{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2015:3HYDYENTEULPDZ7HG6RBY3RFMX","short_pith_number":"pith:3HYDYENT","schema_version":"1.0","canonical_sha256":"d9f03c11b32516f1e7e737a21c6e2565dd707b5b5ea40c4c507636799874f8b8","source":{"kind":"arxiv","id":"1511.09348","version":1},"attestation_state":"computed","paper":{"title":"Energy-limited escape revised","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.EP","authors_text":"J. H. M. M. Schmitt, M. Salz, P. C. Schneider, S. Czesla","submitted_at":"2015-11-30T15:30:56Z","abstract_excerpt":"Gas planets in close proximity to their host stars experience photoevaporative mass loss. The energy-limited escape concept is generally used to derive estimates for the planetary mass-loss rates. Our photoionization hydrodynamics simulations of the thermospheres of hot gas planets show that the energy-limited escape concept is valid only for planets with a gravitational potential lower than $\\log_\\mathrm{10}\\left( -\\Phi_{\\mathrm{G}}\\right) < 13.11~$erg$\\,$g$^{-1}$ because in these planets the radiative energy input is efficiently used to drive the planetary wind. Massive and compact planets w"},"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":"1511.09348","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.EP","submitted_at":"2015-11-30T15:30:56Z","cross_cats_sorted":[],"title_canon_sha256":"a4bb5d6cc7bfd1b4d786336801a61c74775ca8ea20fa0f50e21ecf5aef903bd0","abstract_canon_sha256":"ebb307685d51138389a47cc984269c6278475598943ad73d0f87ed80cac954b9"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:23:53.883632Z","signature_b64":"ptY35h4rWFv/ZYQH0wHutizF+XkcAjUMtp3hN/MMlTuzqv0qYYOUmDaYfqJspcuEgwXiya+Z5SjwHn5RwtO3Bg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"d9f03c11b32516f1e7e737a21c6e2565dd707b5b5ea40c4c507636799874f8b8","last_reissued_at":"2026-05-18T01:23:53.882893Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:23:53.882893Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Energy-limited escape revised","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.EP","authors_text":"J. H. M. M. Schmitt, M. Salz, P. C. Schneider, S. Czesla","submitted_at":"2015-11-30T15:30:56Z","abstract_excerpt":"Gas planets in close proximity to their host stars experience photoevaporative mass loss. The energy-limited escape concept is generally used to derive estimates for the planetary mass-loss rates. Our photoionization hydrodynamics simulations of the thermospheres of hot gas planets show that the energy-limited escape concept is valid only for planets with a gravitational potential lower than $\\log_\\mathrm{10}\\left( -\\Phi_{\\mathrm{G}}\\right) < 13.11~$erg$\\,$g$^{-1}$ because in these planets the radiative energy input is efficiently used to drive the planetary wind. Massive and compact planets w"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1511.09348","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":""},"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":"1511.09348","created_at":"2026-05-18T01:23:53.883010+00:00"},{"alias_kind":"arxiv_version","alias_value":"1511.09348v1","created_at":"2026-05-18T01:23:53.883010+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1511.09348","created_at":"2026-05-18T01:23:53.883010+00:00"},{"alias_kind":"pith_short_12","alias_value":"3HYDYENTEULP","created_at":"2026-05-18T12:29:02.477457+00:00"},{"alias_kind":"pith_short_16","alias_value":"3HYDYENTEULPDZ7H","created_at":"2026-05-18T12:29:02.477457+00:00"},{"alias_kind":"pith_short_8","alias_value":"3HYDYENT","created_at":"2026-05-18T12:29:02.477457+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/3HYDYENTEULPDZ7HG6RBY3RFMX","json":"https://pith.science/pith/3HYDYENTEULPDZ7HG6RBY3RFMX.json","graph_json":"https://pith.science/api/pith-number/3HYDYENTEULPDZ7HG6RBY3RFMX/graph.json","events_json":"https://pith.science/api/pith-number/3HYDYENTEULPDZ7HG6RBY3RFMX/events.json","paper":"https://pith.science/paper/3HYDYENT"},"agent_actions":{"view_html":"https://pith.science/pith/3HYDYENTEULPDZ7HG6RBY3RFMX","download_json":"https://pith.science/pith/3HYDYENTEULPDZ7HG6RBY3RFMX.json","view_paper":"https://pith.science/paper/3HYDYENT","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1511.09348&json=true","fetch_graph":"https://pith.science/api/pith-number/3HYDYENTEULPDZ7HG6RBY3RFMX/graph.json","fetch_events":"https://pith.science/api/pith-number/3HYDYENTEULPDZ7HG6RBY3RFMX/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/3HYDYENTEULPDZ7HG6RBY3RFMX/action/timestamp_anchor","attest_storage":"https://pith.science/pith/3HYDYENTEULPDZ7HG6RBY3RFMX/action/storage_attestation","attest_author":"https://pith.science/pith/3HYDYENTEULPDZ7HG6RBY3RFMX/action/author_attestation","sign_citation":"https://pith.science/pith/3HYDYENTEULPDZ7HG6RBY3RFMX/action/citation_signature","submit_replication":"https://pith.science/pith/3HYDYENTEULPDZ7HG6RBY3RFMX/action/replication_record"}},"created_at":"2026-05-18T01:23:53.883010+00:00","updated_at":"2026-05-18T01:23:53.883010+00:00"}