{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2026:TDAEMJCIJ3NKHZOI5KKLI7AXWL","short_pith_number":"pith:TDAEMJCI","schema_version":"1.0","canonical_sha256":"98c04624484edaa3e5c8ea94b47c17b2e6e58e4047b9215ab1d76af21fc53e0b","source":{"kind":"arxiv","id":"2607.24733","version":1},"attestation_state":"computed","paper":{"title":"Atmospheric Escape Rates of Planets in Stellar Tidal Fields from 3-D Hydrodynamic Simulations1","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.EP","authors_text":"Morgan MacLeod, Ritika Sethi, Sarah Millholland","submitted_at":"2026-07-27T17:57:18Z","abstract_excerpt":"Thermally driven atmospheric escape, including photo-evaporation and core-powered mass-loss, plays a key role in shaping the evolution of close-in exoplanets, yet most current models rely on simplified one-dimensional descriptions of atmospheric escape. In this work, we perform 3D hydrodynamic simulations of atmospheric outflows from a Jupiter-sized planet embedded in the gravitational potential of a solar-type host star, and compare these results with 1D models to identify the regimes where they perform well and where they break down. We explore a range of configurations by varying the degree"},"verification_status":{"content_addressed":true,"pith_receipt":true,"author_attested":false,"weak_author_claims":0,"strong_author_claims":0,"externally_anchored":false,"storage_verified":false,"citation_signatures":0,"replication_records":0,"graph_snapshot":true,"references_resolved":false,"formal_links_present":false},"canonical_record":{"source":{"id":"2607.24733","kind":"arxiv","version":1},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"astro-ph.EP","submitted_at":"2026-07-27T17:57:18Z","cross_cats_sorted":[],"title_canon_sha256":"1dae1b2657564712e1e30de5d61f7d77011b10818072f69c2fac579b1871fbb5","abstract_canon_sha256":"d19aac56ce0550526addc8879b768e6e4c5b9bb62d191ac1356f324bdfa43db6"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-28T02:24:24.809344Z","signature_b64":"L+ZPJ5yE/1QQi4K+8uedDjRimRhngNtzhybtD0J2bbtxnQNp541binS5wjheWNL3SW/Rbt3x1NF+FK4GJWXsAA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"98c04624484edaa3e5c8ea94b47c17b2e6e58e4047b9215ab1d76af21fc53e0b","last_reissued_at":"2026-07-28T02:24:24.808464Z","signature_status":"signed_v1","first_computed_at":"2026-07-28T02:24:24.808464Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Atmospheric Escape Rates of Planets in Stellar Tidal Fields from 3-D Hydrodynamic Simulations1","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.EP","authors_text":"Morgan MacLeod, Ritika Sethi, Sarah Millholland","submitted_at":"2026-07-27T17:57:18Z","abstract_excerpt":"Thermally driven atmospheric escape, including photo-evaporation and core-powered mass-loss, plays a key role in shaping the evolution of close-in exoplanets, yet most current models rely on simplified one-dimensional descriptions of atmospheric escape. In this work, we perform 3D hydrodynamic simulations of atmospheric outflows from a Jupiter-sized planet embedded in the gravitational potential of a solar-type host star, and compare these results with 1D models to identify the regimes where they perform well and where they break down. We explore a range of configurations by varying the degree"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2607.24733","kind":"arxiv","version":1},"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/2607.24733/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"},"aliases":[{"alias_kind":"arxiv","alias_value":"2607.24733","created_at":"2026-07-28T02:24:24.808902+00:00"},{"alias_kind":"arxiv_version","alias_value":"2607.24733v1","created_at":"2026-07-28T02:24:24.808902+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2607.24733","created_at":"2026-07-28T02:24:24.808902+00:00"},{"alias_kind":"pith_short_12","alias_value":"TDAEMJCIJ3NK","created_at":"2026-07-28T02:24:24.808902+00:00"},{"alias_kind":"pith_short_16","alias_value":"TDAEMJCIJ3NKHZOI","created_at":"2026-07-28T02:24:24.808902+00:00"},{"alias_kind":"pith_short_8","alias_value":"TDAEMJCI","created_at":"2026-07-28T02:24:24.808902+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":0,"internal_anchor_count":0,"sample":[]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/TDAEMJCIJ3NKHZOI5KKLI7AXWL","json":"https://pith.science/pith/TDAEMJCIJ3NKHZOI5KKLI7AXWL.json","graph_json":"https://pith.science/api/pith-number/TDAEMJCIJ3NKHZOI5KKLI7AXWL/graph.json","events_json":"https://pith.science/api/pith-number/TDAEMJCIJ3NKHZOI5KKLI7AXWL/events.json","paper":"https://pith.science/paper/TDAEMJCI"},"agent_actions":{"view_html":"https://pith.science/pith/TDAEMJCIJ3NKHZOI5KKLI7AXWL","download_json":"https://pith.science/pith/TDAEMJCIJ3NKHZOI5KKLI7AXWL.json","view_paper":"https://pith.science/paper/TDAEMJCI","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2607.24733&json=true","fetch_graph":"https://pith.science/api/pith-number/TDAEMJCIJ3NKHZOI5KKLI7AXWL/graph.json","fetch_events":"https://pith.science/api/pith-number/TDAEMJCIJ3NKHZOI5KKLI7AXWL/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/TDAEMJCIJ3NKHZOI5KKLI7AXWL/action/timestamp_anchor","attest_storage":"https://pith.science/pith/TDAEMJCIJ3NKHZOI5KKLI7AXWL/action/storage_attestation","attest_author":"https://pith.science/pith/TDAEMJCIJ3NKHZOI5KKLI7AXWL/action/author_attestation","sign_citation":"https://pith.science/pith/TDAEMJCIJ3NKHZOI5KKLI7AXWL/action/citation_signature","submit_replication":"https://pith.science/pith/TDAEMJCIJ3NKHZOI5KKLI7AXWL/action/replication_record"}},"created_at":"2026-07-28T02:24:24.808902+00:00","updated_at":"2026-07-28T02:24:24.808902+00:00"}