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Machine learning-based detection of nonaxisymmetric fast neutrino flavor instabilities in core-collapse supernovae
IF 5 2区 物理与天体物理 Q1 Physics and Astronomy Pub Date : 2025-03-31 DOI: 10.1103/physrevd.111.063077
Sajad Abbar, Akira Harada, Hiroki Nagakura
In dense neutrino environments like core-collapse supernovae (CCSNe) and neutron star mergers, neutrinos can undergo fast flavor conversions when their angular distribution of neutrino electron lepton number (νELN) crosses zero along some directions. While previous studies have demonstrated the detection of axisymmetric νELN crossings in these extreme environments, nonaxisymmetric crossings have remained elusive, mostly due to the absence of models for their angular distributions. In this study, we present a pioneering analysis of the detection of nonaxisymmetric νELN crossings using machine learning (ML) techniques. Our ML models are trained on data from two CCSN simulations, one with rotation and one without, where nonaxisymmetric features in neutrino angular distributions play a crucial role. We demonstrate that our ML models achieve detection accuracies exceeding 90%. This is an important improvement, especially considering that a significant portion of νELN crossings in these models eluded detection by earlier methods. Published by the American Physical Society 2025
{"title":"Machine learning-based detection of nonaxisymmetric fast neutrino flavor instabilities in core-collapse supernovae","authors":"Sajad Abbar, Akira Harada, Hiroki Nagakura","doi":"10.1103/physrevd.111.063077","DOIUrl":"https://doi.org/10.1103/physrevd.111.063077","url":null,"abstract":"In dense neutrino environments like core-collapse supernovae (CCSNe) and neutron star mergers, neutrinos can undergo fast flavor conversions when their angular distribution of neutrino electron lepton number (ν</a:mi>ELN</a:mi></a:math>) crosses zero along some directions. While previous studies have demonstrated the detection of axisymmetric <c:math xmlns:c=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"><c:mi>ν</c:mi><c:mi>ELN</c:mi></c:math> crossings in these extreme environments, nonaxisymmetric crossings have remained elusive, mostly due to the absence of models for their angular distributions. In this study, we present a pioneering analysis of the detection of nonaxisymmetric <e:math xmlns:e=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"><e:mi>ν</e:mi><e:mi>ELN</e:mi></e:math> crossings using machine learning (ML) techniques. Our ML models are trained on data from two CCSN simulations, one with rotation and one without, where nonaxisymmetric features in neutrino angular distributions play a crucial role. We demonstrate that our ML models achieve detection accuracies exceeding 90%. This is an important improvement, especially considering that a significant portion of <g:math xmlns:g=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"><g:mi>ν</g:mi><g:mi>ELN</g:mi></g:math> crossings in these models eluded detection by earlier methods. <jats:supplementary-material> <jats:copyright-statement>Published by the American Physical Society</jats:copyright-statement> <jats:copyright-year>2025</jats:copyright-year> </jats:permissions> </jats:supplementary-material>","PeriodicalId":20167,"journal":{"name":"Physical Review D","volume":"183 1","pages":""},"PeriodicalIF":5.0,"publicationDate":"2025-03-31","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"143736696","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":2,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
引用次数: 0
Circadian coupling orchestrates cell growth
IF 19.6 1区 物理与天体物理 Q1 PHYSICS, MULTIDISCIPLINARY Pub Date : 2025-03-31 DOI: 10.1038/s41567-025-02838-4
Nica Gutu, Malthe S. Nordentoft, Marlena Kuhn, Carolin Ector, Marie Möser, Anna-Marie Finger, Mathias Spliid Heltberg, Mogens Høgh Jensen, Ulrich Keilholz, Achim Kramer, Hanspeter Herzel, Adrián E. Granada

Single-cell circadian oscillators exchange extracellular information to sustain coherent circadian rhythms at the tissue level. The circadian clock and the cell cycle couple within cells but the mechanisms underlying this interplay are poorly understood. We show that the loss of extracellular circadian synchronization disrupts circadian and cell cycle coordination within individual cells, impeding collective tissue growth. We use the theory of coupled oscillators combined with live population, and single-cell recordings and precise experimental perturbations. Coherent circadian rhythms yield oscillatory growth patterns, which unveil a global timing regulator of tissue dynamics. Knocking out core circadian elements abolishes the observed effects, highlighting the central role of circadian clock regulation. Our results underscore the role of tissue-level circadian disruption in regulating proliferation, thereby linking disrupted circadian clocks with oncogenic processes. These findings illuminate the intricate interplay between circadian rhythms, cellular signalling and tissue physiology and enhance our understanding of tissue homeostasis and growth regulation in the context of both health and disease.

