Received: 9 August 2022 Revised: 26 May 2023 Accepted: 22 June 2023 DOI: 10.1002/mp.16604 M E D I C A L P H Y S I C S DATA S E T A R T I C L E A comprehensive open-access database of electron backscattering coefficients for energies ranging from 0.1 keV to 15 MeV Fatemeh Akbari Department of Radiation Oncology, University of Toledo Health Science Campus, Toledo, Ohio, USA Correspondence Fatemeh Akbari, 3000 Arlington Avenue, Toledo, OH 43614, USA. Email: f.akbari1@gmail.com Abstract Purpose: The characterization of electron backscattering is essential in medical physics for accurately assessing dose deposited around inhomogeneities where backscattering alters the spatial energy distribution pattern and for determining Monte-Carlo code’s ability to effectively describe electron scattering and does calculation in a target volume. Recent machine learning advances have provided physicists with powerful tools for effectively extracting information and trends from extensive experiment observations if sufficiently sizeable datasets are available for data mining. We report on the development of a publicly accessible database on electron backscattering coefficients for solid targets. Acquisition and validation methods: The first database on electron-solid interactions was assembled in 1995. Data for bulk materials, limited to normal incidence and energies up to 100 keV, were primarily focusing on electron microscopy. To accommodate broad high-energy applications and include the most recent publications we have created a comprehensive database of electron backscattering coefficients, listed as a function of target atomic number and thickness, electron energy, and incidence angle. These additions resulted in a database of 3566 data points, compared to the previous database of 1430. The data collection includes only published experimental observations (no calculations or results fitting) with no attempt to judge their accuracy or quality. A limited number of data points were compared to recently published Monte-Carlo results. Data format and usage notes: The presented database provides values of electron backscattering coefficients for 50 elements and 19 compounds at electron energies ranging from 0.1 keV to 15 MeV, presented in ASCII files. Each file contains the electron energy and backscattering coefficient with target thickness or electron incidence angle included where available, and the reference number shown in the last column. Additionally, the presented data were shown in the graphs for better visualization. The online database can be accessed from the website https://doi.org/10.5281/zenodo.7810951. Potential applications: The database provides the most up-to-date source of experimentally obtained electron backscattering coefficients that can be used in theoretical and MC calculations and modeling validations.The data availability is still very limited for many solids and almost non-existent for compounds. Novel machine learning methods should be well adapted to predict these unknown values for various targets, thicknesses, energies, and incident angles utilizing the presented cleaned dataset. This is an open access article under the terms of the Creative Commons Attribution-NonCommercial-NoDerivs License, which permits use and distribution in any medium, provided the original work is properly cited, the use is non-commercial and no modifications or adaptations are made. © 2023 The Authors. Medical Physics published by Wiley Periodicals LLC on behalf of American Association of Physicists in Medicine. 5920 wileyonlinelibrary.com/journal/mp Med Phys. 2023;50:5920–5929. 5921 KEYWORDS database, electron backscattering, open-access 1 INTRODUCTION When a primary electron beam is incident on a target material, there is penetration and interaction with the target’s atoms. The electrons continuously change their direction of motion due to the elastic scattering with the targets’ atoms nuclei, whereby they lose part of their energy due to the inelastic scattering with the targets’ atom’s electrons. This process is often characterized in terms of the backscattering coefficient (“η” or “eta”), defined as the ratio of the total electron current reflected into the hemisphere above the target surface to the incident electron current.1 These electrons allow valuable information regarding the characteristics of the target materials to be collected. These electrons contain variable information regarding the characteristics of the target materials. There is considerable variation between the definitions of the parameters used by different researchers to characterize the backscattering of charged particles. For