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f(X, Y, E) gravity and cosmological models f(X, Y, E)引力和宇宙学模型
IF 1.7 4区 物理与天体物理 Q2 PHYSICS, MULTIDISCIPLINARY Pub Date : 2026-03-28 DOI: 10.1007/s12648-026-03975-z
M. M. Tantawy, M. A. Bakry, G. M. Moatimid

In the present article, we employ the geometry of absolute parallelism and parameterized absolute parallelism to develop a new theory, denoted as f(X, Y, E) gravity, where X = X (R, T) represents a parameterized curvature scalar, Y = Y(T) a parameterized torsion scalar, and E refers to the trace of the stress-energy tensor. From this new theory, we derive the modified theories f(R) gravity, f(R, E) gravity and f(T) gravity as special cases, where R represents a curvature scalar, T a torsion scalar. We introduce the f(X, Y, E) = λ X + γ Y + 2η E, where λ, γ and η are constants, and apply a quadratic deceleration parameter to describe the cosmological models of the Big Bang, Big Rip, and Big Crunch. Our study demonstrates that the evolution of the universe exhibits remarkably similar behavior across all proposed modified theories. Additionally, we discuss the energy conditions, revealing that the Dominant Energy Condition, Strong Energy Condition, and Weak Energy Condition are violated for these models.

在本文中,我们利用绝对平行和参数化绝对平行的几何构造了一个新的理论,记作f(X, Y, E)重力,其中X = X (R, T)表示参数化曲率标量,Y = Y(T)表示参数化扭转标量,E表示应力-能量张量的轨迹。在这个新理论的基础上,我们导出了修正后的f(R)引力理论,f(R, E)引力理论和f(T)引力理论作为特例,其中R表示曲率标量,T表示扭转标量。我们引入f(X, Y, E) = λ X + γ Y + 2η E,其中λ, γ和η为常数,并应用二次减速参数来描述大爆炸,大撕裂和大收缩的宇宙学模型。我们的研究表明,宇宙的演化在所有提出的修正理论中都表现出非常相似的行为。此外,我们还讨论了这些模型的能量条件,揭示了这些模型违反了优势能量条件、强能量条件和弱能量条件。
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引用次数: 0
Analysis of the temperature controlled magneto-transport properties and magnetization: role of introducing Au in La2/3Ca1/3MnO3 (LCMO) La2/3Ca1/3MnO3 (LCMO)中引入Au的温控磁输运特性及磁化性能分析
IF 1.7 4区 物理与天体物理 Q2 PHYSICS, MULTIDISCIPLINARY Pub Date : 2026-03-27 DOI: 10.1007/s12648-026-03946-4
Navjyoti Boora, Rana Tabassum, Shafaque Rahman, A. K. Hafiz

Ortho-manganites are considered as promising candidates in ferro-electro-magnetism. The colossal magneto-resistive material demonstrates a first-order phase transition from a paramagnetic to a ferromagnetic state (TC), along with a transition from insulator to metallic behavior, meaning a change in resistivity. Here, we report synthesis and characterization of colossal magneto-resistive material 'pure LCMO' and 'LCMO-30% Au doped composite'. The results indicate that metal–insulator transition temperature was approximately 268 K for the LCMO-30% Au composite along with highest magneto-resistance (MR) of ~ − 63.8% at 268 K under 7 T applied magnetic field. Meanwhile, for the LCMO-30% Au composite, the maximum temperature coefficient of resistance (TCR) of ~ 11.02%/K was observed at 263 K and 1.77% at 275 K; in contrast, the pure LCMO exhibited a TCR of 2.36%/K at 260 K. The results indicate that the magneto-resistive properties of the LCMO-30% Au composite are significantly superior compared to the pure LCMO which is due to the fact that gold either accumulates at the grain boundaries (GBs) or on the surfaces of the LCMO grains, acting as an additive at the GBs without integrating into the primary LCMO lattice. Ultimately, results obtained were compared with the existing ones and demonstrated improvements over previously reported findings.

