{"paper":{"title":"On the CSL Scalar Field Relativistic Collapse Model","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"quant-ph","authors_text":"Daniel Bedingham, Philip Pearle","submitted_at":"2019-06-27T09:05:28Z","abstract_excerpt":"The CSL dynamical collapse structure, adapted to the relativistically invariant model where the collapse-generating operator is a one-dimensional scalar field $\\hat\\phi(x,t)$ (mass $m$) is discussed. A complete solution for the density matrix is given, for an initial state $|\\psi,0\\rangle=\\frac{1}{\\sqrt{2}}[|L\\rangle+|R\\rangle]$ when the Hamiltonian $\\hat H$ is set equal to 0, and when $\\hat H$ is the free field Hamiltonian. Here $|L\\rangle, |R\\rangle$ are coherent states which represent clumps of particles, with mean particle number density $N\\chi_{i}^{2}(x)$, where $\\chi_{1}(x),\\chi_{1}(x) $"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1906.11510","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"}