consistent terminology, we define E (in keV) as the kinetic energy of the incident monoenergetic charged particle beam. Z is the target’s atomic number, t is the film thickness, and 0 < = α < 90◦ is the incidence angle, which is formed by the incident beam’s vector and the vector perpendicular to the target surface. Electron backscattering is of great interest in many applications, such as scanning electron microscopy (SEM) and image analysis, electron microlithography, Auger electron spectroscopy, and film thickness determination. This phenomenon is crucial in medical physics for radiation damage studies and accurately assessing the doses deposited around inhomogeneities where backscattering alters the spatial energy distribution pattern.2,3 Investigations in radiotherapy and radiobiology should consider the backscattering of electrons at interfaces such as tissue-bone, lung-bone, lung-tissue or air-tissue since it changes dosimetry and causes overdosing of lower density tissue. The significance of backscattering while irradiating inhomogeneous tissues during radiotherapy has led to the introduction of proper corrections in treatment planning systems.4 The backscattering process is involved in the dosage adjustment from internal shielding with high-Z materials. For example, using lead or tungsten in electron beam therapy for lip cancer or superficial lesions like those of the eyelid, buccal mucosa, and ear. Backscattering simulations are also a critical framework for determining a Monte Carlo transport code’s ability to effectively describe electron multiple scattering, which in turn affects the backscattered fraction, their energy spectrum and angular distribution, and calculated energy deposition in a target volume.5 In recent decades, many studies have explored the general tendency of the dependence of the backscattering coefficient on the atomic number of the target and incident electron energy. It was observed that the high Z targets exhibit stronger elastic scattering and, correspondingly, more significant deflections, amplifying the yields of backscattered electrons. The general behavior of the primary energy dependence of the backscattering coefficient was also found. Since higher energy electrons are more forward-directed, η decreases as the incident energy increases. Additionally, electron backscattering depends on material thickness, reaching a bulk specimen value known as the saturation thickness, when the layer thickness reaches close to twice the electron range in the material. It was also observed that η is surface sensitive, that is, its value when a thin film is deposited on the top of different materials is different from those in the absence of the substrate. Furthermore, studies on the orientation dependence of electron backscattering have been shown that in general, η increases with the angle of the oblique incident. Recent machine learning (ML) advances have provided physicists with powerful tools to extract information and trends from extensive simulations or experiment datasets. The power of machine learning has previously been demonstrated in numerous fields of materials science, particularly in the prediction of a variety of material’s mechanical, thermodynamic, and electrical properties.6–11 Other possible applications for ML include the prediction of electron inelastic mean free paths, band gaps in semiconductors, stopping power predictions, and machine learning on neutron and x-ray scattering and spectroscopies.12–15 In addition to various investigations in imaging applications, the ML technique has been of interest to medical physicists for the prediction of radiation treatment side effects or patients who would benefit from adaptive radiotherapy.16–18 However, the lack of sufficiently sizeable datasets for data mining restricts the application of ML techniques. If publicly open, such data resources would also enable research by scientists without access to particular experimental equipment. A database of measured electron backscattering as a function of the atomic number of the target and the incident beam energy has been created by Joy19 for several elements and compounds for low energy electron beams. This quantity, however, varies greatly depending on the electron incidence angle and target thickness. Additionally, missing higher energy data can be critical for various spectroscopy applications and the measurement of radiation fields in radiotherapy. Unfortunately, 24734209, 2023, 9, Downloaded from https://aapm.onlinelibrary.wiley.com/doi/10.1002/mp.16604 by University Of Toronto Mississauga, Wiley Online Library on [18/09/2023]. See the Terms and Conditions (https://onlinelibrary.wiley.com/terms-and-conditions) on Wiley Online Library for rules of use; OA articles are governed by the applicable Creative Commons License ELECTRON BACKSCATTERING COEFFICIENTS DATABASE there appear to be no comprehensive collections of the results of such experiments and investigations. Here, we report on developing a freely accessible experimental electron backscattering database (https://doi.org/10. 