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Antimatter and antistars in the universe and in the Galaxy
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We consider consequences of hypothetical existence of baryo-dense stars created in the very early universe within an extension of Affleck-Dine scenario of baryogenesis. New constraints on the possible number of compact antimatter objects are derived. The contemporary observational data do not exclude significant amount of antimatter in the Galaxy (and in other galaxies) in the form of the baryo-dense low-massive stars.
Forward citations
Cited by 2 Pith papers
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Effect of post-recombination accretion on primordial binary black hole mergers within virialized dark matter halos
BHL-type post-recombination accretion can raise late three-body PBH merger rates enough for TianQin detections at f~10^{-6} and for LVK limits to bound delayed virialization.
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Antimatter in the universe and Milky Way
A review-style paper asserts that primordial antimatter produced during inflation populates the Milky Way and that observations of positrons, antihelium, and antistar candidates confirm this prediction.
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