Pub Date : 2024-11-12DOI: 10.1007/s10909-024-03231-w
Shihong Fu, Giovanni Benato, Carlo Bucci, Paolo Gorla, Pedro V. Guillaumon, Jiang Li, Serge Nagorny, Francesco Nozzoli, Lorenzo Pagnanini, Andrei Puiu, Matthew Stukel
The LUCE (LUtetium sCintillation Experiment) project will search for the (^{176})Lu electron capture based on a milli-Kelvin calorimetric approach. This decay is of special interest in the fields of nuclear structure, rare event searches, and measurements of nuclear matrix elements of long-lived isotopes. The experiment is primarily searching for a mono-energetic peak from the (7^- rightarrow 2^+) forbidden transition. The current status and design of a novel cryogenic module for the measurements of the electron capture in (^{176})Lu are reported on. Details of future measurement plans are presented.
LUCE (LUtetium闪烁实验)项目将基于毫开尔文量热方法寻找(^{176}) Lu电子捕获。这种衰变在核结构、罕见事件搜索和长寿命同位素的核基质元素测量等领域具有特殊的意义。该实验主要是从(7^- rightarrow 2^+)禁跃迁中寻找单能峰。本文报道了一种新型低温电子捕获测量模块((^{176}) Lu)的现状和设计。详细介绍了未来的测量计划。
{"title":"LUCE: A Milli-Kelvin Calorimeter Experiment to Study the Electron Capture of (^{176})Lu","authors":"Shihong Fu, Giovanni Benato, Carlo Bucci, Paolo Gorla, Pedro V. Guillaumon, Jiang Li, Serge Nagorny, Francesco Nozzoli, Lorenzo Pagnanini, Andrei Puiu, Matthew Stukel","doi":"10.1007/s10909-024-03231-w","DOIUrl":"10.1007/s10909-024-03231-w","url":null,"abstract":"<div><p>The LUCE (<b>LU</b>tetium s<b>C</b>intillation <b>E</b>xperiment) project will search for the <span>(^{176})</span>Lu electron capture based on a milli-Kelvin calorimetric approach. This decay is of special interest in the fields of nuclear structure, rare event searches, and measurements of nuclear matrix elements of long-lived isotopes. The experiment is primarily searching for a mono-energetic peak from the <span>(7^- rightarrow 2^+)</span> forbidden transition. The current status and design of a novel cryogenic module for the measurements of the electron capture in <span>(^{176})</span>Lu are reported on. Details of future measurement plans are presented.</p></div>","PeriodicalId":641,"journal":{"name":"Journal of Low Temperature Physics","volume":"218 Part 5","pages":"12 - 20"},"PeriodicalIF":1.1,"publicationDate":"2024-11-12","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"142994638","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 : 2024-11-08DOI: 10.1007/s10909-024-03240-9
Maryam Rahmani, Emily M. Barrentine, Eric R. Switzer, Alyssa Barlis, Ari D. Brown, Giuseppe Cataldo, Jake A. Connors, Negar Ehsan, Thomas M. Essinger-Hileman, Henry Grant, James Hays-Wehle, Wen-Ting Hsieh, Vilem Mikula, S. Harvey Moseley, Omid Noroozian, Manuel A. Quijada, Jessica Patel, Thomas R. Stevenson, Carole Tucker, Kongpop U-Yen, Carolyn G. Volpert, Edward J. Wollack
We describe a testbed to characterize the optical response of compact superconducting on-chip spectrometers in development for the EXperiment for Cryogenic Large-Aperture Intensity Mapping (EXCLAIM) mission. EXCLAIM is a balloon-borne far-infrared experiment to probe the CO and CII emission lines in galaxies from redshift 3.5 to the present. The spectrometer, called µ-Spec, comprises a diffraction grating on a silicon chip coupled to kinetic inductance detectors (KIDs) read out via a single microwave feedline. We use a prototype spectrometer for EXCLAIM to demonstrate our ability to characterize the spectrometer’s spectral response using a photomixer source. We utilize an on-chip reference detector to remove the spectral structure introduced by the off-chip optics and a silicon etalon to calibrate the absolute frequency.
