Hi,
Just found this forum topic and thought I might contribute some answers since it is up my alley. Sorry if some of my answers overlap with others, although I'll try to avoid repeating too much.
GRB 080319B said:
I have plethora of questions about light:
1.) I understand that light is created when the electrons in an atom jump to a higher level and fall back down to their ground state. When light is emitted, is it emitted orthogonal to the electron or at the angle of absorption? How is light emitted orthogonal to the nucleus when the electron jumps and falls back orthogonal to the nucleus? Isn't light emitted perpendicular to the direction that the electron jumps? Or are the electrons not orbiting parallel to the nucleus? Do photons/light waves propagate outward in all directions, e.g. a ripple in a pond, or unidirectionally?
In quantum optics, there are basically two kinds of photon emission from an atom: stimulated emission and spontaneous emission. Stimulated emission means the photon is emitted due to the presence of a second nearby photon. In essence, the second photon encourages the new photon to be emitted. For this case, the new photon will occupy the same "mode" as the first photon, or in other words it will travel in the same direction with the same polarization, same phase, etc. This is how lasers work. A photon comes by, stimulates another photon to be emitted with the same properties. The two photons can then stimulate more photons and so on. If you have enough excited atoms this becomes a run-away process until eventually there is an equilibrium between losses in the system and new photons being created into this system via stimulated emission.
The second method for an atom to emit light is spontaneous emission. Like with radioactive decay, there is a lifetime associated with an excited atom. During this lifetime, there is a chance that the atom will return to an un-excited state and emit a photon in the process. Because this process is random and not prompted by other photons, there is no preference for the "mode" of the photon. There is equal probability over all directions that the photon will be detected. In the classical picture, this is most like the spherical wave emanating from the atom.
Oh, and to say the electron is orbiting the nucleus isn't very accurate when talking in the quantum sense. We usually say the electron has a wavefunction which describes the (spatial) probability distribution for measuring the electron at that location. The weird quantum thing is that the electron is simultaneously in
all locations where the wavefunction is non-zero although an actual measurement might show it as being at a particular point. It would be as if an entire ocean wave would instantly disappear as soon as it made a buoy move up-and-down (i.e. it was measured).
GRB 080319B said:
2.) Is light from a reflective surface like a mirror really absorbed and re-emitted or is it just reflected? Is any energy lost in the process of re-emitting light, i.e. is some of the energy of the absorbed photon turned into heat, or is it a complete conversion? Is their any way to modulate the amount/wavelength of photons re-emitted? Do ionized atoms emit different wavelengths than their electrically neutral counterparts would? Does light in the form of photons/waves lose energy as it propagates through space and if so how?
There are several questions here that I will try and address. To start, there are two aspects of light interaction with matter. The first (discussed in the answer above) is absorption/emission. The second is what we call the "index of refraction" for a material. If you want, you could say the absorption/emission affects the strength of the light while the index of refraction affects the phase. Reflection and index of refraction fall into this second category where only the phase of the light is affected. From a classical picture, the electric field (which is part of a light wave) causes electrons in the material to oscillate. These oscillating electrons create new light waves. The atoms in the material however have their own natural resonance frequency they want to oscillate at. If the incident light is not exatly at this resonance frequency, then the new light will have a different phase than the old light. In this classical picture, you add the electric fields up to get the net light wave, and because of this phase difference you get effects such as slowed down propagation or even reflection. Most of this can be translated into an equivalent semi-classical or even quantum description, but I have never gained much additional insight from doing so.
As for light changing frequency, it can happen, but you have to work at it. For instance, there is a thing called a Doppler shift. Imagine shining a lser pointer at a mirror that is flying away from you. The light coming back will actually be slightly redder in color (lower frequency) than the light coming out of the pointer. This is called the Doppler effect, and has been exploted for neat science tricks. In fact, it makes up the bulk of laser cooling (my specialty) which can take a room temperature gas and cool it to within a milli-Kelvin above absolute zero within a fraction of a second! Additional tricks can then get you colder, and eventually into Bose-Einstein condensation which you may have heard about.
As for ionized atoms, I am not an expert, but I don't think things change much. The color (frequency) of light depends only on atomic transitions, which I believe stay the same with ionization.
