Pub Date : 2025-12-18DOI: 10.3103/S1068335625603711
A. B. Loginov, R. R. Ismagilov, N. R. Arutyunyan, I. V. Sapkov, E. D. Obraztsova, A. N. Chulkov
Films consisting of arrays of MoS2 crystallites (nanowalls), which are oriented perpendicular to the substrate, attract the attention of researchers as a promising material for creating photonic, optoelectronic, and sensor devices. The additional ordering of the structure of such layers by orientating nanowalls along a certain direction in the substrate plane allows creation of materials with unique characteristics. For their formation, we use the method of selective laser ablation of MoS2 films formed via deposition from the vapor phase and consisting of nanowalls on the surfaces of silicon substrates. The parameters of a laser pulse, which lead to the emergence of the maximum degree of ordering of nanowalls in the film, are determined. The photoluminescence (PL) and Raman scattering (RS) have been studied. In particular, the degree of polarization of PL and RS signals was determined as a function of the angle between a selected direction in the film plane and the polarization of exciting radiation. It was revealed that exactly nanowalls are responsible for the optical properties of such films but not the underlying film. The possible applications of the materials obtained using the selective ablation method in photonics are discussed.
{"title":"Formation of Oriented MoS2 Nanowalls by Selective Laser Ablation and Their Properties","authors":"A. B. Loginov, R. R. Ismagilov, N. R. Arutyunyan, I. V. Sapkov, E. D. Obraztsova, A. N. Chulkov","doi":"10.3103/S1068335625603711","DOIUrl":"10.3103/S1068335625603711","url":null,"abstract":"<p>Films consisting of arrays of MoS<sub>2</sub> crystallites (nanowalls), which are oriented perpendicular to the substrate, attract the attention of researchers as a promising material for creating photonic, optoelectronic, and sensor devices. The additional ordering of the structure of such layers by orientating nanowalls along a certain direction in the substrate plane allows creation of materials with unique characteristics. For their formation, we use the method of selective laser ablation of MoS<sub>2</sub> films formed via deposition from the vapor phase and consisting of nanowalls on the surfaces of silicon substrates. The parameters of a laser pulse, which lead to the emergence of the maximum degree of ordering of nanowalls in the film, are determined. The photoluminescence (PL) and Raman scattering (RS) have been studied. In particular, the degree of polarization of PL and RS signals was determined as a function of the angle between a selected direction in the film plane and the polarization of exciting radiation. It was revealed that exactly nanowalls are responsible for the optical properties of such films but not the underlying film. The possible applications of the materials obtained using the selective ablation method in photonics are discussed.</p>","PeriodicalId":503,"journal":{"name":"Bulletin of the Lebedev Physics Institute","volume":"52 7","pages":"S735 - S745"},"PeriodicalIF":0.7,"publicationDate":"2025-12-18","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"145772245","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 : 2025-12-18DOI: 10.3103/S0027134925700985
I. I. Mokhov, I. R. Eremin
This paper presents an analysis of spring atmospheric blockings (SAB) in the Northern Hemisphere (NH) for the period 1992–2023. The results of the analysis indicate a significant increase in blocking activity in the NH atmosphere in recent decades. This trend is observed against the background of a general increase in near-surface temperature in the NH during the spring seasons. The following SAB parameters were used in the study: quantity, average duration, total duration, intensity, and size. Statistically significant increases were obtained for the total duration, quantity, and size of SAB, associated with an increase in the average spring near-surface temperature in the NH.
