Spread fo wavefunctions - filling the universe?

In summary, wavefunctions spread with time for particles that do not interact, which is the case for many particles in the universe such as cosmic ray protons. This means that most of space in the universe is filled with overlapping wavefunctions. However, this does not cause any problems with the exclusion principle. Shankar discusses this concept and explains that the wavefunction for an electron extends throughout all space, but this does not mean the electron itself exists everywhere. When observed, an electron will only be found in one place due to the exclusion principle. This concept may also help explain the expansion of the universe.
  • #1
franoisbelfor
42
0
Wavefunctions spread with time, if the particle does not interact.
Now, the universe is filled with particles that do not interact for
thousands and millions of years, for example cosmic ray protons.

This would mean most space in the universe is filled with
wavefunctions, all overlapping.

Does this give problems with the exclusion principle?
Did anybody calculate such effects?
Does this explain the expansion of the universe?


François
 
Physics news on Phys.org
  • #2
It doesn't give any problems with the exclusion principle (thankfully). If the particles are far away, we don't make a big mistake if we don't include them in the anti-symmetrization of the wavefunction. Shankar discusses this I think.
 
  • #3
the wave function for, say an electron, extends throughout all space. but, this does not mean the electron itself exists everywhere. there's a probability (specifically, the square of the wave function) that when you look, you'll find the electron at a given place. you don't know if it's at a given place or not for sure until you look. you'll never see two electrons on top of each other when you do look, though, due to the exclusion principle.
 

FAQ: Spread fo wavefunctions - filling the universe?

What is the concept of spread of wavefunctions?

The spread of wavefunctions refers to the distribution of probabilities associated with the position and momentum of a particle described by a wavefunction. It is a measure of the uncertainty in the particle's location and momentum.

How does the spread of wavefunctions affect the filling of the universe?

The spread of wavefunctions is a fundamental concept in quantum mechanics and affects the behavior of particles at the subatomic level. It determines the probability of a particle's position and momentum, which ultimately affects the structure and dynamics of the universe.

What factors affect the spread of wavefunctions?

The spread of wavefunctions is affected by the energy of the particle, the potential energy of the system, and the temperature of the environment. It is also influenced by the shape and size of the wavefunction and the potential barriers present in the system.

Can the spread of wavefunctions be measured?

Yes, the spread of wavefunctions can be measured through experiments such as the double-slit experiment or the Stern-Gerlach experiment. These experiments involve observing the behavior of particles and their probability distributions to determine the spread of their wavefunctions.

What implications does the spread of wavefunctions have for our understanding of the universe?

The spread of wavefunctions plays a crucial role in our understanding of the universe at the quantum level. It helps explain the behavior of particles and the formation of structures in the universe. It also has implications for technological advancements in fields such as quantum computing and quantum communication.

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