5281/zenodo.7810951). This dataset is the first publicly available extensive experimental data collection for electron backscattering coefficients from solid targets as a function of beam energy, angle of incident, and target thickness. 2 ACQUISITION AND VALIDATION METHODS The electron backscattering coefficient can be measured experimentally or calculated theoretically. Many experimental investigations have been reported in the literature for the backscattering of electrons from solid targets; the results of these investigations were found to show considerable inconsistencies.20–23 One reason would be that most of the reported experimental results have been measured under conventional vacuum conditions, with some at different pressure levels. Also, in situ surface cleaning was considered in few of these investigations, while most of the reported η measurements are from samples with a thin surface film of contaminants. Such layers can change the target thickness, altering its backscattering behavior to another target material. The theoretical treatment of the fundamental scattering process is complicated. The electron backscattering coefficient is mainly calculated analytically or statistically using the Monte Carlo simulation. In recent decades there has been continuous improvement in Monte Carlo modeling of electron beam interactions with solids as a powerful theoretical tool widely used to study electron backscattering. CASINO Monte Carlo simulation software24 and an EGSnrc usercode25 customized for backscatter calculations are the most frequently used approaches to obtain electron backscattering. Analytically, some theoretical expressions have been developed based on a single elastic scatter collision assumption in which the backscatter coefficient depends only on the atomic number (Z) of the scatterer and is independent of electron energy; such as Everhart’s single scattering approach,26 Archard’s point source diffusion model,27 and Thiimmel’s continuous-diffusion-depth model.28 However, a good model describing the backscattering of solids should include single scattering and diffusion, and the contributions of double and multiple scattering processes. Despite many investigations on electron backscattering, there is some disagreement among the proposed theories and various viewpoints. Furthermore, some methods were not significantly predictive of the experimental results. The papers typically describe certain limiting cases where the results are difficult to evaluate. On the other hand, some empirical formulas ELECTRON BACKSCATTERING COEFFICIENTS DATABASE fit the electron backscattering data with linear or polynomial functions of the atomic number (Z), others with exp(−Z) or log(Z+1) functions. While some theoretical formulae are energy independent, it was experimentally indicated that backscatter depends on the electron energy.29–31 Existing theories commonly describe certain limiting cases or are challenging to evaluate. Also, because of the essentially random manner in which electrons lose their energy, current theoretical treatments are not totally satisfactory. By simulation methods, on the other hand, numerical results can be obtained, requiring expensive computer calculations to achieve the acceptance uncertainty. Due to the mentioned limitations of the theoretical and simulation approaches, experimental measurements are considered as the most reliable method to obtain backscatter coefficients. A reasonable amount of experimental data are available for electron backscattering, representing an extensive range of incident projectile angles and energies, target species, and experimental geometries. Available measured data are mainly in the form of research papers written in several different languages. They are inserted within text documents in a table or graph format, stated in different units, and with different levels of precision. Joy’s database of measured electron backscattering as a function of the atomic number of the target and the incident beam energy assembled for 45 elements and 13 compounds of bulk materials was limited to normal incidence and energies up to 100 keV, primarily focusing on electron microscopy and microanalysis