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Outline

Charged- and • Radiation equilibrium Radiation Equilibria • Charged particle equilibrium • Causes of CPE failure Chapter 4 • Transient CPE • Summary F.A. Attix, Introduction to Radiological and Radiation Dosimetry

Introduction Radiation equilibrium • The concepts of radiation equilibrium (RE) and • Consider an extended volume charged-particle equilibrium (CPE) are useful V containing a distributed in relating certain basic quantities radioactive source with a smaller internal volume v • CPE allows the equating of the absorbed dose about a point of interest, P D to the collision kerma Kc and exposure X • Radioactivity is emitted • Radiation equilibrium makes dose D equal to isotropically on average the net rest mass converted to energy per unit • V is required to be large enough so that the maximum distance of penetration d of any emitted ray and its mass at the point of interest progeny (i.e., scattered and secondary rays) is less than the minimum separation s of the boundaries of V and v

Radiation equilibrium Radiation equilibrium • Consider a plane T that is tangent to • Radiation equilibrium (RE) exists for the volume the volume v at a point P´, and the v if the following four conditions exist throughout rays crossing the plane per unit area V (in the nonstochastic limit): • In the nonstochastic limit there will

be perfect reciprocity of rays of each a. The atomic composition of the medium is homogeneous type and energy crossing both ways, b. The density of the medium is homogeneous due to uniform distribution of the c. The radioactive source is uniformly distributed radioactive source within the sphere S d. There are no electric or magnetic fields present to • This will be true for all possible orientations of tangent planes perturb the charged-particle paths, except the fields associated with the randomly oriented individual around the volume v; therefore, in the nonstochastic limit, for each type and energy of ray entering v, another identical ray leaves • This condition is called radiation equilibrium (RE) with respect to v

1 Radiation equilibrium Radiation equilibrium • As a consequence of radiation equilibrium the energy carried in and that carried out of v are balanced for • In non-stochastic consideration the volume v both indirectly and directly ionizing radiation: can be reduced to infinitesimal dv, then RE exists at the point P Rin u  Routu and Rin c  Routc • The energy imparted can then be simplified to • Since D  d  / dm , under condition of radiation equilibrium at a point in a medium, the   Q  absorbed dose is equal to the expectation • Therefore under RE conditions the expectation value value of the energy released by the radioactive of the energy imparted to the matter in the volume v is d material per unit mass at that point, Q equal to that emitted by the radioactive material in v dm 

Radiation equilibrium Radiation equilibrium

• Presence of homogeneous constant magnetic • The concept of RE has practical importance in the and/or throughout V can make fields of nuclear medicine and radiobiology, radiation field anisotropic where distributed radioactive sources may be • RE will still be satisfied if the flow of radiation is introduced into the human body or other balanced biological systems for diagnostic, therapeutic, or analytical purposes • Consider flows of between • The resulting absorbed dose at any given point dv`, dv, and dv``: a+B=A+b depends on the size of the object relative to the • If anisotropy is homogeneous radiation range and on the location of the point everywhere in V, the same balance within the object of flow is held

Charged-particle equilibrium Charged-particle equilibrium

• Charged particle equilibrium (CPE) exists for the • In many practical cases RE condition is not volume v if each charged particle of a given type satisfied, but cab be adequately approximated if and energy leaving v is replaced by an identical CPE condition exists particle of the same energy entering (in terms of • Consider two general situations: expectation values) 1. distributed radioactive sources • If CPE exists, 2. indirectly ionizing radiation from external sources

• RE condition is sufficient for CPE to exist

2 CPE for distributed sources – case 1 CPE for distributed sources – case 2

• For the trivial case of a distributed source emitting • Consider now the case where both charged particles only charged particles, in a system where radiative and relatively more penetrating indirectly ionizing losses are negligible radiation are emitted • The dimension s (the minimum separation of v from • Let the distance d be the maximum range of the the boundary) is taken to be greater than the charged particles only, and distance s > d maximum range d of the particles Distributed source of charged Distributed source of charged particles and () • Conditions a through d are satisfied particles only • If all of the four conditions a - d • Only CPE exists in this case are satisfied, both RE and CPE • RE is not attained since rays exist (they are identical for this case) escaping from the volume v are not replaced, Routu  Rin u

