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The Tutorial X-ray This article criteria meets fcr 1.0 the I of .c A u’ard. To obtain the credit, see questionnaire pp on 45 1-456. T Bushberg, The of the beam. The information quantity After reading tbis article and taking The test, t/,c isms of x-ray . Be scattering, leigh be in imaging and the relative probability of photoelectric interac- various procedures LS a function of the . Be able types, of x-ray the and number absnber. to predict and x-ray . following interaction Auger image dose as use range, photoof atimage appropriate and of contrast the modes is to optimize the the by ac- contrast scattered radiation material and in dedicated and degree quality pair the and production in diagnostic differences in these diagnostic are utility types of the presented but of x-ray inter- examination. do not Ray- occur to any sig- radiography. U INTRODUCTION Understanding of x-ray specific exposure together with ray the interaction kilovolt will of the predominate. to obtain tient Finally, the tissues The imaging and are examination. The objective of this interactions the and highest these for peak), quality a variety x-ray being of reasons. target and imaged, predominant impact on patient dose, utility. An understanding radiologist medical is important (eg, characteristics that a substantial diagnostic dose. interactions parameters Selection filter all affect x-ray the interaction the quality of the radiograph, of these issues enhances the diagnostic types of interactions often the topic for article is to provide mechanisms by which images are some at the fundamental of the physics an overview these lowest to the of x- in turn and ability its ultiof the possible of the various occur. type will pa- understanding portion of the interactions of combinations, types of board of x-ray In addition, x the type exploit the electrons. Understand of each nostic in- characteristic and on the of second- the rays ener- understand radiations eluding the the characteristics ary patient such equipment scattering have mate atomic calculate gies, minimizing photo- which would to predominate tiOflS while techniques to improve nificant flOde energs tissues major and predominant obtain of four influenced energy the imaging to percentage are scattering, are diagnostic are attenuation the the x-ray of attenuation interactions in diagnostic x-ray Imaging the scattering challenges controlling image. absorption, to predict interaction likely the of the by There degree is largely incident Compton The In the Compton the is delivered scattering, in image from recorded. production. composition. and mammography scatter- production. able between actions Compton pair by image successfully involved tissue One quisition the pair removed interactions, photoelectric and mechan- Rayleigh including ing, tenuation. will. the and absorption not (coherent) and mechanisms energy are Rayleigh or fluoroscopic are of the that absorption, electric that content photons interactions: x-ray in a radiograph of x rays information noninteracting predominant Understand PhD diagnostic result electric I Residents Interactions1 Jerrold x-ray reader for credit hour in category tI.)e AAIIA Physician Recognition Physics AAPM/RSNA impact of interaction quality in diag- Index terms: Radiography RadloGraphics 1998; Physics 18:457-468 radiology. ‘From CA 9581. revision the 1)cpartment From requested the ol Radiology. AAPM/RSNA October 22 and School Phvsics received of Medicine. Tutorial at the November University 1996 RSNA 19; accepted of California scientific November l)avis. 231 5 Stockton assembly. 28. Address Received reprint Blvd. September requests Sacramento, 19. 1997: to the author. . RSNA. 1998 457 Scattered photon 1. Figure ing. Rayleigh Diagram dent photon with an tered scatter- shows the atom and photon the being 2 with approximately wavelength. Rayleigh tered photons emitted tion, seat- Incident photon emitted the same seat- are typically in the fairly mci- X1 interacting forward diree- to trajee- close the tory of the incident photon. K, L, and M are electron shells. (Redrawn, with permission, from reference discussions of x-ray of the factors interaction influence the nally, examples tions that can 1 8.) that and x-ray how images are of differences be affect the these presented. in x-ray exploited mode interactions Fiinterac- to enhance utility of a diagnostic examination presented. The specific modes of x-ray clinical tions include Rayleigh scattering, the are interac- Compton the incident photon. This type of interaction has a low probability of occurrence in the diagnostic energy range and typically accounts for less than 5% of x-ray interactions. Rayleigh interactions are also referred to as coherent scattering or classical scattering. During a Rayleigh interaction, the electric