Search:
Match:
28 results

Analysis

This paper introduces a novel application of Fourier ptychographic microscopy (FPM) for label-free, high-resolution imaging of human brain organoid slices. It demonstrates the potential of FPM as a cost-effective alternative to fluorescence microscopy, providing quantitative phase imaging and enabling the identification of cell-type-specific biophysical signatures within the organoids. The study's significance lies in its ability to offer a non-invasive and high-throughput method for studying brain organoid development and disease modeling.
Reference

Nuclei located in neurogenic regions consistently exhibited significantly higher phase values (optical path difference) compared to nuclei elsewhere, suggesting cell-type-specific biophysical signatures.

CNN for Velocity-Resolved Reverberation Mapping

Published:Dec 30, 2025 19:37
1 min read
ArXiv

Analysis

This paper introduces a novel application of Convolutional Neural Networks (CNNs) to deconvolve noisy and gapped reverberation mapping data, specifically for constructing velocity-delay maps in active galactic nuclei. This is significant because it offers a new computational approach to improve the analysis of astronomical data, potentially leading to a better understanding of the environment around supermassive black holes. The use of CNNs for this type of deconvolution problem is a promising development.
Reference

The paper showcases that such methods have great promise for the deconvolution of reverberation mapping data products.

Physics#Nuclear Physics🔬 ResearchAnalyzed: Jan 3, 2026 15:41

Nuclear Structure of Lead Isotopes

Published:Dec 30, 2025 15:08
1 min read
ArXiv

Analysis

This paper investigates the nuclear structure of lead isotopes (specifically $^{184-194}$Pb) using the nuclear shell model. It's important because understanding the properties of these heavy nuclei helps refine our understanding of nuclear forces and the behavior of matter at the atomic level. The study provides detailed calculations of energy spectra, electromagnetic properties, and isomeric state characteristics, comparing them with experimental data to validate the model and potentially identify discrepancies that could lead to new insights.
Reference

The paper reports results for energy spectra, electromagnetic properties such as quadrupole moment ($Q$), magnetic moment ($μ$), $B(E2)$, and $B(M1)$ transition strengths, and compares the shell-model results with the available experimental data.

Paper#Astrophysics🔬 ResearchAnalyzed: Jan 3, 2026 16:46

AGN Physics and Future Spectroscopic Surveys

Published:Dec 30, 2025 12:42
1 min read
ArXiv

Analysis

This paper proposes a science case for future wide-field spectroscopic surveys to understand the connection between accretion disk, X-ray corona, and ionized outflows in Active Galactic Nuclei (AGN). It highlights the importance of studying the non-linear Lx-Luv relation and deviations from it, using various emission lines and CGM nebulae as probes of the ionizing spectral energy distribution (SED). The paper's significance lies in its forward-looking approach, outlining the observational strategies and instrumental requirements for a future ESO facility in the 2040s, aiming to advance our understanding of AGN physics.
Reference

The paper proposes to use broad and narrow line emission and CGM nebulae as calorimeters of the ionising SED to trace different accretion "states".

Analysis

This paper provides a detailed analysis of the active galactic nucleus Mrk 1040 using long-term X-ray observations. It investigates the evolution of the accretion properties over 15 years, identifying transitions between different accretion regimes. The study examines the soft excess, a common feature in AGN, and its variability, linking it to changes in the corona and accretion flow. The paper also explores the role of ionized absorption and estimates the black hole mass, contributing to our understanding of AGN physics.
Reference

The source exhibits pronounced spectral and temporal variability, indicative of transitions between different accretion regimes.

Halo Structure of 6He Analyzed via Ab Initio Correlations

Published:Dec 30, 2025 10:13
1 min read
ArXiv

Analysis

This paper investigates the halo structure of 6He, a key topic in nuclear physics, using ab initio calculations. The study's significance lies in its detailed analysis of two-nucleon spatial correlations, providing insights into the behavior of valence neutrons and the overall structure of the nucleus. The use of ab initio methods, which are based on fundamental principles, adds credibility to the findings. Understanding the structure of exotic nuclei like 6He is crucial for advancing our knowledge of nuclear forces and the limits of nuclear stability.
Reference

The study demonstrates that two-nucleon spatial correlations, specifically the pair-number operator and the square-separation operator, encode important details of the halo structure of 6He.

