Dark Matter Balls Help Supernovae to Explode
Colin D. Froggatt, Holger B. Nielsen

TL;DR
This paper proposes that dark matter balls can provide an energy source to revive stalled shock waves in supernovae, potentially explaining observed multiple neutrino bursts and offering a novel solution to supernova explosion mechanisms.
Contribution
It introduces a new dark matter model involving large dark matter balls that can inject heat into supernova cores, aiding shock wave revival and explaining multiple neutrino signals.
Findings
Dark matter balls can absorb neutrons and release heat, aiding supernova explosions.
The model explains the multiple neutrino bursts observed in SN1987A.
Heating from dark matter balls can cause two separate collapses in supernova progenitors.
Abstract
As a solution to the well-known problem that the shock wave potentially responsible for the explosion of a supernova actually tends to stall, we propose a new energy source arising from our model for dark matter. Our earlier model proposed that dark matter should consist of cm-large white dwarf-like objects kept together by a skin separating two different sorts of vacua. These dark matter balls or pearls will collect in the middle of any star throughout its lifetime. At some stage during the development of a supernova the balls will begin to take in neutrons and then other surrounding material. By passing into a ball nucleons fall through a potential of order 10 MeV, causing a severe production of heat - of order 10 foe for a solar mass of material eaten by the balls. The temperature in the iron core will thereby be raised, splitting up the iron into smaller nuclei. This provides a…
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