{"title":"Circadian coupling orchestrates cell growth","authors":"Nica Gutu, Malthe S. Nordentoft, Marlena Kuhn, Carolin Ector, Marie Möser, Anna-Marie Finger, Mathias Spliid Heltberg, Mogens Høgh Jensen, Ulrich Keilholz, Achim Kramer, Hanspeter Herzel, Adrián E. Granada","doi":"10.1038/s41567-025-02838-4","DOIUrl":"https://doi.org/10.1038/s41567-025-02838-4","url":null,"abstract":"<p>Single-cell circadian oscillators exchange extracellular information to sustain coherent circadian rhythms at the tissue level. The circadian clock and the cell cycle couple within cells but the mechanisms underlying this interplay are poorly understood. We show that the loss of extracellular circadian synchronization disrupts circadian and cell cycle coordination within individual cells, impeding collective tissue growth. We use the theory of coupled oscillators combined with live population, and single-cell recordings and precise experimental perturbations. Coherent circadian rhythms yield oscillatory growth patterns, which unveil a global timing regulator of tissue dynamics. Knocking out core circadian elements abolishes the observed effects, highlighting the central role of circadian clock regulation. Our results underscore the role of tissue-level circadian disruption in regulating proliferation, thereby linking disrupted circadian clocks with oncogenic processes. These findings illuminate the intricate interplay between circadian rhythms, cellular signalling and tissue physiology and enhance our understanding of tissue homeostasis and growth regulation in the context of both health and disease.</p>","PeriodicalId":19100,"journal":{"name":"Nature Physics","volume":"69 1","pages":""},"PeriodicalIF":19.6,"publicationDate":"2025-03-31","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"143736736","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":1,"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}
引用次数: 0
Crystal-symmetry-paired spin–valley locking in a layered room-temperature metallic altermagnet candidate
IF 19.6 1区 物理与天体物理 Q1 PHYSICS, MULTIDISCIPLINARY Pub Date : 2025-03-31 DOI: 10.1038/s41567-025-02864-2
Fayuan Zhang, Xingkai Cheng, Zhouyi Yin, Changchao Liu, Liwei Deng, Yuxi Qiao, Zheng Shi, Shuxuan Zhang, Junhao Lin, Zhengtai Liu, Mao Ye, Yaobo Huang, Xiangyu Meng, Cheng Zhang, Taichi Okuda, Kenya Shimada, Shengtao Cui, Yue Zhao, Guang-Han Cao, Shan Qiao, Junwei Liu, Chaoyu Chen

Previous theoretical efforts have predicted a type of unconventional antiferromagnet characterized by a crystal symmetry that connects antiferromagnetic sublattices in real space and simultaneously couples spin and momentum in reciprocal space. This results in a unique crystal-symmetry-paired spin–valley locking and related properties including piezomagnetism and non-collinear spin current even without spin–orbit coupling. However, most known unconventional antiferromagnets do not meet the necessary symmetry requirements for non-relativistic spin current, and this limits applications in spintronic devices. Here we demonstrate crystal-symmetry-paired spin–valley locking in a layered room-temperature antiferromagnetic compound, Rb1−δV2Te2O. Spin-resolved photoemission measurements directly show the opposite spin splitting between crystal-symmetry-paired valleys. Quasi-particle interference patterns show the suppression of intervalley scattering due to the spin selection rules that are a direct consequence of the spin–valley locking. These results suggest that Rb1−δV2Te2O is a potential room-temperature altermagnet candidate. Our observations highlight a methodology that enables both the advantages of layered materials and possible control through crystal symmetry manipulation for advancements in magnetism, electronics and information technology.

{"title":"Crystal-symmetry-paired spin–valley locking in a layered room-temperature metallic altermagnet candidate","authors":"Fayuan Zhang, Xingkai Cheng, Zhouyi Yin, Changchao Liu, Liwei Deng, Yuxi Qiao, Zheng Shi, Shuxuan Zhang, Junhao Lin, Zhengtai Liu, Mao Ye, Yaobo Huang, Xiangyu Meng, Cheng Zhang, Taichi Okuda, Kenya Shimada, Shengtao Cui, Yue Zhao, Guang-Han Cao, Shan Qiao, Junwei Liu, Chaoyu Chen","doi":"10.1038/s41567-025-02864-2","DOIUrl":"https://doi.org/10.1038/s41567-025-02864-2","url":null,"abstract":"<p>Previous theoretical efforts have predicted a type of unconventional antiferromagnet characterized by a crystal symmetry that connects antiferromagnetic sublattices in real space and simultaneously couples spin and momentum in reciprocal space. This results in a unique crystal-symmetry-paired spin–valley locking and related properties including piezomagnetism and non-collinear spin current even without spin–orbit coupling. However, most known unconventional antiferromagnets do not meet the necessary symmetry requirements for non-relativistic spin current, and this limits applications in spintronic devices. Here we demonstrate crystal-symmetry-paired spin–valley locking in a layered room-temperature antiferromagnetic compound, Rb<sub>1−<i>δ</i></sub>V<sub>2</sub>Te<sub>2</sub>O. Spin-resolved photoemission measurements directly show the opposite spin splitting between crystal-symmetry-paired valleys. Quasi-particle interference patterns show the suppression of intervalley scattering due to the spin selection rules that are a direct consequence of the spin–valley locking. These results suggest that Rb<sub>1−<i>δ</i></sub>V<sub>2</sub>Te<sub>2</sub>O is a potential room-temperature altermagnet candidate. Our observations highlight a methodology that enables both the advantages of layered materials and possible control through crystal symmetry manipulation for advancements in magnetism, electronics and information technology.</p>","PeriodicalId":19100,"journal":{"name":"Nature Physics","volume":"183 1","pages":""},"PeriodicalIF":19.6,"publicationDate":"2025-03-31","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"143736737","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":1,"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}
