{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2011:Y27JSYRVLL4GY5WAMKE6T64ND7","short_pith_number":"pith:Y27JSYRV","schema_version":"1.0","canonical_sha256":"c6be9962355af86c76c06289e9fb8d1fc741f1113876c3c34fd84275fdc4bf89","source":{"kind":"arxiv","id":"1108.5569","version":1},"attestation_state":"computed","paper":{"title":"Scale-dependent bias from the primordial non-Gaussianity with a Gaussian-squared field","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["gr-qc","hep-th"],"primary_cat":"astro-ph.CO","authors_text":"Shuichiro Yokoyama","submitted_at":"2011-08-29T14:28:37Z","abstract_excerpt":"We investigate the halo bias in the case where the primordial curvature fluctuations, $\\Phi$, are sourced from both a Gaussian random field and a Gaussian-squared field, as $\\Phi({\\bf x}) = \\phi({\\bf x}) + \\psi({\\bf x})^2 - <\\psi({\\bf x})^2>$, so-called \"ungaussiton model\". We employ the peak-background split formula and find a new scale-dependence in the halo bias induced from the Gaussian-squared field."},"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":"1108.5569","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2011-08-29T14:28:37Z","cross_cats_sorted":["gr-qc","hep-th"],"title_canon_sha256":"626f49a274453210795621479ad02ac44197c15a37a886191a17a344b219717c","abstract_canon_sha256":"84b9155f8ee06e89127b391c264a939e43d949cb349f1b2e1b2a4c6ea8f33533"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:00:45.445072Z","signature_b64":"JTKTRHptk6k0c22gaIYmnEChas/DcLWPEBb1i7hnIlLlEc/UlBnmL5SJ2nCnUD5i5Wvq2FFP6qhQ9K+D2pn8Ag==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"c6be9962355af86c76c06289e9fb8d1fc741f1113876c3c34fd84275fdc4bf89","last_reissued_at":"2026-05-18T02:00:45.444430Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:00:45.444430Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Scale-dependent bias from the primordial non-Gaussianity with a Gaussian-squared field","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["gr-qc","hep-th"],"primary_cat":"astro-ph.CO","authors_text":"Shuichiro Yokoyama","submitted_at":"2011-08-29T14:28:37Z","abstract_excerpt":"We investigate the halo bias in the case where the primordial curvature fluctuations, $\\Phi$, are sourced from both a Gaussian random field and a Gaussian-squared field, as $\\Phi({\\bf x}) = \\phi({\\bf x}) + \\psi({\\bf x})^2 - <\\psi({\\bf x})^2>$, so-called \"ungaussiton model\". We employ the peak-background split formula and find a new scale-dependence in the halo bias induced from the Gaussian-squared field."},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1108.5569","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":"1108.5569","created_at":"2026-05-18T02:00:45.444529+00:00"},{"alias_kind":"arxiv_version","alias_value":"1108.5569v1","created_at":"2026-05-18T02:00:45.444529+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1108.5569","created_at":"2026-05-18T02:00:45.444529+00:00"},{"alias_kind":"pith_short_12","alias_value":"Y27JSYRVLL4G","created_at":"2026-05-18T12:26:47.523578+00:00"},{"alias_kind":"pith_short_16","alias_value":"Y27JSYRVLL4GY5WA","created_at":"2026-05-18T12:26:47.523578+00:00"},{"alias_kind":"pith_short_8","alias_value":"Y27JSYRV","created_at":"2026-05-18T12:26:47.523578+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/Y27JSYRVLL4GY5WAMKE6T64ND7","json":"https://pith.science/pith/Y27JSYRVLL4GY5WAMKE6T64ND7.json","graph_json":"https://pith.science/api/pith-number/Y27JSYRVLL4GY5WAMKE6T64ND7/graph.json","events_json":"https://pith.science/api/pith-number/Y27JSYRVLL4GY5WAMKE6T64ND7/events.json","paper":"https://pith.science/paper/Y27JSYRV"},"agent_actions":{"view_html":"https://pith.science/pith/Y27JSYRVLL4GY5WAMKE6T64ND7","download_json":"https://pith.science/pith/Y27JSYRVLL4GY5WAMKE6T64ND7.json","view_paper":"https://pith.science/paper/Y27JSYRV","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1108.5569&json=true","fetch_graph":"https://pith.science/api/pith-number/Y27JSYRVLL4GY5WAMKE6T64ND7/graph.json","fetch_events":"https://pith.science/api/pith-number/Y27JSYRVLL4GY5WAMKE6T64ND7/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/Y27JSYRVLL4GY5WAMKE6T64ND7/action/timestamp_anchor","attest_storage":"https://pith.science/pith/Y27JSYRVLL4GY5WAMKE6T64ND7/action/storage_attestation","attest_author":"https://pith.science/pith/Y27JSYRVLL4GY5WAMKE6T64ND7/action/author_attestation","sign_citation":"https://pith.science/pith/Y27JSYRVLL4GY5WAMKE6T64ND7/action/citation_signature","submit_replication":"https://pith.science/pith/Y27JSYRVLL4GY5WAMKE6T64ND7/action/replication_record"}},"created_at":"2026-05-18T02:00:45.444529+00:00","updated_at":"2026-05-18T02:00:45.444529+00:00"}