检索结果-内蒙古大学图书馆

Higher-order correlations between different moments of two flow amplitudes in Pb-Pb collisions at sNN=5.02 TeV

Physical Review C 2023年第5期108卷 055203-055203页

作者： S. Acharya D. Adamová A. Adler G. Aglieri Rinella M. Agnello N. Agrawal Z. Ahammed S. Ahmad S. U. Ahn I. Ahuja A. Akindinov M. Al-Turany D. Aleksandrov B. Alessandro H. M. Alfanda R. Alfaro Molina B. Ali A. Alici N. Alizadehvandchali A. Alkin J. Alme G. Alocco T. Alt I. Altsybeev M. N. Anaam C. Andrei A. Andronic V. Anguelov F. Antinori P. Antonioli N. Apadula L. Aphecetche H. Appelshäuser C. Arata S. Arcelli M. Aresti R. Arnaldi J. G. M. C. A. Arneiro I. C. Arsene M. Arslandok A. Augustinus R. Averbeck M. D. Azmi A. Badalà J. Bae Y. W. Baek X. Bai R. Bailhache Y. Bailung A. Balbino A. Baldisseri B. Balis D. Banerjee Z. Banoo R. Barbera F. Barile L. Barioglio M. Barlou G. G. Barnaföldi L. S. Barnby V. Barret L. Barreto C. Bartels K. Barth E. Bartsch N. Bastid S. Basu G. Batigne D. Battistini B. Batyunya D. Bauri J. L. Bazo Alba I. G. Bearden C. Beattie P. Becht D. Behera I. Belikov A. D. C. Bell Hechavarria F. Bellini R. Bellwied S. Belokurova G. Bencedi S. Beole A. Bercuci Y. Berdnikov A. Berdnikova L. Bergmann M. G. Besoiu L. Betev P. P. Bhaduri A. Bhasin M. A. Bhat B. Bhattacharjee L. Bianchi N. Bianchi J. Bielčík J. Bielčíková J. Biernat A. P. Bigot A. Bilandzic G. Biro S. Biswas N. Bize J. T. Blair D. Blau M. B. Blidaru N. Bluhme C. Blume G. Boca F. Bock T. Bodova A. Bogdanov S. Boi J. Bok L. Boldizsár M. Bombara P. M. Bond G. Bonomi H. Borel A. Borissov A. G. Borquez Carcamo H. Bossi E. Botta Y. E. M. Bouziani L. Bratrud P. Braun-Munzinger M. Bregant M. Broz G. E. Bruno M. D. Buckland D. Budnikov H. Buesching S. Bufalino P. Buhler Z. Buthelezi A. Bylinkin S. A. Bysiak M. Cai H. Caines A. Caliva E. Calvo Villar J. M. M. Camacho P. Camerini F. D. M. Canedo M. Carabas A. A. Carballo F. Carnesecchi R. Caron L. A. D. Carvalho J. Castillo Castellanos F. Catalano C. Ceballos Sanchez I. Chakaberia P. Chakraborty S. Chandra S. Chapeland M. Chartier S. Chattopadhyay T. G. Chavez T. Cheng C. Cheshkov B. Cheynis V. Chibante Barroso D. D. Chinellato E. S. Chizzali J. Cho S. Cho P. Chochula P. Christakoglou C. H. Christe Université Clermont Auvergne CNRS/IN2P3 LPC Clermont-Ferrand France Nuclear Physics Institute of the Czech Academy of Sciences Husinec-Řež Czech Republic Fachbereich Informatik und Mathematik Johann-Wolfgang-Goethe Universität Frankfurt Institut für Informatik Frankfurt Germany European Organization for Nuclear Research (CERN) Geneva Switzerland Dipartimento DISAT del Politecnico and Sezione INFN Turin Italy INFN Sezione di Bologna Bologna Italy Variable Energy Cyclotron Centre Homi Bhabha National Institute Kolkata India Department of Physics Aligarh Muslim University Aligarh India Korea Institute of Science and Technology Information Daejeon Republic of Korea Faculty of Science P.J. Šafárik University Košice Slovak Republic Affiliated with an institute covered by a cooperation agreement with CERN Research Division and ExtreMe Matter Institute EMMI GSI Helmholtzzentrum für Schwerionenforschung GmbH Darmstadt Germany INFN Sezione di Torino Turin Italy Central China Normal University Wuhan China Instituto de Física Universidad Nacional Autónoma de México Mexico City Mexico Dipartimento di Fisica e Astronomia dell'Università and Sezione INFN Bologna Italy University of Houston Houston Texas USA Department of Physics and Technology University of Bergen Bergen Norway INFN Sezione di Cagliari Cagliari Italy Institut für Kernphysik Johann Wolfgang Goethe-Universität Frankfurt Frankfurt Germany Horia Hulubei National Institute of Physics and Nuclear Engineering Bucharest Romania Institut für Kernphysik Westfälische Wilhelms-Universität Münster Münster Germany Physikalisches Institut Ruprecht-Karls-Universität Heidelberg Heidelberg Germany INFN Sezione di Padova Padova Italy Lawrence Berkeley National Laboratory Berkeley California USA SUBATECH IMT Atlantique Nantes Université CNRS-IN2P3 Nantes France Laboratoire de Physique Subatomique et de Cosmologie Université Grenoble-Alpes CNRS-IN2P3 Grenoble France Universidade de São Paulo (USP) São Paulo

