Synchronization is a universal phenomenon underpinning various natural processes and finds direct application in control engineering and photonics. Among several synchronization mechanisms, subharmonic entrainment (SHE) is a nonlinear synchronization phenomenon where an oscillator locks to an external drive with a fraction of the oscillator's frequency. While its mechanism is well understood for scalar couplings and finds application in the stabilization of ultrafast laser pulses, the potential of SHE with vectorial coupling is still unexplored. In this work, we demonstrate vector SHE (VSHE) using a passively mode-locked fiber laser as a testbed. We unveil the mechanism of vector SHE, in which weak external signals can entrain internal laser dynamics through vector coupling. Vector SHE presents in the form of synchronization between the subharmonic of mode-locking-driven oscillations and continuous wave (CW) signal with an evolving state of polarization. This CW signal, driven by the internal dynamics of the injected signal, causes VSHE with the frequencies' ratios of multiples of ten, resulting in a partially mode locking regime operation. Our findings offer new control techniques over mode-locking and additional dimension such as polarization states.
{"title":"Nonlinear synchronization through vector subharmonic entrainment.","authors":"Dmitrii Stoliarov, Sergey Sergeyev, Hani Kbashi, Fan Wu, Qianqian Huang, Chengbo Mou","doi":"10.1038/s42005-026-02509-7","DOIUrl":"https://doi.org/10.1038/s42005-026-02509-7","url":null,"abstract":"<p><p>Synchronization is a universal phenomenon underpinning various natural processes and finds direct application in control engineering and photonics. Among several synchronization mechanisms, subharmonic entrainment (SHE) is a nonlinear synchronization phenomenon where an oscillator locks to an external drive with a fraction of the oscillator's frequency. While its mechanism is well understood for scalar couplings and finds application in the stabilization of ultrafast laser pulses, the potential of SHE with vectorial coupling is still unexplored. In this work, we demonstrate vector SHE (VSHE) using a passively mode-locked fiber laser as a testbed. We unveil the mechanism of vector SHE, in which weak external signals can entrain internal laser dynamics through vector coupling. Vector SHE presents in the form of synchronization between the subharmonic of mode-locking-driven oscillations and continuous wave (CW) signal with an evolving state of polarization. This CW signal, driven by the internal dynamics of the injected signal, causes VSHE with the frequencies' ratios of multiples of ten, resulting in a partially mode locking regime operation. Our findings offer new control techniques over mode-locking and additional dimension such as polarization states.</p>","PeriodicalId":10540,"journal":{"name":"Communications Physics","volume":"9 1","pages":"71"},"PeriodicalIF":5.8,"publicationDate":"2026-01-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://www.ncbi.nlm.nih.gov/pmc/articles/PMC12923357/pdf/","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"147270132","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":1,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"OA","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
Pub Date : 2026-01-01Epub Date: 2026-02-04DOI: 10.1038/s42005-025-02471-w
Jayaprasath Elumalai, Mohammed Salih, Martyn Fice, Adam Brown, Lianhe Li, Edmund H Linfield, Alexander Valavanis, Alwyn J Seeds, Alexander Giles Davies, Joshua R Freeman
Terahertz-frequency (THz) carrier waves in free-space optical (FSO) communications offer the potential for > 1 Tbit/s data rates and stable latency. They offer wider bandwidths than available in the microwave region, together with reduced scattering and relaxed pointing requirements compared with visible and near-infrared regions. However, 1-10 THz FSO communications systems have thus far been limited to data rates several orders of magnitude lower than those of infrared systems. This work describes an experimental demonstration of multi-gigabit-per-second FSO communication using a THz quantum cascade laser (QCL), opening a new frontier for next-generation wireless communications. The FSO communication system consists of a 2.4 THz QCL source as the transmitter and a room-temperature Schottky barrier diode detector as the receiver. By directly modulating the terahertz QCL, we achieved non-return-to-zero on-off keying (NRZ-OOK) with a transmission rate of up to 4 Gbit/s. We evaluated the performance of the communication link by analyzing the bit error rate (BER) of the demodulated signal at the receiver while examining its relation to received optical power, QCL modulation power, and various bias points. Our work establishes the foundation for high-speed optical wireless communication based on terahertz QCL technology systems.
