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arXiv 2021年

作者： Luger, Rodrigo Foreman-Mackey, Daniel Hedges, Christina Hogg, David W. Center for Computational Astrophysics Flatiron Institute New YorkNY United States Virtual Planetary Laboratory University of Washington SeattleWA United States Bay Area Environmental Research Institute Moffett Field CA United States NASA Ames Research Center Moffett Field CA United States Center for Cosmology and Particle Physics New York University New YorkNY United States Center for Data Science New York University New YorkNY United States Max-Planck-Institut für Astronomie Heidelberg Germany

Thanks to missions like Kepler and TESS, we now have access to tens of thousands of high precision, fast cadence, and long baseline stellar photometric observations. In principle, these light curves encode a vast amount of information about stellar variability and, in particular, about the distribution of starspots and other features on their surfaces. Unfortunately, the problem of inferring stellar surface properties from a rotational light curve is famously ill-posed, as it often does not admit a unique solution. Inference about the number, size, contrast, and location of spots can therefore depend very strongly on the assumptions of the model, the regularization scheme, or the prior. The goal of this paper is twofold: (1) to explore the various degeneracies affecting the stellar light curve "inversion" problem and their effect on what can and cannot be learned from a stellar surface given unresolved photometric measurements;and (2) to motivate ensemble analyses of the light curves of many stars at once as a powerful data-driven alternative to common priors adopted in the literature. We further derive novel results on the dependence of the null space on stellar inclination and limb darkening and show that single-band photometric measurements cannot uniquely constrain quantities like the total spot coverage without the use of strong priors. This is the first in a series of papers devoted to the development of novel algorithms and tools for the analysis of stellar light curves and spectral time series, with the explicit goal of enabling statistically robust inference about their surface properties. Copyright © 2021, The Authors. All rights reserved.

关键词： Stars

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Stable attractors in the three-dimensional general relativistic Poynting-Robertson effect

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Physical Review D 2020年第2期101卷 024025-024025页

作者： Vittorio De Falco Pavel Bakala Research Centre for Computational Physics and Data Processing Faculty of Philosophy & Science Silesian University in Opava Bezručovo namesti 13 CZ-746 01 Opava Czech Republic M. R. Štefánik Observatory and Planetarium Sládkovičova 41 920 01 Hlohovec Slovak Republic

We prove the stability of the critical hypersurfaces associated with the three-dimensional general relativistic Poynting-Robertson effect. The equatorial ring configures to be as a stable attractor and the whole critical hypersurface as a basin of attraction for this dynamical system. We introduce a new, simpler (in terms of calculations), and more physical approach within the Lyapunov theory. We propose three different Lyapunov functions, each one carrying important information and very useful for understanding such phenomenon under different aspects.

关键词： General relativity General relativity equations & solutions Gravitation Numerical simulations in gravitation & astrophysics

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Image-guided patient-specific optimization of catheter placement for convection-enhanced nanoparticle delivery in recurrent glioblastoma

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Computers in Biology and Medicine 2024年 179卷 108889-108889页

作者： Wu, Chengyue Hormuth, David A. Christenson, Chase D. Woodall, Ryan T. Abdelmalik, Michael R.A. Phillips, William T. Hughes, Thomas J.R. Brenner, Andrew J. Yankeelov, Thomas E. Oden Institute for Computational Engineering and Sciences The University of Texas at Austin AustinTX78712 United States Department of Biomedical Engineering The University of Texas at Austin AustinTX78712 United States Department of Aerospace Engineering and Engineering Mechanics The University of Texas at Austin AustinTX78712 United States Department of Diagnostic Medicine The University of Texas at Austin AustinTX78712 United States Department of Oncology The University of Texas at Austin AustinTX78712 United States Livestrong Cancer Institutes The University of Texas at Austin AustinTX78712 United States Department of Imaging Physics The University of Texas MD Anderson Cancer Center HoustonTX77030 United States Department of Breast Imaging The University of Texas MD Anderson Cancer Center HoustonTX77030 United States Department of Biostatistics The University of Texas MD Anderson Cancer Center HoustonTX77030 United States Institute for Data Science in Oncology The University of Texas MD Anderson Cancer Center HoustonTX77030 United States Division of Mathematical Oncology Beckman Research Institute City of Hope National Medical Center 1500 East Duarte Rd DuarteCA91010 United States Department of Mechanical Engineering Eindhoven University of Technology Eindhoven Netherlands Department of Radiology UT Health San Antonio San AntonioTX78229 United States Mays Cancer Center UT Health San Antonio San AntonioTX78229 United States

