The Ghirardi--Rimini--Weber theory modifies unitary time evolution by random Gaussian position localizations. Each constituent collapses at a small fixed rate, while the rate for an entangled macroscopic body grows with its number of constituents.
For localization length , the GRW localization operator acting on particle is
A collapse centred at sends to the normalized state with probability density .
For equal particle rates in the GRW model, the next centre falls in with probability . With zero Hamiltonian operator, two successive centres in have joint probability . Dividing by the first-event probability gives the conditional second event, including repeated particle labels. Spatial probabilities depend on actual packet mass, not solely the nominal packet centres.
For entangled constituents, independent localization rates add to approximately . One constituent's collapse localizes the correlated macroscopic configuration, rapidly suppressing macroscopically separated branches.
A first localization near one macroscopically separated branch suppresses the other branch through the Gaussian GRW localization operator. This selects a correlated pointer alternative. However, if a region contains only packet centres and excludes substantial packet mass, the next centre need not lie in that region's small enlargement. Probabilities for the first event and approximately one for the next require regions containing essentially all corresponding branch mass. The general GRW collapse-centre event probabilities retain the geometry exactly.
GRW position localization increases the ensemble mean momentum variance. In three dimensions one collapse adds to , producing mean kinetic-energy increase .

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