{"title":"Free-space optical communications at 4 Gbit/s data rate with a terahertz laser.","authors":"Jayaprasath Elumalai, Mohammed Salih, Martyn Fice, Adam Brown, Lianhe Li, Edmund H Linfield, Alexander Valavanis, Alwyn J Seeds, Alexander Giles Davies, Joshua R Freeman","doi":"10.1038/s42005-025-02471-w","DOIUrl":"https://doi.org/10.1038/s42005-025-02471-w","url":null,"abstract":"<p><p>Terahertz-frequency (THz) carrier waves in free-space optical (FSO) communications offer the potential for > 1 Tbit/s data rates and stable latency. They offer wider bandwidths than available in the microwave region, together with reduced scattering and relaxed pointing requirements compared with visible and near-infrared regions. However, 1-10 THz FSO communications systems have thus far been limited to data rates several orders of magnitude lower than those of infrared systems. This work describes an experimental demonstration of multi-gigabit-per-second FSO communication using a THz quantum cascade laser (QCL), opening a new frontier for next-generation wireless communications. The FSO communication system consists of a 2.4 THz QCL source as the transmitter and a room-temperature Schottky barrier diode detector as the receiver. By directly modulating the terahertz QCL, we achieved non-return-to-zero on-off keying (NRZ-OOK) with a transmission rate of up to 4 Gbit/s. We evaluated the performance of the communication link by analyzing the bit error rate (BER) of the demodulated signal at the receiver while examining its relation to received optical power, QCL modulation power, and various bias points. Our work establishes the foundation for high-speed optical wireless communication based on terahertz QCL technology systems.</p>","PeriodicalId":10540,"journal":{"name":"Communications Physics","volume":"9 1","pages":"33"},"PeriodicalIF":5.8,"publicationDate":"2026-01-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://www.ncbi.nlm.nih.gov/pmc/articles/PMC12915521/pdf/","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"146225439","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":1,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"OA","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
Pub Date : 2026-01-01Epub Date: 2026-02-02DOI: 10.1038/s42005-026-02505-x
Slav Ivanov, Bernhard Ersfeld, Feng Dong, Dino A Jaroszynski
Ultra-high power lasers are becoming important tools for advancing high-field physics and fusion research. However, their development is constrained by the damage thresholds of conventional optical components; it is challenging to design optical elements capable of withstanding high powers without them becoming impractically large. Here we show that transient plasma photonic structures, formed by the interaction of intercepting laser pulses in gas, can act as compact and robust reflective elements. Because these structures evolve in space and time, and rely on many interdependent parameters, designing optical components using traditional trial-and-error design methods is challenging. We show that machine learning can efficiently explore this complex parameter space to rapidly design robust, high reflectivity plasma mirrors. Moreover, this design process unexpectedly discovers a regime where unchirped laser pulses are compressed. This work demonstrates machine learning as a powerful tool for design, discovery and development of ultra-compact optical components for next-generation lasers.
