{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2016:PDFG4ULHPLZ5KEINTLDHIKE3X6","short_pith_number":"pith:PDFG4ULH","schema_version":"1.0","canonical_sha256":"78ca6e51677af3d5110d9ac674289bbf80b4e0efb4d2c7314ed421684bc24788","source":{"kind":"arxiv","id":"1611.07966","version":2},"attestation_state":"computed","paper":{"title":"An effective description of dark matter and dark energy in the mildly non-linear regime","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["gr-qc","hep-ph","hep-th"],"primary_cat":"astro-ph.CO","authors_text":"Azadeh Maleknejad, Leonardo Senatore, Matthew Lewandowski","submitted_at":"2016-11-23T20:34:01Z","abstract_excerpt":"In the next few years, we are going to probe the low-redshift universe with unprecedented accuracy. Among the various fruits that this will bear, it will greatly improve our knowledge of the dynamics of dark energy, though for this there is a strong theoretical preference for a cosmological constant. We assume that dark energy is described by the so-called Effective Field Theory of Dark Energy, which assumes that dark energy is the Goldstone boson of time translations. Such a formalism makes it easy to ensure that our signatures are consistent with well-established principles of physics. Since"},"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":"1611.07966","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2016-11-23T20:34:01Z","cross_cats_sorted":["gr-qc","hep-ph","hep-th"],"title_canon_sha256":"465bbfede84a4d154d18e1ff51b5c0c08b59dc7a0a532a078da3cbfd29464d0c","abstract_canon_sha256":"a005db88d081ecde7f4ee12308ef7853db263c668c748846890692216d96647c"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:35:35.294962Z","signature_b64":"YbGChlWDJTlRelD415dUpFGHScjvzAXNiedYSdI4uTmwp45mlnQwTWHPGtxX4VNIgbkIoNoceva5X6XS97DDDA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"78ca6e51677af3d5110d9ac674289bbf80b4e0efb4d2c7314ed421684bc24788","last_reissued_at":"2026-05-18T00:35:35.294266Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:35:35.294266Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"An effective description of dark matter and dark energy in the mildly non-linear regime","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["gr-qc","hep-ph","hep-th"],"primary_cat":"astro-ph.CO","authors_text":"Azadeh Maleknejad, Leonardo Senatore, Matthew Lewandowski","submitted_at":"2016-11-23T20:34:01Z","abstract_excerpt":"In the next few years, we are going to probe the low-redshift universe with unprecedented accuracy. Among the various fruits that this will bear, it will greatly improve our knowledge of the dynamics of dark energy, though for this there is a strong theoretical preference for a cosmological constant. We assume that dark energy is described by the so-called Effective Field Theory of Dark Energy, which assumes that dark energy is the Goldstone boson of time translations. Such a formalism makes it easy to ensure that our signatures are consistent with well-established principles of physics. Since"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1611.07966","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":"1611.07966","created_at":"2026-05-18T00:35:35.294398+00:00"},{"alias_kind":"arxiv_version","alias_value":"1611.07966v2","created_at":"2026-05-18T00:35:35.294398+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1611.07966","created_at":"2026-05-18T00:35:35.294398+00:00"},{"alias_kind":"pith_short_12","alias_value":"PDFG4ULHPLZ5","created_at":"2026-05-18T12:30:39.010887+00:00"},{"alias_kind":"pith_short_16","alias_value":"PDFG4ULHPLZ5KEIN","created_at":"2026-05-18T12:30:39.010887+00:00"},{"alias_kind":"pith_short_8","alias_value":"PDFG4ULH","created_at":"2026-05-18T12:30:39.010887+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2605.05114","citing_title":"Effective Field Theory of Large Scale Structure and Newtonian Motion Gauges","ref_index":33,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/PDFG4ULHPLZ5KEINTLDHIKE3X6","json":"https://pith.science/pith/PDFG4ULHPLZ5KEINTLDHIKE3X6.json","graph_json":"https://pith.science/api/pith-number/PDFG4ULHPLZ5KEINTLDHIKE3X6/graph.json","events_json":"https://pith.science/api/pith-number/PDFG4ULHPLZ5KEINTLDHIKE3X6/events.json","paper":"https://pith.science/paper/PDFG4ULH"},"agent_actions":{"view_html":"https://pith.science/pith/PDFG4ULHPLZ5KEINTLDHIKE3X6","download_json":"https://pith.science/pith/PDFG4ULHPLZ5KEINTLDHIKE3X6.json","view_paper":"https://pith.science/paper/PDFG4ULH","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1611.07966&json=true","fetch_graph":"https://pith.science/api/pith-number/PDFG4ULHPLZ5KEINTLDHIKE3X6/graph.json","fetch_events":"https://pith.science/api/pith-number/PDFG4ULHPLZ5KEINTLDHIKE3X6/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/PDFG4ULHPLZ5KEINTLDHIKE3X6/action/timestamp_anchor","attest_storage":"https://pith.science/pith/PDFG4ULHPLZ5KEINTLDHIKE3X6/action/storage_attestation","attest_author":"https://pith.science/pith/PDFG4ULHPLZ5KEINTLDHIKE3X6/action/author_attestation","sign_citation":"https://pith.science/pith/PDFG4ULHPLZ5KEINTLDHIKE3X6/action/citation_signature","submit_replication":"https://pith.science/pith/PDFG4ULHPLZ5KEINTLDHIKE3X6/action/replication_record"}},"created_at":"2026-05-18T00:35:35.294398+00:00","updated_at":"2026-05-18T00:35:35.294398+00:00"}