{"title":"Spring Atmospheric Blockings in the Northern Hemisphere: Changes in Recent Decades (1992–2023)","authors":"I. I. Mokhov, I. R. Eremin","doi":"10.3103/S0027134925700985","DOIUrl":"10.3103/S0027134925700985","url":null,"abstract":"<p>This paper presents an analysis of spring atmospheric blockings (SAB) in the Northern Hemisphere (NH) for the period 1992–2023. The results of the analysis indicate a significant increase in blocking activity in the NH atmosphere in recent decades. This trend is observed against the background of a general increase in near-surface temperature in the NH during the spring seasons. The following SAB parameters were used in the study: quantity, average duration, total duration, intensity, and size. Statistically significant increases were obtained for the total duration, quantity, and size of SAB, associated with an increase in the average spring near-surface temperature in the NH.</p>","PeriodicalId":711,"journal":{"name":"Moscow University Physics Bulletin","volume":"80 5","pages":"943 - 949"},"PeriodicalIF":0.4,"publicationDate":"2025-12-18","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"145772262","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 : 2025-12-18DOI: 10.1016/j.physletb.2025.140109
Mengke Li, Gail C. Mclaughlin, Rebecca Surman
{"title":"Implications of a Weakening N = 126 Shell Closure Away from Stability for r-Process Astrophysical Conditions","authors":"Mengke Li, Gail C. Mclaughlin, Rebecca Surman","doi":"10.1016/j.physletb.2025.140109","DOIUrl":"https://doi.org/10.1016/j.physletb.2025.140109","url":null,"abstract":"","PeriodicalId":20162,"journal":{"name":"Physics Letters B","volume":"1 1","pages":""},"PeriodicalIF":4.4,"publicationDate":"2025-12-18","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"145784683","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":2,"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 : 2025-12-18DOI: 10.1051/0004-6361/202557558
Aristeidis Polychronakis, Ioannis Liodakis, Anastasia Glykopoulou, Dmitry Blinov, Iván Agudo, Svetlana G. Jorstad, Beatriz Agís-González, Sara Capecchiacci, Alberto Floris, Sebastian Kielhmann, John A. Kypriotakis, Dimitrios A. Langis, Nikos Mandarakas, Karan Pal, Francisco J. Aceituno, Giacomo Bonnoli, Víctor Casanova, Gabriel Emery, Juan Escudero Pedrosa, Jorge Otero-Santos, Daniel Morcuende, Alfredo Sota, Vilppu Piirola
Blazars are known for their extreme variability across the electromagnetic spectrum. Variability at very short timescales can allow us to discriminate between competing models. This is particularly true for polarization variability, which allows us to probe particle acceleration and high-energy emission models in blazars. Here we present results from the first pilot study of intra-night optical polarization monitoring conducted using RoboPol at the Skinakas Observatory; these results are supplemented by observations from the Calar Alto, Perkins, and Sierra Nevada observatories. Our results show that while variability patterns can vary widely between sources, variability on timescales as short as minutes is prevalent in blazar jets. The amplitudes of the variations are typically small, a few percent for the polarization degree and less than 20° for the polarization angle, pointing to a significant contribution to the optical emission from a turbulent magnetic field component. The overall stability of the polarization angle over time points to a preferred magnetic field orientation.
{"title":"Intra-night optical polarization monitoring of blazars","authors":"Aristeidis Polychronakis, Ioannis Liodakis, Anastasia Glykopoulou, Dmitry Blinov, Iván Agudo, Svetlana G. Jorstad, Beatriz Agís-González, Sara Capecchiacci, Alberto Floris, Sebastian Kielhmann, John A. Kypriotakis, Dimitrios A. Langis, Nikos Mandarakas, Karan Pal, Francisco J. Aceituno, Giacomo Bonnoli, Víctor Casanova, Gabriel Emery, Juan Escudero Pedrosa, Jorge Otero-Santos, Daniel Morcuende, Alfredo Sota, Vilppu Piirola","doi":"10.1051/0004-6361/202557558","DOIUrl":"https://doi.org/10.1051/0004-6361/202557558","url":null,"abstract":"Blazars are known for their extreme variability across the electromagnetic spectrum. Variability at very short timescales can allow us to discriminate between competing models. This is particularly true for polarization variability, which allows us to probe particle acceleration and high-energy emission models in blazars. Here we present results from the first pilot study of intra-night optical polarization monitoring conducted using RoboPol at the Skinakas Observatory; these results are supplemented by observations from the Calar Alto, Perkins, and Sierra Nevada observatories. Our results show that while variability patterns can vary widely between sources, variability on timescales as short as minutes is prevalent in blazar jets. The amplitudes of the variations are typically small, a few percent for the polarization degree and less than 20° for the polarization angle, pointing to a significant contribution to the optical emission from a turbulent magnetic field component. The overall stability of the polarization angle over time points to a preferred magnetic field orientation.","PeriodicalId":8571,"journal":{"name":"Astronomy & Astrophysics","volume":"3 1","pages":""},"PeriodicalIF":6.5,"publicationDate":"2025-12-18","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"145784706","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":2,"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 : 2025-12-18DOI: 10.1016/j.ascom.2025.101051
