Pub Date : 2025-07-13DOI: 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.
{"title":"Electromagnetic Form Factors of the Deuteron in the Dibaryon Model of the (mathbf{NN}) Interaction","authors":"M. N. Platonova, I. T. Obukhovsky","doi":"10.3103/S0027134925700250","DOIUrl":"10.3103/S0027134925700250","url":null,"abstract":"<p>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 <span>(NN)</span> 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 <span>(Q<0.8)</span> GeV/<span>(c)</span>. At higher <span>(Q)</span>, 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.</p>","PeriodicalId":711,"journal":{"name":"Moscow University Physics Bulletin","volume":"80 2","pages":"244 - 254"},"PeriodicalIF":0.4,"publicationDate":"2025-07-13","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"145165289","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 : 2025-07-13DOI: 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.
{"title":"Numerical Models of Nonlinear Acoustic Wave Propagation in Medical Ultrasound Problems and Certain Applications of Aeroacoustics and Underwater Acoustics","authors":"P. V. Yuldashev, O. A. Sapozhnikov, M. M. Karzova, S. A. Tsysar, A. V. Kvashennikova, E. O. Konnova, V. A. Khokhlova","doi":"10.3103/S0027134925700316","DOIUrl":"10.3103/S0027134925700316","url":null,"abstract":"<p>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.</p>","PeriodicalId":711,"journal":{"name":"Moscow University Physics Bulletin","volume":"80 2","pages":"195 - 225"},"PeriodicalIF":0.4,"publicationDate":"2025-07-13","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"145164580","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 : 2025-07-13DOI: 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.
{"title":"Reservoir Network Based on Single Impurity Atoms in Silicon","authors":"A. S. Andreeva, A. S. Trifonov, V. V. Shorokhov, D. E. Presnov, O. V. Snigirev, V. A. Krupenin","doi":"10.3103/S0027134925700420","DOIUrl":"10.3103/S0027134925700420","url":null,"abstract":"<p>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.</p>","PeriodicalId":711,"journal":{"name":"Moscow University Physics Bulletin","volume":"80 2","pages":"277 - 285"},"PeriodicalIF":0.4,"publicationDate":"2025-07-13","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"145164581","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 : 2025-07-13DOI: 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}})。
{"title":"FeSe({}_{mathbf{0.5}})Te({}_{mathbf{0.5}}) Films on Glass with CeO({}_{mathbf{2}}) Doping","authors":"A. V. Petrov, O. V. Snigirev, E. A. Ovchenkov, Yu. V. Blinova, N. V. Porokhov, A. R. Shevchenko, D. A. Chareev, A. G. Maresov","doi":"10.3103/S002713492570033X","DOIUrl":"10.3103/S002713492570033X","url":null,"abstract":"<p>Deposition modes for thin films of FeSe<span>({}_{0.5})</span>Te<span>({}_{0.5})</span> on an amorphous substrate made of K-208 glass, containing cerium oxide (CeO<span>({}_{2})</span>), have been found. The transition temperature of the film, <span>(T_{textrm{C}}=9.5)</span> K, to the superconducting state turned out to be higher than that on borosilicate glass from Fischer Scientific, which does not contain CeO<span>({}_{2})</span>, but lower than the superconducting transition temperature of the target, <span>(T_{textrm{C}}(M)=14)</span> K. This behavior contrasts with the well-known properties of thin films in the FeSe and FeSe<span>({}_{x})</span>Te<span>({}_{1-x})</span> family on crystalline substrates. Based on the measurement results, the vortex activation energy (<i>U</i>), the critical current density (<span>(j_{textrm{C}})</span>), the upper critical field (<span>(H_{C2})</span>), and the irreversibility field (<span>(H_{textrm{irr}})</span>) have been obtained.</p>","PeriodicalId":711,"journal":{"name":"Moscow University Physics Bulletin","volume":"80 2","pages":"306 - 313"},"PeriodicalIF":0.4,"publicationDate":"2025-07-13","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"145165247","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 : 2025-07-13DOI: 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.
