{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2023:PXNIU5B3354PZ3QBZNF2HX2NAH","short_pith_number":"pith:PXNIU5B3","schema_version":"1.0","canonical_sha256":"7dda8a743bdf78fcee01cb4ba3df4d01f00f574803dd00966ab26302b65443ed","source":{"kind":"arxiv","id":"2301.07116","version":2},"attestation_state":"computed","paper":{"title":"Arkenstone I: A Novel Method for Robustly Capturing High Specific Energy Outflows In Cosmological Simulations","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Blakesley Burkhart, Chang-Goo Kim, Chia-Yu Hu, Drummond B. Fielding, Eve C. Ostriker, Greg L. Bryan, John C. Forbes, Jonathan Stern, Kung-Yi Su, Lars Hernquist, Matthew C. Smith, Rachel S. Somerville, Rainer Weinberger, Yuan Li","submitted_at":"2023-01-17T19:00:01Z","abstract_excerpt":"Arkenstone is a new model for multiphase, stellar feedback driven galactic winds designed for inclusion in coarse resolution cosmological simulations. In this first paper of a series, we describe the features that allow Arkenstone to properly treat high specific energy wind components and demonstrate them using idealised non-cosmological simulations of a galaxy with a realistic CGM, using the Arepo code. Hot, fast gas phases with low mass loadings are predicted to dominate the energy content of multiphase outflows. In order to treat the huge dynamic range of spatial scales involved in cosmolog"},"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":"2301.07116","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2023-01-17T19:00:01Z","cross_cats_sorted":[],"title_canon_sha256":"f3d127677ce9516692141d3536c8c5b7851017c2990c1f3e7f7400f8e235428f","abstract_canon_sha256":"deb36d69b40dd67180935183dbab296b20b12cb715530cea16fa3e7985edf595"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T07:53:06.754247Z","signature_b64":"LwlhgvkwjsUZUEJpnzlVjVmMvrsMECPR6wMZfX8lzxpr8xMvScuabHvn9sNtJHOQaCx9nY7j5cHMeaRiHMB5Bg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"7dda8a743bdf78fcee01cb4ba3df4d01f00f574803dd00966ab26302b65443ed","last_reissued_at":"2026-07-05T07:53:06.753744Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T07:53:06.753744Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Arkenstone I: A Novel Method for Robustly Capturing High Specific Energy Outflows In Cosmological Simulations","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Blakesley Burkhart, Chang-Goo Kim, Chia-Yu Hu, Drummond B. Fielding, Eve C. Ostriker, Greg L. Bryan, John C. Forbes, Jonathan Stern, Kung-Yi Su, Lars Hernquist, Matthew C. Smith, Rachel S. Somerville, Rainer Weinberger, Yuan Li","submitted_at":"2023-01-17T19:00:01Z","abstract_excerpt":"Arkenstone is a new model for multiphase, stellar feedback driven galactic winds designed for inclusion in coarse resolution cosmological simulations. In this first paper of a series, we describe the features that allow Arkenstone to properly treat high specific energy wind components and demonstrate them using idealised non-cosmological simulations of a galaxy with a realistic CGM, using the Arepo code. Hot, fast gas phases with low mass loadings are predicted to dominate the energy content of multiphase outflows. In order to treat the huge dynamic range of spatial scales involved in cosmolog"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2301.07116","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/2301.07116/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":"2301.07116","created_at":"2026-07-05T07:53:06.753803+00:00"},{"alias_kind":"arxiv_version","alias_value":"2301.07116v2","created_at":"2026-07-05T07:53:06.753803+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2301.07116","created_at":"2026-07-05T07:53:06.753803+00:00"},{"alias_kind":"pith_short_12","alias_value":"PXNIU5B3354P","created_at":"2026-07-05T07:53:06.753803+00:00"},{"alias_kind":"pith_short_16","alias_value":"PXNIU5B3354PZ3QB","created_at":"2026-07-05T07:53:06.753803+00:00"},{"alias_kind":"pith_short_8","alias_value":"PXNIU5B3","created_at":"2026-07-05T07:53:06.753803+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2507.08925","citing_title":"Cosmological Simulations of Galaxies","ref_index":277,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/PXNIU5B3354PZ3QBZNF2HX2NAH","json":"https://pith.science/pith/PXNIU5B3354PZ3QBZNF2HX2NAH.json","graph_json":"https://pith.science/api/pith-number/PXNIU5B3354PZ3QBZNF2HX2NAH/graph.json","events_json":"https://pith.science/api/pith-number/PXNIU5B3354PZ3QBZNF2HX2NAH/events.json","paper":"https://pith.science/paper/PXNIU5B3"},"agent_actions":{"view_html":"https://pith.science/pith/PXNIU5B3354PZ3QBZNF2HX2NAH","download_json":"https://pith.science/pith/PXNIU5B3354PZ3QBZNF2HX2NAH.json","view_paper":"https://pith.science/paper/PXNIU5B3","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2301.07116&json=true","fetch_graph":"https://pith.science/api/pith-number/PXNIU5B3354PZ3QBZNF2HX2NAH/graph.json","fetch_events":"https://pith.science/api/pith-number/PXNIU5B3354PZ3QBZNF2HX2NAH/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/PXNIU5B3354PZ3QBZNF2HX2NAH/action/timestamp_anchor","attest_storage":"https://pith.science/pith/PXNIU5B3354PZ3QBZNF2HX2NAH/action/storage_attestation","attest_author":"https://pith.science/pith/PXNIU5B3354PZ3QBZNF2HX2NAH/action/author_attestation","sign_citation":"https://pith.science/pith/PXNIU5B3354PZ3QBZNF2HX2NAH/action/citation_signature","submit_replication":"https://pith.science/pith/PXNIU5B3354PZ3QBZNF2HX2NAH/action/replication_record"}},"created_at":"2026-07-05T07:53:06.753803+00:00","updated_at":"2026-07-05T07:53:06.753803+00:00"}