D. Gasparri , L. Morelli , U. Battino , J. Méndez-Abreu , A. de Lorenzo-Cáceres
The increasing availability of high-quality optical and near-infrared spectroscopic data, as well as advances in modelling techniques, have greatly expanded the scientific potential of spectroscopic studies. However, the software tools needed to exploit this potential often remain fragmented across multiple specialised packages, requiring scripting skills and manual integration to handle complex workflows. In this paper we present SPAN (SPectral ANalysis), a cross-platform, Python-based Graphical User Interface (GUI) software that integrates the essential steps of the modern spectroscopic workflow within a single, user-friendly environment. SPAN provides a coherent framework that unifies data preparation, spectral processing, and analysis tasks, using the pPXF software as its core engine for full spectral fitting. SPAN allows users to extract 1D spectra from FITS images and datacubes, perform spectral processing (e.g. Doppler correction, continuum modelling, denoising), and carry out detailed analyses, including equivalent width measurements, stellar and gas kinematics, and stellar population studies. It runs natively on Windows, Linux, macOS, and Android, and is fully task-driven, requiring no prior coding experience. We validate SPAN by comparing its output with existing pipelines and literature studies. By offering a flexible, accessible, and well integrated environment, SPAN simplifies and accelerates the spectral analysis workflow, while maintaining scientific accuracy.
{"title":"SPAN: A cross-platform Python GUI software for optical and near-infrared spectral analysis","authors":"D. Gasparri , L. Morelli , U. Battino , J. Méndez-Abreu , A. de Lorenzo-Cáceres","doi":"10.1016/j.ascom.2025.101051","DOIUrl":"10.1016/j.ascom.2025.101051","url":null,"abstract":"<div><div>The increasing availability of high-quality optical and near-infrared spectroscopic data, as well as advances in modelling techniques, have greatly expanded the scientific potential of spectroscopic studies. However, the software tools needed to exploit this potential often remain fragmented across multiple specialised packages, requiring scripting skills and manual integration to handle complex workflows. In this paper we present <span>SPAN</span> (SPectral ANalysis), a cross-platform, Python-based Graphical User Interface (GUI) software that integrates the essential steps of the modern spectroscopic workflow within a single, user-friendly environment. SPAN provides a coherent framework that unifies data preparation, spectral processing, and analysis tasks, using the pPXF software as its core engine for full spectral fitting. SPAN allows users to extract 1D spectra from FITS images and datacubes, perform spectral processing (e.g. Doppler correction, continuum modelling, denoising), and carry out detailed analyses, including equivalent width measurements, stellar and gas kinematics, and stellar population studies. It runs natively on Windows, Linux, macOS, and Android, and is fully task-driven, requiring no prior coding experience. We validate SPAN by comparing its output with existing pipelines and literature studies. By offering a flexible, accessible, and well integrated environment, SPAN simplifies and accelerates the spectral analysis workflow, while maintaining scientific accuracy.</div></div>","PeriodicalId":48757,"journal":{"name":"Astronomy and Computing","volume":"55 ","pages":"Article 101051"},"PeriodicalIF":1.8,"publicationDate":"2025-12-18","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"145790289","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 : 2025-12-18DOI: 10.3103/S0027134925701061
M. S. Seidaliyeva, V. I. Denisov, I. P. Denisova
Within the framework of parameterized post-Maxwellian vacuum electrodynamics, the propagation of an X-ray and gamma radiation pulse through the electromagnetic field of a relativistically rotating pulsar is investigated. Expressions are obtained for the trajectory of this pulse and for the law of its motion from the point (mathbf{r}_{s}={x_{s},y_{s},z_{s}},) where at the moment of time (t=t_{s}) an X-ray or gamma-ray burst occurs, to the point (mathbf{r}_{d}={x_{s},y_{s},z_{d}},) where the detector of this radiation is located. In the case when the post-Maxwellian parameters of the theory differ, (eta_{1}neqeta_{2}), the time of nonlinear electrodynamic delay of electromagnetic signals carried by different normal modes is calculated. The change in the polarization state of the X-ray or gamma radiation pulse after passing through the electromagnetic field of a relativistically rotating pulsar is analyzed. The possibilities of observing the nonlinear effect of the electromagnetic field of a relativistically rotating pulsar on X-ray and gamma-ray pulses are discussed.