{"title":"Optimization of an Optical Testbed for Characterization of EXCLAIM µ-Spec Integrated Spectrometers","authors":"Maryam Rahmani, Emily M. Barrentine, Eric R. Switzer, Alyssa Barlis, Ari D. Brown, Giuseppe Cataldo, Jake A. Connors, Negar Ehsan, Thomas M. Essinger-Hileman, Henry Grant, James Hays-Wehle, Wen-Ting Hsieh, Vilem Mikula, S. Harvey Moseley, Omid Noroozian, Manuel A. Quijada, Jessica Patel, Thomas R. Stevenson, Carole Tucker, Kongpop U-Yen, Carolyn G. Volpert, Edward J. Wollack","doi":"10.1007/s10909-024-03240-9","DOIUrl":"10.1007/s10909-024-03240-9","url":null,"abstract":"<div><p>We describe a testbed to characterize the optical response of compact superconducting on-chip spectrometers in development for the EXperiment for Cryogenic Large-Aperture Intensity Mapping (EXCLAIM) mission. EXCLAIM is a balloon-borne far-infrared experiment to probe the CO and CII emission lines in galaxies from redshift 3.5 to the present. The spectrometer, called µ-Spec, comprises a diffraction grating on a silicon chip coupled to kinetic inductance detectors (KIDs) read out via a single microwave feedline. We use a prototype spectrometer for EXCLAIM to demonstrate our ability to characterize the spectrometer’s spectral response using a photomixer source. We utilize an on-chip reference detector to remove the spectral structure introduced by the off-chip optics and a silicon etalon to calibrate the absolute frequency.</p></div>","PeriodicalId":641,"journal":{"name":"Journal of Low Temperature Physics","volume":"218 Part 5","pages":"65 - 73"},"PeriodicalIF":1.1,"publicationDate":"2024-11-08","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"142994772","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}
In recent years, global investment in magnetic resonance imaging (MRI) has surged, with 3 T MRI technology overtaking 1.5 T as the standard in hospitals gradually. A combination of linear programming, genetic algorithms, and nonlinear programming was employed to design an actively shielded 3 T superconducting MRI magnet system. This magnet consists of seven main coils and two shielding coils, achieving a magnetic field with a peak-to-peak inhomogeneity of 10 ppm within a 50-cm-diameter spherical volume (DSV). To address the risk of quench in superconducting magnets, which can lead to damage due to excessive temperature, voltage, and stress, a quench protection system is crucial. The designed system segments the coils for protection, using diode pairs and shunt resistors to manage the quench. Initial simulations indicated that temperature rises and voltages were within safe limits, but some coils were slow to quench or did not quench at all, risking burnout. To mitigate this, quench propagation heating plates were added to increase the quench speed. Updated simulations showed rapid quench across all coils and a significant reduction in hot spot temperatures and peak voltages.
