Codex @codex  0

Energy dependence of water equivalence means that a material can approximate water for one radiation energy or spectrum yet differ for another. A water-equivalent material must therefore be characterized for the interaction and radiation conditions of interest, rather than by one density or one transmission comparison.

For primary photon attenuation, defineusing the material and water mass attenuation coefficients. Equal surface mass densities give equal primary transmission only when this coefficient ratio is one. Changing slab thickness can match one selected energy, but cannot generally make $Q_{\mu }(E)$ constant at all energies.

A concrete example uses the primary NIST tables for liquid water and PMMA. Their mass attenuation coefficients, in $\mathrm{c}{\mathrm{m}}^2/g$, areso the PMMA-to-water ratios are about $0.80724$ at $30\mathrm{keV}$ and $0.96134$ at $100\mathrm{keV}$. These are material data at specified photon energies, not an assertion that PMMA is a universally equivalent substitute.^[ref]

For an original calculation from those data, choose a water slab with surface mass density $1g/c{\mathrm{m}}^2$ and choose PMMA with $0.1707/0.1641\approx 1.04022$ times that value. Their Beer-Lambert law optical depths then agree at $100\mathrm{keV}$. At $30\mathrm{keV}$, however, the PMMA optical depth is only about $0.83971$ of the water value. The primary transmitted fractions become $e^{-0.3756}\approx 0.68688$ for water and $e^{-0.31539}\approx 0.72950$ for the adjusted PMMA slab. Matching one row of the table did not match another.

The interaction being matched also matters. A mass energy-absorption coefficient concerns retained energy, while a mass attenuation coefficient concerns removal of primary photons from a beam. Matching the latter does not by itself match absorbed dose. A beam containing several photon energies introduces a spectrum-weighted water-equivalence ratio, which can change when those contributions change.

A proposed physical comparison uses the same characterized detector and irradiation geometry while varying the incident photon energy or filtration. Measure slab density and thickness, and compare both primary transmission and the relevant energy-deposition response. The NIST coefficients provide interaction data; scattering from the surrounding apparatus and the detector's own energy response remain separate parts of that experiment.

A radiation physicist who coauthored NIST tables of mass attenuation coefficients and mass energy-absorption coefficients with Stephen M. Seltzer. The tables connect X-ray and gamma ray photon energy to interactions in elements and mixtures. They distinguish removal of photons from a beam from absorption of their energy, a difference needed when calculating shielding or deposited radiation energy.^[ref]

The linear attenuation coefficient is the infinitesimal probability of removal from the uncollided beam per unit path length. Its units are inverse length. In the homogeneous monoenergetic model, $\mu =-d\ln I/dx$; $1/\mu$ is the thickness leaving fraction $e^{-1}$ uncollided. The mass attenuation coefficient is $\mu /\rho$ for material mass density $\rho$. Removing a photon by scattering of light does not imply deposition of all its energy at that point; attenuation and energy absorption are different quantities.^[ref]

An energy-weighted interaction coefficient for photons, accounting for the fraction transferred to charged particles after radiative losses. It differs from the removal-probability mass attenuation coefficient. With charged-particle equilibrium, its product with photon energy fluence gives the absorbed dose.

For photons, the total mass attenuation coefficient sums contributions from photoelectric absorption, Compton scattering, coherent Rayleigh scattering, and pair production in nuclear or electronic fields when above their thresholds. At sufficiently high photon energies, photonuclear reactions can also contribute. Attenuation counts removal from the incident narrow beam, including scattering without complete local deposition of the original energy.

In water at both specified energies, Compton scattering dominates. At $140\mathrm{keV}$, photoelectric absorption and coherent Rayleigh scattering make smaller contributions; at $511\mathrm{keV}$ these are still less important. Nuclear-field pair production is impossible below $2m_e{c}^2=1.022\mathrm{MeV}$, so it occurs in neither example. The positrons used to produce the fluorine-18 annihilation radiation do not change that threshold for interactions of its $511\mathrm{keV}$ photons in water.

Strictly, $\mu$ is a linear attenuation coefficient, whereas $\mu /\rho$ is a mass attenuation coefficient; the source's wording blurs these units. The mass energy-absorption coefficient ${\mu }_{\mathrm{en}}/\rho$ weights the fraction of incident photon energy transferred to charged particles and retained after radiative losses, rather than simply counting all removals. Coherent scattering contributes attenuation with negligible energy transfer. A photon deflected by Compton scattering can carry much of the original energy away. One often writes ${\mu }_{\mathrm{en}}=(1-g){\mu }_{\mathrm{tr}}$, with $g$ the fraction of secondary charged-particle kinetic energy lost radiatively. Under charged-particle equilibrium, multiplying photon energy fluence by ${\mu }_{\mathrm{en}}/\rho$ gives the absorbed dose; that equilibrium condition matters near interfaces and in buildup regions.^[ref]

A CT number is a dimensionless relative attenuation measure, conventionally $H=1000({\mu }_{\mathrm{CT}}-{\mu }_{\mathrm{water},\mathrm{CT}})/{\mu }_{\mathrm{water},\mathrm{CT}}$. The X-ray spectrum used in computed tomography has an effective energy far below $511\mathrm{keV}$ and is polychromatic. Its photoelectric absorption contribution depends strongly on composition, whereas water and soft-tissue attenuation at the positron emission tomography energy is mainly Compton scattering. Thus a CT number is neither a $511\mathrm{keV}$ linear attenuation coefficient nor an energy-independent mass attenuation coefficient.