The correlations between different moments of two flow amplitudes, extracted with the recently developed asymmetric cumulants, are measured in Pb-Pb collisions at sNN=5.02TeV recorded by the ALICE detector at the CERN Large Hadron Collider. The magnitudes of the measured observables show a dependence on the different moments as well as on the collision centrality, indicating the presence of nonlinear response in all even moments up to the eighth. Furthermore, the higher-order asymmetric cumulants show different signatures than the symmetric and lower-order asymmetric cumulants. Comparisons with state-of-the-art event generators using two different parametrizations obtained from Bayesian optimization show differences between data and simulations in many of the studied observables, indicating a need for further tuning of the models behind those event generators. These results provide new and independent constraints on the initial conditions and transport properties of the system created in heavy-ion collisions.

关键词： Hadron-hadron interactions Particle correlations & fluctuations Relativistic heavy-ion collisions

来源：评论

学校读者我要写书评

暂无评论

Characterization of K2-167 b and CALM, a new stellar activity mitigation method

arXiv

引用

arXiv 2024年

作者： de Beurs, Zoë L. Vanderburg, Andrew Thygesen, Erica Rodriguez, Joseph E. Dumusque, Xavier Mortier, Annelies Malavolta, Luca Buchhave, Lars A. Shallue, Christopher J. Zieba, Sebastian Kreidberg, Laura Livingston, John H. Haywood, R.D. Latham, David W. López-Morales, Mercedes Silva, André M. Department of Earth Atmospheric and Planetary Sciences Massachusetts Institute of Technology CambridgeMA02139 United States NSF Graduate Research Fellow MIT Presidential Fellow United States Department of Physics Kavli Institute for Astrophysics and Space Research Massachusetts Institute of Technology CambridgeMA02139 United States Center for Data Intensive and Time Domain Astronomy Department of Physics and Astronomy Michigan State University East LansingMI48824 United States Observatoire de Genève Université de Genève 51 chemin des Maillettes Versoix1290 Switzerland School of Physics & Astronomy University of Birmingham Edgbaston BirminghamB15 2TT United Kingdom Dipartimento di Fisica e Astronomia "Galileo Galilei" Universitá di Padova Vicolo del l’Osservatorio 3 PadovaI-35122 Italy INAF Osservatorio Astronomico di Padova Vicolo dell’Osservatorio 5 Padova35122 Italy DTU Space National Space Institute Technical University of Denmark Elektrovej 328 Kgs. LyngbyDK-2800 Denmark Center for Astrophysics | Harvard & Smithsonian 60 Garden St CambridgeMA02138 United States Max-Planck-Institut für Astronomie Königstuhl 17 HeidelbergD-69117 Germany Leiden Observatory Leiden University Niels Bohrweg 2 Leiden2333CA Netherlands Astrobiology Center 2-21-1 Osawa Mitaka Tokyo181-8588 Japan National Astronomical Observatory of Japan 2-21-1 Osawa Mitaka Tokyo181-8588 Japan Astronomical Science Program Graduate University for Advanced Studies SOKENDAI 2-21-1 Osawa Mitaka Tokyo181-8588 Japan Astrophysics Group University of Exeter ExeterEX4 2QL United Kingdom STFC Ernest Rutherford Fellow United Kingdom Departamento de Fisica e Astronomia Faculdade de Ciencias Universidade do Porto Rua do Campo Alegre Porto4169-007 Portugal Instituto de Astrofisica e Ciencias do Espaco Universidade do Porto CAUP Rua das Estrelas Porto4150-762 Portugal Quad Fellow

