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Fe Abundances of Early Galaxies at z = 9 − 12 Derived with Deep JWST Spectra

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arXiv 2025年

作者： Nakane, Minami Ouchi, Masami Nakajima, Kimihiko Ono, Yoshiaki Harikane, Yuichi Isobe, Yuki Nomoto, Ken'ichi Ishigaki, Miho N. Yanagisawa, Hiroto Kashino, Daichi Tominaga, Nozomu Takahashi, Koh Nishigaki, Moka Takeda, Yui Watanabe, Kuria Institute for Cosmic Ray Research The University of Tokyo 5-1-5 Kashiwanoha Chiba Kashiwa277-8582 Japan Department of Physics Graduate School of Science The University of Tokyo 7-3-1 Hongo Bunkyo Tokyo113-0033 Japan National Astronomical Observatory of Japan 2-21-1 Osawa Mitaka Tokyo181-8588 Japan 2-21-1 Osawa Mitaka Tokyo181-8588 Japan The University of Tokyo 5-1-5 Kashiwanoha Chiba Kashiwa277-8583 Japan Kavli Institute for Cosmology University of Cambridge Madingley Road CambridgeCB3 0HA United Kingdom Cavendish Laboratory University of Cambridge 19 JJ Thomson Avenue CambridgeCB3 0HE United Kingdom Waseda Research Institute for Science and Engineering Faculty of Science and Engineering Waseda University 3-4-1 Okubo Shinjuku Tokyo169-8555 Japan Astronomical Science Program Graduate Institute for Advanced Studies SOKENDAI 2-21-1 Osawa Mitaka Tokyo181-8588 Japan Department of Physics Faculty of Science and Engineering Konan University 8-9-1 Okamoto Hyogo Kobe658-8501 Japan

We derive Fe-abundance ratios of 6 galaxies at z = 9 − 12 with −22 UV ∼> 0) while that 2 out of 6 galaxies, GS-z11-0 and GN-z11, show Fe enhancements ([O/Fe] +0−03542) beyond the solar-abundance ratio at ∼ 3σ. Because, unlike GS-z11-0, GN-z11 (z = 10.60) may be an AGN, we constrain [O/Fe] via Feii emission under the assumption of AGN and confirm that the Fe enhancement is consistent even in the case of AGN. While [O/Fe] values of the majority of the galaxies are explained by the chemical enrichment of core-collapse supernovae (CCSNe), the Fe enhancements of GS-z11-0 and GN-z11 are puzzling. We develop chemical evolution models, and find that the iron enhancements against oxygen in GS-z11-0 and GN-z11 can be explained by 1) pair-instability supernovae/bright hypernovae with little contribution of CCSNe or 2) Type-Ia supernovae with short delay time (∼ 30 − 50 Myr) with a top-light initial mass function. © 2025, CC BY.

关键词： Oxygen

programming Variational Quantum Circuits with Quantum-Train Agent

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Programming Variational Quantum Circuits with Quantum-Train ...

Quantum Communications, Networking, and Computing (QCNC), International Conference on

作者： Chen-Yu Liu Samuel Yen-Chi Chen Kuan-Cheng Chen Wei-Jia Huang Yen-Jui Chang Graduate Institute of Applied Physics National Taiwan University Taipei Taiwan Hon Hai (Foxconn) Research Institute Taipei Taiwan Wells Fargo New York NY USA Department of Electrical and Electronic Engineering Imperial College London London UK Centre for Quantum Engineering Science and Technology (QuEST) Imperial College London London UK Quantum Information Center Chung Yuan Christian University Taoyuan City Taiwan Master Program in Intelligent Computing and Big Data Chung Yuan Christian University Taoyuan City Taiwan

