On the Energy Increase in Space-Collapse Models
arXiv:quant-ph/0506083 · doi:10.1088/0305-4470/38/37/007
Abstract
A typical feature of spontaneous collapse models which aim at localizing wavefunctions in space is the violation of the principle of energy conservation. In the models proposed in the literature the stochastic field which is responsible for the localization mechanism causes the momentum to behave like a Brownian motion, whose larger and larger fluctuations show up as a steady increase of the energy of the system. In spite of the fact that, in all situations, such an increase is small and practically undetectable, it is an undesirable feature that the energy of physical systems is not conserved but increases constantly in time, diverging for . In this paper we show that this property of collapse models can be modified: we propose a model of spontaneous wavefunction collapse sharing all most important features of usual models but such that the energy of isolated systems reaches an asymptotic finite value instead of increasing with a steady rate.
14 pages, revtex, no figures
References in corpus (13)
- Dynamical Reduction Models
- Why Decoherence has not Solved the Measurement Problem: A Response to P. W. Anderson
- Completely Positive Quantum Dissipation
- Quantum State Diffusion, Density Matrix Diagonalization and Decoherent Histories: A Model
- Martingale Models for Quantum State Reduction
- Towards Quantum Superpositions of a Mirror: an Exact Open Systems Analysis
- Generalized stochastic Schroedinger equations for state vector collapse
- On the quantum description of Einstein's Brownian motion
- Towards Quantum Superpositions of a Mirror: an Exact Open Systems Analysis - Calculational Details
- Non-Abelian linear Boltzmann equation and quantum correction to Kramers and Smoluchowski equation
- Simulating causal collapse models
- Subdynamics of relevant observables: a field theoretical approach
- Reply to Comment on "Completely positive quantum dissipation"
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