field of the electromagnetic wave of the mci- scattering, photoelectric absorption, and pair production. This article discusses the importance of these interactions in medical imaging, some of their characteristics, and their relative probability of occurrence in the energy range of x rays used for diagnostic purposes (ie, the diagnostic energy range). (Further reading on these topics can be found in references 1-8.) dent U RAYLEIGH SCATTERING In Rayleigh scattering, the incident photon interacts with, and “excites, the total atom, as opposed to individual electrons as is common with the other types of x-ray interactions. Because this interaction occurs mainly with very low energy diagnostic x rays, such as those used in mammography (15-30 key), there is no ionization and the scattered photon is emitted with essentially no loss in energy relative to details “ 2 the and atom ting in a photon expends energy, which causes all electrons in the scattering atom to oscillate radiate in phase. The electron cloud of the immediately reradiates this energy, emita photon of the same energy but typically slightly different direction (Fig i). U COMPTON SCAfl’ERING Described by Arthur Compton of Compton by interacting with Imaging & Therapeutic Technology the (3), the factors of occurrence imaging. X-ray scattering do so free or valence shell electrons, in which the incident photon energy greatly exceeds the binding energy of the valence shell electron that is ejected. For example, a iOO-keV photon interacting with a water molecule in soft tissue primarily does so Compton which the binding the water molecules U so-called in i923 and that contribute to its probability are very important to medical photons undergoing Compton through 458 scattering scattering energy (ie, interactions, of the hydrogen in electrons in and oxygen Volume 18 Number 2 Valence electrons Figure 2. ing. Diagram Compton electron dent (Ee.) Compton photon with Angle of deflection are electron ..- . is insignificant compared with the mci- - photon (E1) tive scattermci- energy E() emission of a Compton scattered photon E5 emerging at an angle 8 relative to the trajectory of the incident photon. K, L, and M Scattered -% the interacting with the valence shell electron, which results in the ejection of the Compton ejected electron E and the simultaneous Incident photon (E0) atoms) shows to the incident the incident shells. with permission, enee 8.) photon photon (Redrawn, from is denoted undergoes refer- as 0. Compton dent photon energy. In fact, Compton scattering predominates not only in the diagnostic energy range of x rays in tissue (ie, above 30 key) but continues to predominate well beyond diagnostic energies of x rays (to approximately While 30 The probability of Compton scattering is proportional to the number of electrons per gram. The number of electrons per gram is fairly constant in most materials with the exception of hydrogen, which, because of its lack of neutrons, results in an approximate doubling of electron density. Thus, hydrogenous materi- MeV). When Compton scattering does oc- cur at the lower x-ray energies associated with diagnostic imaging (25- 1 50 kVp), the majority of the incident photon energy interacting with the loosely bound electron is transferred to the scattered photon, which, when detected by the image receptor, contributes to image degradation by reducing the primary photon attenuation differences of the tissues. The components of Compton scattering to keep track of during the interaction are as follows: The incident photon wavelength is denoted as X1 and its energy, as E0. The energy of the Compton electron is denoted as E, whereas the scattered photon wavelength is denoted as X2 with energy equal to The angle of deflection of the scattered photon rela- March-April 1998 scattering, the photon and simultaneously. tening als have resultant Compton scattered ejected (or recoil) electron The process of Compton is illustrated a higher in Figure probability appear scat- 2. of a Compton scat- ten interaction than nonhydnogenous materials of equal mass. However, in radiology, we do not usually compare equal masses. We usually compare regions of an image that correspond to irradiation of adjacent volumes of tissue. Therefore, density-that is, the mass contained within a given volume-plays an important Bushberg U RadioGraphics U 459 role. One can of water glass density radiographically because of the of the ice compared surrounding water Once a Compton the with (Fig ice in a in that of the is ejected from 3). electron kinetic energy through and ionization of atoms in the sunmaterial. The Compton scattered on the other hand, can traverse the medium without interaction or atom, it loses excitation rounding photon, through may visualize differences undergo photon its any of a number of additional including a