Pub Date : 2024-10-21DOI: 10.1007/s13538-024-01621-9
Humberto Araujo Machado, Danton José Fortes Villas Boas, Luis Eduardo Vergueiro Loures da Costa, Denis Guilgim Vieira
This work presents the preliminary thermal analysis of the SPORT microsatellite, based on its initial configuration. A simplified analysis, using control volumes, is conducted, considering the power dissipated by the equipment and solar radiation as heat sources. Internal conduction and radiation processes between components, as well as radiation into space, are also taken into account. A system of ordinary differential equations is constructed and solved using a simple time-marching method. The results are presented as the average temperatures of the components over a 24-h period and are compared with the numerical simulation of the definitive configuration performed by CFD. The main objective is to apply a quick and simplified version of the thermal lumped method to identify which elements may exceed temperature limits during operation, using the results to adjust the design where those limits are not met. The results are compared with CFD data for the final configuration, showing that the overall temperature behavior is consistent, and that all elements remained below the temperature limits. This validates the use of the methodology in the early phases of nanosatellite design, though some improvements may still be required.
这项工作以 SPORT 微型卫星的初始配置为基础,对其进行了初步热分析。使用控制体积进行了简化分析,将设备耗散的功率和太阳辐射视为热源。同时还考虑了部件之间的内部传导和辐射过程,以及向空间的辐射。该研究构建了一个常微分方程系统,并使用简单的时间行进法进行求解。计算结果以 24 小时内各部件的平均温度表示,并与 CFD 对确定配置进行的数值模拟进行了比较。主要目的是应用快速简化版热叠加法来确定哪些元件在运行过程中可能会超过温度限值,并利用结果来调整未达到限值的设计。将结果与最终配置的 CFD 数据进行了比较,结果表明,整体温度行为是一致的,所有元件都保持在温度限值以下。这验证了在超小型卫星设计的早期阶段使用该方法的有效性,尽管可能仍需要进行一些改进。
{"title":"Preliminary Thermal Analysis of the Sport Microsatellite","authors":"Humberto Araujo Machado, Danton José Fortes Villas Boas, Luis Eduardo Vergueiro Loures da Costa, Denis Guilgim Vieira","doi":"10.1007/s13538-024-01621-9","DOIUrl":"10.1007/s13538-024-01621-9","url":null,"abstract":"<div><p>This work presents the preliminary thermal analysis of the SPORT microsatellite, based on its initial configuration. A simplified analysis, using control volumes, is conducted, considering the power dissipated by the equipment and solar radiation as heat sources. Internal conduction and radiation processes between components, as well as radiation into space, are also taken into account. A system of ordinary differential equations is constructed and solved using a simple time-marching method. The results are presented as the average temperatures of the components over a 24-h period and are compared with the numerical simulation of the definitive configuration performed by CFD. The main objective is to apply a quick and simplified version of the thermal lumped method to identify which elements may exceed temperature limits during operation, using the results to adjust the design where those limits are not met. The results are compared with CFD data for the final configuration, showing that the overall temperature behavior is consistent, and that all elements remained below the temperature limits. This validates the use of the methodology in the early phases of nanosatellite design, though some improvements may still be required.</p></div>","PeriodicalId":499,"journal":{"name":"Brazilian Journal of Physics","volume":"54 6","pages":""},"PeriodicalIF":1.5,"publicationDate":"2024-10-21","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://link.springer.com/content/pdf/10.1007/s13538-024-01621-9.pdf","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"142453052","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":4,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"OA","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
Pub Date : 2024-10-19DOI: 10.1007/s13538-024-01636-2
Nathália M. P. Rosa, Itamar Borges Jr.
