[i]Sunward[/i] describes iron bombardment of the Sun in order to disrupt the normal fusion-processes. As far as I've understood, this is a process wherein [sup]56[/sup]Fe is transmuted to [sup]56[/sup]Ni and subsequently [sup]56[/sup]Co, absorbing energy into mass, then beta-decays back to [sup]56[/sup]Fe, releasing most of the mass as anti-neutrinos with high energy. And because anti-neutrinos aren't "useful" energy as such, this results in a net loss of energy to the Sun.
However, beyond simple descriptions of Type II Supernovae, I haven't been able to find much information about exactly what processes would be involved in the "localized collapse" described in [i]Sunward[/i], nor how the effects of iron-bombardment scales with the mass of iron used. The mass of iron used as an example in the book, all the iron in the Solar System, for example, would only make up about 0.14% of the mass of iron already existing in the Sun (and amass about the same as the Earth). Are there any actual (back-of-envelope) calculations regarding the effects of iron bombardment of the Sun, or are the numbers mostly made up for convenience?
I'm particularly interested in knowing if dire consequences could be enacted with a Pluto-mass of iron, a Charon-mass of iron, and smaller masses of iron down to about 10[sup]17[/sup] kg, since the energy needed to move an Earth-mass of iron from the Solar System into the Sun on a time-scale less than an eon seems to make the Death Star superlaser look like a toy flashlight.
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