1999/05/05 by A. M. Lisewski, Andreas Martin Lisewski, Lisewski, A. M.
Physics and Astronomy · #Black Holes and Theoretical Physics #Cosmology and Gravitation Theories #FOS: Physical sciences #Quantum Physics (quant-ph) #Theoretical and Computational Physics #quant-ph
paper · pdf · doi:10.48550/arxiv.quant-ph/9905014
minor changes, 9 pages, no figures, uses revtex
openalex publication_date 1999/05/05 · arxiv created 1999/06/30 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28
We discuss the transition from a quantum to a classical domain for a model where a separation into environment and system is explicitely not given. Utilizing the coarse graining procedure for free quantum fields we also apply the projection method and the Hamiltonian principle to study possible cases of emergent classicality. General conditions for classical dynamics are given. Eventually, they lead to the equations of motion for a perfect classical fluid.