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Is liquid helium composed of both ortho and para-helium? |
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| Jun23-10, 10:25 PM | #1 |
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Is liquid helium composed of both ortho and para-helium?
In a batch of liquid helium (say < 8* K.) is there a mixture of both ortho and para-helium, or is it only ground state para-helium.?
I was under the impression that ortho was a meta-stable state which cannot decay to ground state Para-helium by radiative emission, but by meta-stable we are talking only a fraction of a second...right? What am I missing here.? Anyone? .. |
| Jun23-10, 10:49 PM | #2 |
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IIRC, the singlet-triplet splitting is quite large, ~20 eV. So it should be entirely in the ground state, unless there are special conditions going on (they've made triplet-helium BECs).
It can decay radiatively, just not by a single-photon process. |
| Jun23-10, 11:18 PM | #3 |
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What special conditions are you referring to ? How do I create triplet state experimentally? |
| Jun23-10, 11:51 PM | #4 |
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Is liquid helium composed of both ortho and para-helium?1/10 of a second.. I'm not sure. An isolated 3He atom would probably have a lifetime orders of magnitude longer. But with gaseous or liquid helium, in a container, etc, you have many more interactions that can go on and assist the process. (For instance formation of a He2 molecule in the [tex]^3\Sigma_u^+[/tex] state.) |
| Jun25-10, 12:45 PM | #5 |
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I have read elsewhere that the most probable decay is thru 'collisional' process, I am not sure what that refers to ...any info there? GW Drake has a later article in which it appears as if he is saying that there is a MORE probable Magnetic dipole transition to ground state decay...am I reading that right? See here: http://cos.cumt.edu.cn/jpkc/dxwl/zl/...atomic/099.pdf Creator |
| Jun25-10, 02:36 PM | #6 |
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![]() Both forms of decay are certainly many orders-of-magnitude less significant than the collision route, in a 'normal' environment. This is all mostly of astrophysical interest, since space is full of helium atoms in high vacuum. |
| Jul1-10, 10:08 PM | #7 |
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The collisional process is interesting...apparently, collision with a container wall can also do the trick. 1st question: At what temperature is there enough kinetic energy to spin flip each He triptlet state? Probably somewhere there is a temperature dependent rate formula? 2. Can collisional spin flip be by mecahnical means, (ex,rotation of the fluid) ? After further reasearch it appears as though I was wrong about the 1/10 sec. excited lifetime. The He(2S^3) state lifetime is about 8000 seconds!! That's a quantum eternity, and surprising...probably the longest"Meta-stable" state around.....but makes sense knowing the fact that it is radiatively forbidden transition to ground. Creator |
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