Dark Dwarfs: new star -like objects can reveal the nature of the dark matter

by SkillAiNest

Astronomers have predicted an unseen class of bodies like a star near the center of our galaxy called “Dark Dwarf”. A new study suggests that these items can shine by eliminating dark matter, not nuclear fusion. The dark matter makes about a quarter of the universe and communicates through gravity. If the particles of dark matter like a vamp accumulate in a brown dwarf, they would remove it and warm it, which would create an unconscious brightness. Dark dwarfs would be very mild to fuse hydrogen, but will keep lithium 7 in their environment while offering signatures. This prediction came from a JCAP study. The discovery of someone can reveal the nature of the dark matter.

Dark Dwarf has been predicted

According to On the paper, all the stellar items will be operated in the dark under the doorstep of hydrogen burning. The authors find that in the shifts above the minimum mass ∼0.075 m⊙ for hydrogen fusion in dense dark matter, therefore light brown dwarves become stable -powered stars (‘dark dwarf’). They predict that such items are only visible in regions that have a very high dark matter density, such as the galaxy center (ρ_dm ≳ 10^3 gev/cm^3), because the hala is too hard. Significantly, the dark dwarf should maintain lithium 7 in the massive limits, where ordinary brown dwarves burn it, which provides clear observation signatures.

Observatory possibilities and implications

Sakstein notes that powerful telescopes like James WebSpace telescope can also detect extremely cold items like deep dwarfs near the galaxy center. Alternatively, astronomers can survey the brown dwarf population for a rare sub -class with abnormal lithium material. In particular, even if anyone confirmed that the Dark Dwarf would fully support the heavy, its own dark matter.

Sakstein explains that the search for a dark dwarf will provide “compulsive proof” for the dark matter that is widespread and interacts with itself – mainly vamps or similar particles. He notes that a light candidate (such as axis) will not produce such stars, so the discovery of a dark dwarf will dislike these models. Although there is no evidence of wamps, the detection of a dark dwarf means that the dark matter means the vamps (interacting heavy and weakness). In fact, future surveys and JWST observations will also examine these predictions.

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