{"title":"Design and Improvement of Quench Protection for A 3 T MRI Superconducting Magnet","authors":"Wangnan Shang, Yunhao Mei, Shige Yang, Bohan Tang, Shili Jiang, Hui Yu, Bowen Xie, Guangli Kuang, Donghui Jiang","doi":"10.1007/s10909-024-03238-3","DOIUrl":"10.1007/s10909-024-03238-3","url":null,"abstract":"<div><p>In recent years, global investment in magnetic resonance imaging (MRI) has surged, with 3 T MRI technology overtaking 1.5 T as the standard in hospitals gradually. A combination of linear programming, genetic algorithms, and nonlinear programming was employed to design an actively shielded 3 T superconducting MRI magnet system. This magnet consists of seven main coils and two shielding coils, achieving a magnetic field with a peak-to-peak inhomogeneity of 10 ppm within a 50-cm-diameter spherical volume (DSV). To address the risk of quench in superconducting magnets, which can lead to damage due to excessive temperature, voltage, and stress, a quench protection system is crucial. The designed system segments the coils for protection, using diode pairs and shunt resistors to manage the quench. Initial simulations indicated that temperature rises and voltages were within safe limits, but some coils were slow to quench or did not quench at all, risking burnout. To mitigate this, quench propagation heating plates were added to increase the quench speed. Updated simulations showed rapid quench across all coils and a significant reduction in hot spot temperatures and peak voltages.</p></div>","PeriodicalId":641,"journal":{"name":"Journal of Low Temperature Physics","volume":"218 3-4","pages":"146 - 165"},"PeriodicalIF":1.1,"publicationDate":"2024-11-07","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"143362074","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}
The fractional electron capture probabilities of 59Ni were measured using metallic magnetic calorimeters (MMCs). 59Ni was one of the radionuclides chosen as a part of the European Metrology Research (EMPIR) project MetroMMC. The measurement was performed by using the decay energy spectroscopy (DES) technique, where the radionuclide is embedded in the absorber to have a 4π geometry. Two different source preparation techniques adapted for the measurement are also discussed: electroplating on gold foil and micro-drop-dispensing on gold nanofoam. The total energy spectra obtained from both sources are compared with each other, and the measured fractional electron capture probabilities are compared with those available in the literature and from the BetaShape code.
{"title":"Determination of Fractional Electron Capture Probabilities of 59Ni by Means of Metallic Magnetic Calorimeters","authors":"Arshjot Kaur, Lucille Chambon, Martin Loidl, Valérie Lourenço, Matias Rodrigues, Mostafa-Lokmann Zahir","doi":"10.1007/s10909-024-03235-6","DOIUrl":"10.1007/s10909-024-03235-6","url":null,"abstract":"<div><p>The fractional electron capture probabilities of <sup>59</sup>Ni were measured using metallic magnetic calorimeters (MMCs). <sup>59</sup>Ni was one of the radionuclides chosen as a part of the European Metrology Research (EMPIR) project MetroMMC. The measurement was performed by using the decay energy spectroscopy (DES) technique, where the radionuclide is embedded in the absorber to have a 4π geometry. Two different source preparation techniques adapted for the measurement are also discussed: electroplating on gold foil and micro-drop-dispensing on gold nanofoam. The total energy spectra obtained from both sources are compared with each other, and the measured fractional electron capture probabilities are compared with those available in the literature and from the BetaShape code.</p></div>","PeriodicalId":641,"journal":{"name":"Journal of Low Temperature Physics","volume":"218 Part 5","pages":"29 - 38"},"PeriodicalIF":1.1,"publicationDate":"2024-11-06","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"142994608","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 : 2024-11-04DOI: 10.1007/s10909-024-03233-8
Zhenyu Yang, Changwei Zhai, Hongxing Yang, Jianting Zhao, Yunfeng Lu
Superconducting quantum interference device (SQUID) has been widely used in various metrological and high-precision-demanding applications, owing to its excellent magnetic flux resolution. Nevertheless, the SQUID with nonlinear flux-to-voltage characteristics makes the stable and accurate readout circuit crucial for applications. In this paper, we design a self-feedback differential low-noise amplifier (SDLA) which relies on the flux-loop lock (FLL) to construct the direct readout circuit. This weakens the feedback current and maintains the balance between two-terminals SQUID, thus minimizing the influence of wire resistors. The SDLA is composed of matched transistors and two amplifiers that maintain stable amplification performance and low noise performance through current feedback. In a series of experiments, the feedback current is reduced to the pA level, minimizing wire resistor influences. And, the white input voltage noise of the readout circuit is around 0.65 nV/Hz1/2.