We investigate theoretically the design and application of nine triazine (Tr)-core star-shaped molecules built with thiophene (Th), phenyl (Ph), and carbazole (Cz) moieties in dye-sensitized solar cells (DSSCs) and bulk heterojunction (BHJ) organic solar cells. Density functional theory and time-dependent density functional theory are employed to rationalize the electronic structure, charge transfer properties, and photovoltaic performance of these systems. Tr-Th-Cz and Tr-Ph-p-Th-Cz display power conversion efficiency ((text{PCE})) values close to 30% due to a favorable alignment of the energy levels. Computed open-circuit voltage values show that lack of π-bridges, as in the Tr-Th and Tr-Cz, favor higher voltage generation. Systems containing thiophene (Th) and carbazole (Cz) present the most favorable values for efficient electron injection and dye regeneration. Furthermore, the incorporation of these Th and Cz donor substituents into the triazine core combined with π-bridges significantly impacts other optoelectronic properties of the organic solar cells. The computed high singlet–triplet gap values indicate limited potential of these molecules as thermally activated delayed fluorescence (TADF) emitters for applications in organic light-emitting diodes (OLEDs).
{"title":"Star-Shaped Molecules with a Triazine Core: (TD)DFT Investigation of Charge Transfer and Photovoltaic Properties of Organic Solar Cells","authors":"Nathália M. P. Rosa, Itamar Borges Jr.","doi":"10.1007/s13538-024-01636-2","DOIUrl":"10.1007/s13538-024-01636-2","url":null,"abstract":"<div><p>We investigate theoretically the design and application of nine triazine (Tr)-core star-shaped molecules built with thiophene (Th), phenyl (Ph), and carbazole (Cz) moieties in dye-sensitized solar cells (DSSCs) and bulk heterojunction (BHJ) organic solar cells. Density functional theory and time-dependent density functional theory are employed to rationalize the electronic structure, charge transfer properties, and photovoltaic performance of these systems. Tr-Th-Cz and Tr-Ph-<i>p</i>-Th-Cz display power conversion efficiency (<span>(text{PCE})</span>) values close to 30% due to a favorable alignment of the energy levels. Computed open-circuit voltage values show that lack of π-bridges, as in the Tr-Th and Tr-Cz, favor higher voltage generation. Systems containing thiophene (Th) and carbazole (Cz) present the most favorable values for efficient electron injection and dye regeneration. Furthermore, the incorporation of these Th and Cz donor substituents into the triazine core combined with π-bridges significantly impacts other optoelectronic properties of the organic solar cells. The computed high singlet–triplet gap values indicate limited potential of these molecules as thermally activated delayed fluorescence (TADF) emitters for applications in organic light-emitting diodes (OLEDs).</p></div>","PeriodicalId":499,"journal":{"name":"Brazilian Journal of Physics","volume":"54 6","pages":""},"PeriodicalIF":1.5,"publicationDate":"2024-10-19","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"142451065","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":4,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
Pub Date : 2024-10-15DOI: 10.1007/s13538-024-01615-7
S. Somorendro Singh
We evaluate thermodynamic equation of state (EOS) under one loop correction at finite chemical potential. Due to the presence of the chemical potential in the one loop correction, there is change in formation of bubble/droplet of quark-gluon plasma (QGP) and this chemical potential has the effect on the evaluation of EOS. The effect is particularly studied at the values of quark and gluon parametrization ({gamma }_{q} = 1/8) and (12{gamma }_{q} le {gamma }_{g} le 16{gamma }_{q}) at which the equilibrating bubbles/droplets sizes are obtained. The study indicates that the dynamics of the quark, anti-quark, and gluon fluids with the presence of chemical potential improves the results of the EOS from the earlier result of thermodynamic EOS without the chemical potential. It means that the effect of chemical potential in one loop correction cannot be neglected in the bubble/droplet formation of quark-gluon plasma and this chemical potential can signify the presence of a large number of charge particles in the earlier universe formation.
