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Important Formulas

pyTEMlib


OpenInColab

pyTEMlib , a pycroscopy library

Important Formulas

pyTEMlib

a pycroscopy ecosystem package

Notebook by

Gerd Duscher and Darel Pates

Materials Science & Engineering
Joint Institute of Advanced Materials
The University of Tennessee, Knoxville

Collection of usefull Formulas

'0.2025.12.0'

The formula for relativistic corrected wavelength is: λ=h2meEkin∗(1+Ekin2mec2)\lambda = \frac{h}{\sqrt{2m_e E_{kin} *(1+\frac{E_{kin}}{2 m_e c^2})}}

with

  • h: Planck constant

  • m_e: rest mass of electron

  • EkinE_{kin}: kinetic energy of electron (after acceleration)

  • c: speed of light

wavelength is 4.87 pm for  60 keV
Help on function get_wavelength in module __main__:

get_wavelength(e0: float) -> float
    get deBroglie wavelength of electron accelerated by energy e0 (in eV)

    Parameters
    ----------
    e0 : float
        acceleration voltage in eV
    Returns
    -------
    float
        wavelength in meters

Depth of Focus

The depth of focus is

fdepth≈λα2f_{depth} \approx \frac{\lambda}{\alpha^2}
  • wavelength of the electron λ\lambda

  • convergence angle α\alpha

Depth of focus is 25.08 nm for convergence angle 10.0 mrad at 200 keV

Particle Flux and Current

It is important todetermine the order of magitude of how many electrons are hitting the sample.

The defition of an Ampere:

A=CsA = \frac{C}{s}

That definition is enough to calculate the number of electrons per time unit (flux).

Number of electrons per second for 150.0 pA is 9.36e+08 electrons / second

 at 150.0 pAan electron will hit the sample every 1.07 ns