正锰矿被认为是铁电磁研究的有前途的候选者。巨大的磁阻材料显示了从顺磁性到铁磁性状态(TC)的一级相变,以及从绝缘体到金属行为的转变,这意味着电阻率的变化。在这里,我们报道了巨磁阻材料“纯LCMO”和“LCMO-30% Au掺杂复合材料”的合成和表征。结果表明,在7 T外加磁场作用下,LCMO-30% Au复合材料的金属-绝缘体转变温度约为268 K,磁电阻(MR)在268 K时达到~−63.8%。同时,LCMO-30% Au复合材料在263 K和275 K时的最大电阻温度系数(TCR)分别为~ 11.02%和1.77%;而纯LCMO在260 K时的TCR为2.36%/K。结果表明,30% Au - LCMO复合材料的磁阻性能明显优于纯LCMO,这是由于金在晶界处或晶面处作为添加剂,而没有整合到初级LCMO晶格中。最后,将获得的结果与现有的结果进行比较,并证明比先前报道的结果有所改进。
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引用次数: 0
Optoelectronic properties of strontium incorporated nickel cadmium oxalate trihydrate crystals 锶掺杂三水合草酸镍镉晶体的光电性能
IF 1.7 4区 物理与天体物理 Q2 PHYSICS, MULTIDISCIPLINARY Pub Date : 2026-03-27 DOI: 10.1007/s12648-026-04027-2
B. V. Veekshitha, P. S. Rohith, A. S. Ganavi

Novel crystals of strontium incorporated nickel cadmium oxalate (SNCO) trihydrate were grown by single diffusion method in silica hydro gel by optimizing various growth parameters. Field emission scanning electron microscopic (FESEM) images show the morphology of the crystal surface and the existence of Sr, Ni, Cd, C and O elements in the crystal lattice were identified using energy dispersive X-ray (EDX) analysis. The occurrences of C–O, C=O, C–C, O–H and M–O bonds were observed using Fourier transform infrared (FTIR) spectrophotometer. Powder X-ray diffractogram reveals the high crystallinity of the SNCO crystals, and exhibit triclinic crystal system with P-1 space group. Thermal studies (TG/DTG/DTA/DSC) show the high thermal stability (TS > 600º C) of grown crystals. The high energy gap (Eg = 5.420 eV) from the UV–Visible absorption spectroscopy confirms the insulating behaviour of the crystals. Low electrical conductivity (μA), high leakage resistance (MΩ) and the variation of dielectric constant, dielectric loss, AC conductivity with frequency were studied and reported.

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引用次数: 0
Viscosity of (R^2) modified AdS black brane (R^2)改性AdS黑膜的粘度
IF 1.7 4区 物理与天体物理 Q2 PHYSICS, MULTIDISCIPLINARY Pub Date : 2026-03-27 DOI: 10.1007/s12648-026-03942-8
Razieh Golmoradifard, Mehdi Sadeghi, Behrooz Malekolkalami

We investigate the Einstein-Hilbert black brane solution in four-dimensional Anti-de Sitter (AdS) spacetime supplemented by a quadratic Ricci scalar term (q L^2 R^2), where q is a dimensionless coupling constant and L is the AdS radius. The shear viscosity to entropy density ratio, (frac{eta }{s}), is calculated holographically, and deviations from the universal Kovtun-Son-Starinets (KSS) bound are analyzed. Our results indicate that (frac{eta }{s} = frac{1}{{4pi }}left( {1 - 24q} right)), demonstrating that the ratio falls below the conjectured lower limit for positive q, while it respects the bound for negative q. We confirm that our solutions smoothly reduce to the standard Einstein-Hilbert case when (q rightarrow 0), consistent with expectations. The physical implications of violating the KSS bound are discussed in depth, particularly regarding stability, causality, and the strongly coupled nature of the dual field theory. These findings provide valuable insights into the influence of higher curvature terms on holographic transport properties.

我们研究了二次Ricci标量项(q L^2 R^2)补充的四维反德西特(AdS)时空中的爱因斯坦-希尔伯特黑膜解,其中q为无量纲耦合常数,L为AdS半径。用全息方法计算了剪切粘度与熵密度比(frac{eta }{s}),并分析了与通用的Kovtun-Son-Starinets (KSS)界的偏差。我们的结果表明(frac{eta }{s} = frac{1}{{4pi }}left( {1 - 24q} right)),表明该比率低于正q的推测下限,而它尊重负q的界。我们确认,当(q rightarrow 0)时,我们的解平滑地约为标准爱因斯坦-希尔伯特情况,与期望一致。深入讨论了违反KSS界的物理含义,特别是关于对偶场论的稳定性、因果关系和强耦合性质。这些发现为高曲率项对全息输运性质的影响提供了有价值的见解。
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引用次数: 0
Structural phase transition, intermediate phases and electronic properties of SnO2 metal dioxide (Cassiterite) under high pressure 高压下二氧化锡(锡石)的结构相变、中间相及电子性能
IF 1.7 4区 物理与天体物理 Q2 PHYSICS, MULTIDISCIPLINARY Pub Date : 2026-03-26 DOI: 10.1007/s12648-026-04012-9
Ganimet Mülazımoğlu Kızılırmak, Hülya Öztürk