我们评估了有限化学势下单圈修正的热力学状态方程(EOS)。由于一环修正中化学势的存在,夸克-胶子等离子体(QGP)气泡/液滴的形成发生了变化,这种化学势对 EOS 的评估产生了影响。特别研究了夸克和胶子参数化值({gamma }_{q} = 1/8)和(12{gamma }_{q} le {gamma }_{g} le 16{gamma }_{q})的影响,在这些参数化值上可以得到平衡气泡/液滴的大小。研究表明,存在化学势的夸克流体、反夸克流体和胶子流体的动力学EOS结果比之前不存在化学势的热力学EOS结果要好。这意味着在夸克-胶子等离子体的气泡/液滴形成过程中,化学势的单圈修正效应不容忽视,而且这种化学势可以表明在早期宇宙形成过程中存在大量的电荷粒子。
{"title":"Thermodynamic Equation of State Under One Loop Correction at Finite Chemical Potential","authors":"S. Somorendro Singh","doi":"10.1007/s13538-024-01615-7","DOIUrl":"10.1007/s13538-024-01615-7","url":null,"abstract":"<div><p>We evaluate thermodynamic equation of state (EOS) under one loop correction at finite chemical potential. Due to the presence of the chemical potential in the one loop correction, there is change in formation of bubble/droplet of quark-gluon plasma (QGP) and this chemical potential has the effect on the evaluation of EOS. The effect is particularly studied at the values of quark and gluon parametrization <span>({gamma }_{q} = 1/8)</span> and <span>(12{gamma }_{q} le {gamma }_{g} le 16{gamma }_{q})</span> at which the equilibrating bubbles/droplets sizes are obtained. The study indicates that the dynamics of the quark, anti-quark, and gluon fluids with the presence of chemical potential improves the results of the EOS from the earlier result of thermodynamic EOS without the chemical potential. It means that the effect of chemical potential in one loop correction cannot be neglected in the bubble/droplet formation of quark-gluon plasma and this chemical potential can signify the presence of a large number of charge particles in the earlier universe formation.</p></div>","PeriodicalId":499,"journal":{"name":"Brazilian Journal of Physics","volume":"54 6","pages":""},"PeriodicalIF":1.5,"publicationDate":"2024-10-15","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"142438724","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":4,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
Pub Date : 2024-10-14DOI: 10.1007/s13538-024-01628-2
Marcus Vinicius Santos da Silva, Denis Gilbert Francis David, Victor Mancir da Silva Santana, Christian Godet
Diffuse reflectance spectroscopy (DRS) and photoacoustic absorption spectroscopy (PAS) are investigated in model systems that mimic topological structures found in vegetal fibers, e.g., made of oriented hollow channels. Among this wide family, the shiny optical aspect of Golden grass stems has motivated detailed investigations of their chemical composition, microstructure, and electronic properties. In this work, diffuse reflectance and absorption of a photon flux within a collection of parallel hollow fibers are addressed using 2D optical models, neglecting interface scattering. Analytical results obtained for hollow square tube (HST) and plane parallel membrane (PPM) arrays are validated by full ray-tracing calculations. Optical paths with multiple reflection/refraction events at air-fiber interfaces selectively enhance DRS and PAS intensities and thus explain the shiny golden-like aspect of Golden grass, in contrast with specular reflectance calculated from the complex refractive index. A simple method is proposed to retrieve the complex dielectric function of fiber walls from the measured PAS and DRS intensities, using analytical equations obtained with hollow fiber topologies, in a low-energy region not easily accessible by photoelectron energy loss spectroscopy.
