Topics in dynamical wave function collapse
APA
Pearle, P. (2009). Topics in dynamical wave function collapse. Perimeter Institute. https://pirsa.org/09090091
MLA
Pearle, Philip. Topics in dynamical wave function collapse. Perimeter Institute, Sep. 29, 2009, https://pirsa.org/09090091
BibTex
@misc{ pirsa_PIRSA:09090091, doi = {10.48660/09090091}, url = {https://pirsa.org/09090091}, author = {Pearle, Philip}, keywords = {Quantum Foundations}, language = {en}, title = {Topics in dynamical wave function collapse}, publisher = {Perimeter Institute}, year = {2009}, month = {sep}, note = {PIRSA:09090091 see, \url{https://pirsa.org}} }
Hamilton College
Talk Type
Subject
Abstract
It will be shown how the CSL (continuous spontaneous localization) dynamical collapse equations work. A mathematically equivalent, non-collapse, Hamiltonian formulation will be described, with interpretative differences between it and CSL briefly discussed. A random field engenders collapse in CSL, and particle energies increase due to collapse. Energy of the random field will be treated, such that energy of particles plus field is conserved. A conserved energy-momentum-stress density tensor for the random field will be presented, enabling gravitational applications. Finally, a possible role for collapse in the beginning of the universe is modeled.