In this study, a simulation of the structural phase transition mechanism of SnO2 (Cassiterite), selected among the rutile-type stable metal dioxides, has been carried out. Calculations were performed in the frame of density functional theory (DFT). Using the ab-initio technique, the structural phase transition behaviors and intermediate phases of SnO2 under high pressure were investigated with the Siesta code. Generalized gradient approximation (GGA) was selected to find the exchange–correlation energy. Initially, the rutile-type SnO2 structure was optimized at zero pressure, and then the pressure was increased up to 170 GPa with an increment of 10 GPa. The initial rutile-type structure of SnO2 with space group P42/mnm (No. 136) transformed into the cotunnite type structure with space group Pnma (No. 62) at 100 GPa. During the phase transformation of SnO2 from rutile type to cotunnite type at 100 GPa pressure, intermediate phases Pnnm (Orthorhombic) → P21 (Monoclinic) → P1 (Triclinic) → Pc (Monoclinic) → P21/c (Monoclinic) were determined for the first time in this study. Energy and enthalpy calculations were performed to investigate the compatibility of the determined stable phase transition with the experimental results. For the electronic properties, the band structures and density of states are calculated and analyzed in detail. The findings obtained from the calculations are in accordance with the literature.

本文对金红石型稳定金属氧化物中选择的SnO2(锡石)的结构相变机理进行了模拟。在密度泛函理论(DFT)框架下进行了计算。采用ab-initio方法,利用Siesta程序研究了高压下SnO2的结构相变行为和中间相。采用广义梯度近似(GGA)求交换相关能。首先在零压力下优化金红石型SnO2结构,然后将压力增加到170 GPa,增量为10 GPa。在100 GPa下,初始空间群P42/mnm (No. 136)的SnO2由金红石型结构转变为空间群Pnma (No. 62)的钴矿型结构。在100gpa压力下,SnO2由金红石型向钴长石型相变过程中,首次确定了中间相Pnnm(正交相)→P21(单斜相)→P1(三斜相)→Pc(单斜相)→P21/c(单斜相)。通过能量和焓的计算来考察所确定的稳定相变与实验结果的相容性。在电子性能方面,对能带结构和态密度进行了详细的计算和分析。计算结果与文献一致。
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引用次数: 0
Next-generation LiNbCh2 (Ch = O, S, Se) chalcogenides: Ab initio insights into optoelectronic properties 新一代LiNbCh2 (Ch = O, S, Se)硫族化合物:光电性质的从头计算
IF 1.7 4区 物理与天体物理 Q2 PHYSICS, MULTIDISCIPLINARY Pub Date : 2026-03-26 DOI: 10.1007/s12648-026-04029-0
Ishak Mebarkia, Mohamed Khedidji, Rachid Belkada

In this work, we provide comprehensive first-principles insights into the structural, elastic, electronic, and optoelectronic characteristics of layered LiNbCh2 (Ch = O, S, Se) chalcogenides. Elastic analysis confirms mechanical stability and uncovers a systematic softening and anisotropy trend across the series, with all compounds displaying brittle behavior. Electronic band structure calculations reveal a semiconducting nature, where LiNbO2 hosts a direct band gap, while LiNbS2 and LiNbSe2 exhibit indirect gaps. Optical investigations uncover pronounced anisotropy and birefringence, with LiNbO2 showing strong ultraviolet absorption, positioning it as a promising candidate for UV photodetection. Conversely, LiNbS2 and LiNbSe2 exhibit absorption in the visible range, underlining their potential for next-generation optoelectronic and photovoltaic applications.