引用次数: 0
Old neutron stars as a new probe of relic neutrinos and sterile neutrino dark matter
IF 5 2区 物理与天体物理 Q1 Physics and Astronomy Pub Date : 2025-03-31 DOI: 10.1103/physrevd.111.055035
Saurav Das, P. S. Bhupal Dev, Takuya Okawa, Amarjit Soni
We study the kinetic cooling (heating) of old neutron stars due to coherent scattering with relic neutrinos (sterile neutrino dark matter) via Standard Model neutral-current interactions. We take into account several important physical effects, such as coherent enhancement, gravitational clustering, neutron degeneracy, Pauli blocking and weak potential. We find that the anomalous cooling of neutron stars due to relic neutrino scattering is difficult to observe. However, the anomalous heating of neutron stars due to coherent scattering with keV-scale sterile neutrino dark matter may be observed by current and future telescopes operating in the optical to near-infrared frequency band, such as the James Webb Space Telescope (JWST), which would probe hitherto unexplored parameter space in the sterile neutrino mass-mixing plane. Published by the American Physical Society 2025
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引用次数: 0
Yielding behaviour of active particles in bulk and in confinement
IF 19.6 1区 物理与天体物理 Q1 PHYSICS, MULTIDISCIPLINARY Pub Date : 2025-03-31 DOI: 10.1038/s41567-025-02843-7
Yagyik Goswami, G. V. Shivashankar, Srikanth Sastry

Collective behaviour in dense assemblies of self-propelled active particles occurs in a wide range of biological phenomena, including the dynamical transitions of cellular and subcellular biological assemblies such as the cytoskeleton and the cell nucleus. Here, motivated by observations of mechanically induced changes in the dynamics of such systems and the apparent role of confinement geometry, we show that the fluidization transition broadly resembles yielding in amorphous solids, which is consistent with recent suggestions. More specifically, however, we find that a detailed analogy holds with the yielding transition under cyclic shear deformation, for large but finite persistence times. The fluidization transition is accompanied by driving-induced annealing, strong dependence on the initial state of the system, a divergence of timescales to reach steady states and a discontinuous onset of diffusive motion. We also observe a striking dependence of transition on persistence times and on the nature of confinement. Collectively, our results have implications for biological assemblies in confined geometries, including epigenetic cell-state transitions.

{"title":"Yielding behaviour of active particles in bulk and in confinement","authors":"Yagyik Goswami, G. V. Shivashankar, Srikanth Sastry","doi":"10.1038/s41567-025-02843-7","DOIUrl":"https://doi.org/10.1038/s41567-025-02843-7","url":null,"abstract":"<p>Collective behaviour in dense assemblies of self-propelled active particles occurs in a wide range of biological phenomena, including the dynamical transitions of cellular and subcellular biological assemblies such as the cytoskeleton and the cell nucleus. Here, motivated by observations of mechanically induced changes in the dynamics of such systems and the apparent role of confinement geometry, we show that the fluidization transition broadly resembles yielding in amorphous solids, which is consistent with recent suggestions. More specifically, however, we find that a detailed analogy holds with the yielding transition under cyclic shear deformation, for large but finite persistence times. The fluidization transition is accompanied by driving-induced annealing, strong dependence on the initial state of the system, a divergence of timescales to reach steady states and a discontinuous onset of diffusive motion. We also observe a striking dependence of transition on persistence times and on the nature of confinement. Collectively, our results have implications for biological assemblies in confined geometries, including epigenetic cell-state transitions.</p>","PeriodicalId":19100,"journal":{"name":"Nature Physics","volume":"19 1","pages":""},"PeriodicalIF":19.6,"publicationDate":"2025-03-31","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"143736730","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":1,"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}
引用次数: 0
An interference-based method for the detection of strongly lensed gravitational waves
IF 14.1 1区 物理与天体物理 Q1 ASTRONOMY & ASTROPHYSICS Pub Date : 2025-03-31 DOI: 10.1038/s41550-025-02519-5
Xikai Shan, Bin Hu, Xuechun Chen, Rong-Gen Cai

The strongly lensed gravitational wave (SLGW) is a promising transient phenomenon. However, the long-wave nature of gravitational waves poses a considerable challenge in the identification of its host galaxy. Here, to tackle this challenge, we propose a method triggered by the wave optics effect of microlensing. The microlensing interference introduces frequency-dependent fluctuations in the waveform. Our method consists of three steps. First, we reconstruct the waveforms by using template-independent and template-dependent methods. The mismatch of two reconstructions serves as an indicator of SLGWs. This step can identify approximately 10% SLGWs. Second, we pair the multiple images of the SLGWs by using sky localization overlapping. Because we have preidentified at least one image through microlensing, the false-alarm probability for pairing SLGWs is significantly reduced. Third, we search the host galaxy by requiring the consistency of time delays between galaxy–galaxy lensing and SLGW. By combing the stage-IV galaxy survey and the third-generation gravitational wave detectors, we expect to find, on average, one quadruple-image system per 3 years. This method can substantially facilitate the pursuit of time-delay cosmography, discovery of compact objects and multimessenger astronomy.