Spin Fluctuations as a Probe of Nuclear Clustering

Published:Dec 30, 2025 08:41
1 min read
ArXiv

Analysis

This paper investigates how the alpha-cluster structure of light nuclei like Oxygen-16 and Neon-20 affects the initial spin fluctuations in high-energy collisions. The authors use theoretical models (NLEFT and alpha-cluster models) to predict observable differences in spin fluctuations compared to a standard model. This could provide a new way to study the internal structure of these nuclei by analyzing the final-state Lambda-hyperon spin correlations.
Reference

The strong short-range spin--isospin correlations characteristic of $α$ clusters lead to a significant suppression of spin fluctuations compared to a spherical Woods--Saxon baseline with uncorrelated spins.

Research#Physics🔬 ResearchAnalyzed: Jan 4, 2026 06:49

Total decay rate of a muon bound to a light nucleus

Published:Dec 28, 2025 17:51
1 min read
ArXiv

Analysis

This article title suggests a focus on theoretical physics, specifically the study of muon decay within the context of atomic nuclei. The 'ArXiv' source indicates this is a pre-print publication, likely a research paper. The title is concise and descriptive, clearly indicating the subject matter.

Key Takeaways

    Reference

    Halo Formation in Heavy Sodium Isotopes and Orbit Inversion

    Published:Dec 28, 2025 14:49
    1 min read
    ArXiv

    Analysis

    This paper investigates the impact of inverting the p and f shell-model orbits on the formation of halo structures in neutron-rich sodium isotopes. It uses theoretical models to explore the phenomenon, focusing on isotopes like 34, 37, and 39Na. The research is significant because it contributes to our understanding of nuclear structure, particularly in exotic nuclei, and how shell structure influences halo formation. The study also suggests a method (electric dipole response) to experimentally probe these structures.
    Reference

    The halo formation is driven by the weakening of the shell gap and inversion of the 2p3/2 and 1f7/2 orbits.

    Analysis

    This paper proposes a factorized approach to calculate nuclear currents, simplifying calculations for electron, neutrino, and beyond Standard Model (BSM) processes. The factorization separates nucleon dynamics from nuclear wave function overlaps, enabling efficient computation and flexible modification of nucleon couplings. This is particularly relevant for event generators used in neutrino physics and other areas where accurate modeling of nuclear effects is crucial.
    Reference

    The factorized form is attractive for (neutrino) event generators: it abstracts away the nuclear model and allows to easily modify couplings to the nucleon.

    Evidence for Stratified Accretion Disk Wind in AGN

    Published:Dec 27, 2025 14:49
    1 min read
    ArXiv

    Analysis

    This paper provides observational evidence supporting the existence of a stratified accretion disk wind in Active Galactic Nuclei (AGN). The analysis of multi-wavelength spectroscopic data reveals distinct emission line profiles and kinematic signatures, suggesting a structured outflow. This is significant because it provides constraints on the geometry and physical conditions of AGN winds, which is crucial for understanding the processes around supermassive black holes.
    Reference

    High-ionization lines (e.g., Civ λ1549) exhibit strong blueshifts and asymmetric profiles indicative of fast, inner winds, while low-ionization lines (e.g., Hβ, Mgii λ 2800) show more symmetric profiles consistent with predominant emission from slower, denser regions farther out.

    Differentiable Neural Network for Nuclear Scattering

    Published:Dec 27, 2025 06:56
    1 min read
    ArXiv

    Analysis

    This paper introduces a novel application of Bidirectional Liquid Neural Networks (BiLNN) to solve the optical model in nuclear physics. The key contribution is a fully differentiable emulator that maps optical potential parameters to scattering wave functions. This allows for efficient uncertainty quantification and parameter optimization using gradient-based algorithms, which is crucial for modern nuclear data evaluation. The use of phase-space coordinates enables generalization across a wide range of projectile energies and target nuclei. The model's ability to extrapolate to unseen nuclei suggests it has learned the underlying physics, making it a significant advancement in the field.
    Reference

    The network achieves an overall relative error of 1.2% and extrapolates successfully to nuclei not included in training.

