this very much extends to is core collapse. We know a fair amount about the process, we know gravity eventually win's over as fusion in the core falters through increased content of Iron, but in all our attempts to actually model it, it's clear we're missing part of the puzzle.
above, a computer simulation of the inside of a star as it collapses
The problem is, as the core collapses, and gravity crushes down, the rest of the star falls inwards too, and a shockwave moves outwards. We known part of the process that moves a star from main sequence to red giant is that the shockwave pulls in enough fusible material for the star to continue on. In order for a supernova to really occur (or at least, so the theory goes), the shockwave needs to push out beyond the star's atmosphere, but in almost all models, it never does.
The conclusion is, we're clearly missing a bit of the puzzle, and one of the possible causes is that in the final collapse, the shockwave has much more energy than we're assuming, and neutrino's may hold the key to explaining it.
The last nearby supernova was in 1987(although not in the Milky Way itself, in the LMC), when only a handful of neutrino detectors existed, and they were able to capture a few that coincided with sn1987a, but not nearly enough. Today we have many more, but our Milky Way seems reluctant to share a nearby supernova with us, being long overdue for it.
It's quite possible that we actually have had several since the last in the Milky Way (SN1604), but they occurred within what Edwin Hubble coined the zone of avoidance, effectively behind the galaxy centre, meaning we may have missed it due to the dust and gas obscuring our view of it, from this side of the galaxy.
Still, eventually it will happen, and our ability to capture these neutrino's may point to the missing part of our understanding.
Source:
Neutrinos produced inside an exploding star could betray exotic particles that would lead to a deeper theory of physics. Will our detectors
















