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Electromagnetic Form Factors of the Deuteron in the Dibaryon Model of the (mathbf{NN}) Interaction (mathbf{NN})相互作用双重子模型中氘核的电磁形状因子
IF 0.4 4区 物理与天体物理 Q4 PHYSICS, MULTIDISCIPLINARY Pub Date : 2025-07-13 DOI: 10.3103/S0027134925700250
M. N. Platonova, I. T. Obukhovsky

The electromagnetic form factors of the deuteron have been calculated within the dibaryon model for nuclear forces, which is based on the resonance mechanism of six-quark bag (dibaryon) formation in (NN) collisions. The calculations take into account both single-nucleon currents (impulse approximation) and additional contributions induced by the formation of an intermediate dibaryon. Two versions of the dibaryon model, from 2002 and 2022, have been used for the form factor calculations. It is shown that both versions of the model reproduce the experimental data well for all three deuteron form factors in the momentum transfer region (Q<0.8) GeV/(c). At higher (Q), the predictions of the different versions of the model diverge, with one version (2002) providing a better description of the magnetic form factor and the other (2022) better describing the charge form factor. Possible reasons for the observed discrepancy between theoretical calculations and experimental data for large momentum transfers are discussed.

在核力的双重子模型中计算了氘核的电磁形态因子,该模型基于(NN)碰撞中六夸克袋(双重子)形成的共振机制。计算考虑了单核子电流(脉冲近似)和由中间双重子形成引起的附加贡献。2002年和2022年的两个版本的双重子模型被用于形状因子的计算。结果表明,两种模型都能很好地再现动量传递区(Q<0.8) GeV/ (c)内所有三种氘核形式因子的实验数据。在更高的(Q)上,不同版本模型的预测出现分歧,一个版本(2002年)提供了更好的磁性形状因子描述,另一个版本(2022年)更好地描述了电荷形状因子。讨论了观察到的大动量传递理论计算与实验数据之间存在差异的可能原因。
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引用次数: 0
Numerical Models of Nonlinear Acoustic Wave Propagation in Medical Ultrasound Problems and Certain Applications of Aeroacoustics and Underwater Acoustics 医学超声问题中非线性声波传播的数值模型及其在气动声学和水声中的某些应用
IF 0.4 4区 物理与天体物理 Q4 PHYSICS, MULTIDISCIPLINARY Pub Date : 2025-07-13 DOI: 10.3103/S0027134925700316
P. V. Yuldashev, O. A. Sapozhnikov, M. M. Karzova, S. A. Tsysar, A. V. Kvashennikova, E. O. Konnova, V. A. Khokhlova

The paper presents a review of numerical algorithms developed at the Laboratory of Medical and Industrial Ultrasound at Lomonosov Moscow State University, which are used to solve the evolution equations of nonlinear acoustics, such as the Burgers equation, the Khokhlov–Zabolotskaya–Kuznetsov (KZK) equation, and the one-way Westervelt equation. The main results obtained using these numerical models in studying the propagation of intense acoustic waves in various media are presented. In particular, examples of solving problems in medical ultrasound, nonlinear aeroacoustics, and nonlinear underwater acoustics are considered. The generalization of one-way models to account for medium inhomogeneities is discussed, employing wide-angle parabolic approximation methods in three-dimensional problems.

本文综述了莫斯科国立罗蒙诺索夫大学医学和工业超声实验室开发的用于求解非线性声学演化方程的数值算法,如Burgers方程、Khokhlov-Zabolotskaya-Kuznetsov (KZK)方程和单向Westervelt方程。介绍了用这些数值模型研究强声波在不同介质中的传播所得到的主要结果。特别考虑了解决医学超声、非线性气动声学和非线性水下声学问题的实例。在三维问题中,采用广角抛物线近似方法,讨论了考虑介质非均匀性的单向模型的推广。
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引用次数: 0
Reservoir Network Based on Single Impurity Atoms in Silicon 基于硅中单杂质原子的储层网络
IF 0.4 4区 物理与天体物理 Q4 PHYSICS, MULTIDISCIPLINARY Pub Date : 2025-07-13 DOI: 10.3103/S0027134925700420
A. S. Andreeva, A. S. Trifonov, V. V. Shorokhov, D. E. Presnov, O. V. Snigirev, V. A. Krupenin