subsequent interactions, Compton or, if the scattering, photoelectric photon energy is quite :1 absorption, low, Rayleigh scattering. As with and all types momentum energy must of the sum of the and the of interactions, be incident energy conserved. photon of the kinetic both energy Thus, is equal E) scattered of the energy the to the photon ejected Figure 3. Radiograph (acquired at 125 kVp with an antiscatter grid) of two ice cubes in a plastic eontamer of water. The ice cubes can be visualized because of their lower electron density relative to that of liquid water. The small radiolucent objects seen at electron several the locations are the result of air bubbles in water. E: The binding ejected energies We of the can the that convert and electron compared involved, a photon using energy is so small, (i) E5. + Ee_ = U with it can be between its energy that was the other AX(flfl,) the wavelength of volts by equation: As the (2) 1.24i’X. scattered tered more ‘2 AX: These and = X1 + AX. trajectory of the scattered angle 0 of scatter of the an analysis in wavelength incident of energy between (3) photon relative photon. conservation, the ton for incident Derived the and deto the from change Comp- Imaging & Therapeutic Technology are likely thus of the image observability to be increas- receptor of contrast. scattering transferred angle, to the In the energy frac- scattered pho- with increasing incident for higher energy photons, of the scat(Fig is transferred photon the to the Compton scattered electron. For example, at a 60#{176} scattering angle, the ratio of the scattered tron energy E E. is 0.9 or 0. 1 or to that 90% 10% at of the 100 Compton keV but elec- approxi- at 5 MeV. Conservation of energy and momentum tate certain limits on both scattering angle energy transfer. For example, the maximum ergy transfer thus the ton energy) scattered U more receptor, a given Thus, majority increases, direction much exposure of energy energy. are the decreases scatter. 460 (4) electrons forward image overall addition, mately The wavelength pends on the by the cosO). - energy and the the reducing tion photon photons by photon X. (1 photons toward detected ing the The lower energy of the scattered photon relative to the incident photon can alternatively be expressed as the increase in wavelength of the scattered photon relative to the wavelength of the incident photon. Stated another way, the scattered photon wavelength S equal to the incident photon wavelength A plus the change in wavelength be expressed 0.00243 = incident both 4). E(ke) can ignored. in kiloelectron conversion ton scattered photons following equation: to the maximum occurs In fact, photon the Compton electron reduction in incident with (and pho- a 180#{176}photon maximum is limited energy to backof the 5 1 1 keV, Volume dieand en- which 18 Number 2 By using I 00 keV 90 Equation photon to the change 80 is 0.02031 70 thus (2). 60 c a. 20 calculated 0 30 60 90 Scatter Figure Graph ifiustrates as a function 20, 140-keV and normalized to 100%. University in tissue. (Courtesy 180 seatfor curve is M. Boone, School tons. Even of Medicine, Davis.) at a 90#{176} scattering angle and a maxi- mum of 255 keV during a backscatter event. These maximum limits on photon energy are maintained even when extremely high energy photons (eg, therapeutic energy range) interact through a Compton scattering event. The scatten angle for the ejected electron may occur at angle up scattered to 90#{176} and photon backscatter. at any In contrast practically electron will discussed concepts. undergoing outer shell binding energy scattered of the phoejected an of less 80-keV scattering of an oxygen than is previously the is the Compton By substituting of the change March-April maximum ejected an atom with The first a transferred 0 (minimum cited maximal the energy to L shell). incident the state The photon atom with energy of the loss, x-ray the scat- energy photon shell a lower fills is ates vacancy, from cascade levels occurs. leased as either vacancy, in- ex- inner shell. An from a transition is filled energy higher this and energy creating This which higher from The in an atom. After in an ionized binding the stable another energy. is left a vacancy with energetically electrons electron electron.” i80#{176}for K or the nearby pho- with 10 eV. energy the electron question is “What is the minimum energy of the scattered photon,” and the second question is “What that is Equation completely absorbed and the electron is ejected (now referred to as an ejected photoelectron) with a kinetic energy equal to the incident photon energy minus the binding energy of the ejected electron. For photoelectric absorption to occur, the photon energy must be at least equal to or greater than the binding energy of the electron that is ejected. The ejected electron is most likely