Background: Proper catheter placement for convection-enhanced delivery (CED) is required to maximize tumor coverage and minimize exposure to healthy tissue. We developed an image-based model to patient-specifically optimize the catheter placement for rhenium-186 (186Re)-nanoliposomes (RNL) delivery to treat recurrent glioblastoma (rGBM). Methods: The model consists of the 1) fluid fields generated via catheter infusion, 2) dynamic transport of RNL, and 3) transforming RNL concentration to the SPECT signal. Patient-specific tissue geometries were assigned from pre-delivery MRIs. Model parameters were personalized with either 1) individual-based calibration with longitudinal SPECT images, or 2) population-based assignment via leave-one-out cross-validation. The concordance correlation coefficient (CCC) was used to quantify the agreement between the predicted and measured SPECT signals. The model was then used to simulate RNL distributions from a range of catheter placements, resulting in a ratio of the cumulative RNL dose outside versus inside the tumor, the "off-target ratio" (OTR). Optimal catheter placement) was identified by minimizing OTR. Results: Fifteen patients with rGBM from a Phase I/II clinical trial (NCT01906385) were recruited to the study. Our model, with either individual-calibrated or population-assigned parameters, achieved high accuracy (CCC > 0.80) for predicting RNL distributions up to 24 h after delivery. The optimal catheter placements identified using this model achieved a median (range) of 34.56 % (14.70 %–61.12 %) reduction on OTR at the 24 h post-delivery in comparison to the original placements. Conclusions: Our image-guided model achieved high accuracy for predicting patient-specific RNL distributions and indicates value for optimizing catheter placement for CED of radiolabeled liposomes. © 2024 Elsevier Ltd

关键词： Nanoparticles

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GRAVITATIONAL SELF-LENSING OF FAST RADIO BURSTS IN NEUTRON STAR MAGNETOSPHERES: I. THE MODEL

arXiv

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arXiv 2024年

作者： Dall'Osso, Simone La Placa, Riccardo Stella, Luigi Bakala, Pavel Possenti, Andrea Istituto Nazionale di Fisica Nucleare - Roma 1 Piazzale Aldo Moro 2 Roma00185 Italy GSC - Goethe University of Frankfurt Max von Laue Strasse 1 Frankfurt Germany Dipartimento di Fisica Università La Sapienza Piazzale Aldo Moro 5 Roma00185 Italy INAF - Osservatorio Astronomico di Roma via Frascati 33 Monte Porzio CatoneI-00078 Italy Dipartimento di Fisica Università di Roma "Tor Vergata" Via della Ricerca Scientifica Roma00133 Italy Research Centre for Computational Physics and Data Processing Silesian University in Opava Bezručovo nám. 13 OpavaCZ-74601 Czech Republic M. R. Štefánik Observatory and Planetarium Sládkovičova 41 Hlohovec920 01 Slovakia INAF Osservatorio Astronomico di Cagliari Via della Scienza 5 Selargius09047 Italy

Fast Radio Bursts (FRBs) are cosmological sub-second bursts of coherent radio emission, whose source is still unknown. To date, the galactic magnetar SGR 1935+2154 is the only astrophysical object known to emit radio bursts akin to FRBs, albeit less powerful, supporting suggestions that FRBs originate from magnetars. Many remarkable properties of FRBs, e.g. the dichotomy between repeaters and one-off sources, and their power-law energy distributions (with typical index ∼ 2 − 3), are not well understood yet. Moreover, the huge radio power released by the most active repeaters is challenging even for the magnetic energy reservoir of magnetars. Here we assume that FRBs originate from co-rotating hot-spots anchored in neutron star magnetospheres and get occasionally amplified by large factors via gravitational self-lensing in the strong NS field. We evaluate the probability of amplification and show that (i) a power-law energy distribution of events ∝ E− (2−3) is generally expected, (ii) all FRB sources may be regarded as repeating, their appearance as one-off sources or repeaters being determined by the critical dependence of the amplification probability on the emission geometry and source orientation relative to Earth and (iii) the most active repeaters, in particular, correspond to extremely rare and finely-tuned orientations (∼ one in 106), leading to large probabilities of amplification which make their bursts frequently detectable. At the same time, their power release appears enhanced, typically by factors 10, easing their energy budget problem. © 2024, CC BY-SA.

