CeasarSalad1979
Registered Member
Just reflect off the nucleus of atoms?
NoJust reflect off the nucleus of atoms?
Just reflect off the nucleus of atoms?
So the reflection of light is more due to electron interactions than passive nuclaic interactions.Perhaps you could be a little more specific in what you are thinking. It's not a simple answer.
Generally though, light does not interact with nucleii. If it did, it might convert a proton into a neutron. More commonly, it will
- get absorbed by the electrons in their orbitals, kicking them up into a higher energy state.
- get absorbed by the bonds between atoms in a molecule and converted into vibrations
- a bunch of other things.
Pretty much. Most things that happen to atoms tend to happen to the electrons.So the reflection of light is more due to electron interactions than passive nuclaic interactions.
Yes.So the reflection of light is more due to electron interactions than passive nuclaic interactions.
This is ejection from the topmost electron, in energy terms, in the partly filled conduction band in the bulk metal. The "work function" is the name given to the energy needed to do it for each metal. I found a table of them here: http://hyperphysics.phy-astr.gsu.edu/hbase/Tables/photoelec.htmlI have a question, which I think may be relevent here: Light, when it interacts with "certain metals" will eject electrons completely. This of course gives rise to the photoelectric effect, known about since the second half of the 19th centuary, but only fully explained by considering light energy as being quantized.
My questions are: what are the properties of the so-called "certain metals"? I know they were originally the alkali metals, but my chemistry is not strong enough to attach any real meaning to that fact
Second: presumably these so-called certain metals will have their properties changed by the loss of electrons?? If so, do they still qualify as "certain metals" in the original sense?
Having thought more about this, and having read a bit more, I think I can add something to explain better the difference between ionisation energy and work function. The latter is the energy to remove an electron from the surface of the metal. At the surface, there is incomplete bonding of the electrons, since there are only +ve charged "cores" (atoms minus the outer electrons that are delocalised into the metallic bonding system) on one side of them. So these electrons are only "half-bound", as it were. That's one reason why it is easier to liberate one than to take one out of the outermost orbital of an isolated atom. There are also, apparently - I did not know this, but it makes obvious sense - a lot of detailed surface effects, arising from oxide films and so, on that can radically change the ease with which a surface electron can be liberated.This is ejection from the topmost electron, in energy terms, in the partly filled conduction band in the bulk metal. The "work function" is the name given to the energy needed to do it for each metal. I found a table of them here: http://hyperphysics.phy-astr.gsu.edu/hbase/Tables/photoelec.html
and you are right that it is lowest for alkali metals. This will be for the same reason the first ionisation energy is lowest for the alkali metals, viz. the alkali metals are starting to populate with electrons the s orbital of the next principal quantum number up, so they are outside the last closed shell and only see a low effective nuclear charge. That results in the alkali metals having one electron that is weakly bound, which is what makes them prone to form cations.
The work function is however not the same as the first ionisation energy, which is the energy needed to strip the first electron off a neutral atom of the metal. Interestingly, I found on comparing them that the work function is typically only about half the first ionisation energy. I found this at first glance counterintuitive, seeing as atoms in the bulk metal, being in a bound state, are of lower energy than isolated atoms would be. However, I suppose that's because we are taking an uppermost electron from the conduction band: there are many more electrons lower down in the band, so there is overall a lower energy state in the metal than in the isolated atom. But I've never made the comparison before, so I'm speculating a bit here.
Since the photoelectric effect is an effect in bulk metals, the metal left behind is a still a metal, just one fractionally deficient in electrons.
Yes, this makes sense. Thanks. I know that ionzing radiation is far more energentic than the visible light one typically sees in the photoelectic effect, though I do know that this effect is more efficient at higher energies. Which raises the question: where is the transition between the two, or does that question makes no sense?Having thought more about this, and having read a bit more, I think I can add something to explain better the difference between ionisation energy and work function. The latter is the energy to remove an electron from the surface of the metal. At the surface, there is incomplete bonding of the electrons, since there are only +ve charged "cores" (atoms minus the outer electrons that are delocalised into the metallic bonding system) on one side of them. So these electrons are only "half-bound", as it were. That's one reason why it is easier to liberate one than to take one out of the outermost orbital of an isolated atom. There are also, apparently - I did not know this, but it makes obvious sense - a lot of detailed surface effects, arising from oxide films and so, on that can radically change the ease with which a surface electron can be liberated.
So the relationship between work function and ionisation energy is not entirely straight forward.
The series limit of an atomic spectrum gives one the wavelength needed to just ionise an electron. For example with hydrogen the Lyman series, which is concerned with transitions to and from the quantum number n=1 (ground state), has a series limit at a wavelength of around 90nm (900Å),which is well into the UV but not into the X-ray region. The term "ionising radiation"normally conjures up radiation from atomic. nuclei (α, β, γ) rather than mere UV, but sufficiently energetic UV can in fact ionise atoms.Yes, this makes sense. Thanks. I know that ionzing radiation is far more energentic than the visible light one typically sees in the photoelectic effect, though I do know that this effect is more efficient at higher energies. Which raises the question: where is the transition between the two, or does that question makes no sense?
My yellowing Phys. Chem. text points out that ionization energy is in general equal to the energy of the incicdent radion less the kinetic energy of the expelled electron. Thus, ionizations that require large energies will leave the expelled electrons with lower kinetic energy and vice versa