{"title":"Design of transient plasma photonic structure mirrors for high-power lasers using deep kernel Bayesian optimisation.","authors":"Slav Ivanov, Bernhard Ersfeld, Feng Dong, Dino A Jaroszynski","doi":"10.1038/s42005-026-02505-x","DOIUrl":"https://doi.org/10.1038/s42005-026-02505-x","url":null,"abstract":"<p><p>Ultra-high power lasers are becoming important tools for advancing high-field physics and fusion research. However, their development is constrained by the damage thresholds of conventional optical components; it is challenging to design optical elements capable of withstanding high powers without them becoming impractically large. Here we show that transient plasma photonic structures, formed by the interaction of intercepting laser pulses in gas, can act as compact and robust reflective elements. Because these structures evolve in space and time, and rely on many interdependent parameters, designing optical components using traditional trial-and-error design methods is challenging. We show that machine learning can efficiently explore this complex parameter space to rapidly design robust, high reflectivity plasma mirrors. Moreover, this design process unexpectedly discovers a regime where unchirped laser pulses are compressed. This work demonstrates machine learning as a powerful tool for design, discovery and development of ultra-compact optical components for next-generation lasers.</p>","PeriodicalId":10540,"journal":{"name":"Communications Physics","volume":"9 1","pages":"34"},"PeriodicalIF":5.8,"publicationDate":"2026-01-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://www.ncbi.nlm.nih.gov/pmc/articles/PMC12915518/pdf/","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"146225185","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":1,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"OA","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
Pub Date : 2026-01-01Epub Date: 2026-01-07DOI: 10.1038/s42005-025-02418-1
Emmanouil T Kokkinakis, Ioannis Komis, Konstantinos G Makris
Two-dimensional non-Hermitian photonic lattices with asymmetric couplings offer rich possibilities for controlling wave localization, through the emergence of the non-Hermitian skin effect at lattice corners or sides. Yet, how optical nonlinearity modifies these boundary-localization characteristics remains largely unexplored. Here we show that in a two-dimensional Hatano-Nelson lattice with Kerr nonlinearity, the interplay between self-trapping and directional propagation leads to position-dependent amplitude thresholds. Single-site excitations having above a critical amplitude become confined to their initial position, with lower thresholds near the position where the linear eigenmodes are localized and higher thresholds within the lattice's bulk. Additionally, we study the differences of this dynamical interplay, for wider initial excitations, between the focusing and defocusing Kerr-nonlinearity regimes. Lastly, we identify skin soliton solutions in a variety of two-dimensional lattice geometries featuring coupling asymmetry. This work paves the way for future investigations regarding transport and soliton formation in higher-dimensional nonlinear non-Hermitian lattices.
{"title":"Self-trapping and skin solitons in two-dimensional non-Hermitian lattices.","authors":"Emmanouil T Kokkinakis, Ioannis Komis, Konstantinos G Makris","doi":"10.1038/s42005-025-02418-1","DOIUrl":"10.1038/s42005-025-02418-1","url":null,"abstract":"<p><p>Two-dimensional non-Hermitian photonic lattices with asymmetric couplings offer rich possibilities for controlling wave localization, through the emergence of the non-Hermitian skin effect at lattice corners or sides. Yet, how optical nonlinearity modifies these boundary-localization characteristics remains largely unexplored. Here we show that in a two-dimensional Hatano-Nelson lattice with Kerr nonlinearity, the interplay between self-trapping and directional propagation leads to position-dependent amplitude thresholds. Single-site excitations having above a critical amplitude become confined to their initial position, with lower thresholds near the position where the linear eigenmodes are localized and higher thresholds within the lattice's bulk. Additionally, we study the differences of this dynamical interplay, for wider initial excitations, between the focusing and defocusing Kerr-nonlinearity regimes. Lastly, we identify skin soliton solutions in a variety of two-dimensional lattice geometries featuring coupling asymmetry. This work paves the way for future investigations regarding transport and soliton formation in higher-dimensional nonlinear non-Hermitian lattices.</p>","PeriodicalId":10540,"journal":{"name":"Communications Physics","volume":"9 1","pages":"22"},"PeriodicalIF":5.8,"publicationDate":"2026-01-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://www.ncbi.nlm.nih.gov/pmc/articles/PMC12819148/pdf/","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"146028519","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":1,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"OA","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
Pub Date : 2026-01-01Epub Date: 2026-02-27DOI: 10.1038/s42005-026-02552-4
Antonio Sanna, Tiago F T Cerqueira, Ekin Dogus Cubuk, Ion Errea, Yue-Wen Fang
Hydrides are considered to be one of the most promising families of compounds for achieving high temperature superconductivity. However, there are very few experimental reports of ambient-pressure hydride superconductivity, and the superconducting critical temperatures (Tc) are typically less than 10 K. At the same time several hydrides have been predicted to exhibit superconductivity around 100 K at ambient pressure but in thermodynamically unfavorable phases. In this work we aim at assessing the superconducting properties of thermodynamically stable hydride superconductors at room pressure by investigating the GNoME material database, which has been recently released and includes thousands of hydrides thermodynamically stable at 0K. To scan this large material space we have adopted a multi stage approach which combines machine learning for a fast initial evaluation and cutting edge ab initio methods to obtain a reliable estimation of Tc. Ultimately we have identified 25 cubic hydrides with Tc above 4.2 K and reach a maximum Tc of 17 K. While these critical temperatures are modest in comparison to some recent predictions, the systems where they are found, being stable, are likely to be experimentally accessible and of potential technological relevance.
