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Summary
| Description |
English: Primordial black holes are formed by the collapse of overdense regions in the inflationary or radiation-dominated universe |
| Date | |
| Source |
https://www.slideserve.com/gema/primordial-black-hole-formation-in-an-axion-like-curvaton-model slide 19. Cropped to remove all elements of original authorship. Based on Kawasaki, Masahiro (2013-03-18). "Primordial black hole formation from an axionlike curvaton model". Physical Review D 87 (6): 063519. DOI:10.1103/PhysRevD.87.063519. |
| Author | Gema White |
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| Date/Time | Thumbnail | Dimensions | User | Comment | |
|---|---|---|---|---|---|
| current | 13:42, 24 April 2023 | | 1,234 × 434 (332 KB) | Sandizer | Uploaded a work by Gema White from https://www.slideserve.com/gema/primordial-black-hole-formation-in-an-axion-like-curvaton-model slide 19. Cropped to remove all elements of original authorship. with UploadWizard |
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