This study is aimed at solving the problem of experimental implementation and investigation of single-electron reservoir networks with As impurity atoms in a quasi-two-dimensional near-surface layer of a solid-state matrix based on silicon-on-insulator (SOI) material. The study of electron transport in the fabricated experimental structures revealed the presence of horizontal Coulomb blockade sections in the current–voltage characteristics (CVC) typical of single-electron transport. The shape of the recorded CVC between a pair of selected control electrodes of the reservoir network significantly depended on the potentials of the remaining surrounding electrodes, which modified the structure of the conductive channels passing through the impurity centers. By adjusting the control voltages and utilizing the intrinsic nonlinearity of the system of disordered single As impurity atoms, which possesses an enormous state space, it was possible to demonstrate the feasibility of implementing a tunable nanoscale current switch and the logical functions ‘‘NOT,’’ ‘‘AND,’’ and ‘‘OR’’ in the single-electron reservoir network. A vector tuning method was employed to determine the required configuration of the reservoir network for the implementation of functional elements.

本研究旨在解决基于绝缘体上硅(SOI)材料的固态基体准二维近表面层中含砷杂质原子的单电子储层网络的实验实现和研究问题。电子在实验结构中的传输研究表明,在单电子传输的典型电流-电压特性(CVC)中存在水平库仑阻塞段。在储层网络的一对选定的控制电极之间记录的CVC的形状很大程度上取决于周围剩余电极的电位,这改变了通过杂质中心的导电通道的结构。通过调节控制电压和利用无序单As杂质原子系统具有巨大状态空间的固有非线性,可以证明在单电子储层网络中实现可调谐纳米级电流开关和“非”、“与”和“或”逻辑功能的可行性。采用矢量调谐方法确定实现功能元件所需的水库网络配置。
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引用次数: 0
FeSe({}_{mathbf{0.5}})Te({}_{mathbf{0.5}}) Films on Glass with CeO({}_{mathbf{2}}) Doping FeSe ({}_{mathbf{0.5}})掺杂CeO ({}_{mathbf{2}})的({}_{mathbf{0.5}})玻璃薄膜
IF 0.4 4区 物理与天体物理 Q4 PHYSICS, MULTIDISCIPLINARY Pub Date : 2025-07-13 DOI: 10.3103/S002713492570033X
A. V. Petrov, O. V. Snigirev, E. A. Ovchenkov, Yu. V. Blinova, N. V. Porokhov, A. R. Shevchenko, D. A. Chareev, A. G. Maresov

Deposition modes for thin films of FeSe({}_{0.5})Te({}_{0.5}) on an amorphous substrate made of K-208 glass, containing cerium oxide (CeO({}_{2})), have been found. The transition temperature of the film, (T_{textrm{C}}=9.5) K, to the superconducting state turned out to be higher than that on borosilicate glass from Fischer Scientific, which does not contain CeO({}_{2}), but lower than the superconducting transition temperature of the target, (T_{textrm{C}}(M)=14) K. This behavior contrasts with the well-known properties of thin films in the FeSe and FeSe({}_{x})Te({}_{1-x}) family on crystalline substrates. Based on the measurement results, the vortex activation energy (U), the critical current density ((j_{textrm{C}})), the upper critical field ((H_{C2})), and the irreversibility field ((H_{textrm{irr}})) have been obtained.

