Wikipedia:Reference desk/Archives/Science/2015 November 21
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November 21
editFree electron density
editInteresting Question: in a typical metal, how many conduction band electrons are present per atom?
My answer: This isn't a topic I know, but a quick search conduction electrons per atom turned up [1]. The "table" link for it provides "free electron number densities" as in the first two columns of the following. I've added atomic weight and density to get a per-atom calculation by what I *think* is a relatively foolproof procedure - though I arbitrarily used white tin's density, and would get a slightly different answer for gray. Then I added Fermi energy and related parameters, which I believe can be calculated from the free electron number density and atomic mass...
Element | N/V x1028/m3 ( x 1022 cm3) |
g/cc | N/g (x 1022 cm3) |
g/mol | N/mol (x 1022 cm3) |
N/atom (x 1) |
Fermi energy (eV) |
Fermi temperature x 104 K |
Fermi velocity x 106 m/s |
---|---|---|---|---|---|---|---|---|---|
Cu | 8.47 | 8.96 | 0.94 | 63.5 | 60.0 | 0.96 | 7.00 | 8.16 | 1.57 |
Ag | 5.86 | 10.49 | 0.559 | 107.9 | 60.27 | 1.00 | 5.49 | 6.38 | 1.39 |
Au | 5.90 | 19.30 | 0.306 | 197.0 | 60.22 | 1.00 | 5.53 | 6.42 | 1.40 |
Be | 24.7 | 1.85 | 13.35 | 9.012 | 120.3 | 2.00 | 14.3 | 16.6 | 2.25 |
Mg | 8.61 | 1.738 | 4.95 | 24.305 | 120.4 | 2.00 | 7.08 | 8.23 | 1.58 |
Ca | 4.61 | 1.55 | 2.97 | 40.08 | 119.2 | 1.98 | 4.69 | 5.44 | 1.28 |
Sr | 3.55 | 2.64 | 1.34 | 87.62 | 117.8 | 1.96 | 3.93 | 4.57 | 1.18 |
Ba | 3.15 | 3.51 | 0.897 | 137.32 | 123.2 | 2.05 | 3.64 | 4.23 | 1.13 |
Nb | 5.56 | 8.57 | 0.649 | 92.906 | 60.3 | 1.00 | 5.32 | 6.18 | 1.37 |
Fe | 17.0 | 7.874 | 2.159 | 55.845 | 120.5 | 2.00 | 11.1 | 13.0 | 1.98 |
Mn (alpha) |
16.5 | 7.21 | 2.288 | 54.938044 | 125.7 | 2.09 | 10.9 | 12.7 | 1.96 |
Zn | 13.2 | 7.14 | 1.849 | 65.38 | 120.9 | 2.01 | 9.47 | 11.0 | 1.83 |
Cd | 9.27 | 8.65 | 1.072 | 112.414 | 120.5 | 2.00 | 7.47 | 8.68 | 1.62 |
Hg (78 K) |
8.65 | 13.534 (not 78 K) |
0.639 | 200.592 | 128.2 | 2.13 | 7.13 | 8.29 | 1.58 |
Al | 18.1 | 2.70 | 6.703 | 26.9815 | 180.9 | 3.00 | 11.7 | 13.6 | 2.03 |
Ga | 15.4 | 5.91 | 2.606 | 69.723 | 181.7 | 3.02 | 10.4 | 12.1 | 1.92 |
In | 11.5 | 7.31 | 1.573 | 114.818 | 180.6 | 3.00 | 8.63 | 10.0 | 1.74 |
Sn | 14.8 | 7.365 (gray) |
2.010 | 118.710 | 238.5 | 3.96 | 10.2 | 11.8 | 1.90 |
Pb | 13.2 | 11.34 | 1.164 | 207.2 | 241.2 | 4.01 | 9.47 | 11.0 | 1.83 |
The relationship given for Fermi energy and free electron density at the link above is the harder part for me at the instant. It should reduce to
EF = (1/8) h2/m [n*3/pi]2/3
h = [[Planck's constant] in J s = kg m2 s-1 m = (presumably) electron mass in daltons x (1.660538921E-27 kg) n is the number from the first column x 1028 m-3, so to the 2/3 power it is that number to the 2/3 power x 4.641589E+18 m-2.
This should get me a result in kg m2 s-2, i.e. in joules, which should be multiplied by 1 eV/(1.6021766208E-19 J) for a result in eV - looks like the units are right...