applications. However, there appears to be no comprehensive collections of the results of such experimental investigations. As a result, anyone requiring specific information has to explore the literature in the hope of discovering a reported value that must then be considered reliable. Augmenting Joy’s database, we established a comprehensive database on electron backscattering as a function of target atomic number and thickness, and electron energy and incident angle. For the period from 1940 to the present, literature searches were done to find all citable, published references in this field; yet the search cannot be affirmed to be complete.Table 1A (see Appendix) contains a numerical list of the references used in the database. Unlike Joy’s database, we included the title of the publication where available. Following Joy’s approach, a set of rules were used for data collection: (a) Only experimental observations were included. Findings from calculations and fittings, as well as values that were not explicitly marked as experimental, were excluded. (b) All experimental data were taken from their original sources. (c) There had been no attempt to eliminate any results due to their accuracy, precision, or quality. Our new set of experimental data were digitized electronically from their original graphs if they were not available in tabular form. The backscattering coefficients were expressed as a percentage to 24734209, 2023, 9, Downloaded from https://aapm.onlinelibrary.wiley.com/doi/10.1002/mp.16604 by University Of Toronto Mississauga, Wiley Online Library on [18/09/2023]. See the Terms and Conditions (https://onlinelibrary.wiley.com/terms-and-conditions) on Wiley Online Library for rules of use; OA articles are governed by the applicable Creative Commons License 5922 5923 For validation, a limited number of data points were compared to recently published MC results.32 The validation set consists of the calculated maximum backscattering coefficients and experimental observations for Cu under 20, 50, and 100 keV electron beam, as presented in Figure 1. The numbers next to the symbols correspond to different references for the experimental observations. The simulation results are denoted as “MC”, shown as solid black circles in the graph. 3 F I G U R E 1 Maximum backscattering coefficient from bulk Cu at 20, 50, and 100 keV electron source. The references for the experimental observations are indicated by the numbers next to each data point. Results of the simulations are shown with black symbols and denoted as “MC”. compile a self -consistent database. All energies and incident angles were expressed in keV and degree units, respectively. Compared to the Joy’s database, data were plotted in the format of graphs to provide a visual representation of data that is easier to interpret than raw data. The information is now presented in a clear and succinct manner,making it simpler for others to comprehend the data. Graphs also allow for easy comparison across multiple dataset as well as making informed predictions about future trends. DATA FORMAT AND USAGE NOTES The presented database is available over the World Wide Web. As a result, the database can be accessed by users using a browser without the need for any additional software or a subscription. As of this writing, a total of 3566 records were stored in the database for 50 solid elements and 19 compounds at electron energies ranging from 0.1 keV to 15 MeV. There are three folders in this web interface for energy, orientation, and thickness dependencies of the electron backscattering coefficient, containing 67, 14, and 14 files, respectively. Figure 2 depicts a portion of the web interface’s folders and files. The database was formatted as a collection of ASCII files for general use. Both the commonly used .csv standard format and the .txt format were used to store the data. Data for different materials are presented in a consistent style so that they may easily be compared. The name of the material and elemental atomic number is included in each file. The first and second columns F I G U R E 2 Folders and files in .txt format within our database. The data files in .csv format are also available in three other similar folders that are part of the Zenodo repository. 