关键词： Budget control

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Synchrotron Radiation Dominates the Extremely Bright GRB 221009A

arXiv

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arXiv 2023年

作者： Yang, Jun Zhao, Xiao-Hong Yan, Zhenyu Wang, Xiangyu Ivy Zhang, Yan-Qiu An, Zheng-Hua Cai, Ce Li, Xin-Qiao Li, Zihan Liu, Jia-Cong Liu, Zi-Ke Ma, Xiang Meng, Yan-Zhi Peng, Wen-Xi Qiao, Rui Shao, Lang Song, Li-Ming Tan, Wen-Jun Wang, Ping Wang, Chen-Wei Wen, Xiang-Yang Xiao, Shuo Xue, Wang-Chen Yang, Yu-Han Yin, Yihan Zhang, Bing Zhang, Fan Zhang, Shuai Zhang, Shuang-Nan Zheng, Chao Zheng, Shi-Jie Xiong, Shao-Lin Zhang, Bin-Bin School of Astronomy and Space Science Nanjing University Nanjing210093 China Key Laboratory of Modern Astronomy and Astrophysics Nanjing University Ministry of Education China Yunnan Observatories Chinese Academy of Sciences Kunming China Center for Astronomical Mega-Science Chinese Academy of Sciences Beijing China Key Laboratory for the Structure and Evolution of Celestial Objects Chinese Academy of Sciences Kunming China Key Laboratory of Particle Astrophysics Institute of High Energy Physics Chinese Academy of Sciences 19B Yuquan Road Beijing100049 China University of Chinese Academy of Sciences Beijing100049 China College of Physics Hebei Key Laboratory of Photophysics Research and Application Hebei Normal University Hebei Shijiazhuang050024 China College of Physics Hebei Normal University Shijiazhuang050024 China Guizhou Provincial Key Laboratory of Radio Astronomy and Data Processing Guizhou Normal University Guiyang550001 China Department of Physics University of Rome "Tor Vergata" via della Ricerca Scientifica 1 RomeI-00133 Italy School of Physics Nanjing University Nanjing210093 China Department of Physics and Astronomy University of Nevada Las Vegas NV89154 United States Purple Mountain Observatory Chinese Academy of Sciences Nanjing210023 China

The brightest Gamma-ray burst, GRB 221009A, has spurred numerous theoretical investigations, with particular attention paid to the origins of ultra-high energy TeV photons during the prompt phase. However, analyzing the mechanism of radiation of photons in the ∼MeV range has been difficult because the high flux causes pile-up and saturation effects in most GRB detectors. In this letter, we present systematic modeling of the time-resolved spectra of the GRB using unsaturated data obtained from Fermi/GBM (precursor) and SATech-01/GECAM-C (main emission and flare). Our approach incorporates the synchrotron radiation model, which assumes an expanding emission region with relativistic speed and a global magnetic field that decays with radius, and successfully fits such a model to the observational data. Our results indicate that the spectra of the burst are fully in accordance with a synchrotron origin from relativistic electrons accelerated at a large emission radius. The lack of thermal emission in the prompt emission spectra supports a Poynting-flux-dominated jet composition. Copyright © 2023, The Authors. All rights reserved.

关键词： Synchrotron radiation

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THE TEMPO SURVEY II: SCIENCE CASES LEVERAGED FROM A PROPOSED 30-DAY TIME DOMAIN SURVEY OF THE ORION NEBULA WITH THE NANCY GRACE ROMAN SPACE TELESCOPE