ISBN: (数字)9798331531591

ISBN: (纸本)9798331531607

This study introduces the Quantum-Train Quantum Fast Weight programmer (QT-QFWP) framework, enabling efficient and scalable programming of variational quantum circuits (VQCs) through quantum-driven parameter updates for the classical slow programmer controlling the fast programmer VQC. By optimizing quantum and classical parameter management, QT-QFWP significantly reduces parameters (by 70–90%) compared to Quantum Long Short-Term Memory (QLSTM) and Quantum Fast Weight programmer (QFWP) while maintaining accuracy. Benchmarking on time-series tasks—including Damped Simple Harmonic Motion (SHM), NARMA5, and Simulated Gravitational Waves (GW)—demonstrates superior efficiency and predictive accuracy. QT-QFWP is particularly advantageous for near-term quantum systems, addressing qubit and gate fidelity constraints, enhancing VQC deployment in time-sensitive applications, and expanding quantum computing’s role in machine learning.

关键词： Quantum system Accuracy Computational modeling Qubit Neural networks programming Predictive models Quantum circuit physics Long short term memory

The SRG/eROSITA All-Sky Survey Subaru/HSC-SSP weak-lensing mass measurements for the eRASS1 Galaxy Clusters

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arXiv 2025年

作者： Okabe, Nobuhiro Reiprich, Thomas Grandis, Sebastian Chiu, I-Non Oguri, Masamune Umetsu, Keiichi Bulbul, Esra Bahar, Emre Balzer, Fabian Clerc, Nicolas Comparat, Johan Ghirardini, Vittorio Kleinebreil, Florian Kluge, Matthias Liu, Ang Lin, Yen-Ting Monteiro-Oliveira, Rogério Pacaud, Florian Ceja, Miriam Ramos Sanders, Jeremy Schrabback, Tim Seppi, Riccardo Sommer, Martin Zhang, Xiaoyuan Physics Program Graduate School of Advanced Science and Engineering Hiroshima University 1-3-1 Kagamiyama Higashi-Hiroshima Hiroshima739-8526 Japan Hiroshima Astrophysical Science Center Hiroshima University 1-3-1 Kagamiyama Higashi-Hiroshima Hiroshima739-8526 Japan Core Research for Energetic Universe Hiroshima University 1-3-1 Kagamiyama Higashi-Hiroshima Hiroshima739-8526 Japan Universität Bonn Auf dem Hügel 71 Bonn53121 Germany Universität Innsbruck Institut für Astro- und Teilchenphysik Technikerstr. 25/8 Innsbruck6020 Austria Center for Frontier Science Chiba University 1-33 Yayoicho Inage-ku Chiba263-8522 Japan Department of Physics Graduate School of Science Chiba University 1-33 Yayoi-Cho Inage-Ku Chiba263-8522 Japan Institute of Astronomy and Astrophysics Academia Sinica P.O. Box 23-141 Taipei10617 Taiwan Max Planck Institute for Extraterrestrial Physics Giessenbachstrasse 1 Garching85748 Germany IRAP Université de Toulouse CNRS UPS CNES Toulouse France Institute for Frontiers in Astronomy and Astrophysics Beijing Normal University Beijing102206 China

We perform individual weak-lensing (WL) mass measurements for 78 eROSITA’s first All-Sky Survey (eRASS1) clusters in the footprint of Hyper Suprime-Cam Subaru Strategic program (HSC-SSP) S19A, without any priors of the eRASS1 X-ray quantities or assumption of the mass and concentration relation. In the sample, we find 3 clusters are mis-associated with optical counterparts and 12 clusters are poorly fitted with an NFW profile. The average mass for the 12 poor-fit clusters changes from ∼ 1014h−701 M☉ to ∼ 2 × 1013h−701 M☉ when lensing contamination from surrounding mass structures is taken into account. The scaling relations between the true mass and cluster richness and X-ray count-rate agree well with the results of the eRASS1 Western Galactic Hemisphere region based on count-rate-inferred masses, which are calibrated with the HSC-SSP, DES, and KiDS surveys. We develop a Bayesian framework for inferring the mass-concentration relation of the cluster sample, explicitly incorporating the effects of weak-lensing mass calibration in the mass-concentration parameter space. The redshift-dependent mass and concentration relation is in excellent agreement with predictions of dark-matter-only numerical simulations and previous studies using X-ray-selected clusters. Based on the two-dimensional (2D) WL analysis, the offsets between the WL-determined centers and the X-ray centroids for 36 eRASS1 clusters with high WL S/N are described by two Gaussian components. We find that the mis-centering effect with X-ray centroids is smaller than that with peaks in the galaxy maps. Stacked mass maps support a small mis-centering effect even for clusters with low WL S/N. The projected halo ellipticity is 〈Ε〉 = 0.45 at M200 ∼ 4 × 1014h−701 M☉, in agreement with results of numerical simulations and previous studies of clusters more than twice our mass. Copyright © 2025, The Authors. All rights reserved.