{"title":"Search for thermodynamically stable ambient-pressure superconducting hydrides in the GNoME database.","authors":"Antonio Sanna, Tiago F T Cerqueira, Ekin Dogus Cubuk, Ion Errea, Yue-Wen Fang","doi":"10.1038/s42005-026-02552-4","DOIUrl":"https://doi.org/10.1038/s42005-026-02552-4","url":null,"abstract":"<p><p>Hydrides are considered to be one of the most promising families of compounds for achieving high temperature superconductivity. However, there are very few experimental reports of ambient-pressure hydride superconductivity, and the superconducting critical temperatures (<i>T</i> <sub>c</sub>) are typically less than 10 K. At the same time several hydrides have been predicted to exhibit superconductivity around 100 K at ambient pressure but in thermodynamically unfavorable phases. In this work we aim at assessing the superconducting properties of thermodynamically stable hydride superconductors at room pressure by investigating the GNoME material database, which has been recently released and includes thousands of hydrides thermodynamically stable at 0K. To scan this large material space we have adopted a multi stage approach which combines machine learning for a fast initial evaluation and cutting edge ab initio methods to obtain a reliable estimation of <i>T</i> <sub>c</sub>. Ultimately we have identified 25 cubic hydrides with <i>T</i> <sub>c</sub> above 4.2 K and reach a maximum <i>T</i> <sub>c</sub> of 17 K. While these critical temperatures are modest in comparison to some recent predictions, the systems where they are found, being stable, are likely to be experimentally accessible and of potential technological relevance.</p>","PeriodicalId":10540,"journal":{"name":"Communications Physics","volume":"9 1","pages":"94"},"PeriodicalIF":5.8,"publicationDate":"2026-01-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://www.ncbi.nlm.nih.gov/pmc/articles/PMC12992110/pdf/","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"147480013","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":1,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"OA","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
Pub Date : 2026-01-01Epub Date: 2026-01-10DOI: 10.1038/s42005-025-02479-2
Dawid A Hryniuk, Marzena H Szymańska
Competition between short- and long-range interactions underpins many emergent phenomena in nature. Despite rapid progress in their experimental control, computational methods capable of accurately simulating open quantum many-body systems with complex long-ranged interactions at scale remain scarce. Here, we address this limitation by introducing an efficient and scalable approach to dissipative quantum lattices in one and two dimensions, combining matrix product operators and time-dependent variational Monte Carlo. We showcase the versatility, effectiveness, and unique methodological advantages of our algorithm by simulating the non-equilibrium dynamics and steady states of spin- lattices with competing algebraically-decaying interactions for as many as N = 200 sites, revealing the emergence of spatially-modulated magnetic order far from equilibrium. This approach offers promising prospects for advancing our understanding of the complex non-equilibrium properties of a diverse variety of experimentally-realizable quantum systems with long-ranged interactions, including Rydberg atoms, ultracold dipolar molecules, and trapped ions.