arXiv

引用

arXiv 2024年

作者： Soares-Furtado, Melinda Limbach, Mary Anne Vanderburg, Andrew Bally, John Becker, Juliette Rosen, Anna L. Bouma, Luke G. Vos, Johanna M. Howell, Steve B. Beatty, Thomas G. Best, William M.J. Cody, Anne Marie Distler, Adam D’Onghia, Elena Heller, René Hensley, Brandon S. Hinkel, Natalie R. Jackson, Brian Kounkel, Marina Kraus, Adam Mann, Andrew W. Marston, Nicholas T. Robberto, Massimo Rodriguez, Joseph E. Steffen, Jason H. Teske, Johanna K. Townsend, Richard Yarza, Ricardo Youngblood, Allison Department of Astronomy University of Wisconsin-Madison 475 N. Charter St. MadisonWI53706 United States Department of Physics Kavli Institute for Astrophysics and Space Research Massachusetts Institute of Technology CambridgeMA02139 United States Department of Astronomy University of Michigan Ann ArborMI48109 United States Center for Astrophysics and Space Astronomy Astrophysical and Planetary Sciences Department University of Colorado BoulderCO80389 United States Department of Astronomy San Diego State University San DiegoCA92182 United States Computational Science Research Center San Diego State University San DiegoCA92182 United States Department of Astronomy MC 249-17 California Institute of Technology PasadenaCA91125 United States School of Physics Trinity College Dublin The University of Dublin Dublin 2 Ireland NASA Ames Research Center Moffett FieldCA94035 United States Department of Astronomy The University of Texas at Austin AustinTX78712 United States SETI Institute 189 N. Bernardo Ave #200 Mountain ViewCA94043 United States Max Planck Institute for Solar System Research Justus-von-Liebig-Weg 3 Göttingen37077 Germany Jet Propulsion Laboratory California Institute of Technology 4800 Oak Grove Drive PasadenaCA91109 United States Physics & Astronomy Department Louisiana State University Baton RougeLA70803 United States Department of Physics Boise State University BoiseID83725-1570 United States Department of Physics & Astronomy Vanderbilt University NashvilleTN37235 United States Department of Physics & Astronomy The University of North Carolina at Chapel Hill Chapel HillNC27599-3255 United States Space Telescope Science Institute 3700 San Martin Drive BaltimoreMD21218 United States Johns Hopkins University 3400 N. Charles St. BaltimoreMD21218 United States Center for Data Intensive and Time Domain Astronomy Department of Physics and Astronomy Michigan State University East LansingMI48824 United States Un

The TEMPO (Transiting Exosatellites, Moons, and Planets in Orion) Survey is a proposed 30-day observational campaign using the Nancy Grace Roman Space Telescope. By providing deep, high-resolution, short-cadence infrared photometry of a dynamic star-forming region, TEMPO will investigate the demographics of exosatellites orbiting free-floating planets and brown dwarfs — a largely unexplored discovery space. Here, we present the simulated detection yields of three populations: extrasolar moon analogs orbiting free-floating planets, exosatellites orbiting brown dwarfs, and exoplanets orbiting young stars. Additionally, we outline a comprehensive range of anticipated scientific outcomes accompanying such a survey. These science drivers include: obtaining observational constraints to test prevailing theories of moon, planet, and star formation;directly detecting widely separated exoplanets orbiting young stars;investigating the variability of young stars and brown dwarfs;constraining the low-mass end of the stellar initial mass function;constructing the distribution of dust in the Orion Nebula and mapping evolution in the near-infrared extinction law;mapping emission features that trace the shocked gas in the region;constructing a dynamical map of Orion members using proper motions;and searching for extragalactic sources and transients via deep extragalactic observations reaching a limiting magnitude of mAB = 29.7 mag (F146 filter). © 2024, CC BY.

关键词： Orbits

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Deep learning based parameter search for an agent based social network model

arXiv

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arXiv 2021年

作者： Murase, Yohsuke Jo, Hang-Hyun Török, János Kertész, János Kaski, Kimmo RIKEN Center for Computational Science Kobe Japan Department of Physics Catholic University of Korea Bucheon Korea Republic of Department of Theoretical Physics Budapest University of Technology and Economics Budapest Hungary Department of Network and Data Science Central European University Vienna Austria MTA-BME Morphodynamics Research Group Budapest University of Technology and Economics Budapest Hungary Department of Computer Science Aalto University Espoo Finland Alan Turing Institute British Library London United Kingdom

