{"title":"Tunable optical properties of silicon nanowires for photovoltaic devices","authors":"Vrishty Kundu, Omita Nanda, Dalip Singh Mehta, Kanchan Saxena","doi":"10.1007/s12648-026-04055-y","DOIUrl":"10.1007/s12648-026-04055-y","url":null,"abstract":"<div><p>In recent times, silicon nanowires (Si-NWs) have been primarily used as an inorganic layer in producing hybrid solar cells, mainly because of their enhanced optical absorption characteristics. This study utilizes the metal-assisted chemical etching (MACE) technology to produce vertically aligned, long Si-NWs with a high aspect ratio. The role of metal nanoparticles in the MACE technique was investigated, and the structure optimization process was performed by altering the etching time. Observations indicate that the concentration of metal solution influences both the size and spacing of Si-NWs, whereas the etching time affects the length of the Si-NWs. The optical characteristics of the Si-NWs were also examined utilizing the experimental diffuse reflection spectra. In addition, a 3D finite difference time domain (FDTD) simulation was conducted to analyse and compare the absorption spectra of the created Si-NWs with the experimental findings. Systematic analysis of absorption as a function of the geometry of nanowires (NWs) indicates that as the length and the diameter increase it demonstrates notable anti-reflection properties. This can be attributed to the larger surface area of the NWs and increased roughness/disordered surface. Hence, the work concisely illustrates the essential significance of improved absorption of Si-NWs in attaining optimal efficiency in hybrid solar cell applications.</p></div>","PeriodicalId":584,"journal":{"name":"Indian Journal of Physics","volume":"100 10","pages":"4405 - 4416"},"PeriodicalIF":1.7,"publicationDate":"2026-05-12","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"148909435","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}
{"title":"Generation of plasmon modes at chiral- black phosphorus interface","authors":"M. Nadeem, M. Umair, A. Ghaffar, Imran Shakir","doi":"10.1007/s12648-026-04054-z","DOIUrl":"10.1007/s12648-026-04054-z","url":null,"abstract":"<div><p>This study presents a numerical analysis at the planar interface of chiral-black phosphorus (BP) and investigates the characteristics of surface plasmon polaritons (SPPs) in the terahertz (THz) spectral region. The extended electromagnetic (EM) wave theory is employed for the numerical calculations, while the impedance boundary condition approach is used to derive the dispersion relation. The results demonstrate that the strong anisotropic dispersion of BP gives direction-dependent plasmon modes. The normalized propagation constant (NPC) of plasmon modes is found to be highly sensitive to electron doping, number of BP layers, chirality, and the refractive index of the chiral medium for the conductivity components of BP along the zigzag <span>({(sigma }_{zz}))</span> and armchair <span>(({sigma}_{ac}))</span> directions. Moreover, the electromagnetic field propagation characteristics can be modified effectively by tuning both the chiral and BP parameters. The presented results can be used to fabricate tunable THz devices, providing an extra degree of freedom arising from the anisotropic conductivity of BP.</p></div>","PeriodicalId":584,"journal":{"name":"Indian Journal of Physics","volume":"100 10","pages":"4397 - 4403"},"PeriodicalIF":1.7,"publicationDate":"2026-05-07","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"148909478","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}
Ahmad Yusof Abdo Jamal, Nurul Shazana Abdul Hamid, Idahwati Sarudin
