Article: Supernovae sparked by dark matter in white dwarfs

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SUMMARY

The article "Supernovae sparked by dark matter in white dwarfs" from Physical Review discusses a novel mechanism for Type Ia supernova explosions, where asymmetric dark matter accumulates in a white dwarf, leading to fusion reactions triggered by gravitational potential energy. The discussion posits that neutron and quark stars may be even more effective at capturing dark matter, potentially leading to significant interactions under extreme conditions. The implications of dark matter conversion and its effects on neutron stars, including mass loss and the formation of black holes, are explored, suggesting a complex relationship between dark matter and stellar evolution.

PREREQUISITES
  • Understanding of Type Ia supernova mechanisms
  • Familiarity with dark matter theories and properties
  • Knowledge of stellar structures, specifically white dwarfs and neutron stars
  • Basic principles of gravitational potential energy and fusion reactions
NEXT STEPS
  • Research the mechanisms of Type Ia supernovae in detail
  • Explore the properties and theories surrounding dark matter, particularly asymmetric dark matter
  • Investigate the role of neutron stars in dark matter interactions and potential evaporation processes
  • Examine the implications of axions and their relationship with neutron and white dwarfs
USEFUL FOR

Astronomers, astrophysicists, and researchers interested in stellar evolution, dark matter interactions, and supernova mechanisms will benefit from this discussion.

.Scott
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TL;DR
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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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?
 
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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