    Analysis

    This paper introduces Bright-4B, a large-scale foundation model designed to segment subcellular structures directly from 3D brightfield microscopy images. This is significant because it offers a label-free and non-invasive approach to visualize cellular morphology, potentially eliminating the need for fluorescence or extensive post-processing. The model's architecture, incorporating novel components like Native Sparse Attention, HyperConnections, and a Mixture-of-Experts, is tailored for 3D image analysis and addresses challenges specific to brightfield microscopy. The release of code and pre-trained weights promotes reproducibility and further research in this area.
    Reference

    Bright-4B produces morphology-accurate segmentations of nuclei, mitochondria, and other organelles from brightfield stacks alone--without fluorescence, auxiliary channels, or handcrafted post-processing.

    Physics#Nuclear Physics🔬 ResearchAnalyzed: Jan 3, 2026 23:54

    Improved Nucleon Momentum Distributions from Electron Scattering

    Published:Dec 26, 2025 07:17
    1 min read
    ArXiv

    Analysis

    This paper addresses the challenge of accurately extracting nucleon momentum distributions (NMDs) from inclusive electron scattering data, particularly in complex nuclei. The authors improve the treatment of excitation energy within the relativistic Fermi gas (RFG) model. This leads to better agreement between extracted NMDs and ab initio calculations, especially around the Fermi momentum, improving the understanding of Fermi motion and short-range correlations (SRCs).
    Reference

    The extracted NMDs of complex nuclei show better agreement with ab initio calculations across the low- and high-momentum range, especially around $k_F$, successfully reproducing both the behaviors of Fermi motion and SRCs.

    Analysis

    This paper investigates the processing of hydrocarbon dust in galaxies, focusing on the ratio of aliphatic to aromatic hydrocarbon emission. It uses AKARI near-infrared spectra to analyze a large sample of galaxies, including (U)LIRGs, IRGs, and sub-IRGs, and compares them to Galactic HII regions. The study aims to understand how factors like UV radiation and galactic nuclei influence the observed emission features.
    Reference

    The luminosity ratios of aliphatic to aromatic hydrocarbons ($L_{ali}/L_{aro}$) in the sample galaxies show considerably large variations, systematically decreasing with $L_{IR}$ and $L_{Brα}$.

    Analysis

    This article reports on research concerning the prediction of spontaneous fission half-lives for heavy and super-heavy nuclei using phenomenological models. The focus is on theoretical calculations and model development within the field of nuclear physics. The source is ArXiv, indicating a pre-print or research paper.

    Key Takeaways

      Reference

      Research#Simulation🔬 ResearchAnalyzed: Jan 10, 2026 07:31

      AI and Galaxy Evolution: A Comparison of AGN Hosts in Simulations

      Published:Dec 24, 2025 19:58
      1 min read
      ArXiv

      Analysis

      This research leverages AI, specifically simulations, to study galaxy evolution focusing on the quenching pathways of Active Galactic Nuclei (AGN) host galaxies. The study compares observational data from the Sloan Digital Sky Survey (SDSS) with the IllustrisTNG and EAGLE simulations to improve our understanding of galaxy formation.
      Reference

      The study confronts SDSS AGN hosts with IllustrisTNG and EAGLE simulations.

      Research#X-ray Model🔬 ResearchAnalyzed: Jan 10, 2026 07:45

      New X-ray Spectral Model Improves Understanding of Dusty Galactic Regions

      Published:Dec 24, 2025 06:36
      1 min read
      ArXiv

      Analysis

      This research introduces a novel X-ray spectral model, IMPACTX, designed to analyze the complex environments of polar dust and clumpy tori. The model's development could provide valuable insights into the structure and evolution of active galactic nuclei and other dusty environments.
      Reference

      IMPACTX is an X-ray spectral model for polar dust and clumpy torus.

      Research#Astronomy🔬 ResearchAnalyzed: Jan 10, 2026 07:57

      BASS.L Near-infrared Data Release 3: A Spectral Atlas for Active Galactic Nuclei

      Published:Dec 23, 2025 19:01
      1 min read
      ArXiv

      Analysis

      This article presents a significant contribution to the field of astrophysics, offering a comprehensive spectral atlas of active galactic nuclei. The data release enhances our understanding of these energetic celestial objects, providing valuable resources for further research.
      Reference

      The article describes the release of near-infrared data.