{"title":"Pattern of solar activity levels and their effects on galactic cosmic ray particle fluxes throughout 23rd and 24th solar cycle","authors":"Ahmad Yusof Abdo Jamal, Nurul Shazana Abdul Hamid, Idahwati Sarudin","doi":"10.1007/s12648-026-03984-y","DOIUrl":"10.1007/s12648-026-03984-y","url":null,"abstract":"<div><p>Since the discovery of sunspots on the Sun’s surface, solar sunspot numbers (SSN) have been widely used to study solar activity (SA) and its cyclical behaviour. These cycles arise from processes in the Sun’s core and surface, which modulate SA intensity over time. Researchers commonly divide each solar cycle (SC) into distinct phases—minimum, inclining, maximum, and declining—each characterised by different activity levels. However, few studies have systematically characterised SA intensity across these phases, particularly in relation to space weather events and cosmic ray (CR) fluxes, both of which are strongly influenced by SA. This study investigated the variation of SSN, the F10.7 index, solar flare and geomagnetic storm frequencies, and CR particle intensities across SC23 and SC24. SC phases were defined using SSN and F10.7 data, after which all variables were composited by phase and analysed using phase-averaged values. A percentage difference analysis was also conducted to assess variability between the two cycles, while Spearman correlation was employed to evaluate the alignment between SA proxies, space weather, and CR particle fluxes. The results revealed coherent trends in SA proxies across the SC phases, with SC23 showing higher activity levels than SC24. Solar flare frequency aligned closely with SA phases, while geomagnetic storms showed a lag of one to two phases. Proton flux, helium flux, and neutron counts exhibited inverse correlations with SA proxies due to solar wind modulation, although solar energetic particles introduced minor irregularities. The study recommends further use of phase-based approaches in SA research to improve understanding of the Sun’s influence on space weather and CR variability.</p></div>","PeriodicalId":584,"journal":{"name":"Indian Journal of Physics","volume":"100 6","pages":"2165 - 2178"},"PeriodicalIF":1.7,"publicationDate":"2026-05-07","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"148281080","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}
Shengyi Liu, Duan Gao, Ying Zhu, Xin Chen, Xilai Zhang, Shizhuang Guo, Tianai Zhu, Li Wang, Wenbin Song, Haoyu Liu
{"title":"Synthesis and long afterglow characteristics of Zn2GeO4:Mn2+, Pr3+ phosphors optimized by rotational composite\u0000design","authors":"Shengyi Liu, Duan Gao, Ying Zhu, Xin Chen, Xilai Zhang, Shizhuang Guo, Tianai Zhu, Li Wang, Wenbin Song, Haoyu Liu","doi":"10.1007/s12648-026-04051-2","DOIUrl":"10.1007/s12648-026-04051-2","url":null,"abstract":"<div><p>To maximize the effective afterglow time of Zn<sub>2</sub>GeO<sub>4</sub>: Mn<sup>2+</sup>, Pr<sup>3+</sup> phosphors, a second general rotational composite design strategy was employed to optimize the concentrations of Mn<sup>2+</sup> and Pr<sup>3+</sup>. A quadratic regression equation model was established between the doping concentration of rare-earth ions Mn<sup>2+</sup> and Pr<sup>3+</sup> and the effective afterglow time. The theoretical optimal value of the effective afterglow time was precisely solved through a genetic algorithm. Using the high-temperature solid-state method, we successfully synthesized the phosphor Zn<sub>2</sub>GeO<sub>4</sub>: 0.5 mol% Mn<sup>2+</sup>, 2.3 mol% Pr<sup>3+</sup> with the optimal doping concentration and performed detailed characterization and analysis. The results show that doping with Mn<sup>2+</sup> and Pr<sup>3+</sup> significantly improved the long afterglow properties of Zn<sub>2</sub>GeO<sub>4</sub>. Under 328 nm excitation, a characteristic emission peak at 535 nm was observed, and Zn<sub>2</sub>GeO<sub>4</sub>: Mn<sup>2+</sup>/Pr<sup>3+</sup> exhibited an emission band corresponding to the <sup>4</sup>T<sub>1</sub> → <sup>6</sup>A<sub>1</sub> transition of Mn<sup>2+</sup>. In the Zn<sub>2</sub>GeO<sub>4</sub>: Mn<sup>2+</sup>/Pr<sup>3+</sup> phosphor, Pr<sup>3+</sup> substitution of Zn<sup>2+</sup> generated positive defects of Pr<sup>′</sup><sub>Zn</sub> and vacancy defects of V<sup>′′</sup><sub>Zn</sub>. Furthermore, we measured the thermoluminescent properties of the optimal phosphor, calculating the trap depth to be 0.4608 eV, and discussed the relevant characteristics of long afterglow luminescence.</p></div>","PeriodicalId":584,"journal":{"name":"Indian Journal of Physics","volume":"100 9","pages":"3925 - 3934"},"PeriodicalIF":1.7,"publicationDate":"2026-05-06","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"148751121","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}