{"title":"Effect of Birefringence of Electromagnetic Radiation in the Field of a Relativistically Rotating Pulsar or Magnetar within the Framework of Nonlinear Vacuum Electrodynamics","authors":"M. S. Seidaliyeva, V. I. Denisov, I. P. Denisova","doi":"10.3103/S0027134925701061","DOIUrl":"10.3103/S0027134925701061","url":null,"abstract":"<p>Within the framework of parameterized post-Maxwellian vacuum electrodynamics, the propagation of an X-ray and gamma radiation pulse through the electromagnetic field of a relativistically rotating pulsar is investigated. Expressions are obtained for the trajectory of this pulse and for the law of its motion from the point <span>(mathbf{r}_{s}={x_{s},y_{s},z_{s}},)</span> where at the moment of time <span>(t=t_{s})</span> an X-ray or gamma-ray burst occurs, to the point <span>(mathbf{r}_{d}={x_{s},y_{s},z_{d}},)</span> where the detector of this radiation is located. In the case when the post-Maxwellian parameters of the theory differ, <span>(eta_{1}neqeta_{2})</span>, the time of nonlinear electrodynamic delay of electromagnetic signals carried by different normal modes is calculated. The change in the polarization state of the X-ray or gamma radiation pulse after passing through the electromagnetic field of a relativistically rotating pulsar is analyzed. The possibilities of observing the nonlinear effect of the electromagnetic field of a relativistically rotating pulsar on X-ray and gamma-ray pulses are discussed.</p>","PeriodicalId":711,"journal":{"name":"Moscow University Physics Bulletin","volume":"80 5","pages":"881 - 891"},"PeriodicalIF":0.4,"publicationDate":"2025-12-18","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"145772102","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 : 2025-12-18DOI: 10.3103/S1068335625603723
M. O. Zhulidova, O. E. Nanii, I. I. Shikhaliev, V. N. Treschikov
The paper examines the influence of the delivery scheme and spectral characteristics of remote optically pumped amplifiers (ROPA) on the maximum length of unrepeatered communication lines. It is established that in the backward ROPA (BROPA) scheme, signal amplification due to stimulated Raman scattering (SRS) in the working telecommunication fiber causes a small shift (~5 nm) of optimal pump wavelength toward shorter wavelengths relative to the maximum gain-to-noise ratio of the erbium-doped fiber (max[GainEDF(λpump)/NFEDF(λpump)]). The pump delivery through the working fiber in the case of BROPA has been found to increase the transmission distance due to additional signal amplification caused by SRS and the absence of significant depletion of pump power delivered to the erbium-doped fiber. Conversely, when the signal and pump propagate forward (FROPA) along the working fiber, the pump power decays due to SRS, which makes its delivery via an additional fiber more efficient. It has been determined that for a pump spectral width exceeding 4 GHz, the effect of the Mandelstam-Brillouin stimulated scattering on pump power can be disregarded. Approximate formulas are derived for calculating the dependence of the BROPA gain on the microparameters of the erbium-doped fiber, the signal spectrum, and on the delivered power and pump spectrum subject to the amplified spontaneous emission.
