{"paper":{"title":"Tidal disruptions of main sequence stars -- IV. Relativistic effects and dependence on black hole mass","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.GA","astro-ph.SR"],"primary_cat":"astro-ph.HE","authors_text":"Julian Krolik, Scott C. Noble, Taeho Ryu, Tsvi Piran","submitted_at":"2020-01-08T20:25:00Z","abstract_excerpt":"Using a suite of fully relativistic hydrodynamic simulations applied to main-sequence stars with realistic internal density profiles, we examine full and partial tidal disruptions across a wide range of black hole mass ($10^{5}\\leq M_{\\rm BH}/\\mathrm{M}_{\\odot}\\leq 5\\times 10^{7}$) and stellar mass ($0.3 \\leq M_{\\star} /\\mathrm{M}_{\\odot}\\leq 3$) as larger $M_{\\rm BH}$ leads to stronger relativistic effects. For fixed $M_{\\star}$, as $M_{\\rm BH}$ increases, the ratio of the maximum pericenter distance yielding full disruptions ($\\mathcal{R}_{\\rm t}$) to its Newtonian prediction rises rapidly, "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2001.03504","kind":"arxiv","version":4},"verdict":{"id":null,"model_set":{},"created_at":null,"strongest_claim":"","one_line_summary":"","pipeline_version":null,"weakest_assumption":"","pith_extraction_headline":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/2001.03504/integrity.json","findings":[],"available":true,"detectors_run":[],"snapshot_sha256":"c28c3603d3b5d939e8dc4c7e95fa8dfce3d595e45f758748cecf8e644a296938"},"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"}