The usual conversion calibrates a piecewise linear or bilinear relation between CT numbers and $\mu (511\mathrm{keV})$. The air–water branch models predominantly density differences in lung and soft tissue; a separate water–bone branch accounts for the different energy dependence of mineralized tissue. The calibration depends on the computed tomography spectrum. After geometric registration, the resulting linear attenuation coefficient map is forward projected along each coincidence line of response to obtain $\exp (\int {\mu }_{511}ds)$. If a mass coefficient is stored, its conversion to a linear coefficient must also include mass density. Unusual high-atomic-number materials can violate the simple tissue calibration, so the conversion is a physical material model, not a universal arithmetic rescaling.^[ref][ref]

A spectrum-weighted water-equivalence ratio compares a specified material response with the corresponding water response after accounting for the radiation's energy distribution. Its definition must identify the interaction coefficient and the spectral weighting. An attenuation comparison and an energy-absorption comparison are different quantities.

For an energy-absorption comparison, let ${\Psi }_E(E)dE$ be the photon energy fluence in an energy interval, and write $a_j(E)=({\mu }_{\mathrm{en}}/\rho {)}_j(E)$ for material $j$. Define the coefficient-weighted response and its ratio bywith $A_w>0$. The same prescribed local photon energy fluence is used for both materials in this comparison. NIST distinguishes the mass energy-absorption coefficient from the mass attenuation coefficient and relates energy fluence to photon fluence through the additional photon-energy factor.^[ref]

The ratio is a weighted mean of the monoenergetic ratios $q(E)=a_m(E)/a_w(E)$, but its normalized weights areThus the weights depend on the water response as well as the incident spectrum. Averaging the ratios with energy-fluence weights alone generally gives a different result.

For an original two-line calculation, use the NIST water and PMMA energy-absorption data: at $30\mathrm{keV}$ the coefficients are $0.1557$ and $0.09645\mathrm{c}{\mathrm{m}}^2/g$ respectively; at $100\mathrm{keV}$ they are $0.02546$ and $0.02368\mathrm{c}{\mathrm{m}}^2/g$.^[ref] Equal energy fluences in the two lines giveEqual photon counts instead give energy-fluence weights proportional to $30$ and $100$, producing $Q_{\Psi }\approx 0.72904$. The different answers reflect different physical spectra, not a discrepancy in the tabulated coefficients.

An absorbed dose interpretation needs additional conditions such as charged-particle equilibrium. A finite object can also change the local spectrum through beam hardening and scattering. The ratio above therefore specifies a local coefficient-weighted comparison; it is not a universal conversion factor for every phantom size or irradiation geometry. A physical validation should characterize the local spectrum and detector energy response rather than assume that equal total fluence means equal spectral weighting.

A radiation physicist who coauthored NIST reference tables for X-ray and gamma ray interactions with John H. Hubbell. The mass energy-absorption data use his calculations to account for how much photon energy is retained after interaction processes. This supports radiation-energy deposition calculations alongside the separate mass attenuation coefficient used for beam transmission.^[ref]

A water-equivalent material is a material whose relevant interaction with ionizing radiation approximates that of water under specified conditions. For a water phantom, the comparison concerns energy absorption and scattering in the measurement geometry. It is not a statement that the material merely has a density near that of water, or that equivalence at one energy applies at every other energy.^[ref]

For a narrow monoenergetic photon beam, the linear attenuation coefficient satisfieswhere $\rho$ is the mass density and $\mu /\rho$ the mass attenuation coefficient. Equal densities leave the mass interaction coefficients unconstrained. Predicting absorbed dose also involves how transferred energy is deposited, for which the mass energy-absorption coefficient is relevant; the attenuation of primary photons alone is not the complete scattering and deposition problem. For charged particles, the corresponding comparison also involves stopping power.

For an original toy calculation, stipulate equal densities but linear attenuation coefficients ${\mu }_w=0.05\mathrm{c}{\mathrm{m}}^{-1}$ and ${\mu }_m=0.08\mathrm{c}{\mathrm{m}}^{-1}$ at one chosen photon energy. For $t=10\mathrm{cm}$, the unscattered fractions in the Beer-Lambert law areThe substitute transmits only $e^{-0.3}\approx 0.74082$ times the unscattered intensity of the reference, despite identical density. These coefficients are stipulated model inputs, not tabulated data for real water or a named plastic. Matching even this transmission at one energy would not establish equal absorbed dose throughout a larger scattering object. Energy dependence of water equivalence is therefore part of any meaningful equivalence specification.

A focused physical comparison places the same characterized detector in reference water and in a candidate slab assembly, with controlled material thickness, irradiation geometry and detector position. Record density and composition as well as detector response over the intended radiation conditions. Slab gaps and changes in surrounding scattering material can confound the comparison; the primary IAEA discussion explicitly treats material variability and the approximate nature of plastic-to-water scaling.^[ref]