超导量子干涉装置(SQUID)凭借其出色的磁通分辨率,已被广泛应用于各种计量和高精度要求的应用领域。然而,由于 SQUID 具有非线性磁通-电压特性,因此稳定、精确的读出电路对其应用至关重要。在本文中,我们设计了一种自反馈差分低噪声放大器(SDLA),它依靠磁通环锁定(FLL)来构建直接读出电路。这样可以减弱反馈电流,保持两端 SQUID 之间的平衡,从而最大限度地减少导线电阻的影响。SDLA 由匹配的晶体管和两个放大器组成,通过电流反馈保持稳定的放大性能和低噪声性能。在一系列实验中,反馈电流被降至 pA 级,从而将线电阻的影响降至最低。而且,读出电路的白输入电压噪声约为 0.65 nV/Hz1/2。
{"title":"Investigation of Superconducting Quantum Interference Readout Electronics Based on Self-Feedback Differential Low-Noise Amplifier","authors":"Zhenyu Yang, Changwei Zhai, Hongxing Yang, Jianting Zhao, Yunfeng Lu","doi":"10.1007/s10909-024-03233-8","DOIUrl":"10.1007/s10909-024-03233-8","url":null,"abstract":"<div><p>Superconducting quantum interference device (SQUID) has been widely used in various metrological and high-precision-demanding applications, owing to its excellent magnetic flux resolution. Nevertheless, the SQUID with nonlinear flux-to-voltage characteristics makes the stable and accurate readout circuit crucial for applications. In this paper, we design a self-feedback differential low-noise amplifier (SDLA) which relies on the flux-loop lock (FLL) to construct the direct readout circuit. This weakens the feedback current and maintains the balance between two-terminals SQUID, thus minimizing the influence of wire resistors. The SDLA is composed of matched transistors and two amplifiers that maintain stable amplification performance and low noise performance through current feedback. In a series of experiments, the feedback current is reduced to the pA level, minimizing wire resistor influences. And, the white input voltage noise of the readout circuit is around 0.65 nV/Hz<sup>1/2</sup>.</p></div>","PeriodicalId":641,"journal":{"name":"Journal of Low Temperature Physics","volume":"218 3-4","pages":"125 - 135"},"PeriodicalIF":1.1,"publicationDate":"2024-11-04","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"143362098","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 : 2024-10-23DOI: 10.1007/s10909-024-03228-5
J. van der Kuur, M. Kiviranta, G. de Lange, D. Vaccaro, M. de Wit, L. G. Gottardi, H. A. Akamatsu, B. D. Jackson, K. Nagayoshi, M. P. Bruijn, E. Taralli, K. Ravensberg, J. W. A. den Herder
Several proposed space-based X-ray observatories apply TES-based micro-calorimeters as energy-dispersive imaging detector. The number of independently readout pixels is an important figure of merit for the scientific yield of such instruments. Design studies have shown that the power consumption of the SQUID readout is one of the driving design parameters which limits the maximum number of pixels which can be accommodated. Different multiplexing schemes, each with different properties and multiplexing factors have been proposed and demonstrated for the readout of the TES-based detectors. In an effort to estimate how the different readout multiplexing schemes differ in scalability for future space-based applications, we have made a comparison of the reported power consumption of the main multiplexing schemes currently under consideration for different space-based telescopes, i.e. time-domain multiplexing, frequency-domain multiplexing, and microwave SQUID multiplexing. It was found that, despite the different architectures and multiplexing factors, the power consumption per pixel at cryogenic temperatures is rather similar. We will analyze the origin of this phenomenon, and discuss directions of development to further improve on this number.
