{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2014:7TMXPYVHLHYR36WXEEOJWWM2WN","short_pith_number":"pith:7TMXPYVH","schema_version":"1.0","canonical_sha256":"fcd977e2a759f11dfad7211c9b599ab34074ad85e5a9bf1cad72ab5cd7a9e4d0","source":{"kind":"arxiv","id":"1410.2334","version":3},"attestation_state":"computed","paper":{"title":"Gravitational Wave Detection with High Frequency Phonon Trapping Acoustic Cavities","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["physics.ins-det","quant-ph"],"primary_cat":"gr-qc","authors_text":"Maxim Goryachev, Michael E. Tobar","submitted_at":"2014-10-09T02:24:11Z","abstract_excerpt":"There are a number of theoretical predictions for astrophysical and cosmological objects, which emit high frequency ($10^6-10^9$~Hz) Gravitation Waves (GW) or contribute somehow to the stochastic high frequency GW background. Here we propose a new sensitive detector in this frequency band, which is based on existing cryogenic ultra-high quality factor quartz Bulk Acoustic Wave cavity technology, coupled to near-quantum-limited SQUID amplifiers at $20$~mK. We show that spectral strain sensitivities reaching $10^{-22}$ per $\\sqrt{\\text{Hz}}$ per mode is possible, which in principle can cover the"},"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":"1410.2334","kind":"arxiv","version":3},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"gr-qc","submitted_at":"2014-10-09T02:24:11Z","cross_cats_sorted":["physics.ins-det","quant-ph"],"title_canon_sha256":"fc4385df895e5896bc98e0c63ade1bb6abadf3b25d36ea4af270f311027941d1","abstract_canon_sha256":"a8ddaed43cb4f130d2ba7a6a70a5111a1ef2881ca1bcb2df5128d60ca7fbecca"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T11:22:26.389987Z","signature_b64":"EoPB5G/xV+bK4iyCV5qwd91nICRDY5q62t+cD5gNnMb7HYjHDuMs6Qw0YeN2jH2cKBbzRXj6wRUlAt3g9/ddAw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"fcd977e2a759f11dfad7211c9b599ab34074ad85e5a9bf1cad72ab5cd7a9e4d0","last_reissued_at":"2026-07-05T11:22:26.389459Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T11:22:26.389459Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Gravitational Wave Detection with High Frequency Phonon Trapping Acoustic Cavities","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["physics.ins-det","quant-ph"],"primary_cat":"gr-qc","authors_text":"Maxim Goryachev, Michael E. Tobar","submitted_at":"2014-10-09T02:24:11Z","abstract_excerpt":"There are a number of theoretical predictions for astrophysical and cosmological objects, which emit high frequency ($10^6-10^9$~Hz) Gravitation Waves (GW) or contribute somehow to the stochastic high frequency GW background. Here we propose a new sensitive detector in this frequency band, which is based on existing cryogenic ultra-high quality factor quartz Bulk Acoustic Wave cavity technology, coupled to near-quantum-limited SQUID amplifiers at $20$~mK. We show that spectral strain sensitivities reaching $10^{-22}$ per $\\sqrt{\\text{Hz}}$ per mode is possible, which in principle can cover the"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1410.2334","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/1410.2334/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":"1410.2334","created_at":"2026-07-05T11:22:26.389527+00:00"},{"alias_kind":"arxiv_version","alias_value":"1410.2334v3","created_at":"2026-07-05T11:22:26.389527+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1410.2334","created_at":"2026-07-05T11:22:26.389527+00:00"},{"alias_kind":"pith_short_12","alias_value":"7TMXPYVHLHYR","created_at":"2026-07-05T11:22:26.389527+00:00"},{"alias_kind":"pith_short_16","alias_value":"7TMXPYVHLHYR36WX","created_at":"2026-07-05T11:22:26.389527+00:00"},{"alias_kind":"pith_short_8","alias_value":"7TMXPYVH","created_at":"2026-07-05T11:22:26.389527+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":4,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2606.26736","citing_title":"Coherent collective response in many-qubit systems for dark matter detection","ref_index":37,"is_internal_anchor":false},{"citing_arxiv_id":"2512.19053","citing_title":"Quantum sensing of high-frequency gravitational waves with ion crystals","ref_index":65,"is_internal_anchor":false},{"citing_arxiv_id":"2509.22475","citing_title":"Probing high-frequency gravitational waves with entangled vibrational qubits in linear Paul traps","ref_index":2,"is_internal_anchor":false},{"citing_arxiv_id":"2604.22336","citing_title":"Super-Heisenberg protocol for dark matter and high-frequency gravitational wave search","ref_index":25,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/7TMXPYVHLHYR36WXEEOJWWM2WN","json":"https://pith.science/pith/7TMXPYVHLHYR36WXEEOJWWM2WN.json","graph_json":"https://pith.science/api/pith-number/7TMXPYVHLHYR36WXEEOJWWM2WN/graph.json","events_json":"https://pith.science/api/pith-number/7TMXPYVHLHYR36WXEEOJWWM2WN/events.json","paper":"https://pith.science/paper/7TMXPYVH"},"agent_actions":{"view_html":"https://pith.science/pith/7TMXPYVHLHYR36WXEEOJWWM2WN","download_json":"https://pith.science/pith/7TMXPYVHLHYR36WXEEOJWWM2WN.json","view_paper":"https://pith.science/paper/7TMXPYVH","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1410.2334&json=true","fetch_graph":"https://pith.science/api/pith-number/7TMXPYVHLHYR36WXEEOJWWM2WN/graph.json","fetch_events":"https://pith.science/api/pith-number/7TMXPYVHLHYR36WXEEOJWWM2WN/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/7TMXPYVHLHYR36WXEEOJWWM2WN/action/timestamp_anchor","attest_storage":"https://pith.science/pith/7TMXPYVHLHYR36WXEEOJWWM2WN/action/storage_attestation","attest_author":"https://pith.science/pith/7TMXPYVHLHYR36WXEEOJWWM2WN/action/author_attestation","sign_citation":"https://pith.science/pith/7TMXPYVHLHYR36WXEEOJWWM2WN/action/citation_signature","submit_replication":"https://pith.science/pith/7TMXPYVHLHYR36WXEEOJWWM2WN/action/replication_record"}},"created_at":"2026-07-05T11:22:26.389527+00:00","updated_at":"2026-07-05T11:22:26.389527+00:00"}