在模拟植物纤维拓扑结构的模型系统中研究了漫反射光谱(DRS)和光声吸收光谱(PAS),例如由定向中空通道组成的模型系统。在这一广泛的家族中,金草茎闪亮的光学特性促使人们对其化学成分、微观结构和电子特性进行详细研究。在这项研究中,我们使用二维光学模型,忽略了界面散射,研究了平行中空纤维集合内光子通量的漫反射和吸收。中空方管(HST)和平面平行膜(PPM)阵列的分析结果通过完整的光线跟踪计算得到了验证。在空气-纤维界面上具有多次反射/折射事件的光路选择性地增强了 DRS 和 PAS 强度,从而解释了黄金草闪亮的金色光泽,这与根据复折射率计算的镜面反射形成鲜明对比。本文提出了一种简单的方法,利用中空纤维拓扑结构获得的分析方程,在光电子能量损失光谱不易获取的低能区,从测量到的 PAS 和 DRS 强度中检索纤维壁的复合介电函数。
{"title":"Dielectric Function of Oriented Hollow Vegetal Fibers Retrieved from XPS, Diffuse Reflection, and Photoacoustic Spectroscopies","authors":"Marcus Vinicius Santos da Silva, Denis Gilbert Francis David, Victor Mancir da Silva Santana, Christian Godet","doi":"10.1007/s13538-024-01628-2","DOIUrl":"10.1007/s13538-024-01628-2","url":null,"abstract":"<div><p>Diffuse reflectance spectroscopy (DRS) and photoacoustic absorption spectroscopy (PAS) are investigated in model systems that mimic topological structures found in vegetal fibers, e.g., made of oriented hollow channels. Among this wide family, the shiny optical aspect of Golden grass stems has motivated detailed investigations of their chemical composition, microstructure, and electronic properties. In this work, diffuse reflectance and absorption of a photon flux within a collection of parallel hollow fibers are addressed using 2D optical models, neglecting interface scattering. Analytical results obtained for hollow square tube (HST) and plane parallel membrane (PPM) arrays are validated by full ray-tracing calculations. Optical paths with multiple reflection/refraction events at air-fiber interfaces selectively enhance DRS and PAS intensities and thus explain the shiny golden-like aspect of Golden grass, in contrast with specular reflectance calculated from the complex refractive index. A simple method is proposed to retrieve the complex dielectric function of fiber walls from the measured PAS and DRS intensities, using analytical equations obtained with hollow fiber topologies, in a low-energy region not easily accessible by photoelectron energy loss spectroscopy.</p></div>","PeriodicalId":499,"journal":{"name":"Brazilian Journal of Physics","volume":"54 6","pages":""},"PeriodicalIF":1.5,"publicationDate":"2024-10-14","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"142434925","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":4,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
Pub Date : 2024-10-12DOI: 10.1007/s13538-024-01629-1
M. N. de Oliveira, C. E. Navia, A. A. Nepomuceno
We show evidence of particle acceleration at GeV energies associated directly with protons from the prompt emission of a long-duration M6-class solar flare on July 17, 2023, rather than from protons acceleration by shocks from its associated coronal mass ejection (CME), which erupted with a speed of 1342 km/s. Solar energetic particles (SEP) accelerated by the blast have reached Earth, up to an almost S3 (strong) category of a radiation storm on the NOAA scale. Also, we show a temporal correlation between the fast increase in the GOES-16 proton flux and the ground-level count rate excess of the New-Tupi muon detector, located in the central region of the South Atlantic Anomaly (SAA) an area where the Earth’s magnetic field is anomalously weak. A Monte Carlo spectral analysis based on muon excess at New-Tupi is consistent with the acceleration of electrons and protons (ions) up to relativistic energies (GeV energy range) in the impulsive phase of the flare. In addition, we present another two marginal particle excesses (with low confidence) at ground-level detectors in correlation with the solar flare prompt emission.
