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Particle in superposition of energy eigenstates and conservation of energy. |
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| Dec12-12, 03:02 AM | #18 |
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Particle in superposition of energy eigenstates and conservation of energy.The only way you can have dynamics in the universe is if universe is not in an eigen state of the Hamiltonian. And why should it be in an eigen state? There are infinitely more states than there are eigen states. So we don't need to discuss collapse here. The universe is in some super-position of eigen states, and that's enough. Note that regardless of what kind of superposition you have, [H, H] = 0. So expectation value of energy does not change in time. Yes, energy of the universe is not an eigen energy. But it's always the same, so there are no issues with conservation laws. |
| Dec12-12, 03:37 AM | #19 |
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@Demystifier
Thanks for that, but I'm still mystified ;-) Consider an isolated H-atom in an excited state (for example 2p). This is an energy eigenstate and stationary. However, we know that the H-atom can emit a photon and go to the ground state. The total energy of the system does not change. So can the system evolve from being excited into a superpositon of excited + (ground state +photon)? If not, is the actual photon emission of an excited atom due to some external disturbance? An interaction with the vacuum state of the photon field? |
| Dec12-12, 04:16 AM | #20 |
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| Dec12-12, 04:25 AM | #21 |
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@K^2
Thanks, but I'm still not 100% sure I understand what's going on: Let's assume I "nudge" the system somehow by a quantum process - then it would be in a superposition state. Am I right in assuming that the "nudge-system" itself cannot be in an energy-eigenstate, otherwise it could not change its state and do the nudge? |
| Dec12-12, 04:51 AM | #22 |
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referring to the whole universe and its Hamiltonian may be dangerous b/c (as we know from GR and several QG proposals) energy can neither be defined canonically nor via Noether theorem in general; the problem of the construction of a diff. inv. Dirac observable is - afaik - not yet solved; we have H ~ 0 i.e. H does neither correspond to an energy operator, nor to a time-evolution operator
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| Dec12-12, 05:20 AM | #23 |
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What is the classical surrounding of the whole universe? |
| Dec12-12, 05:22 AM | #24 |
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@tom.stoer Agreed. Unfortunately, we don't really have a better description yet. We can talk what happens if we can treat universe as a closed system with a definite Hamiltonian, under assumption that such a field theory even exists. Whether it does exist is a separate question.
But yes, this is why all the real work is not being done on true closed systems. They are done on partially isolated sub-systems. Hence the golden rule and pretty much the entire stat mech. |
| Dec12-12, 06:31 AM | #25 |
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| Dec12-12, 07:59 AM | #26 |
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| Dec12-12, 08:03 AM | #27 |
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| Dec12-12, 08:08 AM | #28 |
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| Dec12-12, 08:17 AM | #29 |
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| Dec12-12, 08:19 AM | #30 |
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But stability is a separate issue. 2p is unstable even in basic Hydrogen atom Hamiltonian. 2p + ε 1s already has dipole moment and will radiate. So a small perturbation will result in decay. That's the definition of instability. |
| Dec12-12, 09:36 AM | #31 |
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| Dec17-12, 10:51 AM | #32 |
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The notion of a closed universe is quite interesting. Demystifier to expand on what you are saying, if energy eigenstates, so the different superpositions of a particle, must evolve into a coherent state, where does all this excess energy from these states go? Our universe,in accordance with things such as Pauli Exclusion can only have on outcome of a solution, and the physical existence of a particle in two different states seems impossible. Could it be that many worlds theory holds valid in that all these different energy eigenstates come together to form an infinite number of possibly universes, each branching from another, as a wave function collapses and the other superpositions become irrelevant to our world?
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