We report precise radial velocity (RV) observations of HD 212657 (= K2-167), a star shown by K2 to host a transiting sub-Neptune-sized planet in a 10 day orbit. Using Transiting Exoplanet Survey Satellite (TESS) photometry, we refined the planet parameters, especially the orbital period. We collected 74 precise RVs with the HARPS-N spectrograph between August 2015 and October 2016. Although this planet was first found to transit in 2015 and validated in 2018, excess RV scatter originally limited mass measurements. Here, we measure a mass by taking advantage of reductions in scatter from updates to the HARPS-N Data Reduction System (2.3.5) and our new activity mitigation method called CCF Activity Linear Model (CALM), which uses activity-induced line shape changes in the spectra without requiring timing information. Using the CALM framework, we performed a joint fit with RVs and transits using EXOFASTv2 and find Mp = 6.3+1.4−1.4 M◦ and Rp = 2.33+0.17−0.15 R◦, which places K2-167 b at the upper edge of the radius valley. We also find hints of a secondary companion at a ∼ 22 day period, but confirmation requires additional RVs. Although characterizing lower-mass planets like K2-167 b is often impeded by stellar variability, these systems especially help probe the formation physics (i.e. photoevaporation, core-powered mass loss) of the radius valley. In the future, CALM or similar techniques could be widely applied to FGK-type stars, help characterize a population of exoplanets surrounding the radius valley, and further our understanding of their formation. © 2024, CC BY.