{"title":"An interference-based method for the detection of strongly lensed gravitational waves","authors":"Xikai Shan, Bin Hu, Xuechun Chen, Rong-Gen Cai","doi":"10.1038/s41550-025-02519-5","DOIUrl":"https://doi.org/10.1038/s41550-025-02519-5","url":null,"abstract":"<p>The strongly lensed gravitational wave (SLGW) is a promising transient phenomenon. However, the long-wave nature of gravitational waves poses a considerable challenge in the identification of its host galaxy. Here, to tackle this challenge, we propose a method triggered by the wave optics effect of microlensing. The microlensing interference introduces frequency-dependent fluctuations in the waveform. Our method consists of three steps. First, we reconstruct the waveforms by using template-independent and template-dependent methods. The mismatch of two reconstructions serves as an indicator of SLGWs. This step can identify approximately 10% SLGWs. Second, we pair the multiple images of the SLGWs by using sky localization overlapping. Because we have preidentified at least one image through microlensing, the false-alarm probability for pairing SLGWs is significantly reduced. Third, we search the host galaxy by requiring the consistency of time delays between galaxy–galaxy lensing and SLGW. By combing the stage-IV galaxy survey and the third-generation gravitational wave detectors, we expect to find, on average, one quadruple-image system per 3 years. This method can substantially facilitate the pursuit of time-delay cosmography, discovery of compact objects and multimessenger astronomy.</p>","PeriodicalId":18778,"journal":{"name":"Nature Astronomy","volume":"2 1","pages":""},"PeriodicalIF":14.1,"publicationDate":"2025-03-31","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"143736740","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":1,"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}
引用次数: 0
Global Hall-magnetohydrodynamic simulations of transition disks
IF 6.5 2区 物理与天体物理 Q1 ASTRONOMY & ASTROPHYSICS Pub Date : 2025-03-31 DOI: 10.1051/0004-6361/202452121
Eleftheria Sarafidou, Oliver Gressel, Barbara Ercolano
Context. Transition disks (TDs) are a type of protoplanetary disk characterized by a central dust and gas cavity. The processes behind how these cavities are formed and maintained, along with their observed high accretion rates of 10−8−10−7 M yr−1, continue to be subjects of active research.Aims. This work aims to investigate how the inclusion of the Hall effect (HE) alongside Ohmic resistivity (OR) and ambipolar diffusion (AD) affects the structure of the TD. Of key interest is the dynamical evolution of the cavity and whether it can indeed produce transonic accretion, as predicted by theoretical models in order to account for the observed high accretion rates despite the inner disk’s low density.Methods. We present our results of 2D axisymmetric global radiation magnetohydrodynamic (MHD) simulations of TDs for which all three non ideal MHD effects are accounted. We used the NIRVANA-III fluid code and initialized our model with a disk cavity reaching up to R = 8 au with a density contrast of 105 . We performed three runs, one with only OR and AD, and one for each of the two configurations that arise when additionally including the HE, that is, with the field aligned (anti-aligned) with respect to the rotation axis.Results. For all three runs, our models maintain an intact inner cavity and an outer standard disk. MHD winds are launched both from the cavity and from the disk. Notably, when the HE is included, ring-like structures develop within the cavity. We moreover obtain accretion rates of 3−8 × 10−8 M yr−1, comparable to typical values seen in full disks. Importantly, we clearly observe (tran)sonic accretion (vacccs) in the cavity. Additionally, outward magnetic flux transport occurs in all three runs.
{"title":"Global Hall-magnetohydrodynamic simulations of transition disks","authors":"Eleftheria Sarafidou, Oliver Gressel, Barbara Ercolano","doi":"10.1051/0004-6361/202452121","DOIUrl":"https://doi.org/10.1051/0004-6361/202452121","url":null,"abstract":"<i>Context.<i/> Transition disks (TDs) are a type of protoplanetary disk characterized by a central dust and gas cavity. The processes behind how these cavities are formed and maintained, along with their observed high accretion rates of 10<sup>−8<sup/>−10<sup>−7<sup/> <i>M<i/><sub>⊙<sub/> yr<sup>−1<sup/>, continue to be subjects of active research.<i>Aims.<i/> This work aims to investigate how the inclusion of the Hall effect (HE) alongside Ohmic resistivity (OR) and ambipolar diffusion (AD) affects the structure of the TD. Of key interest is the dynamical evolution of the cavity and whether it can indeed produce transonic accretion, as predicted by theoretical models in order to account for the observed high accretion rates despite the inner disk’s low density.<i>Methods.<i/> We present our results of 2D axisymmetric global radiation magnetohydrodynamic (MHD) simulations of TDs for which all three non ideal MHD effects are accounted. We used the NIRVANA-III fluid code and initialized our model with a disk cavity reaching up to <i>R<i/> = 8 au with a density contrast of 10<sup>5<sup/> . We performed three runs, one with only OR and AD, and one for each of the two configurations that arise when additionally including the HE, that is, with the field aligned (anti-aligned) with respect to the rotation axis.<i>Results.<i/> For all three runs, our models maintain an intact inner cavity and an outer standard disk. MHD winds are launched both from the cavity and from the disk. Notably, when the HE is included, ring-like structures develop within the cavity. We moreover obtain accretion rates of 3−8 × 10<sup>−8<sup/> <i>M<i/><sub>⊙<sub/> yr<sup>−1<sup/>, comparable to typical values seen in full disks. Importantly, we clearly observe (tran)sonic accretion (<i>v<i/><sub>acc<sub/> ≳ <i>c<i/><sub>s<sub/>) in the cavity. Additionally, outward magnetic flux transport occurs in all three runs.","PeriodicalId":8571,"journal":{"name":"Astronomy & Astrophysics","volume":"103 1","pages":""},"PeriodicalIF":6.5,"publicationDate":"2025-03-31","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"143737137","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":2,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