Interactions between humans give rise to complex social networks that are characterized by heterogeneous degree distribution, weight-topology relation, overlapping community structure, and dynamics of links. Understanding such networks is a primary goal of science due to serving as the scaffold for many emergent social phenomena from disease spreading to political movements. An appropriate tool for studying them is agent-based modeling, in which nodes, representing persons, make decisions about creating and deleting links, thus yielding various macroscopic behavioral patterns. Here we focus on studying a generalization of the weighted social network model, being one of the most fundamental agent-based models for describing the formation of social ties and social networks. This Generalized Weighted Social Network (GWSN) model incorporates triadic closure, homophilic interactions, and various link termination mechanisms, which have been studied separately in the previous works. Accordingly, the GWSN model has an increased number of input parameters and the model behavior gets excessively complex, making it challenging to clarify the model behavior. We have executed massive simulations with a supercomputer and using the results as the training data for deep neural networks to conduct regression analysis for predicting the properties of the generated networks from the input parameters. The obtained regression model was also used for global sensitivity analysis to identify which parameters are influential or insignificant. We believe that this methodology is applicable for a large class of complex network models, thus opening the way for more realistic quantitative agent-based modeling. Copyright © 2021, The Authors. All rights reserved.

关键词： Simulation platform

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An extreme test case for planet formation: a close-in Neptune orbiting an ultracool star

arXiv

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arXiv 2023年

作者： Stefánsson, Guðmundur Mahadevan, Suvrath Miguel, Yamila Robertson, Paul Delamer, Megan Kanodia, Shubham Cañas, Caleb Winn, Joshua Ninan, Joe Terrien, Ryan Holcomb, Rae Ford, Eric Zawadzki, Brianna Bowler, Brendan P. Bender, Chad Cochran, William Diddams, Scott Endl, Michael Fredrick, Connor Halverson, Samuel Hearty, Fred Hill, Gary J. Lin, Andrea Metcalf, Andrew Monson, Andrew Ramsey, Lawrence Roy, Arpita Schwab, Christian Wright, Jason Zeimann, Gregory Princeton University Department of Astrophysical Sciences United States Department of Astronomy & Astrophysics The Pennsylvania State University United States Center for Exoplanets and Habitable Worlds The Pennsylvania State University United States ETH Zurich Institute for Particle Physics & Astrophysics Switzerland Leiden Observatory University of Leiden Netherlands SRON Netherlands Institute for Space Research Netherlands Department of Physics & Astronomy University of California Irvine United States Earth and Planets Laboratory Carnegie Institution for Science United States NASA Goddard Space Flight Center United States Department of Astronomy & Astrophysics Tata Institute of Fundamental Research India Carleton College United States Center for Astrostatistics The Pennsylvania State University United States Institute for Computational & Data Sciences The Pennsylvania State University United States Department of Astronomy The University of Texas at Austin AustinTX78712 United States Steward Observatory The University of Arizona United States Center for Planetary Systems Habitability and McDonald Observatory UT Austin United States Electrical Computer and Energy Engineering University of Colorado United States National Institute of Standards & Technology United States Department of Physics University of Colorado United States Jet Propulsion Laboratory California Institute of Technology United States McDonald Observatory UT Austin United States Space Vehicles Directorate Air Force Research Laboratory United States Space Telescope Science Institute United States Department of Physics and Astronomy Johns Hopkins University United States School of Mathematical and Physical Sciences Macquarie University Australia Penn State Extraterrestrial Intelligence Center The Pennsylvania State University United States Hobby-Eberly Telescope University of Texas Austin AustinTX78712 United States

In current theories of planet formation, close-orbiting planets as massive as Neptune are expected to be very rare around low-mass stars. We report the discovery of a Neptune-mass planet orbiting the 'ultracool' star LHS 3154, which is nine times less massive than the Sun. The planet's orbital period is 3.7 days and its minimum mass is 13.2 Earth masses, giving it the largest known planet-to-star mass ratio among short-period planets ( Copyright © 2023, The Authors. All rights reserved.

