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The stopping power of a medium toward a charged particle refers to the energy loss of the particle per unit path length in the medium. It is specified by the differential -dE/dx, in which -dE represents the energy loss and dx represents the increment of path length. What is of interest to the radiation scientist is the spatial distribution...
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The stopping power of a medium toward a charged particle refers to the energy loss of the particle per unit path length in the medium. It is specified by the differential -dE/dx, in which -dE represents the energy loss and dx represents the increment of path length. What is of interest to the radiation scientist is the spatial distribution...
The bulk of energy deposition resulting from the passage of a fast-moving, charged particle is concentrated in the “infratrack,” a very narrow region extending typically on the order of 10 interatomic distances perpendicular to the particle trajectory. The extent of the infratrack is dependent on the velocity of the particle, and it is defined as the distance over which the electric...
...and Rufus H. Ritchie and independently by Myron Luntz. The region outside the infratrack is beyond the direct influence of the penetrating particle. Energy deposition in this outer region, or “ultratrack,” is due primarily to electronic excitation and ionization by secondary electrons having sufficient energy to escape from the infratrack. In contrast to the infratrack, the...
...power, is numerically equal to the linear energy transfer and changes smoothly to a constant value, called the Fermi plateau, as the ratio β approaches unity. The other half, called the unrestricted stopping power, increases without limit, but its effect at extreme relativistic velocities (those very near the speed of light) becomes small compared with energy loss by nuclear...
...screening, the relativistic stopping power tends to infinity as the electron velocity approaches the speed of light (v/c = β → 1). One-half of the stopping power, called the restricted stopping power, is numerically equal to the linear energy transfer and changes smoothly to a constant value, called the Fermi plateau, as the ratio β approaches unity. The other half,...
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