Lower and Upper Bounds on CSL Parameters from Latent Image Formation and IGM Heating

dc.creatorAdler, Stephen L.
dc.date2006-05-07
dc.date2007-09-24
dc.date.accessioned2026-07-07T11:07:44Z
dc.date.available2026-07-07T11:07:44Z
dc.descriptionWe study lower and upper bounds on the parameters for stochastic state vector reduction, focusing on the mass-proportional continuous spontaneous localization (CSL) model. We show that the assumption that the state vector is reduced whan a latent image is formed, in photography or etched track detection, requires a CSL rate parameter $λ$ that is larger than conventionally assumed by a factor of roughly $2 \times 10^{9\pm 2}$, for a correlation length $r_C$ of $10^{-5}{\rm cm}$. We reanalyze existing upper bounds on the reduction rate and conclude that all are compatible with such an increase in $λ$. The best bounds that we have obtained come from a consideration of heating of the intergalactic medium (IGM), which shows that $λ$ can be at most $\sim 10^{8\pm 1}$ times as large as the standard CSL value, again for $r_C=10^{-5} {\rm cm}$. (For both the lower and upper bounds, quoted errors are not purely statistical errors, but rather are estimates reflecting modeling uncertainties.) We discuss modifications in our analysis corresponding to a larger value of $r_C$. With a substantially enlarged rate parameter, CSL effects may be within range of experimental detection (or refutation) with current technologies. ADDED NOTE: A careful calculation of radiation from atomic systems in the CSL model (Adler and Ramazanoglu, arXiv:0707.3134) has reinstated the bound obtained by Fu as the best upper bound on lambda, with significant implications for CSL model phenomenology.
dc.descriptionTex, 50p To appear in J. Phys. A: Math-Gen, in the special issue ``The Quantum Universe'' in honor of G. C. Ghirardi. Version 9(apart from minor copy-editing style changes) is the final published version. SEE ADDED NOTE IN ABSTRACT
dc.identifierhttps://arxiv.org/abs/quant-ph/0605072
dc.identifierhttp://arxiv.org/abs/quant-ph/0605072
dc.identifierJ.Phys.A40:2935-2958,2007; Erratum-ibid.A40:13501,2007
dc.identifierdoi:10.1088/1751-8113/40/12/S03 10.1088/1751-8121/40/44/C01
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/189947
dc.subjectQuantum Physics
dc.subjectHigh Energy Physics - Phenomenology
dc.subjectHigh Energy Physics - Theory
dc.titleLower and Upper Bounds on CSL Parameters from Latent Image Formation and IGM Heating
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