{"title":"Variational approach to open quantum systems with long-range competing interactions.","authors":"Dawid A Hryniuk, Marzena H Szymańska","doi":"10.1038/s42005-025-02479-2","DOIUrl":"10.1038/s42005-025-02479-2","url":null,"abstract":"<p><p>Competition between short- and long-range interactions underpins many emergent phenomena in nature. Despite rapid progress in their experimental control, computational methods capable of accurately simulating open quantum many-body systems with complex long-ranged interactions at scale remain scarce. Here, we address this limitation by introducing an efficient and scalable approach to dissipative quantum lattices in one and two dimensions, combining matrix product operators and time-dependent variational Monte Carlo. We showcase the versatility, effectiveness, and unique methodological advantages of our algorithm by simulating the non-equilibrium dynamics and steady states of spin- <math> <mfrac><mrow><mn>1</mn></mrow> <mrow><mn>2</mn></mrow> </mfrac> </math> lattices with competing algebraically-decaying interactions for as many as <i>N</i> = 200 sites, revealing the emergence of spatially-modulated magnetic order far from equilibrium. This approach offers promising prospects for advancing our understanding of the complex non-equilibrium properties of a diverse variety of experimentally-realizable quantum systems with long-ranged interactions, including Rydberg atoms, ultracold dipolar molecules, and trapped ions.</p>","PeriodicalId":10540,"journal":{"name":"Communications Physics","volume":"9 1","pages":"45"},"PeriodicalIF":5.8,"publicationDate":"2026-01-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://www.ncbi.nlm.nih.gov/pmc/articles/PMC12884967/pdf/","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"146156309","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":1,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"OA","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
Pub Date : 2026-01-01Epub Date: 2026-01-10DOI: 10.1038/s42005-026-02489-8
Jason R Shuster, Naoki Bessho, John C Dorelli, Daniel J Gershman, Jason M H Beedle, Harsha Gurram, Jonathan Ng, Li-Jen Chen, Roy B Torbert, James L Burch, Barbara L Giles, Richard E Denton, Paul A Cassak, M Hasan Barbhuiya, Steven J Schwartz, Yi-Hsin Liu, Cecilia Norgren, Daniel E da Silva, Kevin J Genestreti, Steven V Heuer, Matthew R Argall, Hanieh Karimi, Andy T Marshall, Rumi Nakamura, Haoming Liang, Vadim M Uritsky, Arya Afshari, Dominic S Payne
The electron diffusion region is central to NASA's Magnetospheric Multiscale (MMS) mission to understand collisionless magnetic reconnection, the plasma physics phenomenon crucial to triggering the explosive energy release of solar flares, powering auroras generated in planetary magnetospheres, and driving sawtooth crashes in laboratory fusion devices. Inside the diffusion region, electron velocity distributions exhibit highly-structured velocity-space signatures critical for elucidating the kinetic mechanisms fueling reconnection. Recent multi-spacecraft analysis techniques enabled observational study of the spatial gradient in the electron velocity distribution, which has been reported in electron-scale current layers to explain the kinetic origins of electron pressure gradients. However, electron gradient distributions have not yet been investigated inside the reconnection diffusion region. In this work, we discover that electron gradient distributions exhibit a smile-shaped velocity-space structure in the electron diffusion region of asymmetric magnetic reconnection at Earth's magnetopause. Characterizing the nature and prevalence of these smile-shaped electron gradient distributions offers a kinetic perspective into how electrons spatially evolve to provide the net electron pressure divergence that self-consistently supports non-ideal electric fields in the electron diffusion region of magnetopause reconnection. These results are relevant to space, astrophysical, and laboratory plasma communities working to understand the long-standing mystery of collisionless magnetic reconnection.
