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arXiv 2019年

作者： Gautam, Rekha Xiang, Yinxiao Lamstein, Josh Liang, Yi Bezryadina, Anna Liang, Guo Hansson, Tobias Wetzel, Benjamin Preece, Daryl White, Adam Silverman, Matthew Kazarian, Susan Xu, Jingjun Morandotti, Roberto Chen, Zhigang Department of Physics and Astronomy San Francisco State University San FranciscoCA94132 United States Department of Biomedical Engineering Vanderbilt University NashvilleTN37240 United States MOE Key Lab of Weak-Light Nonlinear Photonics TEDA Applied Physics Institute School of Physics Nankai University Tianjin300457 China Guangxi Key Lab for Relativistic Astrophysics Guangxi Colleges Universities Key Lab of Novel Energy Materials and Related Technology School of Physical Science and Technology Guangxi University Nanning Guangxi530004 China Department of Physics and Astronomy California State University Northridge NorthridgeCA91330 United States Institut National de la Recherche Scientifique Université du Québec VarennesQCJ3X 1S2 Canada Department of Physics Chemistry and Biology Linköping University LinköpingSE-581 83 Sweden School of Mathematical and Physical Sciences University of Sussex Sussex House Falmer BrightonBN1 9RH United Kingdom Department of Biomedical Engineering University of California Irvine IrvineCA United States Clinical Laboratory Science Program San Francisco State University San FranciscoCA94132 United States Institute of Fundamental and Frontier Sciences University of Electronic Science and Tech. of China Chengdu610054 China ITMO University Saint Petersburg197101 Russia

Osmotic conditions play an important role in the cell properties of human red blood cells (RBCs), which are crucial for the pathological analysis of some blood diseases such as malaria. Over the past decades, numerous efforts have mainly focused on the study of the RBC biomechanical properties that arise from the unique deformability of erythrocytes. Here, we demonstrate nonlinear optical effects from human RBCs suspended in different osmotic solutions. Specifically, we observe self-trapping and scattering-resistant nonlinear propagation of a laser beam through RBC suspensions under all three osmotic conditions, where the strength of the optical nonlinearity increases with osmotic pressure on the cells. This tunable nonlinearity is attributed to optical forces, particularly the forward scattering and gradient forces. Interestingly, in aged blood samples (with lysed cells), a notably different nonlinear behavior is observed due to the presence of free hemoglobin. We use a theoretical model with an optical force-mediated nonlocal nonlinearity to explain the experimental observations. Our work on light self-guiding through scattering bio-soft-matter may introduce new photonic tools for noninvasive biomedical imaging and medical diagnosis. Copyright © 2019, The Authors. All rights reserved.

关键词： Nonlinear optics

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A demonstration of improved constraints on primordial gravitational waves with delensing

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Physical Review D 2021年第2期103卷 022004-022004页

