On the CSL Scalar Field Relativistic Collapse Model
Daniel Bedingham, Philip Pearle

TL;DR
This paper discusses a relativistic CSL collapse model using a scalar field, providing solutions for the density matrix and analyzing collapse behavior and energy production, highlighting its theoretical soundness despite physical limitations.
Contribution
It introduces a relativistic CSL model with a scalar field operator and provides explicit solutions for the density matrix in different Hamiltonian scenarios.
Findings
Collapse favors eigenstates close to initial Gaussian states
Particle production dominates the density matrix over time
Model is theoretically sound but not physically viable due to energy increase
Abstract
The CSL dynamical collapse structure, adapted to the relativistically invariant model where the collapse-generating operator is a one-dimensional scalar field (mass ) is discussed. A complete solution for the density matrix is given, for an initial state when the Hamiltonian is set equal to 0, and when is the free field Hamiltonian. Here are coherent states which represent clumps of particles, with mean particle number density , where are gaussians of width with mean positions separated by distance . It is shown that, with high probability, the solution for (identical to the short time solution for ) favors collapse toward eigenstates of the scalar field whose eigenvalues are…
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Taxonomy
TopicsQuantum Mechanics and Applications · Cosmology and Gravitation Theories · Quantum Information and Cryptography