Looking at the table there's a monotonic relationship between N and Fermi energy (sort by column), so I'm thinking the "m" is actually the electron mass 9.10938215E-31 kg. Putting that in I get EV = 1.692532 N 2/3
Then for copper I calculate 7.03 eV from N, very close to the value given, and for lead 9.45 eV ... this is looking like I might have it, haven't checked all though. Wnt (talk) 21:29, 22 November 2015 (UTC)
From this I should be able to expand the table to cover some values at the above link's table where N is not given, but Fermi energy is. Computing (EV / 1.692532) ** 3/2 to fill the first column,
Element | N/V x1028/m3 ( x 1022 cm3) |
g/cc | N/g (x 1022 cm3) |
g/mol | N/mol (x 1022 cm3) |
N/atom (x 1) |
Fermi energy (eV) |
Fermi temperature x 104 K |
Fermi velocity x 106 m/s |
---|---|---|---|---|---|---|---|---|---|
Li | 4.68 | 0.534 | 8.76 | 6.94 | 60.8 | 1.01 | 4.74 | 5.51 | 1.29 |
Na | 2.65 | 0.968 | 2.74 | 22.990 | 63.0 | 1.05 | 3.24 | 3.77 | 1.07 |
K | 1.40 | 0.862 | 1.62 | 39.098 | 63.5 | 1.05 | 2.12 | 2.46 | 0.86 |
Rb | 1.14 | 1.532 | 0.744 | 85.468 | 63.6 | 1.06 | 1.85 | 2.15 | 0.81 |
Cs | 0.911 | 1.93 | 0.472 | 132.905 | 62.7 | 1.04 | 1.59 | 1.84 | 0.75 |
Tl | 10.56 | 11.85 | 0.891 | 204.38 | 182.1 | 3.02 | 8.15 | 9.46 | 1.69 |
Bi | 14.15 | 9.78 | 1.447 | 208.98 | 302.3 | 5.02 | 9.90 | 11.5 | 1.87 |
Sb | 16.34 | 6.697 | 2.440 | 121.760 | 297.0 | 4.93 | 10.9 | 12.7 | 1.96 |
Not very surprisingly, all the alkali metals come out close to one conduction electron per atom. The others seem plausible. The number of free electrons is never more than the number in the outermost shell, but we see in the first table it can be less... and that part may indeed be complicated. Wnt (talk) 22:16, 22 November 2015 (UTC)
- The link worked for me just now when I retested it - anyone else having trouble? I've been having some damn witchy internet performance today. As for the temperature, well - in the case of Hg the number given for N was at 78 K, and the density was at room temp, and I presume the disagreement between the two is to blame for the non-integer result. It looks like the Fermi temperature and free electron number per volume are interchangeable; either of these can be calculated based on the number per atom, the density of the material and the atomic weight. One thing I don't know at the moment is which quantities are obtained most accurately, and which is derived from which in practice by calculation. I cannot guarantee the number of conduction band electrons doesn't change with temperature, though I'm thinking that ought to be some kind of a phase transition at least. Wnt (talk) 04:07, 23 November 2015 (UTC)
- Note: well, that last comment was stupid, since the whole point of the Fermi distribution is it changes with temperature... what I mean, though, is that I think of the number of holes and mobile electrons in a semiconductor as being comparatively small. To change the integer part of the N/atom value above, I think you'd have to have an empty spot in half of the atoms of the metal, which I'd think would be an unusually hot temperature. But I realize now I don't actually know this. Wnt (talk) 15:24, 23 November 2015 (UTC)
Banned user |
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The following discussion has been closed. Please do not modify it. |
In a metal, electrical conduction is said to be provided by electrons flying about within the metal, not bound to any one atom or being an inter-atom bond. Only some electrons do this, I think, certainly not all electrons each atom could contribute. In TYPICAL pure metals, what is the ratio of the number of conduction electrons to the number of atoms? For COMMON alloys? 124.178.79.219 (talk) 02:53, 21 November 2015 (UTC)
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Is there more than two caves in an human skull?
editI know two caves: nasal cave and orbital cave. Is there more? 92.249.70.153 (talk) 03:19, 21 November 2015 (UTC)
- Do you mean cavity rather than cave? The skull has a nasal cavity, orbital cavity and sinus cavity. --Jayron32 04:48, 21 November 2015 (UTC)
- I found also middle ear cavity as well as oral cavity and carnial cavity. Is there a difference between sinuses to the cavities? 92.249.70.153 (talk) 06:27, 21 November 2015 (UTC)
- There's also the cranial cavity - containing the brain. Roger (Dodger67) (talk) 16:39, 22 November 2015 (UTC)
- I found also middle ear cavity as well as oral cavity and carnial cavity. Is there a difference between sinuses to the cavities? 92.249.70.153 (talk) 06:27, 21 November 2015 (UTC)
Fruit Preservation
editAs a result of chemical or physical reactions when heating/cooking foods: 1.will it make certain fruits(example plums,durian,banana,apple) to change from sour to sweet or vice –versa? 2.will it help to make foods that has gone slightly bad to be safer for eating? Please also state the reasons for your answers.
- This sounds an awful lot like homework. Why not try answering the questions yourself and then coming back here if you get stuck? You could even post your answer here and we'll likely vet it for you. In particular, think about what makes something sweet or sour and about how food is made more safe for eating. Is cooking used to accomplish either of these things? 99.235.223.170 (talk) 19:59, 21 November 2015 (UTC)