{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2017:YYXW6UEZZWS53JZDHCBGFT2DSE","short_pith_number":"pith:YYXW6UEZ","schema_version":"1.0","canonical_sha256":"c62f6f5099cda5dda723388262cf439134ab6c895587965d07eade5be17355ba","source":{"kind":"arxiv","id":"1711.03988","version":1},"attestation_state":"computed","paper":{"title":"Heavy-Lifting of Gauge Theories By Cosmic Inflation","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO","gr-qc"],"primary_cat":"hep-ph","authors_text":"Raman Sundrum, Soubhik Kumar","submitted_at":"2017-11-10T19:10:25Z","abstract_excerpt":"Future measurements of primordial non-Gaussianity can reveal cosmologically produced particles with masses of order the inflationary Hubble scale and their interactions with the inflaton, giving us crucial insights into the structure of fundamental physics at extremely high energies. We study gauge-Higgs theories that may be accessible in this regime, carefully imposing the constraints of gauge symmetry and its (partial) Higgsing. We distinguish two types of Higgs mechanisms: (i) a standard one in which the Higgs scale is constant before and after inflation, where the particles observable in n"},"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":"1711.03988","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-ph","submitted_at":"2017-11-10T19:10:25Z","cross_cats_sorted":["astro-ph.CO","gr-qc"],"title_canon_sha256":"39c031176a8a68fab3e76c2f3913419f8afa78941462cf87f0b06dad024dadc9","abstract_canon_sha256":"75df72e6dde84834b03356be6b7dd30cbff1c8aff10d88c17b986951dc330500"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:16:08.372173Z","signature_b64":"C2R0tDXkJY6O/yiSqVil9lya49HNJspWubqhQG1kxKzACZ47wXh9zEpuxD2nNpYToTtntUoI3sIHnHiUFQMTCQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"c62f6f5099cda5dda723388262cf439134ab6c895587965d07eade5be17355ba","last_reissued_at":"2026-05-18T00:16:08.371529Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:16:08.371529Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Heavy-Lifting of Gauge Theories By Cosmic Inflation","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO","gr-qc"],"primary_cat":"hep-ph","authors_text":"Raman Sundrum, Soubhik Kumar","submitted_at":"2017-11-10T19:10:25Z","abstract_excerpt":"Future measurements of primordial non-Gaussianity can reveal cosmologically produced particles with masses of order the inflationary Hubble scale and their interactions with the inflaton, giving us crucial insights into the structure of fundamental physics at extremely high energies. We study gauge-Higgs theories that may be accessible in this regime, carefully imposing the constraints of gauge symmetry and its (partial) Higgsing. We distinguish two types of Higgs mechanisms: (i) a standard one in which the Higgs scale is constant before and after inflation, where the particles observable in n"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1711.03988","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":"1711.03988","created_at":"2026-05-18T00:16:08.371627+00:00"},{"alias_kind":"arxiv_version","alias_value":"1711.03988v1","created_at":"2026-05-18T00:16:08.371627+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1711.03988","created_at":"2026-05-18T00:16:08.371627+00:00"},{"alias_kind":"pith_short_12","alias_value":"YYXW6UEZZWS5","created_at":"2026-05-18T12:31:59.375834+00:00"},{"alias_kind":"pith_short_16","alias_value":"YYXW6UEZZWS53JZD","created_at":"2026-05-18T12:31:59.375834+00:00"},{"alias_kind":"pith_short_8","alias_value":"YYXW6UEZ","created_at":"2026-05-18T12:31:59.375834+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":2,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2605.21419","citing_title":"Cosmological Collider Signatures from Right-Handed Neutrino Loop","ref_index":17,"is_internal_anchor":true},{"citing_arxiv_id":"2604.07434","citing_title":"Scalars at the Cosmological Collider: Full Shapes of Tree Diagrams and Bispectrum Searches using Planck Data","ref_index":29,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/YYXW6UEZZWS53JZDHCBGFT2DSE","json":"https://pith.science/pith/YYXW6UEZZWS53JZDHCBGFT2DSE.json","graph_json":"https://pith.science/api/pith-number/YYXW6UEZZWS53JZDHCBGFT2DSE/graph.json","events_json":"https://pith.science/api/pith-number/YYXW6UEZZWS53JZDHCBGFT2DSE/events.json","paper":"https://pith.science/paper/YYXW6UEZ"},"agent_actions":{"view_html":"https://pith.science/pith/YYXW6UEZZWS53JZDHCBGFT2DSE","download_json":"https://pith.science/pith/YYXW6UEZZWS53JZDHCBGFT2DSE.json","view_paper":"https://pith.science/paper/YYXW6UEZ","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1711.03988&json=true","fetch_graph":"https://pith.science/api/pith-number/YYXW6UEZZWS53JZDHCBGFT2DSE/graph.json","fetch_events":"https://pith.science/api/pith-number/YYXW6UEZZWS53JZDHCBGFT2DSE/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/YYXW6UEZZWS53JZDHCBGFT2DSE/action/timestamp_anchor","attest_storage":"https://pith.science/pith/YYXW6UEZZWS53JZDHCBGFT2DSE/action/storage_attestation","attest_author":"https://pith.science/pith/YYXW6UEZZWS53JZDHCBGFT2DSE/action/author_attestation","sign_citation":"https://pith.science/pith/YYXW6UEZZWS53JZDHCBGFT2DSE/action/citation_signature","submit_replication":"https://pith.science/pith/YYXW6UEZZWS53JZDHCBGFT2DSE/action/replication_record"}},"created_at":"2026-05-18T00:16:08.371627+00:00","updated_at":"2026-05-18T00:16:08.371627+00:00"}