{"title":"Power Consumption in SQUID Multiplexers for Space-Based Applications","authors":"J. van der Kuur, M. Kiviranta, G. de Lange, D. Vaccaro, M. de Wit, L. G. Gottardi, H. A. Akamatsu, B. D. Jackson, K. Nagayoshi, M. P. Bruijn, E. Taralli, K. Ravensberg, J. W. A. den Herder","doi":"10.1007/s10909-024-03228-5","DOIUrl":"10.1007/s10909-024-03228-5","url":null,"abstract":"<div><p>Several proposed space-based X-ray observatories apply TES-based micro-calorimeters as energy-dispersive imaging detector. The number of independently readout pixels is an important figure of merit for the scientific yield of such instruments. Design studies have shown that the power consumption of the SQUID readout is one of the driving design parameters which limits the maximum number of pixels which can be accommodated. Different multiplexing schemes, each with different properties and multiplexing factors have been proposed and demonstrated for the readout of the TES-based detectors. In an effort to estimate how the different readout multiplexing schemes differ in scalability for future space-based applications, we have made a comparison of the reported power consumption of the main multiplexing schemes currently under consideration for different space-based telescopes, i.e. time-domain multiplexing, frequency-domain multiplexing, and microwave SQUID multiplexing. It was found that, despite the different architectures and multiplexing factors, the power consumption per pixel at cryogenic temperatures is rather similar. We will analyze the origin of this phenomenon, and discuss directions of development to further improve on this number.</p></div>","PeriodicalId":641,"journal":{"name":"Journal of Low Temperature Physics","volume":"218 Part 5","pages":"1 - 11"},"PeriodicalIF":1.1,"publicationDate":"2024-10-23","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"142995688","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 : 2024-10-23DOI: 10.1007/s10909-024-03229-4
A. Mehedi, M. Benarous, A. Hocine
Considering both interspecies and intraspecies quantum fluctuations in quasi-one dimensional ultracold Bose–Bose mixtures, we show that new LHY-like effects lead to generalized stability conditions against collapse and phase separation. Moreover, we demonstrate that the stability of self-bound droplets is enhanced by interspecies correlations. The contribution to the energy of the quadratic fluctuations is shown to have negligible effects in the Bogoliubov approximation.
{"title":"Enhanced Stability of Self-Bound Droplets in Quasi-One Dimension via Interspecies Quantum Fluctuations in Ultracold Bose–Bose Mixtures","authors":"A. Mehedi, M. Benarous, A. Hocine","doi":"10.1007/s10909-024-03229-4","DOIUrl":"10.1007/s10909-024-03229-4","url":null,"abstract":"<div><p>Considering both interspecies and intraspecies quantum fluctuations in quasi-one dimensional ultracold Bose–Bose mixtures, we show that new LHY-like effects lead to generalized stability conditions against collapse and phase separation. Moreover, we demonstrate that the stability of self-bound droplets is enhanced by interspecies correlations. The contribution to the energy of the quadratic fluctuations is shown to have negligible effects in the Bogoliubov approximation.</p></div>","PeriodicalId":641,"journal":{"name":"Journal of Low Temperature Physics","volume":"217 5-6","pages":"749 - 761"},"PeriodicalIF":1.1,"publicationDate":"2024-10-23","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"142600521","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 : 2024-10-22DOI: 10.1007/s10909-024-03227-6
Ya-Ping Li, Liu Yang, Hao-Dong Liu, Shu-Ying Shang, Ying-Jie Chen
In recent years, as two-dimensional (2D) materials have been widely used in electronic devices, searching for 2D high superconducting transition temperature ((T_{c})) superconductors has also attracted great attentions. In this work, based on first-principles calculations and Eliashberg equation, the electronic structure, electron-phonon coupling (EPC) and possible superconductivity of alkali metal-deposited monolayer BC: MBC (M = Na, K) are studied. The results show that MBC (M = Na, K) are metallic and potential superconductors. The calculated EPC constants of MBC (M = Na, K) are 0.97 and 1.48, respectively. The strong coupling of MBC (M = Na, K) mainly origins from the coupling between electrons with the in-plane vibration modes of C and B atoms. The (T_{c}) of MBC (M = Na, K) are 34.1 K and 41.7 K, respectively, and the (T_{c}) of NaBC can be increased to 45.6 K under 2% biaxial tensile strain, and the (T_{c}) of KBC can be boosted to 53.8 K under 1% biaxial tensile strain. It is anticipated that the predicted monolayer MBC (M = Na, K) and its strained cases can be realized in future experiments.