发现了FeSe ({}_{0.5}) Te ({}_{0.5})薄膜在含氧化铈(ceo2 ({}_{2}))的K-208玻璃非晶衬底上的沉积模式。该薄膜的超导态转变温度(T_{textrm{C}}=9.5) K高于Fischer Scientific公司的硼硅酸盐玻璃(不含CeO ({}_{2})),但低于目标的超导态转变温度(T_{textrm{C}}(M)=14) K。这种行为与FeSe和FeSe ({}_{x}) Te ({}_{1-x})家族薄膜在晶体衬底上的众所周知的特性形成对比。根据测量结果,得到了涡活化能U、临界电流密度(j_{textrm{C}})、上临界场(H_{C2})和不可逆性场(H_{textrm{irr}})。
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引用次数: 0
A Simple Finite-Dimensional Model of the Metastable State 亚稳态的简单有限维模型
IF 0.4 4区 物理与天体物理 Q4 PHYSICS, MULTIDISCIPLINARY Pub Date : 2025-07-13 DOI: 10.3103/S0027134925700298
A. I. Dubikovsky, P. K. Silaev

We have constructed an approximate analytical solution to the spectral problem for a finite-dimensional matrix of a special form, which proves to be a very simple and sufficiently satisfactory model of the metastable state. This model reproduces most of the characteristic properties of the metastable state, including the line shape, decay dynamics, and density of states. The accuracy of the approximate analytical solution was verified through direct numerical calculations. The proposed model represents a finite-dimensional analog of the Fano formalism.

我们构造了一类特殊形式的有限维矩阵的谱问题的近似解析解,证明了它是一个非常简单和足够令人满意的亚稳态模型。该模型再现了亚稳态的大部分特性,包括线形、衰变动力学和态密度。通过直接数值计算验证了近似解析解的准确性。所提出的模型代表了法诺形式主义的有限维模拟。
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引用次数: 0
Reproduction of Hydrothermodynamic Characteristics of the Western Arctic Seas of Russia with Assimilation of Sea Surface Temperature and Sea Ice Concentration Data 利用海面温度和海冰浓度同化资料再现俄罗斯北极西部海域的水热力特征
IF 0.4 4区 物理与天体物理 Q4 PHYSICS, MULTIDISCIPLINARY Pub Date : 2025-07-13 DOI: 10.3103/S0027134925700286
I. I. Panasenkova, V. V. Fomin, N. A. Diansky

Reliable forecasting of meteorological, hydrothermodynamic, and ice characteristics in the waters of the Western Arctic Seas of Russia using atmospheric circulation, marine circulation, and sea ice models is currently impossible without observational data assimilation. Data assimilation improves the quality of the initial state of hydrophysical and ice characteristics in models for forecasting simulations, thereby enhancing their accuracy. This study presents a technique for assimilating satellite data on sea surface temperature (SST) and sea ice concentration (SIC) into the INMOM marine circulation model using the Data Assimilation Research Testbed (DART) software, with an assessment of the validity of the employed assimilation algorithm. A comparative analysis of the accuracy of hydrothermodynamic state forecasts with and without satellite SST and SIC data assimilation has been conducted. It is shown that assimilating satellite data reduce the root-mean-square deviation (RMSD) of 24-h forecast results from observational data by approximately 80(%) for SST and by 60–70(%) for SIC compared to the simulation without assimilation. The temporal variability of RMSD in SST and SIC forecasts indicates that the largest errors occur during periods of intense upper sea layer heating and ice melting. The importance of simultaneous assimilation of SST and SIC data is highlighted: more accurate SST reproduction improves the accuracy of heat and salt flux calculations at the ocean-ice boundary, which regulate the thermal accretion/melting processes of ice, consequently enhancing the reproduction of ice area and its edge. In turn, a more accurate SIC calculation directly improves the accuracy of heat flux calculations at the water–air boundary and, consequently, SST.

