{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2025:IHAMA2B2HDAO3PSHOD7LVWIOPK","short_pith_number":"pith:IHAMA2B2","schema_version":"1.0","canonical_sha256":"41c0c0683a38c0edbe4770febad90e7a97aa65768d0044978c53996ce0b1e4e7","source":{"kind":"arxiv","id":"2506.03756","version":3},"attestation_state":"computed","paper":{"title":"Cosmological Dynamics of Accelerating Model in $f(T)$ Gravity with Special Forms of Deceleration Parameter","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"gr-qc","authors_text":"Gauree Shanker, Gyan Prakash Singh, Romanshu Garg, Shivank Pal","submitted_at":"2025-06-04T09:22:54Z","abstract_excerpt":"In this paper, the dynamical behavior of the accelerated expansion of the universe is discussed within the framework of $f(T)$ gravity, considering power law functional form of $ f(T)=\\alpha (-T)^{n}$. Two distinct redshift-dependent parameterization of the deceleration parameter such as $q(z)=q_{0}+ q_{1}\\left(\\frac{ \\ln(N+z)}{z+1}-\\ln N \\right)$ and $ q(z)=\\frac{1}{2}+ \\frac{q_{1}z+ q_{2}}{(1+z)^2} $ are considered. We have derived the Hubble parameter in terms of redshift and discussed its effect on other cosmological parameters. Using Bayesian statistical analysis and $\\chi^2$-minimization"},"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":"2506.03756","kind":"arxiv","version":3},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"gr-qc","submitted_at":"2025-06-04T09:22:54Z","cross_cats_sorted":[],"title_canon_sha256":"1042fe8b2bd9a5ac59f4b8a228491e42dc26f5558a40841658f02b6619e1dda8","abstract_canon_sha256":"b6e0173f6a81cfb2af964680a11f2fadda81570ad14718ad1269c7b8893abf79"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T12:00:50.437158Z","signature_b64":"1nQmg2rBlKBfPmUphSLNI6lX52zNejp3IzTf8trz6TI8E+8OqT2RA1JxuSmhl1gCC9SdXF0iJCOqBgWuidXqAA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"41c0c0683a38c0edbe4770febad90e7a97aa65768d0044978c53996ce0b1e4e7","last_reissued_at":"2026-07-05T12:00:50.436666Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T12:00:50.436666Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Cosmological Dynamics of Accelerating Model in $f(T)$ Gravity with Special Forms of Deceleration Parameter","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"gr-qc","authors_text":"Gauree Shanker, Gyan Prakash Singh, Romanshu Garg, Shivank Pal","submitted_at":"2025-06-04T09:22:54Z","abstract_excerpt":"In this paper, the dynamical behavior of the accelerated expansion of the universe is discussed within the framework of $f(T)$ gravity, considering power law functional form of $ f(T)=\\alpha (-T)^{n}$. Two distinct redshift-dependent parameterization of the deceleration parameter such as $q(z)=q_{0}+ q_{1}\\left(\\frac{ \\ln(N+z)}{z+1}-\\ln N \\right)$ and $ q(z)=\\frac{1}{2}+ \\frac{q_{1}z+ q_{2}}{(1+z)^2} $ are considered. We have derived the Hubble parameter in terms of redshift and discussed its effect on other cosmological parameters. Using Bayesian statistical analysis and $\\chi^2$-minimization"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2506.03756","kind":"arxiv","version":3},"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/2506.03756/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":"2506.03756","created_at":"2026-07-05T12:00:50.436727+00:00"},{"alias_kind":"arxiv_version","alias_value":"2506.03756v3","created_at":"2026-07-05T12:00:50.436727+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2506.03756","created_at":"2026-07-05T12:00:50.436727+00:00"},{"alias_kind":"pith_short_12","alias_value":"IHAMA2B2HDAO","created_at":"2026-07-05T12:00:50.436727+00:00"},{"alias_kind":"pith_short_16","alias_value":"IHAMA2B2HDAO3PSH","created_at":"2026-07-05T12:00:50.436727+00:00"},{"alias_kind":"pith_short_8","alias_value":"IHAMA2B2","created_at":"2026-07-05T12:00:50.436727+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/IHAMA2B2HDAO3PSHOD7LVWIOPK","json":"https://pith.science/pith/IHAMA2B2HDAO3PSHOD7LVWIOPK.json","graph_json":"https://pith.science/api/pith-number/IHAMA2B2HDAO3PSHOD7LVWIOPK/graph.json","events_json":"https://pith.science/api/pith-number/IHAMA2B2HDAO3PSHOD7LVWIOPK/events.json","paper":"https://pith.science/paper/IHAMA2B2"},"agent_actions":{"view_html":"https://pith.science/pith/IHAMA2B2HDAO3PSHOD7LVWIOPK","download_json":"https://pith.science/pith/IHAMA2B2HDAO3PSHOD7LVWIOPK.json","view_paper":"https://pith.science/paper/IHAMA2B2","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2506.03756&json=true","fetch_graph":"https://pith.science/api/pith-number/IHAMA2B2HDAO3PSHOD7LVWIOPK/graph.json","fetch_events":"https://pith.science/api/pith-number/IHAMA2B2HDAO3PSHOD7LVWIOPK/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/IHAMA2B2HDAO3PSHOD7LVWIOPK/action/timestamp_anchor","attest_storage":"https://pith.science/pith/IHAMA2B2HDAO3PSHOD7LVWIOPK/action/storage_attestation","attest_author":"https://pith.science/pith/IHAMA2B2HDAO3PSHOD7LVWIOPK/action/author_attestation","sign_citation":"https://pith.science/pith/IHAMA2B2HDAO3PSHOD7LVWIOPK/action/citation_signature","submit_replication":"https://pith.science/pith/IHAMA2B2HDAO3PSHOD7LVWIOPK/action/replication_record"}},"created_at":"2026-07-05T12:00:50.436727+00:00","updated_at":"2026-07-05T12:00:50.436727+00:00"}