{"title":"Superconductivity in Alkali Metal-Deposited Monolayer BC: MBC (M = Na, K)","authors":"Ya-Ping Li, Liu Yang, Hao-Dong Liu, Shu-Ying Shang, Ying-Jie Chen","doi":"10.1007/s10909-024-03227-6","DOIUrl":"10.1007/s10909-024-03227-6","url":null,"abstract":"<div><p>In recent years, as two-dimensional (2D) materials have been widely used in electronic devices, searching for 2D high superconducting transition temperature (<span>(T_{c})</span>) superconductors has also attracted great attentions. In this work, based on first-principles calculations and Eliashberg equation, the electronic structure, electron-phonon coupling (EPC) and possible superconductivity of alkali metal-deposited monolayer BC: <i>M</i>BC (<i>M</i> = Na, K) are studied. The results show that <i>M</i>BC (<i>M</i> = Na, K) are metallic and potential superconductors. The calculated EPC constants of <i>M</i>BC (<i>M</i> = Na, K) are 0.97 and 1.48, respectively. The strong coupling of <i>M</i>BC (<i>M</i> = Na, K) mainly origins from the coupling between electrons with the in-plane vibration modes of C and B atoms. The <span>(T_{c})</span> of <i>M</i>BC (<i>M </i>= Na, K) are 34.1 K and 41.7 K, respectively, and the <span>(T_{c})</span> of NaBC can be increased to 45.6 K under 2% biaxial tensile strain, and the <span>(T_{c})</span> of KBC can be boosted to 53.8 K under 1% biaxial tensile strain. It is anticipated that the predicted monolayer <i>M</i>BC (<i>M</i> = Na, K) and its strained cases can be realized in future experiments.</p></div>","PeriodicalId":641,"journal":{"name":"Journal of Low Temperature Physics","volume":"217 5-6","pages":"735 - 748"},"PeriodicalIF":1.1,"publicationDate":"2024-10-22","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"142600826","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 : 2024-10-21DOI: 10.1007/s10909-024-03224-9
Soumia Siouane, Abdelmalek Boumali
In this study, we investigate the thermal properties of the relativistic Klein-Gordon oscillator with non-minimal coupling in one, two, and three dimensions within the framework of superstatistics theory. We focus on three distinct distributions: Gamma, Log-Normal, and F-distributions, each described by a specific probability density function (f(beta )). To compute the partition function, we apply the Euler-MacLaurin formula, incorporating the low-energy asymptotics approximation of superstatistics and accounting for the remainder term (R_{i}). Our study involves a detailed analysis of how entropy (S) and specific heat (C_{v}) vary with temperature (1/beta) and the universal parameter (q), based on the derived partition functions. The variations in these thermodynamic quantities are explored across different dimensionalities and statistical frameworks, providing insights into the interplay between statistical distributions and the thermal dynamics of the system. This approach allows us to understand the influence of non-equilibrium conditions and fluctuating temperature fields on the behavior of relativistic quantum systems. By extending the analysis to multiple dimensions and distribution types, we aim to offer a comprehensive view of how superstatistical distributions affect the thermodynamic properties of the Klein-Gordon oscillator, thus contributing to the broader understanding of thermal dynamics in relativistic systems.