引用次数: 0
Thermopower probes of emergent local moments in magic-angle twisted bilayer graphene
IF 19.6 1区 物理与天体物理 Q1 PHYSICS, MULTIDISCIPLINARY Pub Date : 2025-03-31 DOI: 10.1038/s41567-025-02849-1
Ayan Ghosh, Souvik Chakraborty, Ranit Dutta, Adhip Agarwala, K. Watanabe, T. Taniguchi, Sumilan Banerjee, Nandini Trivedi, Subroto Mukerjee, Anindya Das

Recent experiments on magic-angle twisted bilayer graphene have shown the formation of flat bands, suggesting that electronic correlation effects are likely to dominate in this material. However, a global transport measurement showing distinct signatures of strong correlations—such as local moments arising from the flat bands—is missing. Here we demonstrate the presence of emergent local moments through their impact on entropy extracted from thermopower measurements. In addition to sign changes in the thermopower at the Dirac point and full filling of the flat bands, we observe sign changes near the quarter-filled bands that do not vary with temperature from 5 K to 60 K. This is in contrast to temperature-dependent crossing points seen in our study on twisted bilayer graphene devices with weaker correlations. Furthermore, we find that applying a magnetic field reduces the thermopower, consistent with spin entropy suppression observed in layered oxides under partial spin polarization. Neither the robust crossing points nor the suppression by a magnetic field can be explained solely from the contributions of band fermions; instead, our data suggest a dominant contribution coming from the entropy of the emergent localized moments of a strongly correlated flat band.

{"title":"Thermopower probes of emergent local moments in magic-angle twisted bilayer graphene","authors":"Ayan Ghosh, Souvik Chakraborty, Ranit Dutta, Adhip Agarwala, K. Watanabe, T. Taniguchi, Sumilan Banerjee, Nandini Trivedi, Subroto Mukerjee, Anindya Das","doi":"10.1038/s41567-025-02849-1","DOIUrl":"https://doi.org/10.1038/s41567-025-02849-1","url":null,"abstract":"<p>Recent experiments on magic-angle twisted bilayer graphene have shown the formation of flat bands, suggesting that electronic correlation effects are likely to dominate in this material. However, a global transport measurement showing distinct signatures of strong correlations—such as local moments arising from the flat bands—is missing. Here we demonstrate the presence of emergent local moments through their impact on entropy extracted from thermopower measurements. In addition to sign changes in the thermopower at the Dirac point and full filling of the flat bands, we observe sign changes near the quarter-filled bands that do not vary with temperature from 5 K to 60 K. This is in contrast to temperature-dependent crossing points seen in our study on twisted bilayer graphene devices with weaker correlations. Furthermore, we find that applying a magnetic field reduces the thermopower, consistent with spin entropy suppression observed in layered oxides under partial spin polarization. Neither the robust crossing points nor the suppression by a magnetic field can be explained solely from the contributions of band fermions; instead, our data suggest a dominant contribution coming from the entropy of the emergent localized moments of a strongly correlated flat band.</p>","PeriodicalId":19100,"journal":{"name":"Nature Physics","volume":"38 1","pages":""},"PeriodicalIF":19.6,"publicationDate":"2025-03-31","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"143736733","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":1,"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}
引用次数: 0
Integrated Microwave Photonics Multi-Parameter Measurement System
IF 11 1区 物理与天体物理 Q1 OPTICS Pub Date : 2025-03-31 DOI: 10.1002/lpor.202500013
Yong Zheng, Zhen Han, Liheng Wang, Pu Zhang, Yongheng Jiang, Huifu Xiao, Xudong Zhou, Mingrui Yuan, Mei Xian Low, Aditya Dubey, Thach Giang Nguyen, Qinfen Hao, Guanghui Ren, Arnan Mitchell, Yonghui Tian
Driven by the growing demands in wireless communication, remote sensing and emerging 6G networks, research on microwave signal measurement techniques has attached intensive attention. Unlike conventional electronic-based approaches, photonics chip-based microwave signal measurement systems offer significant advantages, including broad operation bandwidth, reduced weight, and enhanced resistance to unwanted electromagnetic interference. Despite notable progress in integrated microwave photonic measurement systems, the majority remains constrained by bandwidth below 30 GHz, primarily due to the limitation of modulators. Furthermore, most previous studies focus on the measurement of one single parameter, typically the frequency, limiting their applications in more complex, real-world situations. Here, an on-chip photonic microwave multi-parameter measurement system is presented on the thin-film lithium niobate (TFLN) platform. The system enables measurement of microwave frequency, phase, and amplitude, offering an ultra-high bandwidth (up to 60 GHz) with low root-mean-squared errors: 450 MHz for frequency, 3.43° for phase, and 1.64% for amplitude. Additionally, the system is validated by the time-domain reconstruction of unknown sinusoidal microwave signals based on measurement results. This demonstration further broadens the scope of integrated TFLN photonic devices for microwave signal measurement, providing a viable solution to the bandwidth limitations of existing microwave networks and addressing the increasing demands of future information-driven technologies.