24734209, 2023, 9, Downloaded from https://aapm.onlinelibrary.wiley.com/doi/10.1002/mp.16604 by University Of Toronto Mississauga, Wiley Online Library on [18/09/2023]. See the Terms and Conditions (https://onlinelibrary.wiley.com/terms-and-conditions) on Wiley Online Library for rules of use; OA articles are governed by the applicable Creative Commons License ELECTRON BACKSCATTERING COEFFICIENTS DATABASE ELECTRON BACKSCATTERING COEFFICIENTS DATABASE TA B L E 1 Description of the files (.txt format) in the database Folder File name and contents Energy dependence Ag.txt, Al.txt, Ag.txt, As.txt, Au.txt, B.txt, Ba.txt, Be.txt, Bi.txt, C.txt, Ca.txt, Cd.txt, Co.txt, Cr.txt, Cu.txt, Fe.txt, Ga.txt, Ge.txt, Hf.txt, Hg.txt, In.txt, Ir.txt, K.txt, La.txt, Mg.txt, Mn.txt, Mo.txt, Nb.txt, Ni.txt, Pb.txt, Pd.txt, Pt.txt, Sb.txt, Sc.txt, Se.txt, Si.txt, Si-a.txt, Sm.txt, Sn.txt, Sr.txt, Ta.txt, Te.txt, Ti.txt, Tl.txt, U.txt,V.txt, W.txt, Y.txt, Zn.txt, Zr.txt, AlSi.txt, CuAu.txt, COAT725.txt, ITO.txt, IZO.txt, PETEOS.txt, Plastic.txt, Resist.txt, SiO2.txt, TaC.txt, Ti-6Al-4V.txt, TiC.txt, UO2.txt, U-V Resist.txt, V2O5.txt, ZrC.txt, Interconnect-line Al.txt (Electron backscattering coefficients as a function of energy of normal incident electrons for bulk targets) Energy.xlsx (Collected data and plots of backscattering coefficients versus energy) Orientation dependence Ag.txt, Al.txt, Au.txt, Be.txt, C.txt, Cu.txt, Mo.txt, Ta.txt, Ti.txt, U.txt, Fe.txt, Nb.txt, UO2.txt (Electron backscattering coefficients as a function of energy and angle of incident for bulk targets) Orientation.xlsx (Collected data and plots of backscattering coefficients versus beam angle for different energies) Thickness dependence Ag.txt, Al.txt, Au.txt, Bi.txt, Cu.txt, Pb.txt, Ti.txt, U.txt, V.txt, ZnS.txt, PbF2.txt, CuAu.txt, Ti-6Al-4V.txt (Electron backscattering coefficients as a function of energy and film thickness) Thickness.xlsx (Collected data and plots of backscattering coefficients versus film thickness for different energies) were always labeled E, where E denotes the energy values (in keV), and η which is the electron backscattering coefficient (in %), followed by either electron incident angle or target thickness. The last column contains the reference number (see Table 1A in Appendix) for the data. The names of the targets were used to name the files. Additionally, an xlsx file in some folders contains the collected data sorted in ascending order of energy and plotted in graph form for better visualization. The material of interest can be chosen from various alphabetical sheets.High-level visual summaries,trends, and patterns in Excel enables the user to analyze data and better comprehend it. All files in the web-based user interface can be downloaded. Table 1 represents a description of the .txt files in the database. Table 2 and Figure 3 depict an example of information supplied in the three .txt files and the plotted data for Al target, respectively. 4 DISCUSSIONS Although electron backscattering coefficients can be obtained using CASINO, a Monte Carlo code in C language for electron beam interaction, calculations are limited to bulk targets of fixed thicknesses only. Likewise, a customized EGSnrc user code has been developed for backscattering coefficient calculations, but it can only be used for low-energy regimens. Monte Carlo calculations are very time-consuming for higher energies and bulk targets, on the other hand, can only be carried out if sufficient experimental data are available. An open-access database in physics quantities can be incredibly helpful for researchers as it provides them with easy access to a vast amount of data and information. This can save researchers a lot of time and effort in collecting and analyzing data, allowing them to focus on their research and make new discoveries. Additionally, an open-access database can facilitate collaboration and knowledgesharing among researchers, leading to more efficient and effective research outcomes. Collecting the electron backscattering data in this work revealed that there exists little or no data for most elements in the periodic table, while results for complex materials of dosimetric interests are also almost nonexistent, as evident from Table 3. To identify any hidden patterns and problems in the dataset which may not be immediately apparent looking at raw data, we displayed the frequency distribution of existing information by energy and atomic number. As shown in Figure 4, the most experiments were performed using the low energies and low atomic number targets. It was found that only 25% of all data were measured at energies above 100 keV which indicates the lack of data for higher energies of particular importance in radiotherapy applications. Inconsistent experiment results were also found by means of data visualization supplied in the Zenodo repository. This discrepancy was most noticeable in the energy dependence of electron backscattering coefficients. The uncertainty in a measurement arises, in