作者： P. A. R. Ade Z. Ahmed M. Amiri A. J. Anderson J. E. Austermann J. S. Avva D. Barkats R. Basu Thakur J. A. Beall A. N. Bender B. A. Benson F. Bianchini C. A. Bischoff L. E. Bleem J. J. Bock H. Boenish E. Bullock V. Buza J. E. Carlstrom C. L. Chang J. R. Cheshire, IV H. C. Chiang T-L. Chou R. Citron J. Connors C. Corbett Moran J. Cornelison T. M. Crawford A. T. Crites M. Crumrine A. Cukierman T. de Haan M. Dierickx M. A. Dobbs L. Duband W. Everett S. Fatigoni J. P. Filippini S. Fliescher J. Gallicchio E. M. George T. St. Germaine N. Goeckner-Wald D. C. Goldfinger J. Grayson N. Gupta G. Hall M. Halpern N. W. Halverson S. Harrison S. Henderson J. W. Henning S. R. Hildebrandt G. C. Hilton G. P. Holder W. L. Holzapfel J. D. Hrubes N. Huang J. Hubmayr H. Hui K. D. Irwin J. Kang K. S. Karkare E. Karpel S. Kefeli S. A. Kernasovskiy L. Knox J. M. Kovac C. L. Kuo K. Lau A. T. Lee E. M. Leitch D. Li A. Lowitz A. Manzotti J. J. McMahon K. G. Megerian S. S. Meyer M. Millea L. M. Mocanu L. Moncelsi J. Montgomery A. Nadolski T. Namikawa T. Natoli C. B. Netterfield H. T. Nguyen J. P. Nibarger G. Noble V. Novosad R. O’Brient R. W. Ogburn, IV Y. Omori S. Padin S. Palladino S. Patil T. Prouve C. Pryke B. Racine C. L. Reichardt C. D. Reintsema S. Richter J. E. Ruhl B. R. Saliwanchik K. K. Schaffer A. Schillaci B. L. Schmitt R. Schwarz C. D. Sheehy C. Sievers G. Smecher A. Soliman A. A. Stark B. Steinbach R. V. Sudiwala G. P. Teply K. L. Thompson J. E. Tolan C. Tucker A. D. Turner C. Umiltà T. Veach J. D. Vieira A. G. Vieregg A. Wandui G. Wang A. C. Weber N. Whitehorn D. V. Wiebe J. Willmert C. L. Wong W. L. K. Wu H. Yang V. Yefremenko K. W. Yoon E. Young C. Yu L. Zeng C. Zhang Cardiff University Cardiff CF10 3XQ United Kingdom SLAC National Accelerator Laboratory 2575 Sand Hill Road Menlo Park California 94025 USA Kavli Institute for Particle Astrophysics and Cosmology Stanford University 452 Lomita Mall Stanford California 94305 USA Department of Physics and Astronomy University of British Columbia Vancouver British Columbia V6T 1Z1 Canada Fermi National Accelerator Laboratory MS209 P.O. Box 500 Batavia Illinois 60510 USA NIST Quantum Devices Group 325 Broadway Mailcode 817.03 Boulder Colorado 80305 USA Department of Physics University of Colorado Boulder Colorado 80309 USA Department of Physics University of California Berkeley California 94720 USA Harvard-Smithsonian Center for Astrophysics 60 Garden Street Cambridge Massachusetts 02138 USA California Institute of Technology MS 249-17 1216 E. California Blvd. Pasadena California 91125 USA High Energy Physics Division Argonne National Laboratory 9700 S. Cass Avenue Argonne Illinois 60439 USA Kavli Institute for Cosmological Physics University of Chicago 5640 South Ellis Avenue Chicago Illinois 60637 USA Department of Astronomy and Astrophysics University of Chicago 5640 South Ellis Avenue Chicago Illinois 60637 USA School of Physics University of Melbourne Parkville Victoria 3010 Australia Department of Physics University of Cincinnati Cincinnati Ohio 45221 USA Jet Propulsion Laboratory Pasadena California 91109 USA Department of Physics Harvard University Cambridge Massachusetts 02138 USA Minnesota Institute for Astrophysics University of Minnesota Minneapolis Minnesota 55455 USA Department of Physics University of Chicago 5640 South Ellis Avenue Chicago Illinois 60637 USA Enrico Fermi Institute University of Chicago 5640 South Ellis Avenue Chicago Illinois 60637 USA Department of Physics McGill University 3600 Rue University Montreal Quebec H3A 2T8 Canada School of Mathematics Statistics and Computer Science University of KwaZulu-Natal Dur

We present a constraint on the tensor-to-scalar ratio, r, derived from measurements of cosmic microwave background (CMB) polarization B-modes with “delensing,” whereby the uncertainty on r contributed by the sample variance of the gravitational lensing B-modes is reduced by cross-correlating against a lensing B-mode template. This template is constructed by combining an estimate of the polarized CMB with a tracer of the projected large-scale structure. The large-scale-structure tracer used is a map of the cosmic infrared background derived from Planck satellite data, while the polarized CMB map comes from a combination of South Pole Telescope, bicep/Keck, and Planck data. We expand the bicep/Keck likelihood analysis framework to accept a lensing template and apply it to the bicep/Keck dataset collected through 2014 using the same parametric foreground modeling as in the previous analysis. From simulations, we find that the uncertainty on r is reduced by ∼10%, from σ(r)=0.024 to 0.022, which can be compared with a ∼26% reduction obtained when using a perfect lensing template or if there were zero lensing B-modes. Applying the technique to the real data, the constraint on r is improved from r0.05<0.090 to r0.05<0.082 (95% C.L.). This is the first demonstration of improvement in an r constraint through delensing.