关键词： Dark Matter

Study on Free Electrons Generated by Concealed Radioactive Materials under Controlled Gaseous Environment

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Study on Free Electrons Generated by Concealed Radioactive M...

37th International Conference on Infrared, Millimeter, and Terahertz Waves (IRMMW-THz)

作者： Kim, D. S. Lee, W. S. So, J. H. Choi, E. M. Physics Program in Graduate School of UNIST Ulsan National Institute of Science and Technology (UNIST) 689-798 Republic of Korea

We estimate the amount of free electrons generated by concealed radioactive materials using MCNP code. This simulation results show that the existence of radioactive sources enhances the number of photons and backgrou... 详细信息

ISBN: (纸本)9781467315975

关键词： Radioactive materials

AstroPix: A Pixelated HVCMOS Sensor for Space-Based Gamma-Ray Measurement

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arXiv 2025年

作者： Steinhebel, Amanda L. Caputo, Regina Violette, Daniel P. Affolder, Anthony Bauman, Autumn Chinatti, Carolyn Deshmukh, Aware Fadayev, Vitaliy Fukazawa, Yasushi Jadhav, Manoj Kierans, Carolyn Kim, Bobae Kim, Jihee Klest, Henry Kroger, Olivia Kumar, Kavic Kushima, Shin Lauenstein, Jean-Marie Leys, Richard Martinez-Mckinney, Forest Metcalfe, Jessica Metzler, Zachary Mitchell, John W. Nakano, Norito Ott, Jennifer Peric, Ivan Perkins, Jeremy S. Rudin, Max R. Shin, Taylor K.W. Sommer, Grant Striebig, Nicolas Suda, Yusuke Tajima, Hiroyasu Valverde, Janeth Zurek, Maria NASA Postdoctoral Program NASA Goddard Space Flight Center MD United States University of California Santa CruzCA United States University of Colorado DenverCO United States NASA Office of STEM Engagement WashingtonDC United States Carleton College Minnesota United States Center for Research and Exploration in Space Science and Technology Maryland United States Physics Program Graduate School of Advanced Science and Engineering Hiroshima University Japan Argonne National Laboratory Illinois United States University of Maryland MD United States Institute for Space-Earth Environmental Research Nagoya University Japan Karlsruher Institut für Technologie Germany Rice University TX United States The George Washington University WashingtonDC United States Kobayashi-Maskawa Institute for the Origin of Particles and the Universe Nagoya University Japan Department of Physics Center for Space Sciences and Technology University of Maryland Baltimore CountyMD United States

A next-generation medium-energy gamma-ray telescope targeting the MeV range would address open questions in astrophysics regarding how extreme conditions accelerate cosmic-ray particles, produce relativistic jet outflows, and more. One concept, AMEGO-X, relies upon the mission-enabling CMOS Monolithic Active Pixel Sensor silicon chip AstroPix. AstroPix is designed for space-based use, featuring low noise, low power consumption, and high scalability. Desired performance of the device include an energy resolution of 5 keV (or 10% FWHM) at 122 keV and a dynamic range per-pixel of 25 − 700 keV, enabled by the addition of a high-voltage bias to each pixel which supports a depletion depth of 500 μm. This work reports on the status of the AstroPix development process with emphasis on the current version under test, version three (v3), and highlights of version two (v2). Version 3 achieves energy resolution of 10.4 ± 3.2% at 59.5 keV and 94 ± 6 μm depletion in a low-resistivity test silicon substrate. © 2025, CC BY.