关键词： Stars

来源：评论

学校读者我要写书评

暂无评论

Light (anti)nuclei production in Pb-Pb collisions at sNN=5.02 TeV

引用

Physical Review C 2023年第6期107卷 064904-064904页

作者： S. Acharya D. Adamová A. Adler G. Aglieri Rinella M. Agnello N. Agrawal Z. Ahammed S. Ahmad S. U. Ahn I. Ahuja A. Akindinov M. Al-Turany D. Aleksandrov B. Alessandro H. M. Alfanda R. Alfaro Molina B. Ali A. Alici N. Alizadehvandchali A. Alkin J. Alme G. Alocco T. Alt I. Altsybeev M. N. Anaam C. Andrei A. Andronic V. Anguelov F. Antinori P. Antonioli N. Apadula L. Aphecetche H. Appelshäuser C. Arata S. Arcelli M. Aresti R. Arnaldi J. G. M. C. A. Arneiro I. C. Arsene M. Arslandok A. Augustinus R. Averbeck M. D. Azmi A. Badalà J. Bae Y. W. Baek X. Bai R. Bailhache Y. Bailung A. Balbino A. Baldisseri B. Balis D. Banerjee Z. Banoo R. Barbera F. Barile L. Barioglio M. Barlou G. G. Barnaföldi L. S. Barnby V. Barret L. Barreto C. Bartels K. Barth E. Bartsch N. Bastid S. Basu G. Batigne D. Battistini B. Batyunya D. Bauri J. L. Bazo Alba I. G. Bearden C. Beattie P. Becht D. Behera I. Belikov A. D. C. Bell Hechavarria F. Bellini R. Bellwied S. Belokurova V. Belyaev G. Bencedi S. Beole A. Bercuci Y. Berdnikov A. Berdnikova L. Bergmann M. G. Besoiu L. Betev P. P. Bhaduri A. Bhasin M. A. Bhat B. Bhattacharjee L. Bianchi N. Bianchi J. Bielčík J. Bielčíková J. Biernat A. P. Bigot A. Bilandzic G. Biro S. Biswas N. Bize J. T. Blair D. Blau M. B. Blidaru N. Bluhme C. Blume G. Boca F. Bock T. Bodova A. Bogdanov S. Boi J. Bok L. Boldizsár A. Bolozdynya M. Bombara P. M. Bond G. Bonomi H. Borel A. Borissov A. G. Borquez Carcamo H. Bossi E. Botta Y. E. M. Bouziani L. Bratrud P. Braun-Munzinger M. Bregant M. Broz G. E. Bruno M. D. Buckland D. Budnikov H. Buesching S. Bufalino O. Bugnon P. Buhler Z. Buthelezi S. A. Bysiak M. Cai H. Caines A. Caliva E. Calvo Villar J. M. M. Camacho P. Camerini F. D. M. Canedo M. Carabas A. A. Carballo F. Carnesecchi R. Caron L. A. D. Carvalho J. Castillo Castellanos F. Catalano C. Ceballos Sanchez I. Chakaberia P. Chakraborty S. Chandra S. Chapeland M. Chartier S. Chattopadhyay T. G. Chavez T. Cheng C. Cheshkov B. Cheynis V. Chibante Barroso D. D. Chinellato E. S. Chizzali J. Cho S. Cho P. Chochula P. Chri Université Clermont Auvergne CNRS/IN2P3 LPC Clermont-Ferrand France Nuclear Physics Institute of the Czech Academy of Sciences Husinec-Řež Czech Republic Fachbereich Informatik und Mathematik Johann-Wolfgang-Goethe Universität Frankfurt Institut für Informatik Frankfurt Germany European Organization for Nuclear Research (CERN) Geneva Switzerland Dipartimento DISAT del Politecnico and Sezione INFN Turin Italy INFN Sezione di Bologna Bologna Italy Variable Energy Cyclotron Centre Homi Bhabha National Institute Kolkata India Department of Physics Aligarh Muslim University Aligarh India Korea Institute of Science and Technology Information Daejeon Republic of Korea Faculty of Science P. J. Šafárik University Košice Slovak Republic Affiliated with an institute covered by a cooperation agreement with CERN Research Division and ExtreMe Matter Institute EMMI GSI Helmholtzzentrum für Schwerionenforschung GmbH Darmstadt Germany INFN Sezione di Torino Turin Italy Central China Normal University Wuhan China Instituto de Física Universidad Nacional Autónoma de México Mexico City Mexico Dipartimento di Fisica e Astronomia dell'Università and Sezione INFN Bologna Italy University of Houston Houston Texas USA Department of Physics and Technology University of Bergen Bergen Norway INFN Sezione di Cagliari Cagliari Italy Institut für Kernphysik Johann Wolfgang Goethe-Universität Frankfurt Frankfurt Germany Horia Hulubei National Institute of Physics and Nuclear Engineering Bucharest Romania Westfälische Wilhelms-Universität Münster Institut für Kernphysik Münster Germany Physikalisches Institut Ruprecht-Karls-Universität Heidelberg Heidelberg Germany INFN Sezione di Padova Padova Italy Lawrence Berkeley National Laboratory Berkeley California USA SUBATECH IMT Atlantique Nantes Université CNRS-IN2P3 Nantes France Laboratoire de Physique Subatomique et de Cosmologie Université Grenoble-Alpes CNRS-IN2P3 Grenoble France Universidade de São Paulo (USP) São Paul