Lastly, I am not sure how to answer the losing energy question. What I will say is that as you move away from the atom there are more places you can detect the photon, and so the probability of detecting the photon at anyone location decreases. For the stimulated emission description I mentioned above, this is not necessarily true since the photon is emitted in a specific direction, but for the spontaneous emission which has uniform emission with direction it is. To see why, just think of a sphere surrounding the atom. The surface area of the sphere goes as the radius^2. The probability must always be 100% that it can be measured, and so for an equivalent size detector, the probability a photon is detected will fall as 1/radius^2. You can see this just by consideration of the fractional size of your detector with respect to the size of the sphere.
GRB 080319B said:
3.) Light is described as being an electromagnetic wave, with electric and magnetic components. I understand these components come from electrons having magnetic and electric properties. How exactly do the magnetic and electric properties of electrons merge to form electromagnetic waves? Is the electric component caused by the electrons falling from higher energy levels? How is the magnetic component created? How does an electromagnetic wave contain both a magnetic and electric component within one wave? How do current, magnetic and electric fields affect light or produce it, and conversely, how does light affect said fields and current?
I think others have explained this well enough. Classically, light can be thought of as a self-perpetuating electro-magnetic field. The time changing electric field produces a time-varying magnetic field which produces a time-varying electric field, and so on.
GRB 080319B said:
4.) I am familiar with seeing light shown like this: http://upload.wikimedia.org/wikipedia/commons/a/a1/Light-wave.svg"
Is there any way to visualize light in 3D instead of 2D cross sections? Is light a standing wave and does it contain a definite beginning and end point on the wave (does it have a definite length, not wavelength)?
How does light get polarized in the first place, and into circular and elliptical angles? Does the amplitude and intensity of light correspond to the amplitude of the individual photon/wave or is it a property of the sum of the photons/waves of the light?
Technically it is impossible to have infinite extent, although we often approximate things that way. But to answer your question, I'd say that the length of a photon is given by the region where its wavefunction is significant. You can figure out what "significant" means to you.
Polarization is interesting, and has been hit upon already in these messages, but let me add my two cents. In quantum optics, polarization is related to angular momentum. Light has angular momentum, electrons can also have angular momentum depending on the state it is in, and even the nucleus of an atom has angular momentum. Conservation of angular momentum means that when an electron changes from the excited state to ground state, its angular momentum can change, but only if the light carries away that extra angular momentum. Polarization is a characterization of the spin-angular momentum of light, and thus depending on the spin-angular momenta of the two electronic states, you can get different polarizations of light.
For the Hydrogen atom which has only one proton and one electron, the system is simple and the angular momenta of the electronic states can be derived from first principles. Not only that, but by using the rules for quantized angular momenta one can calculate the exact probability that an electron in a particular excited state will decay to a particular ground state and not some other ground state. When I say "some other ground state" or "particular excited state" here, I am referring to the fact that quantum mechanics only allow for specific values of angular momentum (it is quantized), but that the mere presence of the angular momentum means that each energy level can actually have multiple (but finite) degeneracies. To be more concrete, an atom in the ground energy level could be "spin up" (one state) or "spin down" (another state) as an example. Thus in this example there are two possible ground states, each with their own spin-angular momentum.
Anyhow, the short answer to all this is that the polarization for a given photon depends on the change in spin-angular momentum between the two states the electron hops between when the photon is emitted. For simple Hydrogen-like materials the probability for a particular level change can be calculated, but otherwise you are essentially left with random luck. The net polarization for a light beam is a combination of the polarizations for the individual photons.
GRB 080319B said:
5.) I've also seen light shown as loops of electric lines of force: http://www.colorado.edu/physics/PhysicsInitiative/Physics2000.03.99/microwaves/images/fig10.jpg"
I am confused as to how the loop correalates to a wave and why it is expanding. Is the wave increasing in size and if so how?
I have to admit I am not familiar with this particular way of thinking.
GRB 080319B said:
I am struggling to visualize how all these processes are occurring to create light and would appreciate any help. Thank you.
Hopefully some of the above answers help. Although the details are complex, I would try to summarize the generation of light as a consequence of needing conservation of energy and conservation of angular momentum. Quantum mechanics says there are a finite number of energy states an electron can be in. Switching between these states requires a change in energy and angular momentum of the electron, which is balanced by an equal but opposite change which we call a photon. As others have pointed out, a good lesson in quantum mechanics (or at least another thread in these forums) would probably help explain some of the weird effects such as why electrons have a discrete (finite) set of energy levels.