关键词： Planets

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High-throughput investigations of configurational-transformation-dominated serrations in CuZr/Cu nanolaminates

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Journal of Materials Science & Technology 2020年第18期52卷 192-199页

作者： William Yi Wang Bin Gana Deye Lin Jun Wang Yiguang Wang Bin Tang Hongchao Kou Shunli Shang Yi Wang Xingyu Gao Haifeng Song Xidong Hui Laszlo J.Kecskes Zhenhai Xia Karin A.Dahmen Peter K.Liaw Jinshan Lia Zi-Kui Liu State Key Laboratory of Solidification Processing Northwestern Polytechnical UniversityXi'an.710072China Beijing Key Laboratory of Advanced High Temperature Materials Central Iron and Steel Research InstituteBeijing100081China IMDEA Materials Institute Calle Eric Kandel 2GetafeMadrid28906Spain CAEP Software Center for High Performance Numerical Simulation Institute of Applied Physics and Computational MathematicsBeijing100088China Department of Materials Science and Engineering The Pennsylvania State UniversityUniversity ParkPA16802USA State Key Laboratory for Advanced Metals and Materials University of Science and Technology BeijingBeijing100083China Hopkins Extreme Materials Institute Johns Hopkins UniversityBaltimoreMD21218USA Department of Physics University of Illinois at Urbana ChampaignUrbanaIL61801USA Department of Materials Science and Engineering The University of TennesseeKnoxvilleTN37996USA

Metallic amorphous/crystalline(A/C)nanolaminates exhibit excellent ductility while retaining their high ***,the underlying physical mechanisms and the resultant structural changes during plastic deformation still remain *** the present work,the structure-property relationship of CuZr/Cu A/C nanolaminates is established through integrated high-throughput micro-compression tests and molecular dynamics simulations together with high-resolution transmission electron *** serrated flow of nanolaminates results from the formation of hexagonal-close-packed(HCP)-type stacking faults and twins inside the face-centered-cubic(FCC)Cu nano-grains,the body-centered-cubic(BCC)-type ordering at their grain boundaries,and the crystallization of the amorphous CuZr *** serration behavior of CuZr/Cu A/C nanolaminates is determined by several factors,including the formation of dense dislocation networks from the multiplication of initial dislocations that formed after yielding,weak-spots-related configurational-transitions and shear-transition-zone activities,and deformation-induced *** present work provides an insight into the heterogeneous deformation mechanism of A/C nanolaminates at the atomic scale,and mechanistic base for the microstructural design of self-toughening metallic-glass(MG)-based composites and A/C nanolaminates.

关键词： Nanolaminates Serration Configurational transformation Molecular dynamics Metallic glass

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Addendum: Solution epitaxy of polarization-gradient ferroelectric oxide films with colossal photovoltaic current

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Nature communications 2024年第1期15卷 3878-3878页

作者： Lin, Chen Zhang, Zijun Dai, Zhenbang Wu, Mengjiao Liu, Shi Chen, Jialu Hua, Chenqiang Lu, Yunhao Zhang, Fei Lou, Hongbo Dong, Hongliang Zeng, Qiaoshi Ma, Jing Pi, Xiaodong Zhou, Dikui Wu, Yongjun Tian, He Rappe, Andrew M. Ren, Zhaohui Han, Gaorong State Key Laboratory of Silicon and Advanced Semiconductor Materials School of Materials Science and Engineering Zhejiang University Hangzhou 310027 China Center of Electron Microscope School of Materials Science and Engineering Zhejiang University Hangzhou 310027 China Department of Chemistry University of Pennsylvania Philadelphia PA United States Oden Institute for Computational Engineering and Sciences University of Texas at Austin Austin 78712 TX United States Key Laboratory for Quantum Materials of Zhejiang Province Department of Physics School of Science Westlake University Hangzhou 310024 China Zhejiang Province Key Laboratory of Quantum Technology and Device Department of physics Zhejiang University Hangzhou 310027 China Center for High Pressure Science and Technology Advanced Research 201203 Shanghai China State Key Lab of New Ceramics and Fine Processing School of Materials Science and Engineering Tsinghua University 100091 Beijing China Institute of Advanced Semiconductors & Zhejiang Provincial Key Laboratory of Power Semiconductor Materials and Devices ZJU-Hangzhou Global Scientific and Technological Innovation Center Zhejiang University Hangzhou 311215 China Research Center for Intelligent Sensing Zhejiang Lab Hangzhou 311100 China State Key Laboratory of Silicon and Advanced Semiconductor Materials School of Materials Science and Engineering Zhejiang University Hangzhou 310027 China

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