关键词： Cosmology

Metasurfaces for next-generation wireless communication systems

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National science Review 2023年第8期10卷 17-19页

作者： Younes Ra'di Nikita Nefedkin Petar Popovski Andrea Alù Department of Electrical Engineering and Computer Science Syracuse University Photonics Initiative Advanced Science Research Center City University of New York Department of Electronic Systems Aalborg University Physics Program Graduate Center City University of New York

The pace of development in the world of 5G communication systems has proven to be much more demanding than previous generations, with 5G-Advanced seemingly around the corner [1]. Extensive research is already underway to structure the next generation of wireless systems(i.e. 6G), which may potentially enable an unprecedented level of human–machine interaction [2].

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Multi-wavelength fibril dynamics and oscillations above sunspot– I. morphological signature

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Research in Astronomy and Astrophysics 2015年第11期15卷 1843-1856页

作者： Emanuel Sungging Mumpuni Dhani Herdiwijaya Mitra Djamal Thomas Djamaluddin Graduate Program in Astronomy Faculty of Mathematics and Natural Sciences Bandung Institute of TechnologyGedung CAS Lt. 6 ITB Jl. Ganesha 10 Bandung 40132 Indonesia Space Science Center LAPAN Graduate Program in Physics Faculty of Mathematics and Natural Sciences Bandung Institute of Technology Department of PhysicsJl. Ganesha 10 Bandung 40132 Indonesia

In this work we selected one particular fibril from a high resolution observation of the solar chromosphere with the Dutch Open Telescope, and tried to obtain a broad picture of the intricate mechanism that might be operating in the multiple layers of the solar atmosphere visible in high cadence multi-wavelength observations. We analyzed the changing fibril pattern using multi-wavelength tomography, which consists of both the Hα line center and the blue wing, Doppler signal, Ca II H, and the G-band. We have found that the intermittent ejected material through the fibril from Doppler images has clearly shown an oscillation mode, as seen in the Hα blue *** oscillations in the umbrae and penumbrae magnetic field lines that are above the sunspot cause a broadening and the area forms a ring shape from 3 to 15 minute oscillations as a function of height. These made a distinct boundary between the umbrae and penumbrae which suggests a comb structure, and indicates that the oscillations could propagate along the inclined magnetic flux tubes from below. The 3 minute oscillations strongly appeared in the broadly inclined penumbrae magnetic field lines and showed a clear light bridge. The well known 5 minute oscillations were dominant in the umbrae-penumbrae region boundary. The long 7 minute oscillations were transparent in the Hα blue wing, as well as the 10 and 15 minute oscillations. They were concentrated in the inner-penumbrae, as seen in the Hα line center. From these findings we propose that the fibril acts as a fabric for interaction between the layers,as well as related activities around the active region under investigation.

关键词： minute morphological signature picture propagate fabric Figure sector visible concentrated

Terahertz Cavity Phonon Polaritons in Lead Telluride in the Deep-Strong Coupling Regime

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arXiv 2025年

作者： Baydin, Andrey Manjappa, Manukumara Mishra, Sobhan Subhra Xu, Hongjing Doumani, Jacques Tay, Fuyang Kim, Dasom Rappl, Paulo H.O. Abramof, Eduardo Singh, Ranjan Hernandez, Felix G.G. Kono, Junichiro Department of Electrical and Computer Engineering Rice University HoustonTX77005 United States Smalley–Curl Institute Rice University HoustonTX77005 United States Rice Advanced Materials Institute Rice University HoustonTX77005 United States Instrumentation and Applied Physics Department Indian Institute of Science Bangalore560012 India Center for Disruptive Photonic Technologies The Photonics Institute Nanyang Technological University 639798 Singapore Department of Physics and Astronomy Rice University HoustonTX77005 United States Applied Physics Graduate Program Smalley–Curl Institute Rice University HoustonTX77005 United States Group of Research and Development in Materials and Plasma National Institute for Space Research São José dos Campos São Paulo12201-970 Brazil Division of Physics and Applied Physics School of Physical and Mathematical Sciences Nanyang Technological University 637371 Singapore Instituto de Física Universidade de São Paulo São Paulo05508-090 Brazil Department of Material Science and NanoEngineering Rice University HoustonTX77005 United States