{"title":"Influence of Pumping Parameters on the Maximum Length of Unrepeatered Communication Lines with Erbium-Doped Remote Optically Pumped Amplifiers","authors":"M. O. Zhulidova, O. E. Nanii, I. I. Shikhaliev, V. N. Treschikov","doi":"10.3103/S1068335625603723","DOIUrl":"10.3103/S1068335625603723","url":null,"abstract":"<p>The paper examines the influence of the delivery scheme and spectral characteristics of remote optically pumped amplifiers (ROPA) on the maximum length of unrepeatered communication lines. It is established that in the backward ROPA (BROPA) scheme, signal amplification due to stimulated Raman scattering (SRS) in the working telecommunication fiber causes a small shift (~5 nm) of optimal pump wavelength toward shorter wavelengths relative to the maximum gain-to-noise ratio of the erbium-doped fiber (max[Gain<sub>EDF</sub>(λ<sub>pump</sub>)/NF<sub>EDF</sub>(λ<sub>pump</sub>)]). The pump delivery through the working fiber in the case of BROPA has been found to increase the transmission distance due to additional signal amplification caused by SRS and the absence of significant depletion of pump power delivered to the erbium-doped fiber. Conversely, when the signal and pump propagate forward (FROPA) along the working fiber, the pump power decays due to SRS, which makes its delivery via an additional fiber more efficient. It has been determined that for a pump spectral width exceeding 4 GHz, the effect of the Mandelstam-Brillouin stimulated scattering on pump power can be disregarded. Approximate formulas are derived for calculating the dependence of the BROPA gain on the microparameters of the erbium-doped fiber, the signal spectrum, and on the delivered power and pump spectrum subject to the amplified spontaneous emission.</p>","PeriodicalId":503,"journal":{"name":"Bulletin of the Lebedev Physics Institute","volume":"52 7","pages":"S746 - S762"},"PeriodicalIF":0.7,"publicationDate":"2025-12-18","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"145772218","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}
Kwang Jae Lee, Jawad Hadid, Sourish Banerjee, Thomas Nuytten, Ravikiran Lingaparthi, Herwig Hahn, Sebastian M. J. Beer, Md Arif Khan, Karen Geens, Stefaan Decoutere, Robert Langer, Anurag Vohra
Gallium nitride is increasingly recognized as a leading material for power and radio frequency applications, due to its unique electronic properties. However, the phenomenon of wafer bow and warpage during GaN growth on heterogeneous substrates presents significant challenges for vertical-type GaN devices with increasing drift layer thickness (for high voltage applications, 1200 V and above) and substrate diameters scaling to 200 mm. In this study, we introduce a growth scheme in the metalorganic chemical vapor deposition of GaN on 200 mm “engineered” substrates from Qromis substrate technology, specifically to minimize the wafer bow for vertical GaN metal-oxide-semiconductor field-effect transistors featuring an 11.5 μm-thick drift layer, with an overall GaN stack of ∼15 μm. By systematically reducing the pressure during the growth of unintentionally doped GaN from 300 to 150 mbar on an Al0.3Ga0.7N buffer layer, the tensile stress induced during cooldown could be effectively compensated. This yields an overall low residual stress of the thick ∼15 μm epitaxially grown GaN layers on the engineered Qromis substrate technology® substrate.
{"title":"Low-stress MOCVD-grown 15 μm GaN layers on 200 mm engineered substrates with minimal wafer bow","authors":"Kwang Jae Lee, Jawad Hadid, Sourish Banerjee, Thomas Nuytten, Ravikiran Lingaparthi, Herwig Hahn, Sebastian M. J. Beer, Md Arif Khan, Karen Geens, Stefaan Decoutere, Robert Langer, Anurag Vohra","doi":"10.1063/5.0312962","DOIUrl":"https://doi.org/10.1063/5.0312962","url":null,"abstract":"Gallium nitride is increasingly recognized as a leading material for power and radio frequency applications, due to its unique electronic properties. However, the phenomenon of wafer bow and warpage during GaN growth on heterogeneous substrates presents significant challenges for vertical-type GaN devices with increasing drift layer thickness (for high voltage applications, 1200 V and above) and substrate diameters scaling to 200 mm. In this study, we introduce a growth scheme in the metalorganic chemical vapor deposition of GaN on 200 mm “engineered” substrates from Qromis substrate technology, specifically to minimize the wafer bow for vertical GaN metal-oxide-semiconductor field-effect transistors featuring an 11.5 μm-thick drift layer, with an overall GaN stack of ∼15 μm. By systematically reducing the pressure during the growth of unintentionally doped GaN from 300 to 150 mbar on an Al0.3Ga0.7N buffer layer, the tensile stress induced during cooldown could be effectively compensated. This yields an overall low residual stress of the thick ∼15 μm epitaxially grown GaN layers on the engineered Qromis substrate technology® substrate.","PeriodicalId":8094,"journal":{"name":"Applied Physics Letters","volume":"21 1","pages":""},"PeriodicalIF":4.0,"publicationDate":"2025-12-18","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"145770937","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":2,"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 : 2025-12-18DOI: 10.1088/1361-6382/ae272f