关键词： Cosmic microwave background Inflation Large scale structure of the Universe

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High-Temperature Oxidation Behavior of Fe-18Al Alloy Added with 2 %ZrO2 Nanoparticles

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IOP Conference Series: materials science and engineering 2019年第1期515卷

作者： P Pawawoi D H Prajitno A A Dewi A Manaf Postgraduate Program of Materials Science Study Department of Physics Faculty of Mathematics and Natural Sciences Universitas Indonesia Depok 16514 PTNBR- BATAN Jln. Tamansari 71 Bandung 40317 Bandung Metallurgical Engineering of Jenderal Achmad Yani University Jln. Gatot Subroto PO. Box 807 Bandung 40285

The oxidation behaviour of ZrO2 nanoparticles added to Fe-18Al alloy has been studied. Isothermal oxidation behaviour with various temperatures and times was investigated and the results of microstructure showed the presence of Fe3Al intermetallic phases in grey color, Al2O3 oxide in white color, and the porosity indicated by dark color. The results of XRD and SEM-EDS analysis also confirmed the presence of the ZrO2 nanoparticles in addition to Fe3Al intermetallic phases and Al2O3 oxide phases. The addition of ZrO2 nanoparticles tended to decrease oxidation rate by promoting Al2O3 layers.

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Immunotherapy: engineering an Artificial T‐Cell Stimulating Matrix for Immunotherapy (Adv. Mater. 23/2019)

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Advanced materials 2019年第23期31卷

作者： John W. Hickey Yi Dong Jae Wook Chung Sebastian F. Salathe Hawley C. Pruitt Xiaowei Li Calvin Chang Andrew K. Fraser Catherine A. Bessell Andrew J. Ewald Sharon Gerecht Hai‐Quan Mao Jonathan P. Schneck Department of Biomedical Engineering School of Medicine Baltimore MD 21218 USA Institute for Cell Engineering School of Medicine Baltimore MD 21205 USA Department of Pathology School of Medicine Baltimore MD 21287 USA Translational Tissue Engineering Center Baltimore MD 21287 USA Institute for NanoBioTechnology Baltimore MD 21218 USA Graduate Program in Immunology School of Medicine Baltimore MD 21205 USA Department of Chemical and Biomolecular Engineering Whiting School of Engineering Baltimore MD 21218 USA Department of Biology Krieger School of Arts and Sciences Baltimore MD 21218 USA Department of Materials Science and Engineering Whiting School of Engineering Baltimore MD 21218 USA Department of Cell Biology and Center for Cell Dynamics School of Medicine Baltimore MD 21205 USA Department of Oncology School of Medicine Baltimore MD 21205 USA Physical Sciences‐Oncology Center Baltimore MD 21218 USA Department of Medicine School of Medicine Johns Hopkins University Baltimore MD 21205 USA

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The effective increase in atomic scale disorder by doping and superconductivity in Ca3Rh4Sn13

arXiv

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arXiv 2018年

作者： Slebarski, A. Zajdel, P. Fija lkowski, M. Maska, M.M. Witas, P. Goraus, J. Fang, Y. Arnold, D.C. Maple, M.B. Institute of Physics University of Silesia in Katowice Uniwersytecka 4 Katowice40-007 Poland Centre for Advanced Materials and Smart Structures Polish Academy of Sciences Okolna 2 Wroc law50-950 Poland Department of Physics University of California San Diego San DiegoCA92093 United States Materials Science and Engineering Program University of California San Diego San DiegoCA92093 United States School of Physical Sciences University of Kent Canterbury KentCT2 7NH United Kingdom

