On the (im)possibility of extending the GRW model to relativistic particles
arXiv:1907.02370 · doi:10.1103/PhysRevA.103.042216
Abstract
Spontaneous collapse models are proposed modifications to quantum mechanics which aim to solve the measurement problem. In this article we will consider models which attempt to extend a specific spontaneous collapse model, the Ghirardi-Rimini-Weber model (GRW), to be consistent with special relativity. We will present a condition that a relativistic GRW model must meet for three cases: for single particle, for N distinguishable particles, and for indistinguishable particles. We will then show that this relativistic condition implies that one can have a relativistic GRW model for a single particle or for distinguishable non-interacting, non-entangled particles but not otherwise.
14 pages, 11 figures, 1 table. Revised version of the paper, with more context in section II with regards to the definition of Lorentz covariance
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