general, from personal errors, systematic errors, or random errors. The experimenter might take the measurement erroneously, with poor technique, or with bias if they expect that the data will support their prediction. Some inaccuracies can be attributed to faulty design, inaccurate calibration, or the observer’s prejudice and observational style. Identifying exact reasons for inconsistent experiments in the reviewed publications was impossible since the measurements were not always clearly defined and conditions that could affect the measurements were not carefully specified. All measured results were reported in this work regardless of wide disagreements in some measurements. Further investigations are therefore necessary to judge the reliability and uncertainty of any particular data point. This database provides a framework for quantitatively understanding and interpreting electron backscattering, as is required, for example, in semiconductor device research, as well as a comprehensive source of experimental data for testing analytical and Monte Carlo models of electron beam interactions. As noted earlier, this dataset was initially prepared by Joy for limited bulk 24734209, 2023, 9, Downloaded from https://aapm.onlinelibrary.wiley.com/doi/10.1002/mp.16604 by University Of Toronto Mississauga, Wiley Online Library on [18/09/2023]. See the Terms and Conditions (https://onlinelibrary.wiley.com/terms-and-conditions) on Wiley Online Library for rules of use; OA articles are governed by the applicable Creative Commons License 5924 5925 TA B L E 2 An example of information provided in .txt files for the Al target: (a) Energy dependence, (b) Orientation dependence, and (c) Thickness dependence. The first and second columns are energy (in keV), and the electron backscattering coefficient (in %), followed by either electron incident angle or target thickness. The last column contains the reference number for the data, according to Table 1A (see Appendix). (a) (b) (c) E (keV) η (%) Reference E (keV) η (%) Angle (degree) 0.5 21.5 (1) Cleaned sample 20 16.9 10 1 21.2 20 18.6 20 4000 0.49 0.1 1.5 20.6 20 21.6 30 4000 0.57 0.15 2 20.3 20 26 40 4000 1.18 0.3 2.5 20.1 20 32.4 50 4000 1.97 0.5 3 19.7 20 40.9 60 4000 2.68 0.6 3.5 19.5 20 52.6 70 4000 2.74 0.7 4 19.1 20 59.8 75 4000 2.91 0.85 4.5 18.8 20 68.7 80 4000 3.08 0.95 5 18.4 40 15.6 10 4000 3.1 1 6 18 40 17.4 20 4000 3.1 1.25 1 19.1 40 20.4 30 4000 3.16 1.35 1.5 18.6 40 24.9 40 4000 3.28 1.3 2 17.7 40 31.2 50 4000 3.23 1.67 2.5 17.5 40 39.8 60 4000 3.2 1.85 3 17.4 40 50.9 70 8000 0.52 0.16 3.5 16.9 40 58.4 75 8000 0.68 0.34 4 16.7 40 67 80 8000 0.71 0.68 4.5 16.3 60 15.2 10 8000 0.85 0.88 5 16.3 60 16.9 20 8000 1.21 1.38 0.8 19.8 60 19.8 30 8000 1.33 1.57 1 19.5 60 24.3 40 8000 1.24 2.35 1.2 18.9 60 30.6 50 8000 1.26 2.59 1.4 18.2 60 39.3 60 8000 1.26 2.78 1.6 17.9 60 50.5 70 8000 1.25 3.77 1.8 17.5 60 58 75 8000 1.25 4.35 (1) non-cleaned sample (2) targets for energies up to 100 keV. We have expanded Joy’s database to incorporate all relevant details as well as data extracted from more recent research that may be found via reference search engines, such as information on thin films, different incidence angles (if available), and broader energy spectra (up to 15 MeV). Compared to the Joy’s database of 1430, the data were compiled into a database of 3566 data points of electron backscattering coefficients. While the data by itself can be useful in a myriad of clinical and industrial applications related to radiation dose calculations, the cleaned and ordered format of the data could be seen as even more valuable. It can assist physicists in creating more robust theories and identifying more precise relationships between the various factors affecting electron backscattering. Additionally, in one medical application, data can be utilized to estimate the amount of off -focal radiation (stray radiation) produced by backscattering electrons in kilo- Reference E (keV) η (%) Thickness (g/cm2 ) Reference (8) 4000 0.36 0.05 (5) voltage x-ray tubes. Because electron backscattering coefficients from anode materials indicate the amount of off -focal component, researchers can model more realistic and efficient x-ray systems by reducing the effect of off -focal radiation on x-ray tube output, image quality, and patient exposure by knowing these data as a function of incident electron energy, target thickness, and atomic number.33 Moreover, electron backscattering data can be used in designing a multilayer detector structure consisting of a detector-sensitive volume and a metal back-reflector layer. Our database can be utilized to determine the proper material and