CPE for distributed sources – case 2 CPE for distributed sources – case 2 • The equation for the expectation value of the energy imparted • Now assume that the size of the volume V occupied   R  R  Q  in u  outu  by the source is expanded so that distance s • Since the indirectly ionizing rays are so penetrating increases to being greater than the effective range of that they do not interact significantly in v,  is equal the indirectly ionizing rays and their secondaries to the kinetic energy given to charged-particles by • This transition will cause the (Rin)u term to increase the radioactive source in v, less any radiative losses until it equals (Rout)u in value by those particles while in v • RE will be restored • The average absorbed dose in v is thus D   / m • The energy imparted would be transformed into that for CPE condition for RE:   Q

CPE for distributed sources – case 3 CPE for distributed sources

• A distributed source emitting penetrating • The calculation of the absorbed dose is straightforward for either of these limiting cases indirectly ionizing radiation (CPE or RE) • Achieving CPE will also require that RE is • Intermediate situations are more difficult to deal attained with, i.e., when the volume V is larger than necessary • The following equations are applicable to achieve CPE in v, but not large enough for RE • In that case some fraction of the energy of the R  R R  R  in u  outu and  in c  outc indirectly ionizing radiation component will be absorbed, and it is relatively difficult to determine what that fraction is

3 CPE for indirectly ionizing CPE for indirectly ionizing radiation from external sources radiation from external sources • A volume V contains a smaller volume v • These conditions are similar to those of RE, except for: • The boundaries of v and V are required to be separated by at least the maximum distance of penetration of any secondary – Condition c: uniform field of radiation replaces the uniform charged particle present radioactive source • If the following conditions are satisfied throughout V, CPE – The separation of boundaries of v and V are required to be at will exist for the volume v: least the maximum distance of penetration of any secondary a. The atomic composition of the medium is homogeneous charged particle, rather than that of the most penetrating b. The density of the medium is homogeneous radiation (indirectly ionizing) c. There exists a uniform field of indirectly ionizing radiation – The last condition d has been shown to be a sufficient (rays are only negligibly attenuated passing through the medium) substitute for the requirement of a complete absence of d. No inhomogeneous electric or magnetic fields are present electric or magnetic fields

CPE for indirectly ionizing CPE for indirectly ionizing radiation from external sources radiation from external sources • Analogy with the distributed source case: since the • Homogeneous anisotropy, together with a uniform medium in which the charged particles can slow down throughout V radiation field is uniform, the number of charged (as guaranteed by the first two conditions) is sufficient to particles produced per unit volume in each energy produce CPE for the volume v interval and element of solid angle will be uniform • Example: a simplified case of straight charged-particle • However, since and interactions tracks, all emitted at angle q through identical interactions at generally result in anisotropic angular distributions different points of secondary and scattered radiations, these • Three charged particles e1-e3 will particles are not emitted isotropically as in the case contribute the same kinetic energy as e alone would, if its entire track of radioactive point sources 1 remained inside of v • This anisotropy will be homogeneous throughout V • Thus CPE exists inside of v

Rin c  Routc

CPE for indirectly ionizing CPE for indirectly ionizing radiation from external sources radiation from external sources r Ru  hv1 Since e1 n originated in V; • Relating  tr and  for CPE conditions: Routu  hv2 the resultant radiative loss can non-r R non-r  0 be outside of V  n    R  R  R r out u tr  outu  outu u • However, under those same conditions we may

Under CPE e1 and e2 also assume that any radiative interaction by a are equivalent charged particle after it leaves v will be replaced (4.4b) by an identical interaction inside of v, resulting in

non-r r Routu  Routu  Ru

4 CPE for indirectly ionizing CPE for indirectly ionizing radiation from external sources radiation from external sources • Provided that the volume v is small enough to allow • The derivation of this equation proves that radiative-loss photons to escape under CPE conditions at a point in a n    tr medium, the absorbed dose is equal to the • Reducing v to the infinitesimal volume dv, containing collision kerma there mass dm about a point of interest P, we can write • That is true irrespective of radiative losses d d n  tr • This relationship equates the measurable

dm dm quantity D with the calculable quantity hence under CPE: CPE Kc =  • en/ D  Kc