利用大气环流、海洋环流和海冰模式对俄罗斯北冰洋西部海域的气象、水热力学和冰的特征进行可靠的预报,目前不可能没有观测资料同化。数据同化提高了预报模拟模式中水物理和冰特征初始状态的质量,从而提高了预报模拟模式的精度。本文提出了一种利用数据同化研究试验台(data Assimilation Research Testbed, DART)软件将卫星海表温度(SST)和海冰浓度(SIC)数据同化到INMOM海洋环流模型中的方法,并对同化算法的有效性进行了评估。对有无卫星海表温度和SIC资料同化的水热力状态预报精度进行了比较分析。结果表明,与不同化的模拟相比,同化卫星数据可使观测数据的24小时预报结果的均方根偏差(RMSD)降低约80 (%),海温降低约60-70 (%)。海温和SIC预报RMSD的时间变率表明,误差最大的时段出现在强烈的上层加热和冰融化期间。同时同化海温和碳化硅资料的重要性得到强调:更精确的海温再现提高了海冰边界热盐通量计算的准确性,从而调节了冰的热吸融过程,从而增强了冰区及其边缘的再现。反过来,更精确的SIC计算直接提高了水气边界热通量计算的精度,从而提高了海温。
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引用次数: 0
Measurement of the Power Output of the VVER-1000 Reactor Based on the Antineutrino Flux from the Core 基于堆芯反中微子通量的VVER-1000反应堆输出功率测量
IF 0.4 4区 物理与天体物理 Q4 PHYSICS, MULTIDISCIPLINARY Pub Date : 2025-07-13 DOI: 10.3103/S0027134925700365
A. V. Abramov, R. R. Alyev, M. B. Gromov, I. N. Zhutikov, S. M. Kiselev, A. V. Konstantinov, D. S. Kuznetsov, E. A. Litvinovich, I. N. Machulin, A. E. Murchenko, A. M. Nemeryuk, R. R. Nugmanov, A. Yu. Oralbaev, D. V. Popov, A. A. Rastimeshin, M. D. Skorokhvatov, M. A. Strizh, S. V. Sukhotin, V. A. Khvatov, A. S. Chepurnov, D. A. Chmykhalo, A. V. Etenko

The results of measuring the power output of an industrial nuclear reactor based on the antineutrino flux from the core are presented. The measurements were conducted using the iDREAM detector at a distance of 19.5 m from the center of the core of the VVER-1000 reactor at Unit 3 of the Kalinin Nuclear Power Plant. Estimates of the sensitivity of the iDREAM detector to changes in reactor power over 2-, 4-, and 6-h intervals of antineutrino interaction statistics collection were obtained.

本文介绍了基于堆芯反中微子通量测量工业反应堆输出功率的结果。利用iDREAM探测器在距离加里宁核电站3号机组VVER-1000反应堆堆芯中心19.5 m处进行了测量。估计了iDREAM探测器在反中微子相互作用统计收集的2、4和6小时间隔内对反应堆功率变化的灵敏度。
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引用次数: 0
Two Supernovae in NGC 4666: ASASSN-14lp and 2019yvr NGC 4666中的两颗超新星:ASASSN-14lp和2019yvr
IF 0.4 4区 物理与天体物理 Q4 PHYSICS, MULTIDISCIPLINARY Pub Date : 2025-07-13 DOI: 10.3103/S0027134925700389
D. Yu. Tsvetkov, N. N. Pavlyuk, N. P. Ikonnikova, M. A. Burlak, A. A. Belinskii, A. V. Dodin, S. A. Potanin, N. I. Shatsky, I. M. Volkov, P. V. Baklanov, M. G. Ushakova, V. A. Echeistov, V. M. Lipunov

The results of photometric observations of two supernovae in NGC 4666, SN Ia ASASSN-14lp and SN Ib 2019yvr, as well as spectroscopic observations of SN 2019yvr, are presented. Light curves have been constructed, and their main parameters have been derived. Supernova ASASSN-14lp is a fairly typical Type Ia object with low rate of brightness decline and large interstellar extinction. Using the dependence of the maximum luminosity of SNe Ia on the light curve parameters, an estimate of the distance to the galaxy NGC 4666 has been obtained. The spectrum of SN 2019yvr near maximum light, its peak luminosity, and the shapes of the light curves during the first 90 days after maximum revealed characteristics of a typical Type Ib supernova, with interstellar extinction exceeding that of ASASSN-14lp. A decrease in the rate of brightness decline at a phase of approximately 90 days has been detected. Light curve modeling was performed using the STELLA code, and the physical parameters of the optimal model were determined. It is shown that the agreement between the model and observations breaks down after ({sim})40 days post-maximum; to explain this divergence, a model with an extra energy source due to the spin-down of the magnetar formed in the explosion has been proposed.

