{"paper":{"title":"The Planckonions","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"physics.gen-ph","authors_text":"Farook Rahaman, Jitesh R Bhatt, Mofazzal Azam, M Sami","submitted_at":"2016-11-06T08:28:09Z","abstract_excerpt":"We consider a spherically symmetric stellar configuration with a density profile $\\rho(r)=\\frac{c^2}{8\\pi G r^2} $. This configuration satisfies the Schwarzchild black hole condition $\\frac {2GM}{c^2 R}=~1$ for every $ r =R $. We refer it as \"Planckonion\". The interesting thing about the Plankonion is that it has an onion like structure. The central sphere with radius of the Plank-lenght $ L_p=\\sqrt{(\\frac {2\\hbar G}{c^3})}$ has one unit of the Planck-mass $M_p=\\sqrt {(\\frac {c\\hbar}{2G})}$. Subsequent spherical shells of radial width $L_p$ contain exactly one unit of $M_p$. We study this stel"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1611.04895","kind":"arxiv","version":2},"verdict":{"id":null,"model_set":{},"created_at":null,"strongest_claim":"","one_line_summary":"","pipeline_version":null,"weakest_assumption":"","pith_extraction_headline":""},"references":{"count":0,"sample":[],"resolved_work":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57","internal_anchors":0},"formal_canon":{"evidence_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"author_claims":{"count":0,"strong_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"builder_version":"pith-number-builder-2026-05-17-v1"}