在这项工作中,我们对层状LiNbCh2 (Ch = O, S, Se)硫属化合物的结构、弹性、电子和光电子特性提供了全面的第一性原理见解。弹性分析证实了机械稳定性,揭示了整个系列的系统软化和各向异性趋势,所有化合物都表现出脆性行为。电子能带结构计算揭示了其半导体性质,其中LiNbO2具有直接带隙,而LiNbS2和LiNbSe2具有间接带隙。光学研究揭示了明显的各向异性和双折射,其中LiNbO2表现出强烈的紫外线吸收,使其成为紫外光探测的有希望的候选者。相反,LiNbS2和LiNbSe2在可见光范围内表现出吸收,强调了它们在下一代光电和光伏应用中的潜力。
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引用次数: 0
A linear variable optical filter for the mid-infrared spectrum 中红外光谱的线性可变滤光片
IF 1.7 4区 物理与天体物理 Q2 PHYSICS, MULTIDISCIPLINARY Pub Date : 2026-03-25 DOI: 10.1007/s12648-026-04026-3
Nisham Kumari, Pijus Kundu, Ashok Chauhan, Manish Mathew, Kuldip Singh

This work details the design and simulation of a linear variable optical filter (LVOF) that has been optimized for the mid-infrared (MIR) spectrum, specifically within the range of 2500–5500 nm. The filter employs a silicon substrate and a distributed Bragg reflector (DBR) architecture composed of Si, Ge, and SiO2 thin-film layers, incorporating a laterally tapered SiO2 cavity to achieve continuous wavelength tuning. The implementation of high-contrast Si/SiO2 and Ge/SiO2 layer pairs enables broad spectral coverage with a reduced number of DBR periods while maintaining high reflectivity. Simulations demonstrate transmission exceeding 90%, cut-off depth below 0.1%, and spectral resolution between 0.6 and 5%. The proposed structure provides multichannel filtering capability using a monolithic design, enabling compact, low-cost MIR detection systems suitable for gas-sensing applications.

这项工作详细介绍了线性可变光学滤波器(LVOF)的设计和仿真,该滤波器已针对中红外(MIR)光谱进行了优化,特别是在2500-5500 nm范围内。该滤波器采用硅衬底和由Si、Ge和SiO2薄膜层组成的分布式布拉格反射器(DBR)结构,并结合横向锥形SiO2腔来实现连续波长调谐。高对比度Si/SiO2和Ge/SiO2层对的实现可以在保持高反射率的同时减少DBR周期数,实现广谱覆盖。模拟结果表明,透射率超过90%,截止深度低于0.1%,光谱分辨率在0.6 ~ 5%之间。提出的结构采用单片设计提供多通道滤波能力,使紧凑,低成本的MIR检测系统适合气体传感应用。
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引用次数: 0
Optical properties of the most stable GaxPy (x + y = 2 to 5) nanoclusters predicted through first principles 利用第一性原理预测了最稳定的GaxPy (x + y = 2 ~ 5)纳米团簇的光学性质
IF 1.7 4区 物理与天体物理 Q2 PHYSICS, MULTIDISCIPLINARY Pub Date : 2026-03-25 DOI: 10.1007/s12648-026-04018-3
Dheeraj Kumar Pandey,  Anilesh

A Time-Dependent Density Functional Theory (TDDFT) based study has been performed for the optical properties of the previously identified most stable GaxPy (x + y = 2 to 5) nanoclusters. The structures of GaxPy nanoclusters are optimized using the B3LYP-DFT/6-31G(d) method, and after that TDDFT is applied to explore the optical properties of the most stable configurations. The Zero-point energy correction is also considered in determining the most stable structures. This study presents the calculated optical absorption spectra, which are similar to the electron energy loss spectra (EELS) and the corresponding oscillator strength (f) for the most stable GaP nanoclusters of each configuration. Nearly all nanoclusters exhibit strong absorption in the ultraviolet or extreme ultraviolet regions. Some nanoclusters also show appreciable absorption in the visible region. The results reveal a trend where, in most nanoclusters, absorption occurs at lower energies in Ga-rich nanoclusters and at higher energies in P-rich nanoclusters. The development of these theoretically identified most stable GaP nanoclusters could have potential applications in the fabrication of nanodevices, depending on their specific physical properties.

基于时间依赖密度泛函理论(TDDFT)对先前确定的最稳定的GaxPy (x + y = 2至5)纳米团簇的光学性质进行了研究。利用B3LYP-DFT/6-31G(d)方法对GaxPy纳米团簇结构进行优化,然后利用TDDFT研究最稳定构型的光学性质。零点能量修正在确定最稳定结构时也被考虑在内。本研究给出了计算的光学吸收光谱,其与每种构型最稳定的GaP纳米团簇的电子能量损失光谱(EELS)和相应的振荡器强度(f)相似。几乎所有的纳米团簇在紫外线或极紫外线区域都表现出很强的吸收。一些纳米团簇在可见光区也表现出明显的吸收。结果显示,在大多数纳米团簇中,吸收发生在低能量的富ga纳米团簇和高能量的富p纳米团簇中。这些理论上确定的最稳定的GaP纳米团簇的发展可能在纳米器件的制造中有潜在的应用,这取决于它们特定的物理性质。
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引用次数: 0
Traveling wave solutions for a normalized time-fractional predator–prey model 归一化时间分数型捕食者-猎物模型的行波解
IF 1.7 4区 物理与天体物理 Q2 PHYSICS, MULTIDISCIPLINARY Pub Date : 2026-03-25 DOI: 10.1007/s12648-026-04021-8
Seokjun Ham, Soobin Kwak, Ana Yun,  Jyoti, Yunjae Nam, Hyundong Kim, Junseok Kim