{"title":"Prompt Emission of Relativistic Protons up to GeV Energies from M6.4-Class Solar Flare on July 17, 2023","authors":"M. N. de Oliveira, C. E. Navia, A. A. Nepomuceno","doi":"10.1007/s13538-024-01629-1","DOIUrl":"10.1007/s13538-024-01629-1","url":null,"abstract":"<div><p>We show evidence of particle acceleration at GeV energies associated directly with protons from the prompt emission of a long-duration M6-class solar flare on July 17, 2023, rather than from protons acceleration by shocks from its associated coronal mass ejection (CME), which erupted with a speed of 1342 km/s. Solar energetic particles (SEP) accelerated by the blast have reached Earth, up to an almost S3 (strong) category of a radiation storm on the NOAA scale. Also, we show a temporal correlation between the fast increase in the GOES-16 proton flux and the ground-level count rate excess of the New-Tupi muon detector, located in the central region of the South Atlantic Anomaly (SAA) an area where the Earth’s magnetic field is anomalously weak. A Monte Carlo spectral analysis based on muon excess at New-Tupi is consistent with the acceleration of electrons and protons (ions) up to relativistic energies (GeV energy range) in the impulsive phase of the flare. In addition, we present another two marginal particle excesses (with low confidence) at ground-level detectors in correlation with the solar flare prompt emission.</p></div>","PeriodicalId":499,"journal":{"name":"Brazilian Journal of Physics","volume":"54 6","pages":""},"PeriodicalIF":1.5,"publicationDate":"2024-10-12","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"142411492","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":4,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
Pub Date : 2024-10-12DOI: 10.1007/s13538-024-01630-8
Marlon S. Ribeiro, Karen C. Ribeiro, Rozane de F. Turchiello, Sergio L. Gómez
Plasmonic nanoparticles exhibit remarkable photothermal properties, making them valuable in various fields such as renewable energy and medicine. These photothermal properties depend on several factors, including the type of noble metal, particle size, and the stabilizing layer. This study investigates the photothermal properties of colloidal silver nanoparticles synthesized photochemically using UV LEDs. Silver nanoparticles capped with citrate and a combination of citrate and polyvinylpyrrolidone (PVP) were prepared. While the nanoparticle size remained unaffected by the amount of citrate, the nonlinear refractive index did show dependence. As the citrate concentration increased, the nonlinear refractive index decreased. Additionally, increasing the amount of PVP not only reduces the nanoparticle size—suggesting a reverse Ostwald ripening process induced by UV light—but also leads to a diminished photothermal response.
等离子纳米粒子具有显著的光热特性,因此在可再生能源和医学等多个领域具有重要价值。这些光热特性取决于多个因素,包括贵金属类型、粒度和稳定层。本研究探讨了利用紫外线 LED 光化学合成的胶体银纳米粒子的光热特性。研究人员制备了以柠檬酸盐和柠檬酸盐与聚乙烯吡咯烷酮(PVP)组合封端的银纳米粒子。虽然纳米粒子的大小不受柠檬酸盐用量的影响,但非线性折射率却与之相关。随着柠檬酸盐浓度的增加,非线性折射率下降。此外,增加 PVP 的用量不仅会减小纳米粒子的尺寸--这表明紫外线诱导了反向奥斯特瓦尔德熟化过程,而且还会导致光热响应减弱。
{"title":"Photothermal Properties of Plasmonic Nanofluids Containing Ag Nanoparticles Under Off-Resonant Excitation: The Influence of Capping Agents","authors":"Marlon S. Ribeiro, Karen C. Ribeiro, Rozane de F. Turchiello, Sergio L. Gómez","doi":"10.1007/s13538-024-01630-8","DOIUrl":"10.1007/s13538-024-01630-8","url":null,"abstract":"<div><p>Plasmonic nanoparticles exhibit remarkable photothermal properties, making them valuable in various fields such as renewable energy and medicine. These photothermal properties depend on several factors, including the type of noble metal, particle size, and the stabilizing layer. This study investigates the photothermal properties of colloidal silver nanoparticles synthesized photochemically using UV LEDs. Silver nanoparticles capped with citrate and a combination of citrate and polyvinylpyrrolidone (PVP) were prepared. While the nanoparticle size remained unaffected by the amount of citrate, the nonlinear refractive index did show dependence. As the citrate concentration increased, the nonlinear refractive index decreased. Additionally, increasing the amount of PVP not only reduces the nanoparticle size—suggesting a reverse Ostwald ripening process induced by UV light—but also leads to a diminished photothermal response.</p></div>","PeriodicalId":499,"journal":{"name":"Brazilian Journal of Physics","volume":"54 6","pages":""},"PeriodicalIF":1.5,"publicationDate":"2024-10-12","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"142411488","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":4,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
Pub Date : 2024-10-08DOI: 10.1007/s13538-024-01625-5
Emine Avşar Aydin
