|Year : 2018 | Volume
| Issue : 3 | Page : 123-127
A study of energy absorption buildup factors of some steels
L Seenappa1, HC Manjunatha2, N Sowmya2, KN Sridhar3
1 Department of Physics, Government College for Women, Kolar, Karnataka; Research and Development Centre, Bharathiar University, Coimbatore, Tamil Nadu, India
2 Department of Physics, Government College for Women, Kolar, Karnataka, India
3 Department of Physics, Government First Grade College, Kolar, Karnataka, India
|Date of Submission||20-Jun-2018|
|Date of Decision||23-Aug-2018|
|Date of Acceptance||28-Aug-2018|
|Date of Web Publication||19-Nov-2018|
Dr. H C Manjunatha
Department of Physics, Government College for Women, Kolar - 563 101, Karnataka
Source of Support: None, Conflict of Interest: None
We have studied the energy absorption buildup factors of some steels (316 LN, 317 L, 317 LM, 317 LMN, 317 LN, XM-14, XM-17, XM-18, and Nitronic 60) for wide energy range (0.015–15 MeV) up to the penetration depth of 40 mfp using geometric progression fitting method. Buildup factors increase with the increase in the penetration depth. It is found that the shielding parameters such as mass attenuation coefficient, effective atomic number, and buildup factor values are larger for steel type 316 LN than the other studied steels. Hence, the steel type 316 LN is a good shielding material among the studied steels. The present study is useful in the field of radiation shielding.
Keywords: Buildup factor, penetration depth, shielding parameter
|How to cite this article:|
Seenappa L, Manjunatha H C, Sowmya N, Sridhar K N. A study of energy absorption buildup factors of some steels. Radiat Prot Environ 2018;41:123-7
|How to cite this URL:|
Seenappa L, Manjunatha H C, Sowmya N, Sridhar K N. A study of energy absorption buildup factors of some steels. Radiat Prot Environ [serial online] 2018 [cited 2018 Dec 10];41:123-7. Available from: http://www.rpe.org.in/text.asp?2018/41/3/123/245801
| Introduction|| |
When gamma and X-rays enter the medium, they degrade their energy through scattering with the medium, giving rise to secondary radiation which can be estimated by a factor which is called the “buildup factor.” The energy absorption buildup factor is also defined as the buildup factor in which the quantity of interest is the absorbed or deposited energy in the interacting material and the detector response function is that of absorption in the interacting medium. Manjunatha and Rudraswamy studied energy absorption and exposure buildup factors in hydroxyapatite, and these are helpful in dosimetry and diagnostics. The same group, computed the buildup factors and photon relative dose distribution in different regions of teeth, which is useful in dental science. Previous researchers also employed computed buildup factors for the estimation of specific absorbed fractions of energy in the biological samples. Previous researchers used exposure buildup factors for the calculations of secondary radiation dose such as bremsstrahlung., Steel is used for shielding of gamma radiation.
Calculations of the energy absorbed in a medium include not only the contribution of uncollided photons from the source but also the contributions from the collided and secondary photons. In practice, this is done by multiplying the contribution of uncollided photons with the energy absorption buildup factor., The energy absorption buildup factor is the ratio of the total energy absorbed due to uncollided, collided, and secondary photons to the energy absorbed due to only uncollided photons. The buildup factor is an important parameter in the distribution of photon flux in every object. In brnchytherapy, radioactive seeds are implanted into the patient's body to destroy the cancerous tumor., Thus, it is important to consider the photon buildup factor in the calculation of radiation dose received by the cancer cells. The buildup factor data were computed by different codes such as PALLAS-PL, RADHEAT-V4, ADJMOM-1, and ASFIT. Several authors have provided different buildup factor data for extensive utilization of design in radiation shields and other purposes.,,,,, ANSI/ANS 6.4.3 used the geometric progression (GP) fitting method and provided buildup factor data for 23 elements, water, air, and concrete at 25 standard energies in the energy range 0.015–15 MeV with suitable interval up to the penetration depth of 40 mfp. Previous studies compared the computed buildup factors using the GP fitting method with the PALLAS code. Good agreement was observed for penetration depth up to 40 mfp. Shimizu et al. compared the buildup factors obtained by three different methods (GP fitting, invariant embedding, and Monte Carlo method), and only small discrepancies were observed for low-Z elements up to 10 mfp. Singh et al. studied the variation of energy absorption buildup factors with incident photon energy and penetration depth for some solvents. Sidhu et al. computed the exposure buildup factors in biological samples and studied the variation of exposure buildup factors with incident photon energy and effective atomic number. In the present study, we have studied the energy absorption buildup factors of some steels (316 LN, 317 L, 317 LM, 317 LMN, 317 LN, XM-14, XM-17, XM-18, and Nitronic 60) for wide energy range (0.015–15 MeV) up to the penetration depth of 40 mfp using GP fitting method.
| Materials and Methods|| |
The equivalent atomic number of a composite material that will produce the same effect as that of the single element when it interacts with photons is referred as effective atomic number (Zeff). The effective atomic number is a convenient parameter for representing X-ray and gamma interactions. The number of electrons per unit mass is referred as effective electron density (Ne).