The measurement of the production of deuterons, tritons and He3 and their antiparticles in Pb-Pb collisions at sNN=5.02TeV is presented in this article. The measurements are carried out at midrapidity (|y|< 0.5) as a function of collision centrality using the ALICE detector. The pT-integrated yields, the coalescence parameters and the ratios to protons and antiprotons are reported and compared with nucleosynthesis models. The comparison of these results in different collision systems at different center-of-mass collision energies reveals a suppression of nucleus production in small systems. In the Statistical Hadronisation Model framework, this can be explained by a small correlation volume where the baryon number is conserved, as already shown in previous fluctuation analyses. However, a different size of the correlation volume is required to describe the proton yields in the same data sets. The coalescence model can describe this suppression by the fact that the wave functions of the nuclei are large and the fireball size starts to become comparable and even much smaller than the actual nucleus at low multiplicities.

关键词： Particle & resonance production Particle correlations & fluctuations Relativistic heavy-ion collisions A ≤ 5

来源：评论

学校读者我要写书评

暂无评论

Effect of synthesis conditions on the electrical resistivity of TiSe2

arXiv

引用

arXiv 2019年

作者： Moya, Jaime M. Huang, C.-L. Choe, Jesse Costin, Gelu Foster, Matthew S. Morosan, E. Applied Physics Program Rice University Department of Physics and Astronomy Rice University Department of Electrical and Computer Engineering Rice University Department of Earth Environmental and Planetary Sciences Rice University

Dilute impurities and growth conditions can drastically affect the transport properties of TiSe2, especially below the charge density wave transition. In this paper, we discuss the effects of cooling rate, annealing time and annealing temperature on the transport properties of TiSe2: slow cooling of polycrystalline TiSe2 post-synthesis drastically increases the low temperature resistivity, which is in contrast to the metallic behavior of single-crystalline TiSe2 due to charge doping from the residual iodine transport agent. A logarithmic increase of resistivity upon cooling and negative magnetoresistance with a sharp cusp around zero field are observed for the first time for the polycrystalline TiSe2 samples, pointing to weak-localization effects due to low dimensionality. Annealing at low temperatures has a similar, but less drastic effect. Furthermore, rapid quenching of the polycrystalline samples from high temperatures freezes in disorder, leading to a decrease in the low temperature resistivity. Copyright © 2019, The Authors. All rights reserved.

关键词： Titanium compounds

来源：评论

学校读者我要写书评

暂无评论

Effect of concentration of trisodium citrate complexing agent on spray-synthesized ZnS thin films

引用

Materials Today: Proceedings 2021年 36卷 133-140页

作者： P.O. Offor S.N. Ude G.M. Whyte F.U. Otung I.G. Madiba AKH Bashir N. Thovhogi B.A. Okorie Fabian I. Ezema Metallurgical and Materials Engineering Department University of Nigeria Nsukka Nigeria Department of Physics and Astronomy University of Nigeria Nsukka Nigeria Nanosciences African Network (NANOAFNET) iThemba LABS-National Research Foundation 1 Old Faure Road Somerset West 7129 P.O. Box 722 Somerset West Western Cape Province South Africa UNESCO-UNISA Africa Chair in Nanosciences/Nanotechnology College of Graduate Studies University of South Africa (UNISA) Muckleneuk Ridge P.O. Box 392 Pretoria South Africa Biomedical Research and Innovation Platform South African Medical Research Council (SAMRC) Private Bag 19070 Tygerberg 7505 Western Cape Province South Africa Department of Physics Faculty of Natural and Applied Sciences Coal City University Enugu Nigeria