Breast cancer ranks as the second most common cause of mortality among women globally, with the potential to increase survival rates by 97% through early detection. This study focuses on developing an innovative triple-band microstrip patch antenna designed to operate within the 2–6 GHz frequency spectrum. Simulation tests were conducted to evaluate its efficacy in early breast cancer detection. The antenna, constructed from copper tape and five different substrates (Felt, FR4, PET, PLA, TPU), was chosen considering its advantages for various applications. This design prioritizes wearer comfort while ensuring functionality and allows for producing antenna structures in desired geometries using 3D printing, even in complex configurations. With a general size of 30 × 30 mm2, the antenna underwent analyses on tumor-free models with tumors of different shapes and sizes, and additionally, to evaluate the performance of multiple antennas in detecting cancers, tumor models with 2 and 3 antenna numbers were analyzed in a total of six different breast scenarios. Critical performance parameters such as specific absorption rate (SAR), return loss (S11), and voltage standing wave ratio (VSWR) were obtained for each generated model. Simulation outcomes indicated SAR values within the permissible threshold for medical applications. Moreover, VSWR values maintained acceptability, while variations in return losses were contingent upon tumor dimensions, location, and the number of antennas used. Furthermore, the antenna’s adaptability to bending was scrutinized through bending analyses, affirming its robustness, and sustained operational capability. One of the significant contributions of the study is the utilization of recyclable filaments such as PLA, TPU, and Protopasta in experimental investigations, providing a pathway for producing environmentally friendly and flexible antennas and breast phantoms. This study offers a way to develop more sensitive and reliable breast cancer screening and early diagnosis tools.
{"title":"A Novel Triple-Band Microstrip Patch Antenna for Breast Cancer Detection Systems Fabricated with Recyclable Filaments","authors":"Emine Avşar Aydin","doi":"10.1007/s13538-024-01625-5","DOIUrl":"10.1007/s13538-024-01625-5","url":null,"abstract":"<div><p>Breast cancer ranks as the second most common cause of mortality among women globally, with the potential to increase survival rates by 97% through early detection. This study focuses on developing an innovative triple-band microstrip patch antenna designed to operate within the 2–6 GHz frequency spectrum. Simulation tests were conducted to evaluate its efficacy in early breast cancer detection. The antenna, constructed from copper tape and five different substrates (Felt, FR4, PET, PLA, TPU), was chosen considering its advantages for various applications. This design prioritizes wearer comfort while ensuring functionality and allows for producing antenna structures in desired geometries using 3D printing, even in complex configurations. With a general size of 30 × 30 mm<sup>2</sup>, the antenna underwent analyses on tumor-free models with tumors of different shapes and sizes, and additionally, to evaluate the performance of multiple antennas in detecting cancers, tumor models with 2 and 3 antenna numbers were analyzed in a total of six different breast scenarios. Critical performance parameters such as specific absorption rate (SAR), return loss (S11), and voltage standing wave ratio (VSWR) were obtained for each generated model. Simulation outcomes indicated SAR values within the permissible threshold for medical applications. Moreover, VSWR values maintained acceptability, while variations in return losses were contingent upon tumor dimensions, location, and the number of antennas used. Furthermore, the antenna’s adaptability to bending was scrutinized through bending analyses, affirming its robustness, and sustained operational capability. One of the significant contributions of the study is the utilization of recyclable filaments such as PLA, TPU, and Protopasta in experimental investigations, providing a pathway for producing environmentally friendly and flexible antennas and breast phantoms. This study offers a way to develop more sensitive and reliable breast cancer screening and early diagnosis tools.</p></div>","PeriodicalId":499,"journal":{"name":"Brazilian Journal of Physics","volume":"54 6","pages":""},"PeriodicalIF":1.5,"publicationDate":"2024-10-08","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"142410749","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":4,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
Pub Date : 2024-10-05DOI: 10.1007/s13538-024-01618-4
P. Bewyn Joseph, S. K. Suresh Babu, J. Godwin Christus Selvin, B. Sudharsan Bangaru
This study investigates the effects of lanthanum oxide (La₂O₃) and strontium oxide (SrO) on polyvinyl alcohol (PVA) polymer membranes. The PVA membranes, fabricated using an ultrasound-assisted casting method, include variations with (PVA-SrO), (PVA-La₂O₃), and a combination of both metal oxides (PVA-SrO-La₂O₃). X-ray diffraction (XRD) analysis reveals that these membranes exhibit a combination of semi-crystalline and amorphous properties, with the introduction of crystalline peaks due to the addition of SrO and La₂O₃. Electrical performance assessments, conducted using an I-V source meter and impedance spectroscopy, demonstrate that the metal oxide composite membranes showed improved performance. Mechanical properties were evaluated using Load–Displacement curves, where PVA-SrO-La₂O₃ exhibited the highest elongation with a value (ɛ) of 134, as measured by Young's modulus, and a resistance value of 12.230 kΩ.
