{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2014:24YA2VBZ75PU7SCDGPWO3VZ4MU","short_pith_number":"pith:24YA2VBZ","schema_version":"1.0","canonical_sha256":"d7300d5439ff5f4fc84333ecedd73c652ff030b9afe91e3d59286bf90a428085","source":{"kind":"arxiv","id":"1406.3625","version":2},"attestation_state":"computed","paper":{"title":"Modeling jet and outflow feedback during star cluster formation","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.GA","astro-ph.IM","physics.comp-ph","physics.flu-dyn"],"primary_cat":"astro-ph.SR","authors_text":"Christoph Federrath, Martin Schr\\\"on, Ralf S. Klessen, Robi Banerjee","submitted_at":"2014-06-13T20:00:01Z","abstract_excerpt":"Powerful jets and outflows are launched from the protostellar disks around newborn stars. These outflows carry enough mass and momentum to transform the structure of their parent molecular cloud and to potentially control star formation itself. Despite their importance, we have not been able to fully quantify the impact of jets and outflows during the formation of a star cluster. The main problem lies in limited computing power. We would have to resolve the magnetic jet-launching mechanism close to the protostar and at the same time follow the evolution of a parsec-size cloud for a million yea"},"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":"1406.3625","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2014-06-13T20:00:01Z","cross_cats_sorted":["astro-ph.GA","astro-ph.IM","physics.comp-ph","physics.flu-dyn"],"title_canon_sha256":"c8ec9cec5d866fcb8e9af86f62fd9547910bf333b793d492c3feb6dc422a36f0","abstract_canon_sha256":"2523e4ff6d22014716c92dfcccc90a568c9e47ae18a3b3480c2ca6d6ed97ab45"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:46:22.514466Z","signature_b64":"JWPV9Wwd0RJyQbcvZkUDNPSZJ5Y69pLl6PGI55gAH2ghGtt/mMtXA+kO+gUAiL01/oZzAAbMI6TF7GIRBqrSBQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"d7300d5439ff5f4fc84333ecedd73c652ff030b9afe91e3d59286bf90a428085","last_reissued_at":"2026-05-18T02:46:22.513982Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:46:22.513982Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Modeling jet and outflow feedback during star cluster formation","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.GA","astro-ph.IM","physics.comp-ph","physics.flu-dyn"],"primary_cat":"astro-ph.SR","authors_text":"Christoph Federrath, Martin Schr\\\"on, Ralf S. Klessen, Robi Banerjee","submitted_at":"2014-06-13T20:00:01Z","abstract_excerpt":"Powerful jets and outflows are launched from the protostellar disks around newborn stars. These outflows carry enough mass and momentum to transform the structure of their parent molecular cloud and to potentially control star formation itself. Despite their importance, we have not been able to fully quantify the impact of jets and outflows during the formation of a star cluster. The main problem lies in limited computing power. We would have to resolve the magnetic jet-launching mechanism close to the protostar and at the same time follow the evolution of a parsec-size cloud for a million yea"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1406.3625","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"},"aliases":[{"alias_kind":"arxiv","alias_value":"1406.3625","created_at":"2026-05-18T02:46:22.514050+00:00"},{"alias_kind":"arxiv_version","alias_value":"1406.3625v2","created_at":"2026-05-18T02:46:22.514050+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1406.3625","created_at":"2026-05-18T02:46:22.514050+00:00"},{"alias_kind":"pith_short_12","alias_value":"24YA2VBZ75PU","created_at":"2026-05-18T12:28:09.283467+00:00"},{"alias_kind":"pith_short_16","alias_value":"24YA2VBZ75PU7SCD","created_at":"2026-05-18T12:28:09.283467+00:00"},{"alias_kind":"pith_short_8","alias_value":"24YA2VBZ","created_at":"2026-05-18T12:28:09.283467+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":3,"internal_anchor_count":3,"sample":[{"citing_arxiv_id":"2605.16917","citing_title":"The Rapid ASKAP Continuum Survey VII: Spectra and Polarisation In Cutouts of Extragalactic Sources (SPICE-RACS) Second Data Release -- Unveiling the Magnetised Sky","ref_index":159,"is_internal_anchor":true},{"citing_arxiv_id":"2605.16917","citing_title":"The Rapid ASKAP Continuum Survey VII: Spectra and Polarisation In Cutouts of Extragalactic Sources (SPICE-RACS) Second Data Release -- Unveiling the Magnetised Sky","ref_index":159,"is_internal_anchor":true},{"citing_arxiv_id":"2605.13189","citing_title":"The Accretion Process on Protostars","ref_index":175,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/24YA2VBZ75PU7SCDGPWO3VZ4MU","json":"https://pith.science/pith/24YA2VBZ75PU7SCDGPWO3VZ4MU.json","graph_json":"https://pith.science/api/pith-number/24YA2VBZ75PU7SCDGPWO3VZ4MU/graph.json","events_json":"https://pith.science/api/pith-number/24YA2VBZ75PU7SCDGPWO3VZ4MU/events.json","paper":"https://pith.science/paper/24YA2VBZ"},"agent_actions":{"view_html":"https://pith.science/pith/24YA2VBZ75PU7SCDGPWO3VZ4MU","download_json":"https://pith.science/pith/24YA2VBZ75PU7SCDGPWO3VZ4MU.json","view_paper":"https://pith.science/paper/24YA2VBZ","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1406.3625&json=true","fetch_graph":"https://pith.science/api/pith-number/24YA2VBZ75PU7SCDGPWO3VZ4MU/graph.json","fetch_events":"https://pith.science/api/pith-number/24YA2VBZ75PU7SCDGPWO3VZ4MU/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/24YA2VBZ75PU7SCDGPWO3VZ4MU/action/timestamp_anchor","attest_storage":"https://pith.science/pith/24YA2VBZ75PU7SCDGPWO3VZ4MU/action/storage_attestation","attest_author":"https://pith.science/pith/24YA2VBZ75PU7SCDGPWO3VZ4MU/action/author_attestation","sign_citation":"https://pith.science/pith/24YA2VBZ75PU7SCDGPWO3VZ4MU/action/citation_signature","submit_replication":"https://pith.science/pith/24YA2VBZ75PU7SCDGPWO3VZ4MU/action/replication_record"}},"created_at":"2026-05-18T02:46:22.514050+00:00","updated_at":"2026-05-18T02:46:22.514050+00:00"}