本文介绍了NGC 4666中两颗超新星SN Ia ASASSN-14lp和SN Ib 2019yvr的光度观测结果,以及SN 2019yvr的光谱观测结果。构造了光曲线,推导了光曲线的主要参数。超新星ASASSN-14lp是一个相当典型的Ia型天体,亮度下降率低,星际消光大。利用Ia型超新星的最大光度与光曲线参数的关系,估计了它到NGC 4666星系的距离。SN 2019yvr在最大光附近的光谱、峰值亮度以及最大光后90天内的光曲线形状揭示了典型Ib型超新星的特征,其星际消光超过ASASSN-14lp。在大约90天的一个阶段,已经检测到亮度下降的速度下降。利用STELLA代码进行光曲线建模,确定了最优模型的物理参数。结果表明,模型与观测值之间的一致性在最大值后({sim}) 40天后就失效了;为了解释这种分歧,提出了一个由于爆炸中形成的磁星自旋下降而产生额外能量源的模型。
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引用次数: 0
Amplitude Characteristics and Frequency Bias in a Zeeman Ring Laser under Three-Frequency Running Wave Excitation 三频行波激励下塞曼环形激光器的幅值特性和频率偏置
IF 0.4 4区 物理与天体物理 Q4 PHYSICS, MULTIDISCIPLINARY Pub Date : 2025-07-13 DOI: 10.3103/S0027134925700341
M. E. Grushin, E. G. Lariontsev, I. I. Savel’ev, E. V. Soukhov

The characteristics of the Zeeman ring laser (ZRL) have been investigated theoretically and experimentally under conditions of two- and three-frequency generation. The influence of the running wave, excited at the third frequency, on the frequency bias and the intensities of counterpropagating waves is examined. A comparison of experimentally measured characteristics with calculations based on vector theory has been conducted. It has been found that when a running wave is excited in a neighbouring longitudinal mode, kinks appear in the dependence of counterpropagating wave intensities on the detuning of the generation frequency from the gain-line center. It is shown that excitation at the third frequency results in a stronger dependence of the frequency bias on the detuning from the gain-line center compared to the two-frequency generation regime. Based on the comparison of theory with experiment, it is demonstrated that among the known values of the isotopic shift between Ne({}^{20}) and Ne({}^{22}) at a wavelength of 0.63 (mu)m reported in the literature, the value (sigma=1050) MHz leads to results that do not agree with the experiment, allowing for a refinement of the parameter (sigma).

对塞曼环形激光器在二频和三频条件下的特性进行了理论和实验研究。研究了三频激励下的行波对频率偏置和反传播波强度的影响。将实验测量的特性与基于矢量理论的计算结果进行了比较。研究发现,当行波在邻近的纵模中被激发时,反传播波强度与产生频率偏离增益线中心的关系出现了扭曲。结果表明,与双频产生相比,第三频激发导致频率偏置对增益线中心失谐的依赖性更强。通过理论与实验的比较,证明了在已知的文献报道的Ne ({}^{20})和Ne ({}^{22})在0.63 (mu) m波长处的同位素位移值中,(sigma=1050) MHz的值导致的结果与实验不一致,允许对(sigma)参数进行改进。
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引用次数: 0
Reconstruction of Photonic Crystal Structure from a Given Phase Response 从给定相位响应重构光子晶体结构
IF 0.4 4区 物理与天体物理 Q4 PHYSICS, MULTIDISCIPLINARY Pub Date : 2025-07-13 DOI: 10.3103/S0027134925700419
P. S. Emeliantsev, S. E. Svyakhovskiy

We present a method for designing one-dimensional photonic structures whose phase response has a predefined shape and characteristics. An algorithm for constructing such photonic crystal structures has been developed, and numerical modeling of their phase and spectral responses have been performed.

提出了一种设计相位响应具有预定形状和特征的一维光子结构的方法。本文提出了一种构造这种光子晶体结构的算法,并对其相位和光谱响应进行了数值模拟。
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引用次数: 0
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Moscow University Physics Bulletin
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