Bethe formula

For a particle with speed v, charge z (in multiples of the electron charge), and energy E, traveling a distance x into a target of electron number density n and mean excitation energy I (see below), the relativistic version of the formula reads, in SI units:[2]

${\displaystyle -\left\langle {\frac {dE}{dx}}\right\rangle ={\frac {4\pi }{m_{e}c^{2}}}\cdot {\frac {nz^{2}}{\beta ^{2}}}\cdot \left({\frac {e^{2}}{4\pi \varepsilon _{0}}}\right)^{2}\cdot \left[\ln \left({\frac {2m_{e}c^{2}\beta ^{2}}{I\cdot (1-\beta ^{2})}}\right)-\beta ^{2}\right]}$

(1)

where c is the speed of light and ε₀ the vacuum permittivity, ${\displaystyle \beta ={\frac {v}{c}}}$, e and m_e the electron charge and rest mass respectively.

Stopping Power of Aluminum for Protons versus proton energy, and the Bethe formula without (red) and with corrections (blue)

Here, the electron density of the material can be calculated by

${\displaystyle n={\frac {N_{A}\cdot Z\cdot \rho }{A\cdot M_{u}}}\,,}$

where ρ is the density of the material, Z its atomic number, A its relative atomic mass, N_A the Avogadro number and M_u the Molar mass constant.

In the figure to the right, the small circles are experimental results obtained from measurements of various authors, while the red curve is Bethe's formula.[4] Evidently, Bethe's theory agrees very well with experiment at high energy. The agreement is even better when corrections are applied (see below).

For low energies, i.e., for small velocities of the particle β << 1, the Bethe formula reduces to

${\displaystyle -{\frac {dE}{dx}}={\frac {4\pi nz^{2}}{m_{e}v^{2}}}\cdot \left({\frac {e^{2}}{4\pi \varepsilon _{0}}}\right)^{2}\cdot \left[\ln \left({\frac {2m_{e}v^{2}}{I}}\right)\right].}$

(2)

This can be seen by first replacing βc by v in eq. (1) and then neglecting β² because of its small size.

At low energy, the energy loss according to the Bethe formula therefore decreases approximately as v⁻² with increasing energy. It reaches a minimum for approximately E = 3Mc², where M is the mass of the particle (for protons, this would be about at 3000 MeV). For highly relativistic cases β ≈ 1, the energy loss increases again, logarithmically due to the transversal component of the electric field.

The mean excitation energy I of atoms, versus atomic number Z, in eV, divided by Z

In the Bethe theory, the material is completely described by a single number, the mean excitation energy I. In 1933 Felix Bloch showed that the mean excitation energy of atoms is approximately given by

${\displaystyle I=(10~\mathrm {eV} )\cdot Z}$

(3)

where Z is the atomic number of the atoms of the material. If this approximation is introduced into formula (1) above, one obtains an expression which is often called Bethe-Bloch formula. But since we have now accurate tables of I as a function of Z (see below), the use of such a table will yield better results than the use of formula (3).

The figure shows normalized values of I, taken from a table.[5] The peaks and valleys in this figure lead to corresponding valleys and peaks in the stopping power. These are called "Z₂-oscillations" or "Z₂-structure" (where Z₂ = Z means the atomic number of the target).

The Bethe formula is only valid for energies high enough so that the charged atomic particle (the ion) does not carry any atomic electrons with it. At smaller energies, when the ion carries electrons, this reduces its charge effectively, and the stopping power is thus reduced. But even if the atom is fully ionized, corrections are necessary.

Bethe found his formula using quantum mechanical perturbation theory. Hence, his result is proportional to the square of the charge z of the particle. The description can be improved by considering corrections which correspond to higher powers of z. These are: the Barkas-Andersen-effect (proportional to z³, after Walter H. Barkas and Hans Henrik Andersen), and the Felix Bloch-correction (proportional to z⁴). In addition, one has to take into account that the atomic electrons of the material traversed are not stationary ("shell correction").

The corrections mentioned have been built into the programs PSTAR and ASTAR, for example, by which one can calculate the stopping power for protons and alpha particles.[6] The corrections are large at low energy and become smaller and smaller as energy is increased.

At very high energies, Fermi's density correction[5] has to be added.

• Stopping power (particle radiation)
• Landau distribution
• Hans Bethe

• The Straggling function. Energy Loss Distribution of charged particles
• Original Publication: Zur Theorie des Durchgangs schneller Korpuskularstrahlen durch Materie in "Annalen der Physik", Vol. 397 (1930) 325 -400
• Passage of charged particles through matter, with a graph
• Stopping power for protons and alpha particles
• Stopping Power graphs and data
• Recent numerical solutions