A hemispherical electron energy analyzer or hemispherical deflection analyzer is a type of electron energy spectrometer generally used for applications where high energy resolution is needed—different varieties of electron spectroscopy such as angle-resolved photoemission spectroscopy (ARPES), X-ray photoelectron spectroscopy (XPS) and Auger electron spectroscopy (AES) or in imaging applications such as photoemission electron microscopy (PEEM) and low-energy electron microscopy (LEEM). It consists of two concentric conductive hemispheres that serve as electrodes that bend the trajectories of the electrons entering a narrow slit at one end so that their final radii depend on their kinetic energy. The analyzer, therefore, provides a mapping from kinetic energies to positions on a detector.
Function
An ideal hemispherical analyzer consists of two concentric hemispherical electrodes (inner and outer hemispheres) of radii R 1 {\displaystyle R_{1}} and R 2 {\displaystyle R_{2}} held at proper voltages. In such a system, the electrons are linearly dispersed, depending on their kinetic energy, along the direction connecting the entrance and the exit slit, while the electrons with the same energy are first-order focused.
When two voltages, V 1 {\displaystyle V_{1}} and V 2 {\displaystyle V_{2}} , are applied to the inner and outer hemispheres, respectively, the electric potential in the region between the two electrodes follows from the Laplace equation:
V ( r ) = − [ V 2 − V 1 R 2 − R 1 ] ⋅ R 1 R 2 r + c o n s t . {\displaystyle V(r)=-\left[{\frac {V_{2}-V_{1}}{R_{2}-R_{1}}}\right]\cdot {\frac {R_{1}R_{2}}{r}}+const.}
The electric field, pointing radially from the center of the hemispheres out, has the familiar planetary motion 1 / r 2 {\displaystyle 1/r^{2}} form
| E ( r ) | = − [ V 2 − V 1 R 2 − R 1 ] ⋅ R 1 R 2 r 2 {\displaystyle |\mathbf {E} (r)|=-\left[{\frac {V_{2}-V_{1}}{R_{2}-R_{1}}}\right]\cdot {\frac {R_{1}R_{2}}{r^{2}}}}
The voltages are set in such a way that the electrons with kinetic energy E k {\displaystyle E_{k}} equal to the so-called pass energy E P {\displaystyle E_{\textrm {P}}} follow a circular trajectory of radius R P = 1 2 ( R 1 + R 2 ) {\displaystyle R_{\textrm {P}}={\tfrac {1}{2}}(R_{1}+R_{2})} . The centripetal force along the path is imposed by the electric field − e E ( r ) {\displaystyle -e\mathbf {E} (r)} . With this in mind,
V ( r ) = E P e R P r + c o n s t . {\displaystyle V(r)={\frac {E_{\textrm {P}}}{e}}{\frac {R_{\textrm {P}}}{r}}+const.}
The potential difference between the two hemispheres needs to be
… excerpt ends here. Continue reading the full article.