{"title":"Integrated Microwave Photonics Multi-Parameter Measurement System","authors":"Yong Zheng, Zhen Han, Liheng Wang, Pu Zhang, Yongheng Jiang, Huifu Xiao, Xudong Zhou, Mingrui Yuan, Mei Xian Low, Aditya Dubey, Thach Giang Nguyen, Qinfen Hao, Guanghui Ren, Arnan Mitchell, Yonghui Tian","doi":"10.1002/lpor.202500013","DOIUrl":"https://doi.org/10.1002/lpor.202500013","url":null,"abstract":"Driven by the growing demands in wireless communication, remote sensing and emerging 6G networks, research on microwave signal measurement techniques has attached intensive attention. Unlike conventional electronic-based approaches, photonics chip-based microwave signal measurement systems offer significant advantages, including broad operation bandwidth, reduced weight, and enhanced resistance to unwanted electromagnetic interference. Despite notable progress in integrated microwave photonic measurement systems, the majority remains constrained by bandwidth below 30 GHz, primarily due to the limitation of modulators. Furthermore, most previous studies focus on the measurement of one single parameter, typically the frequency, limiting their applications in more complex, real-world situations. Here, an on-chip photonic microwave multi-parameter measurement system is presented on the thin-film lithium niobate (TFLN) platform. The system enables measurement of microwave frequency, phase, and amplitude, offering an ultra-high bandwidth (up to 60 GHz) with low root-mean-squared errors: 450 MHz for frequency, 3.43° for phase, and 1.64% for amplitude. Additionally, the system is validated by the time-domain reconstruction of unknown sinusoidal microwave signals based on measurement results. This demonstration further broadens the scope of integrated TFLN photonic devices for microwave signal measurement, providing a viable solution to the bandwidth limitations of existing microwave networks and addressing the increasing demands of future information-driven technologies.","PeriodicalId":204,"journal":{"name":"Laser & Photonics Reviews","volume":"36 1","pages":""},"PeriodicalIF":11.0,"publicationDate":"2025-03-31","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"143737154","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":1,"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}
引用次数: 0
Investigation of Λc states and D¯N molecule production at the EicC and EIC
IF 5 2区 物理与天体物理 Q1 Physics and Astronomy Pub Date : 2025-03-31 DOI: 10.1103/physrevd.111.056029
Kai-Sa Qiao, Bing-Song Zou
We explore various Λ</a:mi>c</a:mi></a:msub></a:math> states, including <d:math xmlns:d="http://www.w3.org/1998/Math/MathML" display="inline"><d:msub><d:mi mathvariant="normal">Λ</d:mi><d:mi>c</d:mi></d:msub></d:math>, <g:math xmlns:g="http://www.w3.org/1998/Math/MathML" display="inline"><g:msub><g:mi mathvariant="normal">Λ</g:mi><g:mi>c</g:mi></g:msub><g:mo stretchy="false">(</g:mo><g:mn>2595</g:mn><g:mo stretchy="false">)</g:mo></g:math>, <l:math xmlns:l="http://www.w3.org/1998/Math/MathML" display="inline"><l:msub><l:mi mathvariant="normal">Λ</l:mi><l:mi>c</l:mi></l:msub><l:mo stretchy="false">(</l:mo><l:mn>2940</l:mn><l:mo stretchy="false">)</l:mo></l:math>, and the predicted <q:math xmlns:q="http://www.w3.org/1998/Math/MathML" display="inline"><q:mo stretchy="false">(</q:mo><q:mover accent="true"><q:mi>D</q:mi><q:mo stretchy="false">¯</q:mo></q:mover><q:mi>N</q:mi><q:mo stretchy="false">)</q:mo></q:math> hadronic molecular states, in photoproduction and electroproduction to estimate their yields at the EicC and EIC. Assuming <w:math xmlns:w="http://www.w3.org/1998/Math/MathML" display="inline"><w:msub><w:mi mathvariant="normal">Λ</w:mi><w:mi>c</w:mi></w:msub><w:mo stretchy="false">(</w:mo><w:mn>2940</w:mn><w:mo stretchy="false">)</w:mo></w:math> as either a hadronic molecular state or a three-quark state, our analysis demonstrates that its production rates are of the same order of magnitude, posing challenges