Exact(34)
This makes sense, at least if the stellar collapse model is the right one.
To discuss these points, let us briefly review the first consistent Collapse model (Ghirardi, Rimini, and Weber 1985) to appear in the literature.
However, many scientists now agree that the gravitational collapse model could be very important "especially when explaining multiple large planets a long way out from the star".
But the study on the ISO collapse model shows that it is inappropriate to predict the collapse strength of HCC of all sizes.
An energy balance between prebuckling and collapsed configurations obtained from a uniform collapse model yields approximate values of PP2 and PPS.
We have then simply to recall that in a collapse model relating reductions to mass density differences, the dynamics suppresses in extremely short times the embarrassing superpositions of such states to recover the mass distribution corresponding to our perceptions.
Similar(26)
Non-interferometric tests of collapse models.
Figure 11 Decoherence parameter for various collapse models.
In the GRW/Pearle collapse models, wave functions represent the most exhaustive, complete specification of states of individual systems.
Collapse models typically depend more strongly on particle mass than quantum physics, which facilitates their experimental distinction.
In Figure 2, we compare the predictions of several collapse models with that minimum, discernible decoherence rate (Gamma _{mathrm{min}}).
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