For the computation of Zeff, the values of mass attenuation coefficients were computed from WinX Com computer program. Zeff and Ne can be computed from the following equations:
Where ni is the number of atoms of ith element in a given molecule, (μ/ρ)st is the mass attenuation coefficient of steels, N is the Avogadro's number, Ai is the atomic weight of element i. (μ/ρ)st was estimated based on the chemical composition shown in [Table 1] and fi is the fractional abundance.
|Table 1: Chemical composition of different steels used in the present study|
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During the interaction of gamma/X-ray with the medium, it degrades their energy and produces secondary radiations through the different interaction processes. The quantity of secondary radiations produced in the medium and energy deposited/absorbed in the medium is studied by calculating buildup factors. In the present study, we have estimated energy absorption buildup factors (Ben) using GP fitting method.,,,,,, We have evaluated the GP fitting parameters (b, c, a, Xk, and d) for different stent alloys using the following expression which is based on the Lagrange's interpolation technique:
Where lower case z is the atomic number of the element of known GP fitting parameter Pz adjacent to the effective atomic number (Zeff) of the given material whose GP fitting parameter PZeff is desired and upper case Z are atomic numbers of other elements of known GP fitting parameter adjacent to Zeff. GP fitting parameters (b, c, a, Xk, and d) for element adjacent to Zeff are provided by the standard data available in the literature. The computed GP fitting parameters (b, c, a, Xk, and d) were then used to compute the EABF in the energy range of 0.015–15 MeV up to a penetration depth of 40 mfp with the help of GP fitting formula, as given by the following equations:,,,,,,
Where X is the source-detector distance for the medium in mean free paths and b is the value of buildup factor at 1 mfp. K(E, X) is the dose multiplication factor, and b, c, a, Xk, and d are computed GP fitting parameters that depend on attenuating medium and source energy.
| Results and Discussion|| |
The variation of mass attenuation coefficient as a function of energy is shown in [Figure 1]. The value of mass attenuation coefficient is large of low energies due to the dominance of photoelectric effect. The mass attenuation coefficient decreases progressively with the photon energy. We have calculated energy absorption buildup factors using GP fitting method. The calculated energy absorption buildup factors are graphically represented. The variation of energy absorption buildup factors with incident photon energy for steels is shown in [Figure 2]. From [Figure 1] and [Figure 2], it is observed that energy absorption increases up to the Epe (0.1 MeV) and then decreases. Here, Epe is the energy value at which the photoelectric interaction coefficients match with Compton interaction coefficients for a given value of effective atomic number (Zeff). The variation of buildup factors with energy is due to the dominance of photoelectric absorption in the lower end and the dominance of pair production in the higher photon energy region. As the energy of incident photon increases, Compton scattering overtakes the photoelectric absorption. It results in multiple Compton scattering events, which increases the energy absorption buildup factor up to the Epe, and it becomes maximum at Epe. Thereafter (above Epe), pair production starts dominating (absorption process) which reduces the energy absorption buildup factor to a minimum value. The variation of energy absorption buildup factors with the penetration depth at 0.1 MeV, 0.2 MeV, 0.5 MeV, 5 MeV, and 15 MeV is shown in [Figure 3]. The buildup factor increases with the penetration depth.
|Figure 1: Variation of mass attenuation coefficient with energy for different types of steels|
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|Figure 2: Variation of energy absorption buildup factor with photon energy for different types of steels|
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|Figure 3: Variation of energy absorption buildup factor with free mean path for different types of steels|
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We have compared the calculated mass attenuation coefficient among the studied different types of the steels; it is found that mass attenuation coefficient for steel type 316 LN is higher than that of other studied steels. If mass attenuation coefficient is large, penetration properties such as half-value layer, tenth-value layer, and mean free path are small. We have also compared the calculated effective atomic number among the studied different types of the steels; it is found that the effective atomic number for steel type 316 LN is higher than that of other studied steels. The comparison of calculated energy absorption buildup factors among the studied different types of steels shows that build factors for steel type 316 LN is higher than that of other studied steels. This means X-ray and gamma undergo more scattering and absorption in steel type 316 LN. Hence, the steel type 316 LN is a good shielding material for X-ray and gamma among the studied steels.
Financial support and sponsorship
Conflicts of interest
There are no conflicts of interest.
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[Figure 1], [Figure 2], [Figure 3]