Bohmian mechanics and the Ghirardi-Rimini-Weber theory provide opposite resolutions of the quantum measurement problem: the former postulates additional variables (the particle positions) besides the wave function, whereas the latter implements spontaneous collapses of the wave function by a nonlinear and stochastic modification of Schrödinger's equation. Still, both theories, when understood appropriately, share the following structure: They are ultimately not about wave functions but about 'matter' moving in space, represented by either particle trajectories, fields on space-time, or a discrete set of space-time points. The role of the wave function then is to govern the motion of the matter.

A major disagreement between different views about the foundations of quantum mechanics concerns whether for a theory to be intelligible as a fundamental physical theory it must involve a "primitive ontology" (PO), i.e., variables describing the distribution of matter in 4-dimensional space-time. In this paper, we illustrate the value of having a PO. We do so by focussing on the role that the PO plays for extracting predictions from a given theory and discuss valid and invalid derivations of predictions. To this end, we investigate a number of examples based on toy models built from the elements of familiar interpretations of quantum theory. PACS: 03.65.Ta. Key words: quantum theory without observers; Ghirardi-RiminiWeber (GRW) theory of spontaneous wave function collapse; Bohmian mechanics; many-worlds view of quantum mechanics. Dedicated to Tim Maudlin on the occasion of his 50th birthday

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Schrödinger's first proposal for the interpretation of quantum mechanics was based on a postulate relating the wave function on configuration space to charge density in physical space. Schrödinger apparently later thought that his proposal was empirically wrong. We argue here that this is not the case, at least for a very similar proposal with charge density replaced by mass density. We argue that when analyzed carefully this theory is seen to be an empirically adequate many-worlds theory and not an empirically inadequate theory describing a single world. Moreover, this formulation-Schrödinger's first quantum theory-can be regarded as a formulation of the many-worlds view of quantum mechanics that is ontologically clearer than Everett's. PACS: 03.65.Ta. Key words: Everett's many-worlds view of quantum theory; quantum theory without observers; primitive ontology; Bohmian mechanics; quantum nonlocality in the many-worlds view; nature of probability in the many-worlds view; typicality.

Classical physics is about real objects, like apples falling from trees, whose motion is governed by Newtonian laws. In standard quantum mechanics only the wave function or the results of measurements exist, and to answer the question of how the classical world can be part of the quantum world is a rather formidable task. However, this is not the case for Bohmian mechanics, which, like classical mechanics, is a theory about real objects. In Bohmian terms, the problem of the classical limit becomes very simple: when do the Bohmian trajectories look Newtonian?1. The first step is the crucial one: As is well known, and as Bell has emphasized [1], standard quantum mechanics is not a precise microscopic theory because the division between