{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2016:3HMYL7XC3NERJ2NSZSUEN72Y3D","short_pith_number":"pith:3HMYL7XC","schema_version":"1.0","canonical_sha256":"d9d985fee2db4914e9b2cca846ff58d8fc9a4e636cb9ff98673017b8c4674367","source":{"kind":"arxiv","id":"1607.02356","version":2},"attestation_state":"computed","paper":{"title":"Post-Newtonian parameter $\\gamma$ for multiscalar-tensor gravity with a general potential","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO","hep-ph","hep-th"],"primary_cat":"gr-qc","authors_text":"Erik Randla, Laur Jarv, Manuel Hohmann, Ott Vilson, Piret Kuusk","submitted_at":"2016-07-08T13:20:53Z","abstract_excerpt":"We compute the parametrized post-Newtonian parameter $\\gamma$ in the case of a static point source for multiscalar-tensor gravity with completely general nonderivative couplings and potential in the Jordan frame. Similarly to the single massive field case $\\gamma$ depends exponentially on the distance from the source and is determined by the length of a vector of non-minimal coupling in the space of scalar fields and its orientation relative to the mass eigenvectors. Using data from the Cassini tracking experiment, we estimate bounds on a general theory with two scalar fields. Our formalism ca"},"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":"1607.02356","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"gr-qc","submitted_at":"2016-07-08T13:20:53Z","cross_cats_sorted":["astro-ph.CO","hep-ph","hep-th"],"title_canon_sha256":"ac13903431eed12c94f8e8e73827b2756985529a28e1d318386f3ed51f941020","abstract_canon_sha256":"94073eb3328b488588c221f1f04ff96af1c2dbd181fd615a6ba8b800f1ea82f6"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:53:02.438491Z","signature_b64":"M+mil+6lXBhQ5C4gBlPRa46axnxFxpl9/OshHJCvT4aeIb7H3RP6Mgv8V7FNVsBJ/QLacweW+F8OwCksNqCKDg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"d9d985fee2db4914e9b2cca846ff58d8fc9a4e636cb9ff98673017b8c4674367","last_reissued_at":"2026-05-18T00:53:02.437730Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:53:02.437730Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Post-Newtonian parameter $\\gamma$ for multiscalar-tensor gravity with a general potential","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO","hep-ph","hep-th"],"primary_cat":"gr-qc","authors_text":"Erik Randla, Laur Jarv, Manuel Hohmann, Ott Vilson, Piret Kuusk","submitted_at":"2016-07-08T13:20:53Z","abstract_excerpt":"We compute the parametrized post-Newtonian parameter $\\gamma$ in the case of a static point source for multiscalar-tensor gravity with completely general nonderivative couplings and potential in the Jordan frame. Similarly to the single massive field case $\\gamma$ depends exponentially on the distance from the source and is determined by the length of a vector of non-minimal coupling in the space of scalar fields and its orientation relative to the mass eigenvectors. Using data from the Cassini tracking experiment, we estimate bounds on a general theory with two scalar fields. Our formalism ca"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1607.02356","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":"1607.02356","created_at":"2026-05-18T00:53:02.437834+00:00"},{"alias_kind":"arxiv_version","alias_value":"1607.02356v2","created_at":"2026-05-18T00:53:02.437834+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1607.02356","created_at":"2026-05-18T00:53:02.437834+00:00"},{"alias_kind":"pith_short_12","alias_value":"3HMYL7XC3NER","created_at":"2026-05-18T12:29:55.572404+00:00"},{"alias_kind":"pith_short_16","alias_value":"3HMYL7XC3NERJ2NS","created_at":"2026-05-18T12:29:55.572404+00:00"},{"alias_kind":"pith_short_8","alias_value":"3HMYL7XC","created_at":"2026-05-18T12:29:55.572404+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2604.16907","citing_title":"First-order thermodynamics of multi-scalar-tensor gravity","ref_index":36,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/3HMYL7XC3NERJ2NSZSUEN72Y3D","json":"https://pith.science/pith/3HMYL7XC3NERJ2NSZSUEN72Y3D.json","graph_json":"https://pith.science/api/pith-number/3HMYL7XC3NERJ2NSZSUEN72Y3D/graph.json","events_json":"https://pith.science/api/pith-number/3HMYL7XC3NERJ2NSZSUEN72Y3D/events.json","paper":"https://pith.science/paper/3HMYL7XC"},"agent_actions":{"view_html":"https://pith.science/pith/3HMYL7XC3NERJ2NSZSUEN72Y3D","download_json":"https://pith.science/pith/3HMYL7XC3NERJ2NSZSUEN72Y3D.json","view_paper":"https://pith.science/paper/3HMYL7XC","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1607.02356&json=true","fetch_graph":"https://pith.science/api/pith-number/3HMYL7XC3NERJ2NSZSUEN72Y3D/graph.json","fetch_events":"https://pith.science/api/pith-number/3HMYL7XC3NERJ2NSZSUEN72Y3D/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/3HMYL7XC3NERJ2NSZSUEN72Y3D/action/timestamp_anchor","attest_storage":"https://pith.science/pith/3HMYL7XC3NERJ2NSZSUEN72Y3D/action/storage_attestation","attest_author":"https://pith.science/pith/3HMYL7XC3NERJ2NSZSUEN72Y3D/action/author_attestation","sign_citation":"https://pith.science/pith/3HMYL7XC3NERJ2NSZSUEN72Y3D/action/citation_signature","submit_replication":"https://pith.science/pith/3HMYL7XC3NERJ2NSZSUEN72Y3D/action/replication_record"}},"created_at":"2026-05-18T00:53:02.437834+00:00","updated_at":"2026-05-18T00:53:02.437834+00:00"}