Electron-Matter interaction Flashcards
Why electrons allow for better resolution than light?
They can also be used for imaging because of wave particle duality. From Do Broglie relation you can find the wavelength of an accelerated photon. For a 1kV, it is 0.03nm => diffraction limitation is not a problem at all since atoms are like 0.1nm.
What is the wavelength/velocity of an electron in a 1 kV electron microscope?
Electron mass: me = 9.10938356 × 10−31 kg
Electron charge: e = 1.6021766208 × 10−19 C
Planck constant: h = 6.626 x 10-24 m2 kg s-1
1J = 1 kg m2 s-2
E = eU = mv^2/2
=> v = sqrt(2eU/m)
=> lambda = h/mv = h/sqrt(2meU) = hc/sqrt(2mc^2[eV]*E) = 0.04 nm
Describe the different types of electron scattering possible!
- elastic backscattered => high energy/coherent, with preserved energy and phase of the incident electron beam
-inelastically backscattered: also referred to as incoherent, they would ave collided with electrons(see the same for the scattered) - transmission: no interaction
- elastically scattered: they are only deflected but preserve energy and phase
- inelastically scattered: energy is lost/transmitted to a secondary electron which then has low energy compared to the scattered electron. In addition higher shell electron would then fall to the lower orbital state resulting in X-ray photons.
Interaction cross section
doesnt really represent area but the probability of scattering event.
𝜎𝑎𝑡𝑜𝑚 = 𝜋𝑟2
where r is the effective radius of the atom/the matter that the electron will interact with.
A higher r would thus mean that a bigger interaction cross section is present meaning more electron scattering events can occur
Formula for interaction cross section effective radius
Hint: think of the factors that influence this process
The factors are:
1. The atomic number, heavier atoms generally deflect electrons more strongly since they have bigger atom nucleus charge
2. Incident beam voltage: electrons scatter less strongly for higher voltage
3. Scattering into high-angles is less likely since it requires less momentum/energy transfer.
Thus taking all of this into account we get the following formula.
𝑟𝑒𝑙𝑎𝑠𝑡𝑖𝑐 = 𝑍𝑒/𝑈𝜃
Solid angle of scattering
measure of the “spread” of scattering directions
Ω = 2𝜋(1 − 𝑐𝑜𝑠𝜃)
Total scattering cross section
𝜎𝑡 = 𝑁𝜎𝑎𝑡𝑜𝑚 = 𝑁𝜋𝑟2, 𝑁 = 𝑁A * 𝜌/𝑚𝑎
Why do we observe more scattering at high angles for Au foil compared to Cu one?
higher Z
Mean Free path
Mean free path = distance between two scattering events
Λ = 1/𝜎𝑡 = 𝑚𝑎 / (𝑁𝐴𝜎𝑎𝑡𝑜𝑚𝜌)
What are the most commons scattering events?
Plasmon and elastic scattering
events account for the majority
of total scattering cross section.
Why is backscattering more likely if the electron passes close to the nucleus?
The closer it passes the higher pull by the nucleus => deflection angle becomes close to 180 => backscattering
Plasmons and Plasmon scattering
plasmon is a quasiparticle that represents the collective oscillation of free electron density in a material, typically a metal, in response to an external electromagnetic field
When electrons pass through a material, they can excite plasmons, which leads to energy loss. This loss can be measured and analyzed in electron energy loss spectroscopy
Auger scattering
Auger scattering refers to a process in which an atom, excited by the removal of an inner-shell electron, undergoes a series of electron transitions that result in the ejection of a secondary electron, known as an Auger electron. This process, named after the French physicist Pierre Auger, occurs without the emission of an X-ray photon, which would be typical in X-ray fluorescence following inner-shell ionization.
electron interaction volume
the region within a material where incoming electrons interact with the atoms in the sample, undergoing various scattering and energy-loss processes.
When can secondary electrons (SE) be formed?
SE1: SEs directly generated by primary electrons
SE2: SEs generated by BSEs leaving the sample
SE3: SEs generated by BSEs hitting objects in the
vacuum chamber