optimum thickness of the backscattering layer to achieve signal enhancement in radiation dosimetry.32 Besides, as the radiation dose can be calculated using an equation incorporating the electron backscattering coefficients, according to the established linear relationship between the backscattered electron fluence and the deposited dose in the detector’s active volume,32 our database 24734209, 2023, 9, Downloaded from https://aapm.onlinelibrary.wiley.com/doi/10.1002/mp.16604 by University Of Toronto Mississauga, Wiley Online Library on [18/09/2023]. See the Terms and Conditions (https://onlinelibrary.wiley.com/terms-and-conditions) on Wiley Online Library for rules of use; OA articles are governed by the applicable Creative Commons License ELECTRON BACKSCATTERING COEFFICIENTS DATABASE ELECTRON BACKSCATTERING COEFFICIENTS DATABASE F I G U R E 3 Electron backscattering coefficient for Al target. (a) Energy dependence, (b) Electron beam orientation dependence, and (c–f) Target thickness dependence. Y-axis in all graphs represents electron backscattering coefficient η(%). Parts (c–f) show film thickness dependency of the η for a different range of low and high electron energies. The original unit of the thickness was kept. 24734209, 2023, 9, Downloaded from https://aapm.onlinelibrary.wiley.com/doi/10.1002/mp.16604 by University Of Toronto Mississauga, Wiley Online Library on [18/09/2023]. See the Terms and Conditions (https://onlinelibrary.wiley.com/terms-and-conditions) on Wiley Online Library for rules of use; OA articles are governed by the applicable Creative Commons License 5926 5927 TA B L E 3 A list of the target materials included in the references used to compile our database, organized alphabetically. Target material Reference number (see Table 1A in Appendix) Silver (Z = 47) 1–18, 35 TA B L E 3 (Continued) Target material Reference number (see Table 1A in Appendix) Silicon (Z = 14) 6, 10, 12, 14, 15, 17, 18, 24, 25 Si-a (Silicon amorphous) 38 Aluminum (Z = 13) 1–5, 7–23, 35, 36 Silicon Dioxide (SiO2) 29 Al-Si alloy 4 6 Arsenic (Z = 33) Samarium (Z = 62) 13 Tin (Z = 50) 6, 10, 13, 14, 18 Gold (Z = 74) 1–3, 6–10, 12, 14, 15, 17, 18, 19, 24, 35, 36 Strontium (Z = 38) 18 Boron (Z = 5) 6 Tantalum (Z = 73) 5, 6, 8, 13, 14, 18, 21, 26, 0, 31 Barium (Z = 56) 18 Tantalum Carbide (TaC) 31 Beryllium (Z = 4) 7–11, 13, 15, 18, 25 Bismuth (Z = 83) 6, 10, 13, 14, 17, 35 Carbon (Z = 6) 1, 4, 5, 6, 8, 9, 12–14, 16–18, 21, 26 Calcium (Z = 20) 16, 18 Cadmium (Z = 48) 6, 18 Cobalt (Z = 27) 6, 13, 14 COAT725 (wafer coat) 38 Tellurium (Z = 52) 6, 10, 13, 14, 32 Titanium (Z = 22) 6, 8, 12–14, 17–19, 21 Ti-6Al-4V 19 Titanium Carbide (TiC) 31 Thallium (Z = 81) 18 Uranium (Z = 92) 5, 6, 8–10, 13–15, 21 Uranium dioxide (UO2) 21 U-V Resist 29 Vanadium (Z = 23) 6, 14, 17, 19 33 Chromium (Z = 24) 6, 12, 14, 17 Copper (Z = 29) 1–12, 14, 15, 17–20, 26–28 CuAu (50%Cu-50%Au) 19 Vanadium Pentoxide (V2O5) Iron (Z = 26) 6, 8, 12–14, 16, 17, 26 Tungsten (Z = 74) 6, 10, 12–14, 16, 18, 34 Gallium (Z = 31) 18 Yttrium (Z = 39) 18 Germanium (Z = 32) 6, 10, 12, 13, 15, 18 Zinc (Z = 30) 6, 12, 18, 35 Hafnium (Z = 72) 6 6, 14, 17 Mercury (Z = 80) Zirconium (Z = 40) 18 Zirconium Carbide (ZrC) 31 Indium (Z = 49) 10, 18 Interconnect line Aluminum 38 Iridium (Z = 77) 14 Indium tin oxide (ITO) 29 Indium Zinc Oxide (IZO) 29 Potassium (Z = 19) 1 Lanthanum (Z = 57) 18 Magnesium (Z = 12) 6, 14, 18 Manganese (Z = 25) 14 Molybdenum (Z = 42) 10, 12–14, 16, 18, 21, 26 Niobium (Z = 41) 8, 13 Nickel (Z = 28) 6, 12–14, 16–18, 30, 31 Lead (Z = 82) 18, 20, 35, 37 Lead fluoride (PbF2) 35 Palladium (Z = 46) 14 PETEOS 38 Plastic 25 Platinum (Z = 78) 6, 12, 14, 16, 18, 26, 31 Resist (e-beam –PMMA) 38 Antimony (Z = 51) 6, 10, 14 Scandium (Z = 21) 18 Selenium (Z = 34) 18 (Continues) can be utilized to test this theory and demonstrate the accuracy of any suggested dose calculation formula. The present database also assists in the design of internal shields that incorporate appropriate materials to reduce backscattering while minimizing overall shield thickness for improved clinical setup and simplicity of utilization. Furthermore, because thin-films are crucial to modern materials science, microelectronics, semiconductor technology, and biology, and because film thickness and the electron backscattering coefficient are correlated, our database provides an essential tool for determining thin-film thickness and enables scientists to develop an optimized thin-film design. Last but not least, this database provides researchers with knowledge about the backscattering effect on image quality when developing an imaging system since backscattering introduces