Is energy exchange quantized? In the photoelectric effect there is a threshold frequency that must be exceeded, to observe any electron emission, I have two questions about this.
I) Lower than threshold:
What happen with lesser frequency/energy photons? I mean there is no energy transferred? If some energy were transferred, (and it must be transfered quantized), how can be experimentally known it was quantized, if there is no electron emission?
II) Intensity dependence: There is any known dependency with intensity? (I mean a dependency not about the number of electrons (I am already aware of this) but about the energy of them) I thought energy of electron emited was independent with intensity, but then I found this link dependency with intensity (is a paper to buy that I haven't read) but relates energy with intensity.
 A: Energy exchange is quantized when moving a electron from one bound state to another bound state.
This isn't because the exchange is inherently quantized, but because the states the electron may occupy are quantized.
Thus the standard photo-electric effect in which a photon can not excite an atom unless it has a minimum energy.

However,...
There are multi-photon processes by which sub-threshold light can excite transitions. 
Cross-section for them go by intensity-squared (or worse) and are very small for any reasonable light intensity. To study or employ them you get powerful, short pulsed laser systems. Where short pulsed means nano-second or faster pulses and powerful means "Do not look into beam with remaining eye". Even then you don't get a lot of rate.
These processes are utterly negligible for the kind of benchtop experiment we use to teach the photoelectric effect: you just can't get enough intensity. (See below for how negligible.)
The conceptual model here is that the first photon bumps the electron to a short-lived, unstable state without well defined quantum numbers, and the second comes along before that state decays and finishes the job. 
We're currently exploring the application of such a process to calibrating light yields, opacities in a large volume of scintillating material.

From New J.Phys.12:113024, 2010:

For gases the one-photon absorption cross-section $\sigma_1$ is typically of the order of $10^{−17}\text{ cm}^2$, 
  whereas the two-photon and the three-photon cross-sections are of the order of 
  $\sigma_s = W/F_2 \approx 10^{−50}\text{ cm}^4\text{ s}$ 
  and 
  $\sigma_3 = W/F_3 \approx 10^{−83}\text{ cm}^6\text{ s}^2$, 
  respectively.

Where $F$ is intensity in photons/second and W is excitation rate in reciprocal seconds.
A: If the frequency of the incident radiation is lower than the threshold frequency then either a photon is fully absorbed or not absorbed at all. It is absorbed only if it has an energy which is just enough to excite the electron to the higher state but not enough (less than the work  function) to make the electron to leave the surface of the material.
The only way we know that the energy of the electron is quantized in an atom is by analyzing its spectrum.
For a particular frequency above the threshold, the number of the electrons emitted will linearly increase with the intensity of the incident radiation.
A: MC Physics would counter that kinetic energy transfers are fully quantized in every transaction. If the photon has insufficient KE to cause a lowest bound electron to be emitted from an atom, it causes, at least, an increase in vibration of that atom which emits photons (seen as heat). Those emitted photons then transfer to nearby atoms (seen as heat transfer or heating of the material).
If the KE of an absorbed photon is sufficient to cause an atom to emit its lowest bound electron, then it will. The absorbed photonic mono-charges may or may not be emitted. 
The intensity of the light (photon count rate) follows the same rules, but with increased temperature effect on the internal vibration and electron bondings.