{"title":"A Simple Finite-Dimensional Model of the Metastable State","authors":"A. I. Dubikovsky, P. K. Silaev","doi":"10.3103/S0027134925700298","DOIUrl":"10.3103/S0027134925700298","url":null,"abstract":"<p>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.</p>","PeriodicalId":711,"journal":{"name":"Moscow University Physics Bulletin","volume":"80 2","pages":"226 - 235"},"PeriodicalIF":0.4,"publicationDate":"2025-07-13","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"145165290","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 : 2025-07-13DOI: 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。
{"title":"Reproduction of Hydrothermodynamic Characteristics of the Western Arctic Seas of Russia with Assimilation of Sea Surface Temperature and Sea Ice Concentration Data","authors":"I. I. Panasenkova, V. V. Fomin, N. A. Diansky","doi":"10.3103/S0027134925700286","DOIUrl":"10.3103/S0027134925700286","url":null,"abstract":"<p>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<span>(%)</span> for SST and by 60–70<span>(%)</span> 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.</p>","PeriodicalId":711,"journal":{"name":"Moscow University Physics Bulletin","volume":"80 2","pages":"379 - 388"},"PeriodicalIF":0.4,"publicationDate":"2025-07-13","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"145165478","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 : 2025-07-13DOI: 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.
{"title":"Measurement of the Power Output of the VVER-1000 Reactor Based on the Antineutrino Flux from the Core","authors":"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","doi":"10.3103/S0027134925700365","DOIUrl":"10.3103/S0027134925700365","url":null,"abstract":"<p>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.</p>","PeriodicalId":711,"journal":{"name":"Moscow University Physics Bulletin","volume":"80 2","pages":"255 - 261"},"PeriodicalIF":0.4,"publicationDate":"2025-07-13","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"145165291","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 : 2025-07-13DOI: 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。
{"title":"Two Supernovae in NGC 4666: ASASSN-14lp and 2019yvr","authors":"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","doi":"10.3103/S0027134925700389","DOIUrl":"10.3103/S0027134925700389","url":null,"abstract":"<p>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 <span>({sim})</span>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.</p>","PeriodicalId":711,"journal":{"name":"Moscow University Physics Bulletin","volume":"80 2","pages":"358 - 369"},"PeriodicalIF":0.4,"publicationDate":"2025-07-13","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"145165477","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 : 2025-07-13DOI: 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).
{"title":"Amplitude Characteristics and Frequency Bias in a Zeeman Ring Laser under Three-Frequency Running Wave Excitation","authors":"M. E. Grushin, E. G. Lariontsev, I. I. Savel’ev, E. V. Soukhov","doi":"10.3103/S0027134925700341","DOIUrl":"10.3103/S0027134925700341","url":null,"abstract":"<p>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<span>({}^{20})</span> and Ne<span>({}^{22})</span> at a wavelength of 0.63 <span>(mu)</span>m reported in the literature, the value <span>(sigma=1050)</span> MHz leads to results that do not agree with the experiment, allowing for a refinement of the parameter <span>(sigma)</span>.</p>","PeriodicalId":711,"journal":{"name":"Moscow University Physics Bulletin","volume":"80 2","pages":"294 - 298"},"PeriodicalIF":0.4,"publicationDate":"2025-07-13","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"145165250","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 : 2025-07-13DOI: 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.
{"title":"Reconstruction of Photonic Crystal Structure from a Given Phase Response","authors":"P. S. Emeliantsev, S. E. Svyakhovskiy","doi":"10.3103/S0027134925700419","DOIUrl":"10.3103/S0027134925700419","url":null,"abstract":"<p>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.</p>","PeriodicalId":711,"journal":{"name":"Moscow University Physics Bulletin","volume":"80 2","pages":"286 - 293"},"PeriodicalIF":0.4,"publicationDate":"2025-07-13","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"145165535","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}