The comprehensive research of the electronic structure, thermodynamic and electrical transport properties reveals the existence of inhomogeneous superconductivity due to structural disorder in Ca3Rh4Sn13 doped with La (Ca3-xLaxRh4Sn13) or Ce (Ca3-xCexRh4Sn13) with superconducting critical temperatures T? c higher than those (Tc) observed in the parent compounds. The T - x diagrams and the entropy S(x)T isotherms well document the relation between degree of an atomic disorder and separation of the high-temperature T*c and Tc-bulk phases. In these dirty superconductors with the mean free path much smaller than the coherence length, the Werthamer-Helfand-Hohenber theoretical model does not well fits the Hc2(T) data. We suggest that this can result from two-band superconductivity or from the presence of strong inhomogeneity in these systems. The multiband model very well describes the H - T dependencies, but the present results as well as our previous studies give arguments for the scenario based on the presence of nanoscopic inhomogeneity of the superconducting state. We also revisited the nature of structural phase transition at T*∼ 130 - 170 K and documented that there might be another precursor transition at higher temperatures. The impact of the magnetic Ce-Ce correlations on the increase of Tc in respect to the critical temperatures of Ca3-xLaxRh4Sn13 is also discussed. Copyright © 2018, The Authors. All rights reserved.

关键词： Electronic structure

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A generalized family of anisotropic compact object in general relativity

arXiv

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arXiv 2017年

作者： Maurya, S.K. Ray, Saibal Ghosh, Shounak Manna, Sarbajit Smitha, T.T. Department of Mathematical and Physical Sciences College of Arts and Science University of Nizwa Nizwa Oman Department of Physics Government College of Engineering & Ceramic Technology KolkataWest Bengal700010 India Department of Physics Indian Institute of Engineering Science and Technology Shibpur HowrahWest Bengal711103 India Department of Materials Engineering Indian Institute of Science BangaloreKarnataka560012 India

We present model for anisotropic compact star under the general theory of relativity of Einstein. In the study a 4-dimensional spacetime has been considered which is embedded into the 5-dimensional flat metric so that the spherically symmetric metric has class 1. A set of solutions for the field equations are found depending on the index n involved in the physical parameters. The interior solutions have been matched smoothly at the boundary of the spherical distribution to the exterior Schwarzschild solution which necessarily provides values of the unknown constants. We have chosen the values of n as n = 2 and n=10 to 20000 for which interesting and physically viable results can be found out. The investigations on the physical features of the model include several astrophysical issues, like (i) regularity behavior of stars at the centre, (ii) well behaved condition for velocity of sound, (iii) energy conditions, (iv) stabilty of the system via the following three techniques - adiabatic index, Herrera cracking concept and TOV equation, (v) total mass, effective mass and compactification factor and (vi) surface redshift. Specific numerical values of the compact star candidates LMC X-4 and SMC X-1 are calculated for central and surface densities as well as central pressure to compare the model value with actual observational data. Copyright © 2017, The Authors. All rights reserved.

关键词： Relativity

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Organosilica: Mesoporous Organosilica Hollow Nanoparticles: Synthesis and Applications (Adv. Mater. 38/2019)

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Advanced materials 2019年第38期31卷

作者： Zhaogang Teng Wei Li Yuxia Tang Ahmed Elzatahry Guangming Lu Dongyuan Zhao Department of Medical Imaging Jinling Hospital School of Medicine Nanjing University Nanjing 210002 Jiangsu P.R. China State Key Laboratory of Analytical Chemistry for Life Science School of Chemistry and Chemical Engineering Nanjing University Nanjing 210093 Jiangsu P.R. China Department of Chemistry Laboratory of Advanced Materials and iChEM Fudan University Shanghai 200433 P.R. China Materials Science and Technology Program College of Arts and Sciences Qatar University Doha 2713 Qatar

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2D Transition Metal Dichalcogenide: Unraveling High-Yield Phase-Transition Dynamics in Transition Metal Dichalcogenides on Metallic Substrates (Adv. Sci. 7/2019)

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Advanced science 2019年第7期6卷 1970042-1970042页