one whose binding energy is closest to, but less than, scattering of the Consider with teraction, Compton some Compton electron Compton up to a 180#{176} absorbed. involving to reinforce of the energy be locally A problem that angle to the all the presented ton using U PHOTOELECTRIC ABSORPTION Photoelectric absorption is another mechanism of x-ray attenuation important to diagnostic mmaging in which the incident photon interacts with a tightly bound electron (typically one from occurs ton, by nm, energy tered photons still have a relatively high and thus a good probability of detection. Each ofJohn of Radiology, of California, 150 relative Compton of scattering angle photons Department 120 (degrees) Angle 4. ter probability any photon keV remembering added AX of 0.00486 scattered as 61 when - 0 PhD, The 80- of an which, in wavelength nm. Now, wavelength ejected electron is equal to 19 keY (80 keV 61 key). This exercise illustrates an important concept about the energy of the scattered pho- 10 80, the nm, Compton ejected electron is equal to the difference between the incident and scattered photon energies, one can readily see that the kinetic energy associated with the Compton 50 2 (2), is 0.0155 a more crein turn by levels. Thus, an to lower energy difference in energy characteristic x rays is re- or Auger electrons. energy scattered photon) into Equation (4), the in wavelength is equal to 0.00486 nm. 1998 Bushberg U RadioGraphics U 461 1- Binding Energy (keV) 100 keV incident photon Characteristic A:O.6keV(N-’-M) B:4.4keV(M--L) < X3< 22< (L-.-K) C:29keV Figure 5. Photoelectric absorption. Diagram shows a 100-keV photon undergoing photoelectric absorption with an iodine atom. In this case, the K-shell electron is ejected with a kinetic energy equal to the difference between the incident photon energy and the K-shell binding energy of 34 keV or 66 keV. The vacancy created in the K shell results in the transition of an electron from the L shell to the K shell. The difference in their binding energies (ie, 34 and 5 key) results in a 29-keV Ka characteristic x ray. This electron cascade will continue, resulting in the production of other characteristic x rays of lower energies. Note that the sum of the characteristie x-ray energies equals the binding energy of the ejected photoelectrons. Although not shown in this diagram, Auger electrons of various energies could be emitted in lieu of the characteristic x-ray emissions. (Redrawn and modified, with permission, from reference 8.) To conserve transition, energy during characteristic each x rays are electron emitted with an energy that equals the difference between the binding energies of the electrons from the initial and fmal shells. Consider the transition of an electron from the L shell to the K shell in iodine, in which the K-shell binding energy is 34 keV and the L-shell binding energy is 5 keV. A Ka characteristic x ray of 34 5 = 29 keY will be released (Fig 5). The nomenclatune used to identify the characteristic x rays subsequently Auger electron is established istic - U such that the capital letter mdi- Another form of energy dissipation is Auger In this process, the energy that otherwise would appear as a characteristic x ray after an electron transition is transferred to a orbital electron whose binding energy is electron less than that x ray minus characteristic x ray and the binding energy of the from would have a kinetic energy of 29 0.6 = 28.4 keY. Insofar as the electron binding energies of hydrogen and oxygen in tissue are very low and the kinetic energy associated with Auger electrons would be lower than the alternative characteristic x-ray energy, both the character- Imaging M shell to the a indicates electron was & Therapeutic L shell, in which the that the origin of the casthe adjacent M shell. A K, Technology electron. of the ejected. The kinetic energy of the is equal to that of the character- example, as an alternative to a Ka characteristic x-ray emission of 29 keY, that energy may be used to eject an M-shell electron with a binding energy of 0.6 keY within the same atom. The Auger electron the ejected emission. cates the final destination of the cascading electron and the subscript Greek letter indicates whether the transition occurred from an adjacent or nonadjacent shell. For example, an L0 characteristic x ray indicates a transition subscript cading 462 characteristic x ray indicates an electron transition to the K shell from a nonadjacent shell (eg, the M shell). For - Volume 18 Number 2 istic x-ray will be locally photon The benefit that there are tons to and Auger electron an atomic emissions absorbed. of photoelectric no additional degrade the absorption nonprimary image; however, is pho- the local deposition of energy increases the radiation dose in a relatively small area, and this effect must be