      Research#nuclear physics🔬 ResearchAnalyzed: Jan 4, 2026 07:13

      Exploring quark mass dependent three-nucleon forces in medium-mass nuclei

      Published:Dec 23, 2025 15:49
      1 min read
      ArXiv

      Analysis

      This article likely discusses research on nuclear physics, specifically focusing on the impact of quark masses on the interactions between three nucleons within medium-mass nuclei. The research likely uses theoretical models and computational methods to understand the behavior of atomic nuclei.

      Key Takeaways

        Reference

        Analysis

        This article reports on research investigating the relationship between the variability timescale of Active Galactic Nuclei (AGN) and the mass of their central black holes. The study utilizes data from the Gaia, SDSS, and ZTF surveys. The research likely aims to understand the physical processes driving AGN variability and to refine methods for estimating black hole masses.

        Key Takeaways

          Reference

          Analysis

          This article focuses on modeling heavy-ion collisions using fluid dynamics, aiming to understand the transition from colliding nuclei to the quark-gluon plasma. The research likely explores the applicability and limitations of fluid dynamics in describing this complex process.

          Key Takeaways

            Reference

            Research#AGN🔬 ResearchAnalyzed: Jan 10, 2026 09:34

            M87's AGN Feedback: Unveiling Filament Dynamics and Ionization

            Published:Dec 19, 2025 13:32
            1 min read
            ArXiv

            Analysis

            This research delves into the complex interplay between active galactic nuclei (AGN) and their host galaxies, specifically focusing on the impact of AGN-driven feedback mechanisms. The study of the dynamics and ionization of filaments within M87 provides crucial insights into galaxy evolution.
            Reference

            The research focuses on the dynamics and ionization of filaments in M87.

            Analysis

            This article likely presents research on particle physics, specifically exploring constraints on hypothetical bosons beyond the Standard Model. The methodology involves precision spectroscopy of muonic atoms (atoms where an electron is replaced by a muon) using magic nuclei, which are nuclei with specific numbers of protons and neutrons that exhibit enhanced stability. The term "self-consistent bounds" suggests the researchers are aiming for rigorous and reliable limits on the properties of these new bosons.
            Reference

            Research#llm🔬 ResearchAnalyzed: Jan 4, 2026 09:16

            Resolving Galaxy Nuclei and Compact Stellar Systems as Engines of Galaxy Evolution

            Published:Dec 15, 2025 16:20
            1 min read
            ArXiv

            Analysis

            This article likely discusses the role of galactic nuclei and compact stellar systems in the process of galaxy evolution. It suggests that these components are key drivers of how galaxies change over time. The source, ArXiv, indicates this is a research paper.

            Key Takeaways

            Reference

            Analysis

            This article describes a research paper focusing on the application of weak-to-strong generalization in training a Mask-RCNN model for a specific biomedical task: segmenting cell nuclei in brain images. The use of 'de novo' training suggests a focus on training from scratch, potentially without pre-existing labeled data. The title highlights the potential for automation in this process.
            Reference

            Research#Cosmology🔬 ResearchAnalyzed: Jan 10, 2026 11:54

            Cosmic Ray Feedback from AGN Impacts Galaxy Properties, Study Finds

            Published:Dec 11, 2025 19:23
            1 min read
            ArXiv

            Analysis

            This article summarizes research exploring the impact of cosmic ray feedback from Active Galactic Nuclei (AGN) on the characteristics of massive galaxies. The study's findings are likely to contribute to a deeper understanding of galaxy formation and evolution.
            Reference

            The study investigates the effects of varied cosmic ray feedback from AGN on massive galaxy properties.

            Research#Nuclear Physics🔬 ResearchAnalyzed: Jan 10, 2026 14:09

            Nuclear Structure Research on Nobelium Isotopes

            Published:Nov 27, 2025 08:47
            1 min read
            ArXiv

            Analysis

            This article discusses research focused on the nuclear structure of Nobelium isotopes, specifically examining $0^+$ and $8^-$ states. The study, accessible via ArXiv, provides insights into the behavior of heavy nuclei.
            Reference

            The study focuses on even-even $^{250-260}$No isotopes.