作者： Xinmao Yin Chi Sin Tang Di Wu Weilong Kong Changjian Li Qixing Wang Liang Cao Ming Yang Yung-Huang Chang Dianyu Qi Fangping Ouyang Stephen J. Pennycook Yuan Ping Feng Mark B. H. Breese Shi Jie Wang Wenjing Zhang Andrivo Rusydi Andrew T. S. Wee Department of Physics Faculty of Science National University of Singapore Singapore 117542 Singapore Singapore Synchrotron Light Source (SSLS) National University of Singapore Singapore 117603 Singapore NUS Graduate School for Integrative Sciences and Engineering National University of Singapore Singapore 117456 Singapore International Collaborative Laboratory of 2D Materials for Optoelectronics Science and Technology Shenzhen University Shenzhen 518060 China Hunan Key Laboratory of Super-microstructure and Ultrafast Process School of Physics and Electronics Central South University No. 932 South Lushan Road Changsha Hunan Province 410083 China Department of Materials Science and Engineering National University of Singapore 9 Engineering Drive 1 Singapore 117575 Singapore Anhui Province Key Laboratory of Condensed Matter Physics at Extreme Conditions High Magnetic Field Laboratory of the Chinese Academy of Sciences Hefei 230031 China Institute of Materials Research and Engineering A∗STAR (Agency for Science Technology and Research) 2 Fusionopolis Way Singapore 138634 Singapore Bachelor Program in Interdisciplinary Studies National Yunlin University of Science and Technology Yunlin 640 Taiwan

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Measurements of the temperature and E-mode polarization of the cosmic microwave background from the full 500-square-degree SPTpol dataset

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Physical Review D 2025年第12期111卷 123513-123513页

作者： T.-L. Chou P. A. R. Ade A. J. Anderson J. E. Austermann L. Balkenhol J. A. Beall A. N. Bender B. A. Benson F. Bianchini L. E. Bleem J. E. Carlstrom C. L. Chang P. Chaubal H. C. Chiang R. Citron C. Corbett Moran T. M. Crawford A. T. Crites T. de Haan M. A. Dobbs D. Dutcher W. Everett J. Gallicchio E. M. George N. Gupta N. W. Halverson G. P. Holder W. L. Holzapfel J. D. Hrubes N. Huang J. Hubmayr K. D. Irwin L. Knox A. T. Lee D. Li A. Lowitz J. J. McMahon J. Montgomery T. Natoli J. P. Nibarger G. I. Noble V. Novosad Y. Omori S. Padin S. Patil C. Pryke W. Quan C. L. Reichardt J. E. Ruhl B. R. Saliwanchik K. K. Schaffer C. Sievers G. Smecher A. A. Stark C. Tucker T. Veach J. D. Vieira G. Wang N. Whitehorn W. L. K. Wu V. Yefremenko J. A. Zebrowski Department of Astronomy and Astrophysics University of Chicago 5640 South Ellis Avenue Chicago Illinois 60637 USA Kavli Institute for Cosmological Physics University of Chicago 5640 South Ellis Avenue Chicago Illinois 60637 USA Cardiff University Cardiff CF10 3XQ United Kingdom Fermi National Accelerator Laboratory MS209 P.O. Box 500 Batavia Illinois 60510 USA NIST Quantum Devices Group 325 Broadway Mailcode 817.03 Boulder Colorado 80305 USA Department of Physics University of Colorado Boulder Colorado 80309 USA Sorbonne Universit’e CNRS UMR 7095 Institut d’Astrophysique de Paris 98 bis bd Arago 75014 Paris France High Energy Physics Division Argonne National Laboratory 9700 South Cass Avenue Argonne Illinois 60439 USA SLAC National Accelerator Laboratory 2575 Sand Hill Road Menlo Park California 94025 USA Department of Physics University of Chicago 5640 South Ellis Avenue Chicago Illinois 60637 USA Enrico Fermi Institute University of Chicago 5640 South Ellis Avenue Chicago Illinois 60637 USA School of Physics University of Melbourne Parkville Victoria 3010 Australia Department of Physics McGill University 3600 Rue University Montreal Quebec H3A 2T8 Canada School of Mathematics Statistics and Computer Science University of KwaZulu-Natal Durban South Africa University of Chicago 5640 South Ellis Avenue Chicago Illinois 60637 USA Jet Propulsion Laboratory Pasadena California 91109 USA Department of Physics Cornell University Ithaca New York USA Department of Astronomy Cornell University Ithaca New York USA Department of Physics University of California Berkeley California 94720 USA Physics Division Lawrence Berkeley National Laboratory Berkeley California 94720 USA High Energy Accelerator Research Organization (KEK) Tsukuba Ibaraki 305-0801 Japan Canadian Institute for Advanced Research CIFAR Program in Gravity and the Extreme Universe Toronto Ontario M5G 1Z8 Canada Joseph Henry Laboratories of Physics Jadwin Hall Princ

