Article: Supernovae sparked by dark matter in white dwarfs

In summary, the article discusses how a ball of asymmetric dark matter inside a white dwarf could trigger fusion reactions and potentially lead to a Type Ia supernova explosion. The potential for dark matter to accumulate in the cores of neutron and quark stars is also mentioned, and the possibility of dark matter conversion in these conditions is raised. However, the likelihood of this happening depends on the mass of the dark matter particles.
  • #1
.Scott
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TL;DR Summary
The article claims that assymetric dark matter can accumulate in a dwarf star producing a small Black Hole, and then ignite a supernova.
Here is the Physical Review article:
"Supernovae sparked by dark matter in white dwarfs"

"A ball of asymmetric dark matter accumulated inside a white dwarf and collapsing under its own weight sheds enough gravitational potential energy through scattering with nuclei to spark the fusion reactions that precede a Type Ia supernova explosion."

From what I gather, the Supernovae triggering mechanism for some White Dwarf stars has not been discovered.
 
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  • #2
Just thinking...

If the core of white dwarfs can arrest dark matter, then the core of neutron/quark stars should be even more effective at it.

If ever there is a way to convert between dark matter and regular matter, it would be most pronounced under conditions where it is pushed hardest by le chatelier's principle. And if anywhere there is a place where this push would be strongest in the direction of dark matter, it would in the cores of neutron stars.

Could this actually be happening? Over time, should we expect that neutron stars could, in part evaporate to dark matter, and in part accumulate dark matter that will would ultimately push them to a BH?
 
  • #3
If the dark matter particles are very heavy as discussed in the publication then neutron stars won't be able to make them. If they are light then neutron stars might make them and they would escape. This would cool their interior and lead to a smaller mass loss. This has been discussed a lot for axions, e.g. here for neutron stars and here for white dwarfs. If they are in an intermediate mass range then they might co-exist with matter in the core.
 
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1. What is the main finding of the article?

The main finding of the article is that dark matter can trigger supernovae explosions in white dwarfs, which was previously thought to be impossible.

2. How was this discovery made?

The discovery was made by simulating the behavior of white dwarfs in the presence of dark matter using advanced computer models.

3. What implications does this have for our understanding of supernovae?

This discovery challenges previous theories about the cause of supernovae and suggests that dark matter may play a larger role in these explosive events than previously thought.

4. How does this relate to current research on dark matter?

This research adds to the growing body of evidence that dark matter has a significant impact on the behavior of celestial objects, and highlights the need for further study into its properties and effects.

5. What are the potential future implications of this discovery?

This discovery could lead to a better understanding of the role of dark matter in the universe and potentially open up new avenues for research and exploration in this field.

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