Here, we present the effect of molar concentration of trisodium citrate complexant on the solid state attributes of zinc sulphide (ZnS) thin films grown using chemical spray pyrolysis (CSP). The films were synthesized using 0.1 M concentration of ZnCl 2 , 0.1 M concentration of thiourea with addition of 0.01 M, 0.02 M and 0.03 M concentrations of trisodium citrate complexant at 300 °C. The films’ transmittance, band gap, and refractive index are from 55.81% to 82.44%, 3.52 to 3.72 eV and 3.07 to 4.02 respectively. The films possessed cubic and microcrystalline/amorphous structures. The crystallite size of the film deposited with 0.01 M trisodium citrate concentration was 20.454 nm. The surface morphology exhibited separate standing nanodot-like and nanorod-like crystals with increasing molar concentration. Raman spectroscopy revealed C C bond. The Fourier transform infrared (FTIR) spectroscopy showed various bonds inherent in the film with an attendant band edge emissions arising from the photoluminescence (PL) studies. The contact angle disclosed the films’ hydrophilic surface characteristics.

关键词： Chemical spray pyrolysis Zinc sulphide Trisodium-citrate Microcrystalline Band gap

来源：评论

学校读者我要写书评

暂无评论

PRESENT STATUS OF PICOLON PROJECT

arXiv

引用

arXiv 2024年

作者： Fushimi, K. Chernyak, D. Ejiri, H. Hata, K. Hazama, R. Iida, T. Ikeda, H. Imagawa, K. Inoue, K. Ito, H. Kisimoto, T. Koga, M. Kotera, K. Kozlov, A. Kurosawa, S. Nakamura, K. Orito, R. Sakaguchi, A. Sakaue, A. Shima, T. Takaku, Y. Takemoto, Y. Umehara, S. Urano, Y. Yamamoto, Y. Yasuda, K. Yoshida, S. Division of Science and Technology Tokushima University 2-1 Minami Josanajima-cho Tokushima city Tokushima770-8506 Japan Department of Physics and Astronomy University of Alabama TuscaloosaAL35487 United States Research Center for Nuclear Physics Osaka University 10-1 Mihogaoka Ibaraki city Osaka567-0042 Japan Research Center for Neutrino Science Tohoku University 6-3 Aramaki Aza Aoba Aobaku Sendai city Miyagi980-8578 Japan Department of Environmental Science and Technology Osaka Sangyo University 3-1-1 Nakagaito Daito city Osaka574-8530 Japan Faculty of Pure and Applied Sciences University of Tsukuba 1-1-1 Tennoudai Ibaraki Tsukuba city305-8571 Japan I. S. C. Lab. 5-15-24 Torikai Honmachi Settsu city Osaka566-0052 Japan 5-1-5 Kashiwanoha Kashiwa city Chiba277-8583 Japan Department of Physics Faculty of Science and Technology Tokyo University of Science Chiba Noda278-8510 Japan Department of Physics Osaka University 1-1 Machikaneyama-cho Toyonaka city Osaka560-0043 Japan Graduate School of Advanced Technology and Science Tokushima University 2-1 Minami Josanajima-cho Tokushima city Tokushima770-8506 Japan Moscow115409 Russia New Industry Creation Hatchery Center Tohoku University 6-6-10 Aza-Aoba Aramaki Aoba-ku Sendai980-8579 Japan Institute for Materials Research Tohoku University 2-1-1 Katahira Aoba-ku Miyagi Sendai980-8577 Japan Institute of Laser Engineering Osaka University 2-6 Yamadaoka Osaka Suita565-0871 Japan Butsuryo College of Osaka 3-33 Ohtori Kitamachi Nishi ward Sakai city Osaka593-8328 Japan

The existence of cosmic dark matter and neutrino properties are long-standing problems in cosmology and particle physics. These problems have been investigated by using radiation detectors. We will discuss the application of inorganic crystal scintillators to studies on dark matter and neutrino properties. A large volume and high-purity inorganic crystal is a promising detector for investigating dark matter and neutrino. © 2024, CC BY.