considered with respect to its impact on dosimetry. The laws of conservation of energy dictate that the sum of the characteristic x-ray and binding Auger electron energy of the energies ejected equals the photoelectron. The probability of Auger electron emission increases as the atomic number (2) of the absorber increases, and thus this process does not occur frequently for x-ray interactions in soft tissue. The probability of photoelectric increases dramatically with the of the absorber (ie, proportional versely, the probability absorption atomic number to Z3). Con- of photoelectric absorp- tion decreases dramatically with increasing incident photon energy (ie, proportional to lIE03). Thus, for a given absorbing material, there is generally a rapid decrease in attenuation as photon energy is increased. However, at photon energies equal to the binding energy of inner shell electrons, there is a rapid and dramatic increase in attenuation. This rapid increase is referred to as an absorption edge, at which point the number of electrons available for interaction dramatically increases, resulting in a rapid rise in the attenuation cross section. The phenomenon of the absorption edge is used in radiographic contrast agents such as iodine and barium. For these materials, the absorption edges of 33 and 37 keY, respectively, create substantially increased values of x-ray attenuation relative to that of surrounding tissues. The high atomic number of these contrast agents also dramatically increases the probability creases wise of photoelectric scattered degrade radiation, the radiograph. absorption which and would In fact, de- other- photo- electric absorption is the primary mode of interaction of diagnostic x rays with screen phosphors, contrast materials, and bone. A problem involving photoelectric absorption is presented to reinforce some of these concepts. Consider a contrast material A with March-April 1998 number of 25, which with 50-keV photons, terial B with an atomic is irradiated and another contrast ma- of 50, which is irradiated with 100-keY photons. What is the probability of photoelectric absorption in material A relative to material B for the same thickness of material? Because the probability of photoelectric absorption is proportional to Z3/ E03, the probability of photoelectric absorption with respect to atomic number changes as the ratio of (25/50) = ‘/8 or 0. 125. The probability of photoelectric absorption with respect to photon energy changes as i/(50/iOO)3, which is equal to 8. Thus, the overall effect of a decrease to one-eighth number in photoelectric absorp- tion probability for a material of lower atomic number, combined with an eightfold increase in photoelectric absorption probability associated with the lower-energy photons, results in no net difference in the probability of photoelectric absorption. At photon energies below 50 keV, the photoelectric process plays an important role in imaging soft tissue. The photoelectric absorption process can be used to amplify differences in attenuation between tissues with slightly dif- ferent atomic contrast. knowledge ploited numbers, An excellent thus of differential to improve improving example absorption subject contrast mammography. The development of the tube targets and molybdenum cated mammography subject of how this can be is seen ex- in molybdenum x-ray filters for dedi- systems is a case in point. Characteristic x rays of i7 and 19.5 keV are produced in the output energy spectrum of the x-ray tube. The tube port, which is made of beryllium, has low atomic number (Z = 4) to al- low essentially all the photons of importance to be transmitted. Unfortunately, a preponderance of low-energy photons (<1 5 key) are simply absorbed in the breast and a preponderance of high-energy photons (>20 key) reduce the subject contrast. Use of a molybdenum filten (typically 25-30 im thick) allows the preferential transmission of the desired characteristic x rays because their energies are just below Bushberg U RadioGraphics U 463 Relative Photon Intensity 1E 6 I 1.1 2 0iL Photon Mass attenuation coeffIcient Energy spectrum Mo target I (keV) Mass attenuation Molybdenum - 30 kVp unfiltered Bremsstrahlung - Aluminum coefficient srna 80 (cm/gm) 60 (cm2! \j< 40 2: gm) 0 Photon Energy (key) Photon Energy 3 3 with 0.03 mm Mo filter Mo target (keV) Mo target with 0.5 mm Al filter 4 Relative Intensity . - 10 15 Photon absorption ray photons edge. are gies just beyond creased attenuation sorption reduces --_-__. 25 (key) 30 35 energies, absorbed, and, the x- at ener- K-absorption edge, indue to photoelectric abthe transmission of higherenergy photons through the filter. A pseudomonoenergetic spectrum is thus achieved; this spectrum maximizes the subject contrast of the soft tissues of the breast with a minimal radiation dose. Aluminum is the material most commonly used for x-ray applications, of the transmission quently shows results in suboptimal allowing of high-energy photons is illustrated in subject with at- increased and contrast a mammography conse- (Fig 6). 