Tahereh Azizi and Mojtaba Alimoradi
We study a thick brane scenario within the Palatini formulation of gravity, where the metric and affine connection are treated as independent variables. By introducing a non-minimal coupling between a bulk scalar field and the Ricci scalar, we obtain analytic solutions under a flat, four-dimensional Poincaré-invariant metric with a kink-like scalar configuration. The warp factor exhibits a bell-shaped profile, while the scalar potential forms a symmetric volcano-like structure, characteristic of a finite-thickness brane. The corresponding energy density is regular and localized, featuring a central peak with symmetrically placed negative minima. Through the analysis of linear tensor perturbations, we derive a Schrödinger-like equation with supersymmetric factorization, ensuring the absence of tachyonic modes and thus the stability of the background configuration. The effective potential also takes a volcano-like form that supports a localized graviton zero mode, confirming the recovery of four-dimensional gravity on the brane. A numerical study of the massive Kaluza–Klein spectrum reveals the progressive delocalization of massive modes into the bulk. Our results demonstrate a stable and physically consistent thick brane configuration within the Palatini gravity framework, offering new insights into gravity localization and braneworld phenomenology.
{"title":"Thick brane in Palatini formalism with a non-minimally coupled bulk scalar field","authors":"Tahereh Azizi and Mojtaba Alimoradi","doi":"10.1088/1361-6382/ae272f","DOIUrl":"https://doi.org/10.1088/1361-6382/ae272f","url":null,"abstract":"We study a thick brane scenario within the Palatini formulation of gravity, where the metric and affine connection are treated as independent variables. By introducing a non-minimal coupling between a bulk scalar field and the Ricci scalar, we obtain analytic solutions under a flat, four-dimensional Poincaré-invariant metric with a kink-like scalar configuration. The warp factor exhibits a bell-shaped profile, while the scalar potential forms a symmetric volcano-like structure, characteristic of a finite-thickness brane. The corresponding energy density is regular and localized, featuring a central peak with symmetrically placed negative minima. Through the analysis of linear tensor perturbations, we derive a Schrödinger-like equation with supersymmetric factorization, ensuring the absence of tachyonic modes and thus the stability of the background configuration. The effective potential also takes a volcano-like form that supports a localized graviton zero mode, confirming the recovery of four-dimensional gravity on the brane. A numerical study of the massive Kaluza–Klein spectrum reveals the progressive delocalization of massive modes into the bulk. Our results demonstrate a stable and physically consistent thick brane configuration within the Palatini gravity framework, offering new insights into gravity localization and braneworld phenomenology.","PeriodicalId":10282,"journal":{"name":"Classical and Quantum Gravity","volume":"23 1","pages":""},"PeriodicalIF":3.5,"publicationDate":"2025-12-18","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"145771422","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":3,"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 : 2025-12-18DOI: 10.1016/j.radmeas.2025.107594
Zhong-Bin Hang , Chuan-Feng Liu , Yan Zhang , Zi-Wei Liang , Hai Hu , Tian-Tian Zhang , Yun-Tao Liu , Ming-Zhe Song , Ke-Xin Wei , Lin Qin , Xi-Mei Wang , Zuo-Xiang He
Background:
In the clinical application of brachytherapy, the relevant quantities of brachytherapy seed strength must be converted into absorbed dose at a reference depth of 1 cm in water. The current method of obtaining the absorbed dose in water is based on the air kerma strength and dose rate constant, which has an uncertainty of more than 10% (k=2), potentially affecting cancer treatment outcomes.
Purpose:
To ensure accurate dosimetry for 125I brachytherapy seeds, an extrapolation chamber embedded in the water-equivalent material was designed and manufactured to measure the absorbed dose in water directly.
