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This comparison utilizes a calculation of the rate of heating through phonon excitation implied by a general noise power spectrum $\\lambda(\\omega)$. We find that in the standard heating formula, the reduction rate $\\lambda$ is replaced by $\\lambda_{\\rm eff}=\\frac{2}{3 \\pi^{3/2}} \\int d^3w e^{-\\vec w^2} \\vec w^2 \\lambda(\\omega_L(\\vec w/r_c))$, with $\\omega_L(\\vec"},"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":"1801.06857","kind":"arxiv","version":3},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"quant-ph","submitted_at":"2018-01-21T17:23:25Z","cross_cats_sorted":[],"title_canon_sha256":"6eceae09416049df63a0b96e7c6bebef3c1f6131104cb8c8395c1965ca0c5422","abstract_canon_sha256":"e33ef1d3370f57100c1459ea243b00940ab5c93296d1b4e02cf09d04bd9acc08"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:13:28.327941Z","signature_b64":"KA/hFSvDUFQSWH2pZoq/b9HD+n8LGXhcD9nEF5uWctjVtBGcZdZMYLAncj+seg62jnY/fYHcGH/AGUuuvZ06Bg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"c8ef5c4dc35d0c7f3c0a9e93d60aef9ca92325611d733c8d500fa173320baebc","last_reissued_at":"2026-05-18T00:13:28.327493Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:13:28.327493Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Bulk Heating Effects as Tests for Collapse Models","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"quant-ph","authors_text":"Andrea Vinante, Stephen L. 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