CPE for indirectly ionizing CPE for indirectly ionizing radiation from external sources radiation from external sources • If the same photon energy fluence  is present in • It is possible for CPE to exist in a volume without media A and B having two different average satisfying all the requirements, a through d, under energy absorption coefficients, the ratio of certain geometrical conditions absorbed doses under CPE conditions in the two • The -collecting region of a free-air chamber media will be given by represents such a situation (Chapter 12)

D CPE K   /  • Another example is the trivial case of a point A  C A  en A source within a volume large enough so the D K B  C B en / B radiation cannot reach the boundary surface, hence no replacement particles are required • Doses DA and DB can differ due to either different atomic compositions A and B, or radiation spectra

CPE in measurement of exposure Ion chamber operation

• Exposure is only defined for x and  rays, X  K c ( e W ) • v must be small enough for air to allow the escape of • This poses a practical difficulty in the measurement of X, I radiative losses since collision kerma (K ) cannot be readily measured by • Corrections must be c II made for larger volumes any direct means • Ionization from I is • The attainment of CPE in an ionization chamber, however, equivalent to II allows the measurement of the ionization collected within a defined volume and mass of air (in place of the ionization produced everywhere by all the secondary that start within the defined volume, as called for by the exposure definition)

5 Relating absorbed dose to exposure Relating absorbed dose to exposure

• It is sometimes useful to know how much • If D is expressed in rads and X in roentgens, absorbed dose would be deposited at some point in air

air as a result of an exposure X CPE • The relationship is indeterminate in the absence of Dair  Kc air  0.876X CPE, since

CPE W  D  K   X   air c air   • This equation is valid only where X is the  e air where the first equality is valid only if CPE exists exposure at the point of interest in air, under at the point in question CPE conditions

Causes of CPE failure in a field CPE failure: Proximity to the source of indirectly ionizing radiation • If the volume V is too close to the source of the There are four basic causes for CPE failure in indirectly ionizing radiation, then the energy an indirectly ionizing field: fluence will be significantly nonuniform within V, a. Inhomogeneity of atomic composition within being larger on the side nearest to the source volume V • Thus there will be more b. Inhomogeneity of density in V particles (e ) produced at c. Non-uniformity of the field of indirectly 3 points like P than particles ionizing radiation in V 3 e at P => more particles d. Presence of a non-homogeneous electric or 1 1 will enter v than leave it magnetic field in V • CPE consequently fails for v

CPE failure: proximity to a boundary CPE failure: proximity to a of inhomogeneity in the medium boundary of inhomogeneity • If the volume V is divided by a boundary between • Consider a case of a beam of MV photons incident on a solid dissimilar media, loss of CPE may result at v, unit-density air-equivalent phantom • The photon beam is not contaminated by secondary electrons since the number of charged particles arriving at v from the photon source or associated hardware will generally be different than would be the case • The absorbed dose D in the for a homogeneous medium phantom first increases steeply up • This difference may be due to a change in to a maximum, then decreases charged-particle production, or a change in the more gradually in a condition range or geometry for scattering of those particles, called transient charged particle equilibrium (TCPE) or a combination of these effects • We temporarily consider TCPE as

being ~ the same as CPE

6 CPE failure: proximity to a CPE failure: High energy radiation boundary of inhomogeneity • As the energy of indirectly ionizing radiation increases, the • The spherical volume V, having radius d equal to the penetrating power of the secondary charged particles increases maximum range of secondary electrons, must contain a faster than the penetrating power of the primary radiation uniformly irradiated homogeneous medium throughout if • For example, a 7% attenuation of -rays would occur in a water TCPE is to be produced at point P layer equal in thickness ( 5 cm) to the maximum range of secondary electrons produced by 10-MeV -rays • If P is too close to the surface, the • The neutron effect is much smaller (1%) at that energy, portion V of V will project out of assuming hydrogen-recoil secondaries the phantom • To replace the solid missing from that volume, a 1000-fold larger volume V of air is required (distance ac=1000ab) • But V is not homogeneousely (nor even completely) irradiated