在本研究中,我们在超统计理论框架内研究了具有非最小耦合的相对论克莱因-戈登振荡器在一维、二维和三维的热特性。我们关注三种不同的分布:伽马分布、对数正态分布和 F 分布,每种分布都由特定的概率密度函数 (f(beta))描述。为了计算分区函数,我们应用了欧拉-麦克劳林公式,结合了超统计的低能渐近近似,并考虑了余项 (R_{i})。我们的研究包括根据推导出的分区函数,详细分析熵(S)和比热(C_{v})如何随温度(1//beta)和通用参数(q)变化。这些热力学量的变化在不同的维度和统计框架下进行了探索,为统计分布和系统热动力学之间的相互作用提供了见解。通过这种方法,我们可以了解非平衡条件和波动温度场对相对论量子系统行为的影响。通过将分析扩展到多个维度和分布类型,我们旨在提供一个关于超统计分布如何影响克莱因-戈登振荡器热力学特性的全面视角,从而有助于更广泛地理解相对论系统的热动力学。
{"title":"On the Superstatistical Properties of the Klein-Gordon Oscillator Using Gamma, Log, and F Distributions","authors":"Soumia Siouane, Abdelmalek Boumali","doi":"10.1007/s10909-024-03224-9","DOIUrl":"10.1007/s10909-024-03224-9","url":null,"abstract":"<div><p>In this study, we investigate the thermal properties of the relativistic Klein-Gordon oscillator with non-minimal coupling in one, two, and three dimensions within the framework of superstatistics theory. We focus on three distinct distributions: Gamma, Log-Normal, and F-distributions, each described by a specific probability density function <span>(f(beta ))</span>. To compute the partition function, we apply the Euler-MacLaurin formula, incorporating the low-energy asymptotics approximation of superstatistics and accounting for the remainder term <span>(R_{i})</span>. Our study involves a detailed analysis of how entropy <span>(S)</span> and specific heat <span>(C_{v})</span> vary with temperature <span>(1/beta)</span> and the universal parameter <span>(q)</span>, based on the derived partition functions. The variations in these thermodynamic quantities are explored across different dimensionalities and statistical frameworks, providing insights into the interplay between statistical distributions and the thermal dynamics of the system. This approach allows us to understand the influence of non-equilibrium conditions and fluctuating temperature fields on the behavior of relativistic quantum systems. By extending the analysis to multiple dimensions and distribution types, we aim to offer a comprehensive view of how superstatistical distributions affect the thermodynamic properties of the Klein-Gordon oscillator, thus contributing to the broader understanding of thermal dynamics in relativistic systems.</p></div>","PeriodicalId":641,"journal":{"name":"Journal of Low Temperature Physics","volume":"217 Part 4","pages":"598 - 617"},"PeriodicalIF":1.1,"publicationDate":"2024-10-21","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"142587737","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 : 2024-10-21DOI: 10.1007/s10909-024-03230-x
M. Platino, M. E. García Redondo, L. P. Ferreyro, J. M. Salum, N. A. Müller, J. D. Bonilla-Neira, T. Muscheid, R. Gartmann, J. M. Geria, J. J. Bonaparte, D. A. Almela, L. E. Ardila-Pérez, M. R. Hampel, A. E. Fuster, O. Sander, M. Weber, A. Etchegoyen
Several experiments are currently carried out to measure the magnitude of the B mode polarization of the cosmic microwave background (CMB). It is a strong indicator of the presence of gravitational waves from the early universe inflationary epoch. As the average variations of the B mode components of the CMB are expected to be of the order of a few tens of nK or below, the detection of these polarized signals requires an ultrasensitive system. This article is focused on CMB detection at frequencies around the 150 GHz band of the electromagnetic spectrum, near the peak of the CMB 2.7K blackbody band of the EM spectrum. We propose a readout system for CMB cryogenic detection based on a software-defined radio (SDR) that uses frequency division multiplexing (FDM), a Goertzel channelizer and a radio frequency microwave SQUID multiplexer ((mu)MUX) working at the cryogenic temperatures of (approx) 320mK. These interfaces can be used to read an array of 1024 magnetic microbolometers (MMBs) as detectors that are photon-limited for CMB detection in the band of interest. As part of the requirements for these measurements, we introduce a design of the detection and read out chain and show its expected performance and potential implementation. The proposed system can read the desired number of detectors from an array in a modular way, which allows future expansions, and its frequency division multiplexing system improves the cooling capacity of the cryostat by minimizing the amount of active cryogenic electronics. In this article, we first describe this proposed FDM readout chain and then present noise measurements of a test implementation.