Lead telluride is an important thermoelectric material due to its large Seebeck coefficient combined with its unusually low thermal conductivity that is related to the strong anharmonicity of phonons in this material. Here, we have studied the resonant and nonperturbative coupling of transverse optical phonons in lead telluride with cavity photons inside small-mode-volume metallic metasurface cavities that have photonic modes with terahertz frequencies. We observed a giant vacuum Rabi splitting on the order of the bare phonon and cavity frequencies. Through terahertz time-domain spectroscopy experiments, we systematically studied the vacuum Rabi splitting as a function of sample thickness, temperature, and cavity length. Under the strongest light–matter coupling conditions, the strength of coupling exceeded the bare phonon and cavity frequencies, putting the system into the deep-strong coupling regime. These results demonstrate that this uniquely tunable platform is promising for realizing and understanding predicted cavity-vacuum-induced ferroelectric instabilities and exploring applications of light–matter coupling in the ultrastrong and deep-strong coupling regimes in quantum technology. Copyright © 2025, The Authors. All rights reserved.

关键词： Phonons

Directed discovery of high-loading nanoaggregates enabled by drug-matched oligo-peptide excipients

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Chem 2025年

作者： Berisha, Naxhije Farahpour, Atena Ramakrishnan, Maithreyi Chen, Chen McPhee, Scott A. Wang, Tong Li, Tai-De Hema, Kuntrapakam Panagiotakopoulou, Magdalini Athiyarath, Vignesh Coste, Maeva Marciano, Yaron Sherman, Emmet Ulijn, Rein V. Heller, Daniel A. Nanoscience Initiative Advanced Science Research Center CUNY Graduate Center City University of New York New York 10031 NY United States Department of Chemistry and Biochemistry Hunter College City University of New York New York 10065 NY United States PhD Program in Chemistry CUNY Graduate Center City University of New York New York 10016 NY United States Molecular Pharmacology Program Memorial Sloan Kettering Cancer Center New York 10065 NY United States Tri-Institutional PhD Program in Chemical Biology Memorial Sloan Kettering Cancer Center New York 10065 NY United States Department of Physics City College of New York City University of New York New York 10031 NY United States Department of Chemistry Brooklyn College City University of New York 2900 Bedford Avenue Brooklyn 11210 NY United States PhD Program in Biochemistry CUNY Graduate Center City University of New York New York 10016 NY United States Weill Cornell Medicine Cornell University New York 10065 NY United States

Nanoparticles can improve drug pharmacokinetics, but low loading efficiencies can limit treatment efficacy. Drug-aggregation-based nanoparticles have demonstrated improved loadings of up to 90%, but few excipients facilitate efficient co-assembly. We investigated peptides as designer excipients because of their diverse chemical space and inherent biodegradability. We designed pentapeptide scaffolds to mimic the structure of known indocyanine excipients by modulating aromaticity, rigidity, and charge. We screened 184 formulations by using diverse drug cargoes. We found drug-peptide combinations that formed nanoparticles with up to 98% drug loading. Molecular dynamics simulations and mass spectrometry analysis demonstrated that tryptophan-drug interactions and solvent exposure of charged amino acid residues drove the formation of core-shell structures. Peptide-drug formulations containing the JAK2/FLT3 inhibitor lestaurtinib were investigated in acute myeloid leukemia models, resulting in enhanced anti-tumor efficacy. This work found that oligopeptides can be designed to efficiently co-assemble with therapeutic cargoes to result in high-loading nanoparticles that improve anti-tumor efficacy. © 2024

关键词： co-assembly directed discovery drug delivery excipient nanocarrier design nanoparticle oligopeptides SDG3: Good health and well-being