CPE failure: High energy radiation CPE failure: High energy radiation

• As a result, there is a significant attenuation of • Since the measurements of exposure from x- and - primary radiation over the distance d rays relies on the existence of CPE, exposure • The radiation field is not uniform anymore (failure measurements have been conventionally assumed of condition c in CPE definition) to be infeasible for photon energies > 3 MeV

• CPE fails due to the difference in the number of • However, if some known relationship between Dair charged particles produced and (Kc)air can be attained under achievable conditions, and substituted for the simple equality • Due to attenuation fewer photons that exists for CPE, exposure can still be measured, reach P1 than P3 at least in principle • The number of charged particles • Such a relationship does exist for a situation known generated at P3 is greater than at P1 as TCPE

Transient charged-particle equilibrium Transient charged-particle equilibrium • Case 1: Assume negligible radiative losses from secondary charged particles (Kr  0) • TCPE is said to exist at all points within a region in – Strictly true only for incident neutrons

which D ~ Kc, with the constant of proportionality >1 – In low-Z media (carbon, water, air) Kr = K – Kc <1% of K for photons • Consider two cases of a broad “clean” beam of up to 3 MeV indirectly ionizing radiation (no contamination by • The absorbed-dose curve is rising with depth near the surface as the population of charged particles flowing toward the right charged particles) falling perpendicularly on a slab of is augmented by more interactions of indirectly ionizing rays material: • The dose curve reaches a 1. Negligible radiative losses from secondary charged maximum (Dmax) at the depth particles where the rising slope due to 2. Significant radiative losses; photons are allowed to buildup of charged particles is escape from the phantom balanced by the descending slope due to attenuation of the indirectly ionizing radiation

7 Transient charged-particle equilibrium Transient charged-particle equilibrium

• At a somewhat greater depth rmax, equal to the • For a “clean” beam of indirectly ionizing radiation maximum distance the secondary charged particles starting at the surface can penetrate in the direction of Dmax occurs at approximately the same depth as the incident rays, the D-curve becomes parallel to the where the D-curve crosses the Kc-curve Kc– and K–curves, although all may gradually change • The presence of charged-particle “contamination” slope together with depth in the beam is often observed to shift the depth of

Dmax closer to the surface, where it no longer • D therefore becomes approximates the depth at which D = Kc proportional to Kc, and we say that TCPE exists • Thus one should not assume that D = Kc at Dmax

Transient charged-particle equilibrium Transient charged-particle equilibrium

• Roesch suggest a relationship between the D- and K-curves • Case 2: The case of significant radiative losses from for TCPE conditions, in assumption of no radiative secondary charged particles (such as bremsstrahlung interactions, and ignoring scattered photons: interactions) is similar to the previous one

TCPE TCPE 2   x  D  K e x  K 1 x   • The D-curve bears the same relationship to the Kc- c c  2!    curve, which is moved down by the amount Kr TCPE   Kc 1  x K  Kc  Kr • Here D and Kc are for the same given depth, at which TCPE is required,  is the common slope of the D, K, and Kr  tr  en / tr K Kc curves at that depth; and x is the mean distance the secondary charged particles carry their kinetic energy in the direction of the primary rays while depositing it as dose

Transient charged-particle equilibrium Summary

• Existence of a relationship between D and Kc • Radiation equilibrium under transient CPE conditions is valuable for • Charged particle equilibrium high-energy indirectly ionizing radiations, where CPE may fail • Causes of CPE failure • However, a knowledge of x and the effective • Transient CPE attenuation coefficient  is required for each case, so the equation is not as readily applicable as the

simple equality of D and Kc that exists under CPE conditions

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