QUOTE
Your statement is just saying that if you narrow down where you're looking, a smaller range of point locations is included in the area.
Yes. And when you narrow down where you're looking, you define the possible values for position more accurately. The smaller the area you consider, the more inaccurately you can measure the momentum, and the wider the range of possible values there can be.
This, and the Pauli exclusion principle, is the source of 'electron degeneracy pressure, which prevents neutron stars from completely collapsing into black holes.
Wiki on electron degeneracy pressure.QUOTE (->
| QUOTE |
| Your statement is just saying that if you narrow down where you're looking, a smaller range of point locations is included in the area. |
Yes. And when you narrow down where you're looking, you define the possible values for position more accurately. The smaller the area you consider, the more inaccurately you can measure the momentum, and the wider the range of possible values there can be.
This, and the Pauli exclusion principle, is the source of 'electron degeneracy pressure, which prevents neutron stars from completely collapsing into black holes.
Wiki on electron degeneracy pressure.Ron's statement made sense. If you would take a long exposure of a few particles, the pattern would be more likely to be tighter than if you took the same length exposure of many particles.
When Ron said 'the smaller the sample', he was talking about the physical space examined, not the number of particles.