Bethe Feynman Formula BetheBloch Formula Hans Bethe Wiki Hans Bethe Contributions to Science BetheBloch Aimee Blaut BetheBloch Equation Electron Stopping Power
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In nuclear physics and theoretical physics, charged particles moving through matter interact with the electrons of atoms in the material. The interaction excites or ionizes the atoms. This leads to an energy loss of the traveling particle. The Bethe formula describes^{[1]} the energy loss per distance travelled of swift charged particles (protons, alpha particles, atomic ions, but not electrons^{[Footnote 1]}) traversing matter (or alternatively the stopping power of the material). The nonrelativistic version was found by Hans Bethe in 1930; the relativistic version (shown below) was found by him in 1932 (Sigmund 2006).
The Bethe formula is sometimes called "BetheBloch formula", but this is misleading (see below).
For a particle with speed v, charge z, and energy E, traveling a distance x into a target of electron number density n and mean excitation potential I, the relativistic version of the formula reads:^{[citation needed]}

( 
where c is the speed of light and ε_{0} the vacuum permittivity, β = v/c, e and m_{e} the electron charge and rest mass respectively.
Here, the electron density of the material can be calculated by
where ρ is the density of the material, Z its atomic number, 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 (taken from http://www.exphys.unilinz.ac.at/Stopping/). The red curve is Bethe's formula. 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^{[citation needed]}

( 
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 = 3Mc^{2}, 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.
In the Bethe theory, the material is completely described by a single number, the mean excitation potential I. In 1933 Felix Bloch showed that the mean ionization potential of atoms is approximately given by

( 
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 BetheBloch 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.^{[2]} The peaks and valleys in this figure lead to corresponding valleys and peaks in the stopping power. These are called "Z_{2}oscillations" or "Z_{2}structure" (where Z_{2} 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 BarkasAnderseneffect (proportional to z^{3}, after Walter H. Barkas and Hans Henrik Andersen), and the Blochcorrection (proportional to z^{4}). In addition, one has to take into account that the atomic electrons are not stationary ("shell correction").
These corrections have been built into the programs PSTAR and ASTAR, for example, by which one can calculate the stopping power for protons and alpha particles.^{[3]} The corrections are large at low energy and become smaller and smaller as energy is increased.
At very high energies, Fermi's density correction^{[2]} has to be added also.
In describing programs PSTAR and ASTAR, the National Institute of Standards and Technology^{[3]} calls formula (1) "Bethe's stopping power formula".
On the other hand, in the 2008 Review of Particle Physics^{[4]} the formula was called "BetheBloch equation", even though Bloch's expression (3) did not appear in the formula. As of the most recent edition, this seems to have disappeared with the formula being called only the "Bethe formula".^{[5]}
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