We introduce a normalized time-fractional diffusive predator–prey model that accounts for memory effects through a novel fractional time scale. Unlike conventional time-fractional models, the proposed formulation uses a normalized fractional derivative that ensures the total weight of the memory kernel remains unity, which enables a more consistent interpretation of historical influence across all fractional orders. The model is discretized using a finite difference scheme and solved via tridiagonal systems. Numerical simulations are performed to study traveling wave solutions and the dynamics of the system under varying fractional orders. The computational results demonstrate that decreasing the order of the fractional derivative leads to shorter temporal periods and increased spatial wavelengths in the predator–prey oscillations, while simultaneously reducing the amplitude of population fluctuations. These numerical experiments highlight the important role of fractional order in controlling the temporal and spatial evolution of ecological systems and emphasize the advantages of normalization in analyzing such dynamics.

我们引入了一个标准化的时间分数扩散捕食者-猎物模型,该模型通过一个新的分数时间尺度来解释记忆效应。与传统的时间分数模型不同,提出的公式使用标准化分数导数,确保内存核的总权重保持统一,从而能够更一致地解释所有分数阶的历史影响。该模型采用有限差分格式离散化,并通过三对角系统求解。通过数值模拟研究了系统在不同分数阶下的行波解和动力学特性。计算结果表明,降低分数阶导数的阶数可以缩短捕食者-猎物振荡的时间周期和增加空间波长,同时降低种群波动的幅度。这些数值实验突出了分数阶在控制生态系统时空演化中的重要作用,并强调了归一化在分析这种动态过程中的优势。
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引用次数: 0
Cosmological analysis of the rényi holographic dark energy in an inhomogeneous isotropic universe 非均匀各向同性宇宙中全息暗能量的宇宙学分析
IF 1.7 4区 物理与天体物理 Q2 PHYSICS, MULTIDISCIPLINARY Pub Date : 2026-03-25 DOI: 10.1007/s12648-026-03968-y
Mohamed Abdelrashied, Ayman Aly, Mustafa Selim

This work aims to construct the generalized form of holographic dark energy density which is known as the Rényi holographic dark energy within an inhomogeneous universe scenario with interacting dark sectors. This holographic model is investigated using the IR cutoff equals the Hubble horizon. The evolutionary behavior of some basic cosmological parameters, such as the Hubble parameter, the deceleration parameter, and the equation of state parameter is studied and plotted against the redshift. The stability of these models has been studied by investigating the evolution of the square of sound speed of the cosmological matter fluctuations against the redshift. In addition, the evolution of the diagnostic Om and Lm parameters is studied. The obtained results show a very good agreement between the recent values of some of the cosmological parameters with the observations. Some major differences and similarities between these models and previously studied inhomogeneous models have been shown. The features that distinguish these models from each other and the standard cosmological model have been studied by applying the state finder analysis. To investigate the viability of these models and how they are candidates to explain a realistic case of our universe, they have been tested with the violation of the second law of thermodynamics.

本工作旨在构建具有相互作用的暗扇区的非均匀宇宙场景中全息暗能量密度的广义形式,即r尼全息暗能量。这个全息模型是用等同于哈勃视界的红外截止点来研究的。研究了一些基本宇宙学参数,如哈勃参数、减速参数和状态方程参数的演化行为,并绘制了红移图。通过研究宇宙物质波动的声速平方对红移的演化,研究了这些模型的稳定性。此外,还研究了诊断参数Om和Lm的演变。所得结果表明,一些宇宙学参数的最新值与观测值吻合得很好。这些模型与先前研究的非均匀模型之间存在一些主要的异同。应用状态查找器分析研究了这些模型与标准宇宙学模型的区别。为了研究这些模型的可行性,以及它们如何成为解释我们宇宙现实情况的候选者,他们已经用违反热力学第二定律的情况进行了测试。
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引用次数: 0
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Indian Journal of Physics
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