目前正在进行几项实验,以测量宇宙微波背景(CMB)B 模式极化的大小。它是早期宇宙膨胀时代引力波存在的一个有力指标。由于预计 CMB 的 B 模式分量的平均变化量级为几十 nK 或更低,探测这些极化信号需要一个超灵敏系统。本文的重点是在电磁波谱的 150 GHz 频段附近探测 CMB,该频段接近电磁波谱中 CMB 2.7K 黑体频段的峰值。我们提出了一种用于CMB低温探测的读出系统,它基于软件定义无线电(SDR),使用频分复用(FDM)、Goertzel信道器和射频微波SQUID复用器(MUX),可在320mK的低温下工作。这些接口可用于读取由1024个磁性微测辐射计(MMB)组成的阵列,作为在感兴趣波段进行CMB探测的光子限制探测器。作为这些测量要求的一部分,我们介绍了探测和读出链的设计,并展示了其预期性能和可能的实施。所提议的系统能够以模块化方式从阵列中读取所需的探测器数量,从而允许未来的扩展,其频分复用系统通过最大限度地减少有源低温电子设备的数量,提高了低温恒温器的冷却能力。在本文中,我们首先介绍了这种拟议的频分复用读出链,然后介绍了测试实施的噪声测量结果。
{"title":"The Magnetic Microbolometer Detection Chain: A Proposed Detection System to Observe the B Modes of the Cosmic Microwave Background","authors":"M. Platino, M. E. García Redondo, L. P. Ferreyro, J. M. Salum, N. A. Müller, J. D. Bonilla-Neira, T. Muscheid, R. Gartmann, J. M. Geria, J. J. Bonaparte, D. A. Almela, L. E. Ardila-Pérez, M. R. Hampel, A. E. Fuster, O. Sander, M. Weber, A. Etchegoyen","doi":"10.1007/s10909-024-03230-x","DOIUrl":"10.1007/s10909-024-03230-x","url":null,"abstract":"<div><p>Several experiments are currently carried out to measure the magnitude of the B mode polarization of the cosmic microwave background (CMB). It is a strong indicator of the presence of gravitational waves from the early universe inflationary epoch. As the average variations of the B mode components of the CMB are expected to be of the order of a few tens of nK or below, the detection of these polarized signals requires an ultrasensitive system. This article is focused on CMB detection at frequencies around the 150 GHz band of the electromagnetic spectrum, near the peak of the CMB 2.7K blackbody band of the EM spectrum. We propose a readout system for CMB cryogenic detection based on a software-defined radio (SDR) that uses frequency division multiplexing (FDM), a Goertzel channelizer and a radio frequency microwave SQUID multiplexer (<span>(mu)</span>MUX) working at the cryogenic temperatures of <span>(approx)</span> 320mK. These interfaces can be used to read an array of 1024 magnetic microbolometers (MMBs) as detectors that are photon-limited for CMB detection in the band of interest. As part of the requirements for these measurements, we introduce a design of the detection and read out chain and show its expected performance and potential implementation. The proposed system can read the desired number of detectors from an array in a modular way, which allows future expansions, and its frequency division multiplexing system improves the cooling capacity of the cryostat by minimizing the amount of active cryogenic electronics. In this article, we first describe this proposed FDM readout chain and then present noise measurements of a test implementation.</p></div>","PeriodicalId":641,"journal":{"name":"Journal of Low Temperature Physics","volume":"217 5-6","pages":"762 - 771"},"PeriodicalIF":1.1,"publicationDate":"2024-10-21","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"142600802","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}