{"title":"Smile-shaped electron gradient distributions observed during magnetic reconnection at Earth's magnetopause.","authors":"Jason R Shuster, Naoki Bessho, John C Dorelli, Daniel J Gershman, Jason M H Beedle, Harsha Gurram, Jonathan Ng, Li-Jen Chen, Roy B Torbert, James L Burch, Barbara L Giles, Richard E Denton, Paul A Cassak, M Hasan Barbhuiya, Steven J Schwartz, Yi-Hsin Liu, Cecilia Norgren, Daniel E da Silva, Kevin J Genestreti, Steven V Heuer, Matthew R Argall, Hanieh Karimi, Andy T Marshall, Rumi Nakamura, Haoming Liang, Vadim M Uritsky, Arya Afshari, Dominic S Payne","doi":"10.1038/s42005-026-02489-8","DOIUrl":"10.1038/s42005-026-02489-8","url":null,"abstract":"<p><p>The electron diffusion region is central to NASA's Magnetospheric Multiscale (MMS) mission to understand collisionless magnetic reconnection, the plasma physics phenomenon crucial to triggering the explosive energy release of solar flares, powering auroras generated in planetary magnetospheres, and driving sawtooth crashes in laboratory fusion devices. Inside the diffusion region, electron velocity distributions exhibit highly-structured velocity-space signatures critical for elucidating the kinetic mechanisms fueling reconnection. Recent multi-spacecraft analysis techniques enabled observational study of the spatial gradient in the electron velocity distribution, which has been reported in electron-scale current layers to explain the kinetic origins of electron pressure gradients. However, electron gradient distributions have not yet been investigated inside the reconnection diffusion region. In this work, we discover that electron gradient distributions exhibit a smile-shaped velocity-space structure in the electron diffusion region of asymmetric magnetic reconnection at Earth's magnetopause. Characterizing the nature and prevalence of these smile-shaped electron gradient distributions offers a kinetic perspective into how electrons spatially evolve to provide the net electron pressure divergence that self-consistently supports non-ideal electric fields in the electron diffusion region of magnetopause reconnection. These results are relevant to space, astrophysical, and laboratory plasma communities working to understand the long-standing mystery of collisionless magnetic reconnection.</p>","PeriodicalId":10540,"journal":{"name":"Communications Physics","volume":"9 1","pages":"56"},"PeriodicalIF":5.8,"publicationDate":"2026-01-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://www.ncbi.nlm.nih.gov/pmc/articles/PMC12900639/pdf/","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"146200338","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":1,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"OA","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
Pub Date : 2026-01-01Epub Date: 2026-01-08DOI: 10.1038/s42005-025-02486-3
R A Lara, N Sharadhi, A A L Huttunen, L Ansas, E J G Rislakki, G M Bessa, M Backholm
Swimming is ubiquitous in nature and crucial for the survival of a wide range of organisms. The physics of swimming at the viscosity-dominated microscale and inertia-dominated macroscale is well studied. However, in between lies a complicated mesoscale with swimmers affected by non-linear and time-dependent fluid mechanics. The intricate motility strategies, combined with complex and periodically changing body shapes add extra challenges for accurate meso-swimming modelling. Here, we have further developed the micropipette force sensor to directly probe the swimming forces of the meso-organism Artemia. Through deep neural network-based image analysis, we show how Artemia achieves an increased propulsive force by increasing its level of time-reversal symmetry breaking. We present a universal force-based scaling law for a wide range of micro- to meso-organisms with different body shapes, swimming strategies, and level of inertia at the mesoscale. These results capture fundamental aspects of biological meso-swimming dynamics and provide guidance for future biomimicking meso-robot designs.