in identifying its underlying structure. After considering the integral luminosity, the yields of <bb:math xmlns:bb="http://www.w3.org/1998/Math/MathML" display="inline"><bb:msub><bb:mi mathvariant="normal">Λ</bb:mi><bb:mi>c</bb:mi></bb:msub></bb:math> excited states reach <eb:math xmlns:eb="http://www.w3.org/1998/Math/MathML" display="inline"><eb:msup><eb:mn>10</eb:mn><eb:mn>6</eb:mn></eb:msup></eb:math> to <gb:math xmlns:gb="http://www.w3.org/1998/Math/MathML" display="inline"><gb:msup><gb:mn>10</gb:mn><gb:mn>7</gb:mn></gb:msup></gb:math> at the EicC and EIC. The <ib:math xmlns:ib="http://www.w3.org/1998/Math/MathML" display="inline"><ib:mo stretchy="false">(</ib:mo><ib:mover accent="true"><ib:mi>D</ib:mi><ib:mo stretchy="false">¯</ib:mo></ib:mover><ib:mi>N</ib:mi><ib:mo stretchy="false">)</ib:mo></ib:math> molecular states with both isospin <ob:math xmlns:ob="http://www.w3.org/1998/Math/MathML" display="inline"><ob:mi>I</ob:mi><ob:mo>=</ob:mo><ob:mn>0</ob:mn></ob:math> and <qb:math xmlns:qb="http://www.w3.org/1998/Math/MathML" display="inline"><qb:mi>I</qb:mi><qb:mo>=</qb:mo><qb:mn>1</qb:mn></qb:math> are also studied, with yields reaching <sb:math xmlns:sb="http://www.w3.org/1998/Math/MathML" display="inline"><sb:msup><sb:mn>10</sb:mn><sb:mn>5</sb:mn></sb:msup></sb:math>, making them likely to be detectable at these facilities. <jats:supplementary-material> <jats:copyright-statement>Published by the American Physical Society</jats:copyright-statement> <jats:copyright-year>2025</jats:copyright-year> </jats:permissions> </jats:supplem
{"title":"Investigation of Λc states and D¯N molecule production at the EicC and EIC","authors":"Kai-Sa Qiao, Bing-Song Zou","doi":"10.1103/physrevd.111.056029","DOIUrl":"https://doi.org/10.1103/physrevd.111.056029","url":null,"abstract":"We explore various Λ&lt;/a:mi&gt;c&lt;/a:mi&gt;&lt;/a:msub&gt;&lt;/a:math&gt; states, including &lt;d:math xmlns:d=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"&gt;&lt;d:msub&gt;&lt;d:mi mathvariant=\"normal\"&gt;Λ&lt;/d:mi&gt;&lt;d:mi&gt;c&lt;/d:mi&gt;&lt;/d:msub&gt;&lt;/d:math&gt;, &lt;g:math xmlns:g=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"&gt;&lt;g:msub&gt;&lt;g:mi mathvariant=\"normal\"&gt;Λ&lt;/g:mi&gt;&lt;g:mi&gt;c&lt;/g:mi&gt;&lt;/g:msub&gt;&lt;g:mo stretchy=\"false\"&gt;(&lt;/g:mo&gt;&lt;g:mn&gt;2595&lt;/g:mn&gt;&lt;g:mo stretchy=\"false\"&gt;)&lt;/g:mo&gt;&lt;/g:math&gt;, &lt;l:math xmlns:l=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"&gt;&lt;l:msub&gt;&lt;l:mi mathvariant=\"normal\"&gt;Λ&lt;/l:mi&gt;&lt;l:mi&gt;c&lt;/l:mi&gt;&lt;/l:msub&gt;&lt;l:mo stretchy=\"false\"&gt;(&lt;/l:mo&gt;&lt;l:mn&gt;2940&lt;/l:mn&gt;&lt;l:mo stretchy=\"false\"&gt;)&lt;/l:mo&gt;&lt;/l:math&gt;, and the predicted &lt;q:math xmlns:q=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"&gt;&lt;q:mo stretchy=\"false\"&gt;(&lt;/q:mo&gt;&lt;q:mover accent=\"true\"&gt;&lt;q:mi&gt;D&lt;/q:mi&gt;&lt;q:mo stretchy=\"false\"&gt;¯&lt;/q:mo&gt;&lt;/q:mover&gt;&lt;q:mi&gt;N&lt;/q:mi&gt;&lt;q:mo stretchy=\"false\"&gt;)&lt;/q:mo&gt;&lt;/q:math&gt; hadronic molecular states, in photoproduction and electroproduction to estimate their yields at the EicC and EIC. Assuming &lt;w:math xmlns:w=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"&gt;&lt;w:msub&gt;&lt;w:mi mathvariant=\"normal\"&gt;Λ&lt;/w:mi&gt;&lt;w:mi&gt;c&lt;/w:mi&gt;&lt;/w:msub&gt;&lt;w:mo stretchy=\"false\"&gt;(&lt;/w:mo&gt;&lt;w:mn&gt;2940&lt;/w:mn&gt;&lt;w:mo stretchy=\"false\"&gt;)&lt;/w:mo&gt;&lt;/w:math&gt; as either a hadronic molecular state or a three-quark state, our analysis demonstrates that its production rates are of the same order of magnitude, posing challenges in identifying its underlying structure. After considering the integral luminosity, the yields of &lt;bb:math xmlns:bb=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"&gt;&lt;bb:msub&gt;&lt;bb:mi mathvariant=\"normal\"&gt;Λ&lt;/bb:mi&gt;&lt;bb:mi&gt;c&lt;/bb:mi&gt;&lt;/bb:msub&gt;&lt;/bb:math&gt; excited