20 25 30 Energy (key) at 30 kVp, with filter directly that was 35 attenuation curves and below on the left and imaged with both molybde- mammograms of the same spec- breast oh- tamed approximately 10 years apart. The change in imaging techniques over the period results in substantial improvement in subject contrast. The mammogram obtained in the early 1980s used 30 kYp. The higher effective energy, pression spectrum, 15 Photon and aluminum filters (Fig 7). The clinical impact of the x-ray energy trum can also be seen in Figure 8, which is used for mammography. edge of aluminum is not at of interest for mammographic in radiography; 10 num of the a reduction effect phantom how- filters which tenuation This the tube ever, molybdenum The K-absorption the energy range 5 of an unfiltered molybdenum (Mo) target molybdenum filter and a 0.5-mm aluminum with permission, from reference 8.) At lower readily Intensity 20 Energy Figure 6. Output spectrum filtered spectra for a 0.03-mm right, respectively. (Redrawn, the Photon I - . 5 Relative Ii 2 Photon together era and resulted with absence screen-film technology of “substantial” in reduced subject comcontrast 8a). The contemporary mammogram was obtained with 26 kYp. A lower tube voltage and more accurate automatic exposure control results in a energy spectrum “tuned” to provide a beam of lower effective energy (Fig 8b). A (Fig substantial improvement in subject and radio- by enhancements in screen-film technology, such as increasing the gradient of the characteristic curve response of the film and greater breast compres- graphic contrast is achieved sion. 464 U Imaging & Therapeutic Technology Volume 18 Number 2 a. Figure merized b. 7. Images methyl of an American methacrylate (Lucite) College were of Radiology obtained mammography with target and molybdenum filter (a) and with a molybdenum provement in subject contrast for the calcification specks the test phantom is readily evident in a. test phantom a mammography unit with target and aluminum and other test objects made of poly- a molybdenum filter (b). embedded The imwithin Figure 8. Mammograms of the same breast imaged 10 years apart. (a) Mammognam acquired with a mammography unit with a three-phase six-pulse generator (CGR Sentograph 500T; GE Medical Systems, Milwaukee, Wis) at 30 kVp and a Min-R screen with Ortho M film (Eastman Kodak, Rochester, NY) demonstrates the image quality resulting from older imaging techniques, including higher effective energies, film with lower contrast and lower speed, and minimal breast cornpression. (b) Mammogram acquired 10 years later with a mammography unit with a high-frequency generator (CGR Sentograph 600HT; GE Medical Systems) at 26 kVp and a Kodak Min-R screen with Microvision film (Du Pont, Wilmington, Del) demonstrates greater subject contrast and was obtained at lower dose. The much improved image was produced with a lower effeetive energy x-ray beam, higher speed screen-film technology, and better breast compression. (Modified, with a. March-April permission, from reference 8.) b. 1998 Bushberg U RadioGrapbics U 465 The photoelectric when lower energy terials of high diagnostic process photons atomic energy predominates interact with number range, (Fig the ma- photoelectric pro- PRODUCTION converted namely a high-energy into the -U U .b 0 P. 20 C.) 0 B 50i . Cl) 0 2 a. Inpalrproductlon, den the influence Nuclear Medicine 9). In the cess predominates in materials such as lead used in protective aprons, contrast agents, and the sodium iodide in the crystals used in gamma scintigraphic cameras. Conversely, Compton scattering wifi predominate at higher photon energies with materials of lower atomic numbers such as tissue and air. U PAIR Diagnostic Radiology photon, of the atomic a matter electron and un- nucleus, antimatter pair, The andpositron. is keV thresh- old photon energy required for this interaction is 1 .02 MeV, which is equal to the rest mass energy equivalent of the positron-electron pair. Figure 9. Graph plots tion of the photoelectric the (right processes The sues electron loses its energy kinetic through and ionization and becomes ated with another atom or is eventually sorbed into the free electron pool. The tron (a form of antimatter) also loses its excitation energy by is much excitation and different than positron will eventually tron in an annihilation of the combine reaction, ab- posiits fate electron. The with an elecin which the rest mass energy of the positron-electron pair is completely converted into electromagnetic radiation in the form of two 51 1-keV photons. These photons, to one another, attenuation