a source of noise to the detection signal in imaging systems. The data availability is still very limited for many solids and almost non-existent for compounds because experimental physicists are motivated to collect data that are useful to their particular area of study. Machine learning techniques should be well adapted to produce the missing values for various target materials, 24734209, 2023, 9, Downloaded from https://aapm.onlinelibrary.wiley.com/doi/10.1002/mp.16604 by University Of Toronto Mississauga, Wiley Online Library on [18/09/2023]. See the Terms and Conditions (https://onlinelibrary.wiley.com/terms-and-conditions) on Wiley Online Library for rules of use; OA articles are governed by the applicable Creative Commons License ELECTRON BACKSCATTERING COEFFICIENTS DATABASE ELECTRON BACKSCATTERING COEFFICIENTS DATABASE FIGURE 4 Distribution of existing experimental data by energy and atomic number. including thin films, and expanded ranges of energies. LiF, one of the most popular thermoluminescent detectors, or CdTe, which is regarded as the next-generation x-ray detector in medical imaging applications34 are examples of such missing data. This extensive collection of easily accessible data enables researchers to develop sophisticated Monte Carlo simulations of electron-solid interactions and validate their predictions. The literature has demonstrated the benefits of combining powerful machine-learning techniques with conventional computational modeling to develop the required data. Therefore, another substantial application of the presented database is that it could be used with combination of Monte-Carlo to design the optimal detector device for a range of energies. These data are useful in determining the ideal parameters, before running time consuming simulations or pursuing them in the laboratory which in turn helps to reduce the costs of building prototypes. Furthermore, recently introduced physics-based machine learning allows investigators to analyze the physical principles behind electron- solid interactions by extracting features and evaluating their importance. 5 CONCLUSIONS This paper presents a database on electron backscattering coefficients from different target materials. The data were stored in compressed files freely available for all users via the Zenodo repository (https://doi.org/ 10.5281/zenodo.7810951). The present database contains a wide range of data on the backscattering of electrons, including information on the energy and angle of the incident electrons, as well as the composition and structure of the target materials. The database is designed to be used by researchers in a variety of fields, including medical physics, physics, materials science, and engineering. It can be used to help researchers understand the fundamental physics of electron backscattering, as well as to develop new detectors, materials, and technologies that rely on this phenomenon. This is a scientifically valuable open-access resource for researchers who are interested in electron backscattering, as it provides a wealth of data and information that can be used to inform and guide research in this area. It can be freely used by students, universities, and research laboratories in their research endeavors. A reference to this paper should be made whenever the results from using these data are presented or published. AC K N OW L E D G M E N T S I am deeply grateful to all those who played a role in the success of this database article. The author received no financial support for the research and publication of this article. C O N F L I C T O F I N T E R E S T S TAT E M E N T The authors do not have any conflict of interest. REFERENCES 1. 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High-Z Materials for X-ray Detection: Material Properties and Characterization Techniques. Springer; 2023:23-41. S U P P O R T I N G I N F O R M AT I O N Additional supporting information can be found online in the Supporting Information section at the end of this article. How to cite this article: Akbari F. A comprehensive open-access database of electron backscattering coefficients for energies ranging from 0.1 keV to 15 MeV. Med Phys. 2023;50:5920–5929. https://doi.org/10.1002/mp.16604 24734209, 2023, 9, Downloaded from https://aapm.onlinelibrary.wiley.com/doi/10.1002/mp.16604 by University Of Toronto Mississauga, Wiley Online Library on [18/09/2023]. See the Terms and Conditions (https://onlinelibrary.wiley.com/terms-and-conditions) on Wiley Online Library for rules of use; OA articles are governed by the applicable Creative Commons License ELECTRON BACKSCATTERING COEFFICIENTS DATABASE