states reach &lt;eb:math xmlns:eb=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"&gt;&lt;eb:msup&gt;&lt;eb:mn&gt;10&lt;/eb:mn&gt;&lt;eb:mn&gt;6&lt;/eb:mn&gt;&lt;/eb:msup&gt;&lt;/eb:math&gt; to &lt;gb:math xmlns:gb=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"&gt;&lt;gb:msup&gt;&lt;gb:mn&gt;10&lt;/gb:mn&gt;&lt;gb:mn&gt;7&lt;/gb:mn&gt;&lt;/gb:msup&gt;&lt;/gb:math&gt; at the EicC and EIC. The &lt;ib:math xmlns:ib=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"&gt;&lt;ib:mo stretchy=\"false\"&gt;(&lt;/ib:mo&gt;&lt;ib:mover accent=\"true\"&gt;&lt;ib:mi&gt;D&lt;/ib:mi&gt;&lt;ib:mo stretchy=\"false\"&gt;¯&lt;/ib:mo&gt;&lt;/ib:mover&gt;&lt;ib:mi&gt;N&lt;/ib:mi&gt;&lt;ib:mo stretchy=\"false\"&gt;)&lt;/ib:mo&gt;&lt;/ib:math&gt; molecular states with both isospin &lt;ob:math xmlns:ob=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"&gt;&lt;ob:mi&gt;I&lt;/ob:mi&gt;&lt;ob:mo&gt;=&lt;/ob:mo&gt;&lt;ob:mn&gt;0&lt;/ob:mn&gt;&lt;/ob:math&gt; and &lt;qb:math xmlns:qb=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"&gt;&lt;qb:mi&gt;I&lt;/qb:mi&gt;&lt;qb:mo&gt;=&lt;/qb:mo&gt;&lt;qb:mn&gt;1&lt;/qb:mn&gt;&lt;/qb:math&gt; are also studied, with yields reaching &lt;sb:math xmlns:sb=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"&gt;&lt;sb:msup&gt;&lt;sb:mn&gt;10&lt;/sb:mn&gt;&lt;sb:mn&gt;5&lt;/sb:mn&gt;&lt;/sb:msup&gt;&lt;/sb:math&gt;, making them likely to be detectable at these facilities. &lt;jats:supplementary-material&gt; &lt;jats:copyright-statement&gt;Published by the American Physical Society&lt;/jats:copyright-statement&gt; &lt;jats:copyright-year&gt;2025&lt;/jats:copyright-year&gt; &lt;/jats:permissions&gt; &lt;/jats:supplem","PeriodicalId":20167,"journal":{"name":"Physical Review D","volume":"38 1","pages":""},"PeriodicalIF":5.0,"publicationDate":"2025-03-31","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"143736688","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":2,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
引用次数: 0
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全部 ACS Photonics J. Biophotonics Laser Photonics Rev. Comput. Phys. Commun. J. Comput. Phys. Prog. Part. Nucl. Phys. Prog. Quantum Electron. Solid State Commun. IEEE Trans. Plasma Sci. Acoust. Phys. Appl. Magn. Reson. Astrophys. Bull. ASTROPHYSICS+ Braz. J. Phys. B LEBEDEV PHYS INST+ Commun. Math. Phys. Dokl. Phys. EPJ QUANTUM TECHNOL Exp. Astron. Few-Body Syst. Found. Phys. FRONT PHYS-BEIJING Gen. Relativ. Gravitation Indian J. Phys. Int. J. Theor. Phys. Jetp Lett. J. Astrophys. Astron. J CONTEMP PHYS-ARME+ J. Exp. Theor. Phys. J. High Energy Phys. J. Low Temp. Phys. J. Russ. Laser Res. J. Stat. Phys. J. Supercond. Novel Magn. J KOREAN PHYS SOC Kinematics Phys. Celestial Bodies Lett. Math. Phys. Living Rev. Relativ. Living Rev. Sol. Phys. Moscow Univ. Phys. Bull. Opt. Rev. Opt. Spectrosc. Phys. At. Nucl. Phys. Part. Nucl. Phys. Solid State PHYS WAVE PHENOM Plasma Phys. Rep. Plasmonics Quantum Inf. Process. Russ. J. Math. Phys. Russ. Phys. J. SCI CHINA PHYS MECH Sol. Phys. Sol. Syst. Res. Tech. Phys. Tech. Phys. Lett. Theor. Math. Phys. ACTA PHYS SIN-CH ED Acta Phys. Pol. B 光学学报 光子学报 Acta Phys. Pol. A Adv. Phys. ADV PHYS-X Adv. Condens. Matter Phys. Adv. High Energy Phys. Am. J. Phys. Ann. Phys. Annu. Rev. Condens. Matter Phys. Annu. Rev. Nucl. Part. Sci. Appl. Phys. Express Appl. Phys. Lett. Annu. Rev. Astron. Astrophys. ARCH ACOUST APL Photonics Appl. Phys. Rev. Ann. Phys. ASTRON ASTROPHYS Astrophys. J. Suppl. Ser. Astrophys. Space Sci. ASTROBIOLOGY Can. J. Phys. 液晶与显示 Chin. Phys. C Chin. Phys. B Classical Quantum Gravity CHIN OPT LETT Chin. J. Phys. Chin. Phys. Lett. Condens. Matter Phys. Commun. Phys. Commun. Theor. Phys. Contrib. Plasma Phys. Curr. Appl Phys. ENTROPY-SWITZ EPL-EUROPHYS LETT EUR PHYS J-SPEC TOP EUR PHYS J-APPL PHYS Front. Phys. High Pressure Res.
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