{"title":"Effects of La2O3 and SrO on the Electrical and Mechanical Properties of Ultrasound-Assisted Cast Polyvinyl Alcohol (PVA) Polymer Membranes","authors":"P. Bewyn Joseph, S. K. Suresh Babu, J. Godwin Christus Selvin, B. Sudharsan Bangaru","doi":"10.1007/s13538-024-01618-4","DOIUrl":"10.1007/s13538-024-01618-4","url":null,"abstract":"<div><p>This study investigates the effects of lanthanum oxide (La₂O₃) and strontium oxide (SrO) on polyvinyl alcohol (PVA) polymer membranes. The PVA membranes, fabricated using an ultrasound-assisted casting method, include variations with (PVA-SrO), (PVA-La₂O₃), and a combination of both metal oxides (PVA-SrO-La₂O₃). X-ray diffraction (XRD) analysis reveals that these membranes exhibit a combination of semi-crystalline and amorphous properties, with the introduction of crystalline peaks due to the addition of SrO and La₂O₃. Electrical performance assessments, conducted using an I-V source meter and impedance spectroscopy, demonstrate that the metal oxide composite membranes showed improved performance. Mechanical properties were evaluated using Load–Displacement curves, where PVA-SrO-La₂O₃ exhibited the highest elongation with a value (ɛ) of 134, as measured by Young's modulus, and a resistance value of 12.230 kΩ.</p></div>","PeriodicalId":499,"journal":{"name":"Brazilian Journal of Physics","volume":"54 6","pages":""},"PeriodicalIF":1.5,"publicationDate":"2024-10-05","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"142410052","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":4,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
Pub Date : 2024-10-05DOI: 10.1007/s13538-024-01627-3
Darshan J. Jadav, R. R. Varasada, M. P. Trasadiya, S. M. Vyas, A. M. Vora
Copper selenide (Cu2Se) is a promising semiconductor with notable potential for optoelectronic and thermoelectric applications. This study investigates the impact of film thickness on the physical properties of Cu2Se thin films. Cu2Se thin films of varying thicknesses were synthesized using the thermal evaporation technique. These films were then analyzed for optical properties, structural characteristics, and surface morphology. Optical analysis was conducted using absorption spectra over a wavelength range of 200 to 900 nm. From these spectra, we determined key optical parameters such as the energy band gap (Eg), extinction coefficient (k), and refractive index for films of different thicknesses. Dielectric properties were evaluated, allowing us to calculate the dielectric constant and dielectric loss for various film thicknesses. Additionally, current–voltage (I-V) characteristics and Raman spectroscopy were performed, and the results are presented and discussed in detail.