{"title":"Forces and symmetry breaking of a living meso-swimmer.","authors":"R A Lara, N Sharadhi, A A L Huttunen, L Ansas, E J G Rislakki, G M Bessa, M Backholm","doi":"10.1038/s42005-025-02486-3","DOIUrl":"10.1038/s42005-025-02486-3","url":null,"abstract":"<p><p>Swimming is ubiquitous in nature and crucial for the survival of a wide range of organisms. The physics of swimming at the viscosity-dominated microscale and inertia-dominated macroscale is well studied. However, in between lies a complicated mesoscale with swimmers affected by non-linear and time-dependent fluid mechanics. The intricate motility strategies, combined with complex and periodically changing body shapes add extra challenges for accurate meso-swimming modelling. Here, we have further developed the micropipette force sensor to directly probe the swimming forces of the meso-organism <i>Artemia</i>. Through deep neural network-based image analysis, we show how <i>Artemia</i> achieves an increased propulsive force by increasing its level of time-reversal symmetry breaking. We present a universal force-based scaling law for a wide range of micro- to meso-organisms with different body shapes, swimming strategies, and level of inertia at the mesoscale. These results capture fundamental aspects of biological meso-swimming dynamics and provide guidance for future biomimicking meso-robot designs.</p>","PeriodicalId":10540,"journal":{"name":"Communications Physics","volume":"9 1","pages":"53"},"PeriodicalIF":5.8,"publicationDate":"2026-01-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://www.ncbi.nlm.nih.gov/pmc/articles/PMC12893912/pdf/","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"146200365","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":1,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"OA","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
Pub Date : 2026-01-01Epub Date: 2026-01-06DOI: 10.1038/s42005-025-02458-7
Kristian C Z Haverson, Robin Smith, Moshe Gai, Deran K Schweitzer, Sarah R Stern, Sean W Finch
The carbon oxygen ratio (C/O) at the end of stellar helium burning is a crucial nuclear input to stellar evolution theory. Knowledge of the C/O ratio with sufficient accuracy has eluded measurement over the past five decades. It is determined by the rate of oxygen formation in the fusion of helium with 12C, denoted as 12C(α, γ)16O. Even though recent methods employing a time projection chamber can measure the time-reverse photo-dissociation reaction, the results still do not show unambiguous agreement with the predictions of quantum scattering theory. Here, we improve this method using a N2O gas target. This improvement allows us to eliminate the background caused by 12C photo-dissociation events, obtain complete angular distributions (0∘-180∘), and measure the cross sections over the 1- resonance in 16O at Ecm ~ 2.4 MeV. These measurements resolve the discrepancy that was previously observed between the measured E1-E2 mixing phase angle (ϕ12) of 12C(α, γ)16O and the predictions of quantum scattering theory. This newfound agreement demonstrates the viability of our method for conducting measurements at lower energies.
恒星氦燃烧结束时的碳氧比(C/O)是恒星演化理论的重要核输入。在过去的50年里,对碳氧比有足够精确的了解一直无法测量。它是由氦与12C的聚变生成氧的速率决定的,记为12C(α, γ)16O。尽管使用时间投影室的最新方法可以测量逆时间光解反应,但结果仍不能与量子散射理论的预测完全一致。在这里,我们使用N2O气体靶改进了该方法。这一改进使我们能够消除由12C光解离事件引起的背景,获得完整的角分布(0°-180°),并测量16O在E cm ~ 2.4 MeV下的1-共振截面。这些测量解决了之前观测到的12C(α, γ)16O的E1-E2混合相角(φ 12)与量子散射理论预测之间的差异。这个新发现的一致证明了我们的方法在较低能量下进行测量的可行性。
{"title":"Background-free <sup>12</sup>C(<i>α</i>, <i>γ</i>) angular distribution measurements with a time projection chamber operating in Gamma beams.","authors":"Kristian C Z Haverson, Robin Smith, Moshe Gai, Deran K Schweitzer, Sarah R Stern, Sean W Finch","doi":"10.1038/s42005-025-02458-7","DOIUrl":"10.1038/s42005-025-02458-7","url":null,"abstract":"<p><p>The carbon oxygen ratio (C/O) at the end of stellar helium burning is a crucial nuclear input to stellar evolution theory. Knowledge of the C/O ratio with sufficient accuracy has eluded measurement over the past five decades. It is determined by the rate of oxygen formation in the fusion of helium with <sup>12</sup>C, denoted as <sup>12</sup>C(<i>α</i>, <i>γ</i>)<sup>16</sup>O. Even though recent methods employing a time projection chamber can measure the time-reverse photo-dissociation reaction, the results still do not show unambiguous agreement with the predictions of quantum scattering theory. Here, we improve this method using a