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Dark star

Celestial bodies composed of dark matter
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Dark stars may exist in the super early universe before the formation of ordinary stars (photon period, see Cosmic chronology )。 Most stars are mainly composed of ordinary matter, but dark stars are mainly composed of Neutral neutrino Constitute and pass dark substance Of Annihilation Release energy. These heat can prevent the dark star from collapsing into an ordinary star under the action of gravity, so the ordinary matter atoms in it will not occur nuclear fusion
Chinese name
Dark star
Foreign name
dark star
Energy source
Dark matter annihilation
Classification
Pure theoretical star

brief introduction

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Dark stars are composed of a large group hydrogen and helium The cloud formed in the early universe has a diameter of about 4 to 2000 Astronomical unit Due to the low surface temperature, the dark star will only emit infrared , will not emit visible light

observation

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If there are still dark stars in the modern universe Gamma ray neutrino and Antimatter Release of, and accompanying cold hydrogen Molecular cloud It may be possible to detect their existence. Usually, cold hydrogen molecular clouds do not emit such high-energy particles. Astronomer Katherine Fritz said she planned to launch James in 2018· Weber Space Telescope It should be able to detect the clues of dark stars.

evolution

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Evolution Path 1: Reionization Previously, the temperature of the universe was low, and dark stars may collapse into black hole , which can explain why black holes existed in the early universe.
Evolution Path 2: The dark matter of the dark star is consumed, and the remaining ordinary gas collapses into ordinary gas fixed star
Evolution Path 3: The gas cooling and dark matter heating in the dark star can maintain a balance, allowing the dark star to survive.

Related reports

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In July 2023, astronomers from Colgate University and the University of Texas found evidence of the existence of dark stars based on the data from the James Webb Space Telescope. Relevant research was published in the new issue of Proceedings of the National Academy of Sciences. [1]