{"title":"Synthesize and Investigate Structural, Surface Morphology, Optical, and Electrical Characterization of Cu2Se Thin Films by Thermal Evaporation Technique","authors":"Darshan J. Jadav, R. R. Varasada, M. P. Trasadiya, S. M. Vyas, A. M. Vora","doi":"10.1007/s13538-024-01627-3","DOIUrl":"10.1007/s13538-024-01627-3","url":null,"abstract":"<div><p>Copper selenide (Cu<sub>2</sub>Se) is a promising semiconductor with notable potential for optoelectronic and thermoelectric applications. This study investigates the impact of film thickness on the physical properties of Cu<sub>2</sub>Se thin films. Cu<sub>2</sub>Se thin films of varying thicknesses were synthesized using the thermal evaporation technique. These films were then analyzed for optical properties, structural characteristics, and surface morphology. Optical analysis was conducted using absorption spectra over a wavelength range of 200 to 900 nm. From these spectra, we determined key optical parameters such as the energy band gap (<i>E</i><sub>g</sub>), extinction coefficient (<i>k</i>), and refractive index for films of different thicknesses. Dielectric properties were evaluated, allowing us to calculate the dielectric constant and dielectric loss for various film thicknesses. Additionally, current–voltage (I-V) characteristics and Raman spectroscopy were performed, and the results are presented and discussed in detail.</p></div>","PeriodicalId":499,"journal":{"name":"Brazilian Journal of Physics","volume":"54 6","pages":""},"PeriodicalIF":1.5,"publicationDate":"2024-10-05","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"142410082","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":4,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
Pub Date : 2024-10-04DOI: 10.1007/s13538-024-01626-4
M. Mahmoodi, A. A. Rajabi
In this paper, the fusion cross sections of 6He + 197Au and 8He + 197Au systems have been investigated at center-of-mass energies from below to above the Coulomb barrier, 14.5 to 60.0 and 15.0 to 29.0 MeV, respectively. The required nucleus-nucleus potential has been calculated by using the Monte Carlo method, applying four different phenomenological density distributions. The results obtained from both systems reveal that considering the suitable halo structure for distribution of the nuclear matter increases the height of fusion barrier, giving a better agreement with the experimental data. In addition, by using the generalized function of the two-parameter Fermi distribution for the nuclear density of the halo nucleons of 6He and 8He nuclei, a better agreement with experimental data was achieved. Using the same potential with the above-mentioned density distributions, we also studied the elastic scattering cross sections for the 6He + 197Au system measured at Elab. = 29 MeV and Elab. = 40 MeV, with similar good results as for the fusion reaction.
{"title":"Investigation of the Nuclear Matter Distribution in the 6He and 8HeNuclei","authors":"M. Mahmoodi, A. A. Rajabi","doi":"10.1007/s13538-024-01626-4","DOIUrl":"10.1007/s13538-024-01626-4","url":null,"abstract":"<div><p>In this paper, the fusion cross sections of <sup>6</sup>He + <sup>197</sup>Au and <sup>8</sup>He + <sup>197</sup>Au systems have been investigated at center-of-mass energies from below to above the Coulomb barrier, 14.5 to 60.0 and 15.0 to 29.0 MeV, respectively. The required nucleus-nucleus potential has been calculated by using the Monte Carlo method, applying four different phenomenological density distributions. The results obtained from both systems reveal that considering the suitable halo structure for distribution of the nuclear matter increases the height of fusion barrier, giving a better agreement with the experimental data. In addition, by using the generalized function of the two-parameter Fermi distribution for the nuclear density of the halo nucleons of <sup>6</sup>He and <sup>8</sup>He nuclei, a better agreement with experimental data was achieved. Using the same potential with the above-mentioned density distributions, we also studied the elastic scattering cross sections for the <sup>6</sup>He + <sup>197</sup>Au system measured at <i>E</i><sub>lab.</sub> = 29 MeV and <i>E</i><sub>lab.</sub> = 40 MeV, with similar good results as for the fusion reaction.</p></div>","PeriodicalId":499,"journal":{"name":"Brazilian Journal of Physics","volume":"54 6","pages":""},"PeriodicalIF":1.5,"publicationDate":"2024-10-04","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"142409819","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":4,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}