Methods:
The mathematical model for determining the absorbed dose in water is based on radiation transport theory, where the key term conversion factor is determined using the Monte Carlo (MC) methods. In this paper, the basic structure, the measurement method, and the MC simulation of the extrapolation chamber are described. The dose rate constant of the model 6711 125I brachytherapy seed was obtained using three methods (experimental measurement, MC simulation, and AAPM recommended values), and the results was compared and analyzed.
Results:
The absorbed dose in water of the model 6711 125I brachytherapy seed was determined, and after repeated measurements and uncertainty evaluation, the result was 12.39 mGy/h, with an uncertainty of 3.5% (k=2). In addition, the brachytherapy seed was calibrated using an absolute measurement device for the air kerma strength, and its dose rate constant was calculated, which was in good agreement with both the AAPM-recommended values and MC simulated values.
Conclusions:
We successfully developed an absolute measurement device for the absorbed dose in water, which reduced the measurement uncertainty for 125I brachytherapy seeds and achieved dose accuracy for external radiotherapy. This study contributes to the establishment of primary standards for the absorbed dose in water of 125I brachytherapy seeds.
{"title":"Absolute measurement of absorbed dose in water for 125I brachytherapy seeds","authors":"Zhong-Bin Hang , Chuan-Feng Liu , Yan Zhang , Zi-Wei Liang , Hai Hu , Tian-Tian Zhang , Yun-Tao Liu , Ming-Zhe Song , Ke-Xin Wei , Lin Qin , Xi-Mei Wang , Zuo-Xiang He","doi":"10.1016/j.radmeas.2025.107594","DOIUrl":"10.1016/j.radmeas.2025.107594","url":null,"abstract":"<div><h3>Background:</h3><div>In the clinical application of brachytherapy, the relevant quantities of brachytherapy seed strength must be converted into absorbed dose at a reference depth of 1 cm in water. The current method of obtaining the absorbed dose in water is based on the air kerma strength and dose rate constant, which has an uncertainty of more than 10% (<em>k</em>=2), potentially affecting cancer treatment outcomes.</div></div><div><h3>Purpose:</h3><div>To ensure accurate dosimetry for <sup>125</sup>I brachytherapy seeds, an extrapolation chamber embedded in the water-equivalent material was designed and manufactured to measure the absorbed dose in water directly.</div></div><div><h3>Methods:</h3><div>The mathematical model for determining the absorbed dose in water is based on radiation transport theory, where the key term conversion factor <span><math><mrow><mi>C</mi><mrow><mo>(</mo><msub><mrow><mi>x</mi></mrow><mrow><mi>i</mi><mo>+</mo><mn>1</mn></mrow></msub><mo>,</mo><msub><mrow><mi>x</mi></mrow><mrow><mi>i</mi></mrow></msub><mo>)</mo></mrow></mrow></math></span> is determined using the Monte Carlo (MC) methods. In this paper, the basic structure, the measurement method, and the MC simulation of the extrapolation chamber are described. The dose rate constant of the model 6711 <sup>125</sup>I brachytherapy seed was obtained using three methods (experimental measurement, MC simulation, and AAPM recommended values), and the results was compared and analyzed.</div></div><div><h3>Results:</h3><div>The absorbed dose in water of the model 6711 <sup>125</sup>I brachytherapy seed was determined, and after repeated measurements and uncertainty evaluation, the result was 12.39 mGy/h, with an uncertainty of 3.5% (<em>k</em>=2). In addition, the brachytherapy seed was calibrated using an absolute measurement device for the air kerma strength, and its dose rate constant was calculated, which was in good agreement with both the AAPM-recommended values and MC simulated values.</div></div><div><h3>Conclusions:</h3><div>We successfully developed an absolute measurement device for the absorbed dose in water, which reduced the measurement uncertainty for <sup>125</sup>I brachytherapy seeds and achieved dose accuracy for external radiotherapy. This study contributes to the establishment of primary standards for the absorbed dose in water of <sup>125</sup>I brachytherapy seeds.</div></div>","PeriodicalId":21055,"journal":{"name":"Radiation Measurements","volume":"191 ","pages":"Article 107594"},"PeriodicalIF":2.2,"publicationDate":"2025-12-18","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"145787322","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":3,"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}