Using the full four-year SPTpol 500 deg2 dataset in both the 95 and 150 GHz frequency bands, we present measurements of the temperature and E-mode polarization of the cosmic microwave background (CMB), as well as the E-mode polarization autopower spectrum (EE) and temperature-E-mode cross-power spectrum (TE) in the angular multipole range 50<ℓ<8000. We find the SPTpol dataset to be self-consistent, passing several internal consistency tests based on maps, frequency bands, bandpowers, and cosmological parameters. The full SPTpol dataset is well-fit by the ΛCDM model, for which we find H0=70.48±2.16 km s−1 Mpc−1 and Ωm=0.271±0.026, when using only the SPTpol data and a Planck-based prior on the optical depth to reionization. The ΛCDM parameter constraints are consistent across the 95 GHz-only, 150 GHz-only, TE-only, and EE-only data splits. Between the ℓ<1000 and ℓ>1000 data splits, the ΛCDM parameter constraints are borderline consistent at the ∼2σ level. This consistency improves when including a parameter AL, the degree of lensing of the CMB inferred from the smearing of acoustic peaks. When marginalized over AL, the ΛCDM parameter constraints from SPTpol are consistent with those from Planck. The power spectra presented here are the most sensitive measurements of the lensed CMB damping tail to date for roughly ℓ>1700 in TE and ℓ>2000 in EE.

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Magnetism and the spin state in cubic perovskite CaCoO3 synthesized under high pressure

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Physical Review materials 2017年第2期1卷 024406-024406页

作者： Hailiang Xia Jianhong Dai Yuanji Xu Yunyu Yin Xiao Wang Zhehong Liu Min Liu Michael A. McGuire Xiang Li Zongyao Li Changqing Jin Yifeng Yang Jianshi Zhou Youwen Long Beijng National Laboratory for Condensed Matter Physics Institute of Physics Chinese Academy of Sciences Beijing 100190 China School of Physical Sciences University of Chinese Academy of Sciences Beijing 100190 China Materials Science and Technology Division Oak Ridge National Laboratory Oak Ridge Tennessee 37831 USA Materials Science and Engineering Program Department of Mechanical Engineering University of Texas Austin Texas 78712 USA Collaborative Innovation Center of Quantum Matter Beijing 100190 China

Cubic SrCoO3 with an intermediate spin state can only be stabilized by high pressure and high temperature (HPHT) treatment. It is metallic and ferromagnetic with the highest Curie temperature of the transition-metal perovskites. The chemical substitution by Ca on Sr sites would normally lower crystal symmetry from cubic to orthorhombic as seen in the perovskite family of CaMO3 (M=M4+ of transition metals, Ge4+, Sn4+, and Zr4+) at room temperature. This structural change narrows the bandwidth, so as to further enhance the Curie temperature as the crossover to the localized electronic state is approached. We report a successful synthesis of the perovskite CaCoO3 with a HPHT treatment. Surprisingly, CaCoO3 crystallizes in a simple cubic structure that remains stable down to 20 K, the lowest temperature in the structural study. The new perovskite has been thoroughly characterized by a suite of measurements including transport, magnetization, specific heat, thermal conductivity, and thermoelectric power. Metallic CaCoO3 undergoes two successive magnetic transitions at 86 K and 54 K as temperature decreases. The magnetization at 5 K is compatible with the intermediate spin state t4e1 of Co4+ at the octahedral site. The thermal expansion of the Co-O bond length indicates that the population of high spin state t3e2 increases for T>100K. The shortest Co-O bond length in cubic CaCoO3 is responsible for delocalizing electrons in the π*-band and itinerant-electron ferromagnetism at T<54K. A comprehensive comparison between SrCoO3 and CaCoO3 and the justification of their physical properties by first-principles calculation have also been made in this report. Partially filled π* and σ* bands would make CaCoO3 suitable to study the Hund's coupling effect in a metal.

关键词： Antiferromagnetism Chemical bonding Electrical conductivity Ferromagnetism Magnetic interactions Metals Pressure effects Perovskites Transition metal alloys

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