N<sub>2</sub>O gas target. This improvement allows us to eliminate the background caused by <sup>12</sup>C photo-dissociation events, obtain complete angular distributions (0<sup>∘</sup>-180<sup>∘</sup>), and measure the cross sections over the 1<sup>-</sup> resonance in <sup>16</sup>O at <i>E</i> <sub>cm</sub> ~ 2.4 MeV. These measurements resolve the discrepancy that was previously observed between the measured <i>E</i>1-<i>E</i>2 mixing phase angle (<i>ϕ</i> <sub>12</sub>) of <sup>12</sup>C(<i>α</i>, <i>γ</i>)<sup>16</sup>O and the predictions of quantum scattering theory. This newfound agreement demonstrates the viability of our method for conducting measurements at lower energies.</p>","PeriodicalId":10540,"journal":{"name":"Communications Physics","volume":"9 1","pages":"27"},"PeriodicalIF":5.8,"publicationDate":"2026-01-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://www.ncbi.nlm.nih.gov/pmc/articles/PMC12823443/pdf/","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"146046227","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":1,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"OA","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
Pub Date : 2026-01-01Epub Date: 2025-12-21DOI: 10.1038/s42005-025-02457-8
Tomasz Karpisz, Robert L Lirette, Aaron M Hagerstrom, Nathan D Orloff, Angela C Stelson
Many electrically active devices rely on nonlinear signal mixing (heterodyning) between two electrical signals. Heterodyning between electric and acoustic signals can allow for active control of typically passive components such as transmission lines, acoustic resonators, and electrical resonators built from piezoelectric materials. However, there are few techniques to characterize the nonlinear properties of materials that lead to heterodyning between electric and acoustic signals within the material. Here we demonstrate a proof-of-concept microwave interferometer that uses electromagnetic and acoustic waves to measure second-order mixing from electrical and acoustic signals in a piezoelectric material. The sum and difference frequencies of signal mixing can be detected in the electromagnetic spectrum in our measurement. We show the effect of frequency and power of the fundamental signals on the mixing products. We additionally characterize the heterodyne signal to show that it is electric-acoustic in nature, versus purely electric. Characterizing nonlinear electric-acoustic properties is important to the development of next generation piezoelectric materials models and devices.
{"title":"Measuring electric-acoustic heterodyning in piezoelectric materials.","authors":"Tomasz Karpisz, Robert L Lirette, Aaron M Hagerstrom, Nathan D Orloff, Angela C Stelson","doi":"10.1038/s42005-025-02457-8","DOIUrl":"10.1038/s42005-025-02457-8","url":null,"abstract":"<p><p>Many electrically active devices rely on nonlinear signal mixing (heterodyning) between two electrical signals. Heterodyning between electric and acoustic signals can allow for active control of typically passive components such as transmission lines, acoustic resonators, and electrical resonators built from piezoelectric materials. However, there are few techniques to characterize the nonlinear properties of materials that lead to heterodyning between electric and acoustic signals within the material. Here we demonstrate a proof-of-concept microwave interferometer that uses electromagnetic and acoustic waves to measure second-order mixing from electrical and acoustic signals in a piezoelectric material. The sum and difference frequencies of signal mixing can be detected in the electromagnetic spectrum in our measurement. We show the effect of frequency and power of the fundamental signals on the mixing products. We additionally characterize the heterodyne signal to show that it is electric-acoustic in nature, versus purely electric. Characterizing nonlinear electric-acoustic properties is important to the development of next generation piezoelectric materials models and devices.</p>","PeriodicalId":10540,"journal":{"name":"Communications Physics","volume":"9 1","pages":"26"},"PeriodicalIF":5.8,"publicationDate":"2026-01-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://www.ncbi.nlm.nih.gov/pmc/articles/PMC12823382/pdf/","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"146050710","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":1,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"OA","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}