关键词： Galaxies

来源：评论

学校读者我要写书评

暂无评论

Day-To-Day Quantification of Changes in Global Lightning Activity Based on Schumann Resonances

引用

Journal of Geophysical Research: Atmospheres 2023年第11期128卷 e2023JD038557-e2023JD038557页

作者： T. Bozóki G. Sátori E. Williams A. Guha Y. Liu P. Steinbach A. Leal M. Herein M. Atkinson C. D. Beggan E. DiGangi A. Koloskov A. Kulak J. LaPierre D. K. Milling J. Mlynarczyk A. Neska A. Potapov T. Raita R. Rawat R. Said A. K. Sinha Y. Yampolski Institute of Earth Physics and Space Science (EPSS) Sopron Hungary Department of Optics and Quantum Electronics University of Szeged Szeged Hungary Department of Geophysics and Space Science Eötvös Loránd University Budapest Hungary Parsons Laboratory Massachusetts Institute of Technology Cambridge MA USA Department of Physics Tripura University Agartala India ELKH-ELTE Space Research Group Budapest Hungary Department of Physics and Langmuir Laboratory New Mexico Institute of Mining and Technology Socorro NM USA Graduate Program in Electrical Engineering Federal University of Pará Belem Brazil ELKH-ELTE Theoretical Physics Research Group Budapest Hungary Department of Theoretical Physics Institute of Physics and Astronomy Eötvös Loránd University Budapest Hungary HeartMath Institute Boulder Creek CA USA British Geological Survey Edinburgh UK Advanced Environmental Monitoring (AEM) Germantown MD USA Department of Physics University of New Brunswick Fredericton NB Canada State Institution National Antarctic Scientific Center of Ukraine Kyiv Ukraine Institute of Electronics AGH University of Science and Technology Krakow Poland Department of Physics University of Alberta Edmonton AB Canada Institute of Geophysics Polish Academy of Sciences Warsaw Poland Institute of Solar-Terrestrial Physics SB RAS Irkutsk Russia Sodankylä Geophysical Observatory University of Oulu Sodankylä Finland Indian Institute of Geomagnetism Navi Mumbai India Vaisala Louisville CO USA Department of Physics School of Science University of Bahrain Zallaq Bahrain Institute of Radio Astronomy National Academy of Sciences of Ukraine Kharkiv Ukraine

The importance of lightning has long been recognized from the point of view of climate-related phenomena. However, the detailed investigation of lightning on global scales is currently hindered by the incomplete and spatially uneven detection efficiency of ground-based global lightning detection networks and by the restricted spatio-temporal coverage of satellite observations. We are developing different methods for investigating global lightning activity based on Schumann resonance (SR) measurements. SRs are global electromagnetic resonances of the Earth-ionosphere cavity maintained by the vertical component of lightning. Since charge separation in thunderstorms is gravity-driven, charge is typically separated vertically in thunderclouds, so every lightning flash contributes to the measured SR field. This circumstance makes SR measurements very suitable for climate-related investigations. In this study, 19 days of global lightning activity in January 2019 are analyzed based on SR intensity records from 18 SR stations and the results are compared with independent lightning observations provided by ground-based (WWLLN, GLD360, and ENTLN) and satellite-based (GLM, LIS/OTD) global lightning detection. Daily average SR intensity records from different stations exhibit strong similarity in the investigated time interval. The inferred intensity of global lightning activity varies by a factor of 2–3 on the time scale of 3–5 days which we attribute to continental-scale temperature changes related to cold air outbreaks from polar regions. While our results demonstrate that the SR phenomenon is a powerful tool to investigate global lightning, it is also clear that currently available technology limits the detailed quantitative evaluation of lightning activity on continental scales. Daily average Schumann resonance intensity is a quasi-global invariant quantity that shows good agreement with global daily stroke rates and thunder hours Global lightning activity can vary by a fa

关键词： global lightning activity Schumann resonances extremely low frequency lightning and climate day-to-day variability

