Alvl P1: energy levels and particles of light(ch3) Cheat Sheet by MostAncientDream

a fluore­scent covered tube with mercury vapour inside.

process:

1. thermonic emission to raise electrons to the surface
> energy has to be equal to or greater than the energy gap between energy levels to interact

2. potential difference is applied (V = w/q) so work is done on the electron to accelerate it across the tube

3. electrons will collide with mercury vapour causing excitation (risk of electron capture however unlikely due to mercurys stability)
> electrons will continue to interact even after a single intera­ction as the field continues to accele­ctrate them

4. electrons dexcite, releasing energy certain frequency

5. mercury vapour has small wavelength photons (discrete) of light released in any direction

6. this causes the photon to interact with the phosph­orous which must have the exact energy gap
> small wavelength = large energy

7. most of the phosporous energy levels are visible light spectrum, it has fluoresced
> absorb short, release long wavelength

questions possibly answered:
- how does the fluore­scent tube worked
- why is mercury vapour used
- what does the phosph­orous do
- do the electrons continue to interact after intera­cting once

electron diffra­ction is evidence for wave behaviour.

-as an electron passes through a diffra­ction grating the electron wave spreads out/is diffra­cted.
-an interf­erance pattern is produced, bright rins at where maximum intensity occurs­/in­terfere constr­uct­ively


working out velocity of an electron from an electron gun:

- cathode(-) fires electrons through an anode(+) grating
- there is a potential difference between the cathod­e/anode known as the accele­rating voltage

V = E/Q so E = eV (e is Q)
eV (energy) = 1/2mv²
and rearrange for v

v = square root(2­eV/m)

this can be substi­tuted into de broglie wavelength equation

- when an electron gains energy via a photon, if the photon contains the correct amount of energy for the energy level, an electron will excite to the next energy level
- (if it had enough energy to ionise it becomes a free electron)
- (if it did not have enough energy to get to the next energy level then the photon passes through the atom without intera­cting)

- the electron is now in an unstable state

- to overcome this the electron will eventually de-excite (return to the energy level) and release a corres­ponding photon in the process

an atom could have absorbed a singular photon to excite multiple energy levels.

as it dexcites and releases energy this can be in the form of multiple photons.

for example:

if a photon excites an electron 2 energy levels, then when it dexcites it can either go
n=3 > n=1 (with the corres­ponding energy differ­ence)
or
n=3 > n=2 > n=1

Absorption spectrums:
- these look like rainbom bars with black lines vertically across them

black lines > freque­nci­es/­wav­ele­ngths absorbed


Emission spectrums:
- these look like black bars with single coloured lines vertically across them

coloured line > emitted freque­ncy­/wa­vel­ength


** you should expect more lines on the emission spectrum as there is more paths it can take per photon absorbed when dexciting

photoe­lectric effect:

light is modelled as photons (~discrete packets of energy)
E = hf

if wave theory was correct then the surface electrons should be liberated with any f of light so long as its bright enough

when surface electrons are liberated from the surface, they have Ek.

it is a 1-1 intera­ction
- higher intensity does not equal Ek max
- 1 photon absorbed by 1 electron

- to measure the Ek set up an excavated tube with metal plates on either side connected to a battery.
- turn up the voltage on the battery until no electrons reach the other plate (the ammeter will read 0)
- this is the stopping potential (Vs)

V = E/Q > Vs = Ek/e > Ek max = eVs
(Ek max is electrons liberated from surface)

Graphs:

Ek max - f graph
y = mx +c
into
Ek max = hf - work funtion (always a negative)
the x intercept is the threshold frequency