emitted at approximately 180#{176} are referred to as annihilation and MeY. After cay. a pair production The resultant required for pair pair production U CONCLUSIONS Four types of x-ray unless viewed: high does not energies of 1 .02 scattering energies energies become greatly MeY. In fact, significant exceed the minimum As previously stated, predominates and the beyond in tissue up photon energy Compton at diagnostic to approximately tis- in excess the extremely to occur. for various reaction, any enof 1 .02 MeY is distributed as Idnetic energy to the positron-electron pair. Positrons, however, are important in nuclear imaging, as certain types of radioactive materials emit positrons as a form of radioactive deergy ted from the tron emission production and Compton as a function of energy. When diagnostic energy photons interact with materials of low atomic number (eg, soft tissues), the Compton process dominates. (Redrawn and modified, with permission, from reference 8.) are illustrated in Figure 10. The process of pair production is of no consequence in diagnostic radiography because of radiation of contnibu- scale) kinetic but ionization, that associ- scale) percentage (left 30 annihilation patient can tomographic Rayleigh radiation emit- be detected by posi(PET) scanners (4). interaction scattering, have been Compton photoelectric absorption, and pair tion. As one can see from the summary attenuation coefficients in soft tissue as tion of energy (Fig 1 1), pair production not contribute substantially to the types ing, teractions important in the energy re- scatterproducof mass a funcdoes of in- range used in diagnostic radiology. Photoelectric absorption is an important process in diagnostic studies in which contrast agents are employed because 466 U Imaging & Therapeutic Technology of the high atomic number of the Volume 18 Number 2 n and incident photon (Negation) A (Positron) Annihilation 4rMe”H800 Radiation B 10. Pair production. Diagram illustrates the pair production process in which a high-energy incident photon, under the influence of the atomic nucleus, is converted to a matter and antimatter pair. The electron expends its kinetic energy by excitation and ionization as does the positron. However, when the positron comes to rest, it combines with an electron, producing the two 51 1-keV annihilation radiation photons. K, L, and M are electron shells. (Redrawn, with permission, from reference 8.) Figure 10 E U 3 C 0 U 1 /TOt1 0 0 U \ C 0 0 ,.-.- Photoelectric C 1m...I..uI.__ Compton Rayleigh<1 < U) 0.01 Pair .. 0.003 0.001 10 100 N Energy March-April 1998 Figure Rayleigh, 1,000 (keV) 10,000 11. Graph the Compton, and total mass at- pair production, tenuation coefficients (Z 7) as a function Bushberg plots photoelectric, U for soft tissue of energy. RadioGraphics U 467 absorber. It is also important in special applications such as mammography, in which the photoelectric absorption process aids in the ability to amplify subtle differences in tissue attenuation. Compton scattering interactions predominate energy contrast tissue over the majority of the range in soft tissue is chiefly derived density. Detection Acknowledginent ofJ. Anthony Seibert, the 1996 AAPM/RSNA are greatly in which subject from differences 1 . Anderson DA. Absorption of ionizing radiation. Baltimore, Md: University Park Press, 1984. 2. Evans RE. The atomic nucleus. Malabar, Fl: Knieger, 1982. 3. Compton MI. A quantum theory of the scattering of x-rays by light elements. Phys Rev 1923; in scattered photons by the image receptor results in a loss of radiographic contrast. An understanding of how these interactions occur and their effects on subject contrast and 21:483. 4. Votaw dose allow one to control the imaging acquisition variables and x-ray production equipment to yield the best possible diagnostic mnformation at the lowest possible patient dose. Furthen reading on this and related topics can be found in several excellent texts in medical physics 5. JR. Physics of PET. RadioGraphics 15:1179-1190. Hendee WR, Ritenour ER. Medical imaging This (5-8). 468 U Imaging article meets To obtain & Therapeutic the credit, criteria see for the 1.0 credit questionnaire Technology hour 1995; physics. 3rd ed. St Louis, Mo: Mosby-Year Book, 1992. 6. Sprawls P Jr. Physical principals of medical imaging. 2nd ed. Gaithersburg, Mo: Aspen, 1993. 7. Bushong SC. Radiologic science for technologists: physics, biology, and protection. 6th ed. St Louis, Mo: Mosby, 1997. 8. Bushberg JT, Seibert JA, Leidholdt EM, Boone JM. The essential physics of medical imaging. Baltimore, Awara appreciated. U REFERENCES diagnostic of Compton The comments and suggestions PhD, who served as chair for Physics Tutorial for Residents in category on pp Md: I of the AMA Williams Physician & Wilkins, 199-I. ‘s Recognition 45 1-456 Volume 18 Number 2