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- Path: sparky!uunet!think.com!paperboy.osf.org!hsdndev!husc-news.harvard.edu!blom
- From: blom@husc15.harvard.edu
- Newsgroups: sci.chem
- Subject: Re: Technetium
- Summary: Nucleon shell model, elementary style
- Keywords: nucleon shell model proton electron pairing magic numbers
- Message-ID: <1993Jan21.153756.19628@husc15.harvard.edu>
- Date: 21 Jan 93 20:37:56 GMT
- References: <staff.02r1@rabbit.augs.se> <C0zK8D.Bu1@world.std.com> <staff.02ri@rabbit.augs.se> <C14nyC.Fyp@world.std.com>
- Reply-To: blom@husc.harvard.edu
- Followup-To: sci.chem
- Organization: Harvard University Science Center
- Lines: 127
-
- In article <C14nyC.Fyp@world.std.com>, moroney@world.std.com (Michael Moroney) writes:
- > staff@rabbit.augs.se (Staffan Friberg) writes:
- >
- >>In article <C0zK8D.Bu1@world.std.com> moroney@world.std.com (Michael Moroney) writes:
- >
- >>> There is some sort of structure to the nucleus, similar to electron shells.
- >>> The protons (and neutrons) pair up. The stable odd-proton elements all have
- >>> only one or two stable isotopes, while even-proton elements have as many as
- >>> 10 stable isotopes. It turns out that technecium (and promethium) didn't
- >>> even get one stable isotope.
- >
- >>What does this structure look like. Do they just pair up two by two or is it
- >>more complex than that?
- >
- > There is a shell structure of some sort, like electron shells of atoms.
- > Some numbers are rather stable, much like the noble gas shells of atoms
- > are stable, so like noble gases are stable (don't "want" to gain or lose
- > electrons) these nuclei are stable against nuclear processes. I think
- > 3 of these stable shells are helium, tin and lead. Note that helium nuclei
- > are commonly formed by radioactive alpha decay, lead is the end-point of
- > the decay of the heavy elements, and tin has 10 stable isotopes.
- > I've read a theory that the next number is 114, and element 114, if it
- > can be made, might be stable or have an exceptionally long half-life (anyone
- > know if any progress has been made recently to make elements near 114?)
- >
- > -Mike
-
-
- OK. I'll now proceed to tell you all everything I know. I hope this helps.
- First of all, large nuclei become less stable because the strong force which
- bonds the nucleii acts only at short range because its mediators, the pions,
- are short-lived. Photons, the mediators of the electromagnetic force, are
- very stable, and although this force is 100x weaker than the strong force. As
- nuclei become very large, the strong force dies off very rapidly and the nuclei
- become less stable.
-
- The protons and neutrons are hypothetically assumed to lie in shells because
- this explains nuclear stability. Nucleons have spins which correspond to
- half-integer multiples of h bar. (or, if you like, half integer multiples of
- h/2pi, where h is Planck's constant.) Electrons have spins of 1/2 or -1/2.
- Protons and neutrons have spins of 1/2, -1/2, 3/2, -3/2, 5/2, -5/2, etc.
- Arranging them into shells, we find they fill in a fairly regular pattern:
- (I have filled the shells in pairs, which have opposite spin. By pairing
- particles with opposite spin, we greatly increase their stability. This is the
- reason for the even-even rule.) Oh, and somehow, there are 2 1/2-spin
- nucleons, 6 3/2 spin nucleons, and 2n n/2-spin nucleons per shell. [Insert
- favorite hand-waving argument here.] I guess it has to do with angular
- momentum and quantum number, sort like electron shells, but I don't think
- anyone REALLY knows.
-
- 2: 1/2
-
- 8: 3/2
- 10: 1/2
-
- 20: 5/2
- 26: 3/2
- 28: 1/2
-
- . . .
-
- 2,8,20,28,50,82,and 126 turn out to be "magic" numbers. Nucleii with this
- number of either protons or neutrons are exceptionally stable. Nucleii with
- a magic number of protons and a magic number of neutrons are even more stable.
-
- To previous poster: Element 126 is the one, I believe, which is expected to be
- very stable. (Rather than 114, although that might come pretty close.) By
- really stable people mean "as stable as Radium" or so, although who knows? It
- might not be radioactive... Ha.
-
- Hope this makes some sense. I'm actually a bit fuzzy right now about the above
- nucleon pairing scheme. Somehow I can't get it to work properly. Anyhow,
- that's the general idea. If I figure out what I was doing wrong, I will
- repost. Ciaou, everyone, and have duckie days.
-
- Eric Blom
- Harvard U
-
-
- P.S. OK. I figured out my problem. Somehow there are 2k nucleons with 2k-1/2
- spin. So there are a total of 12 nucleons in an 11/2-spin shell. So the
- diagram goes like this:
-
- *2: 1/2
-
- 6: 3/2
- *8: 1/2
-
- 14: 5/2
- 18: 3/2
- *20: 1/2
-
- *28: 7/2
- 34: 5/2
- 38: 3/2
- 40: 1/2
-
- *50: 9/2
- 58: 7/2
- 64: 5/2
- 68: 3/2
- 70: 1/2
-
- *82: 11/2
- 92: 9/2
- 100: 7/2
- 106: 5/2
- 110: 3/2
- 112: 1/2
-
- *126: 13/2
- 138: 11/2
- 148: 9/2
- ...
-
- By this point, it's all speculation. The shells marked with asterisks show
- special stability, and correspond to magic numbers. Again, both the protons
- and the neutrons form these shells, and they seem to do so independantly. To
- be very stable, a nucleus likes to have filled shells of protons and neutrons.
-
- No one to date has tried to synthesize element 126. Considering it's large
- size, I would be extremely surprised if element 126 has a half life over a
- fraction of a second. After all, if it did, there's a good chance we'd see it
- on Earth or in star spectra.
-
- Eric Blom
- Harvard U
-