来源：评论

学校读者我要写书评

暂无评论

Perfect intrinsic squeezing at the superradiant phase transition critical point

arXiv

引用

arXiv 2020年

作者： Hayashida, Kenji Makihara, Takuma Peraca, Nicolas Marquez Padilla, Diego Fallas Pu, Han Kono, Junichiro Bamba, Motoaki Department of Electrical and Computer Engineering Rice University Houston77005 United States Division of Applied Physics Graduate School and Faculty of Engineering Hokkaido University SapporoHokkaido060-8628 Japan Department of Physics and Astronomy Rice University Houston77005 United States Department of Material Science and NanoEngineering Rice University Houston77005 United States Department of Physics Kyoto University Kyoto606-8502 Japan PRESTO Japan Science and Technology Agency Kawaguchi332-0012 Japan

The ground state of the photon–matter coupled system described by the Dicke model is found to be perfectly squeezed at the quantum critical point of the superradiant phase transition (SRPT). In the presence of the counter-rotating photon–atom coupling, the ground state is analytically expressed as a two-mode squeezed vacuum in the basis of photons and atomic collective excitations. The variance of a quantum fluctuation in the two-mode basis vanishes at the SRPT critical point, with its conjugate fluctuation diverging, ideally satisfying the Heisenberg uncertainty principle. Copyright © 2020, The Authors. All rights reserved.

关键词： Photons

来源：评论

学校读者我要写书评

暂无评论

Detection of an Earth-sized exoplanet orbiting the nearby ultracool dwarf star SPECULOOS-3

arXiv

引用

arXiv 2024年

作者： Gillon, Michaël Pedersen, Peter P. Rackham, Benjamin V. Dransfield, Georgina Ducrot, Elsa Barkaoui, Khalid Burdanov, Artem Y. Schroffenegger, Urs Chew, Yilen Gómez Maqueo Lederer, Susan M. Alonso, Roi Burgasser, Adam J. Howell, Steve B. Narita, Norio de Wit, Julien Demory, Brice-Olivier Queloz, Didier Triaud, Amaury H.M.J. Delrez, Laetitia Jehin, Emmanuël Hooton, Matthew J. Garcia, Lionel J. Muñoz, Clàudia Jano Murray, Catriona A. Pozuelos, Francisco J. Sebastian, Daniel Timmermans, Mathilde Thompson, Samantha J. Zúñiga-Fernández, Sebastián Aceituno, Jesús Aganze, Christian Amado, Pedro J. Baycroft, Thomas Benkhaldoun, Zouhair Berardo, David Bolmont, Emeline Clark, Catherine A. Davis, Yasmin T. Davoudi, Fatemeh de Beurs, Zoë L. de Leon, Jerome P. Ikoma, Masahiro Ikuta, Kai Isogai, Keisuke Fukuda, Izuru Fukui, Akihiko Gerasimov, Roman Ghachoui, Mourad Günther, Maximilian N. Hasler, Samantha Hayashi, Yuya Heng, Kevin Hu, Renyu Kagetani, Taiki Kawai, Yugo Kawauchi, Kiyoe Kitzmann, Daniel Koll, Daniel D.B. Lendl, Monika Livingston, John H. Lyu, Xintong Meier Valdés, Erik A. Mori, Mayuko McCormac, James J. Murgas, Felipe Niraula, Prajwal Pallé, Enric Plauchu-Frayn, Ilse Rebolo, Rafael Sabin, Laurence Schackey, Yannick Schanche, Nicole Selsis, Franck Sota, Alfredo Stalport, Manu Standing, Matthew R. Stassun, Keivan G. Tamura, Motohide Theissen, Christopher A. Turbet, Martin Van Grootel, Valérie Varas, Roberto Watanabe, Noriharu Lang, Francis Zong Astrobiology Research Unit Université de Liège Allée du 6 août 19 Liège4000 Belgium Cavendish Laboratory JJ Thomson Avenue CambridgeCB3 0HE United Kingdom Department of Physics ETH Zurich Wolfgang-Pauli-Strasse 2 ZurichCH-8093 Switzerland Department of Earth Atmospheric and Planetary Science Massachusetts Institute of Technology 77 Massachusetts Avenue CambridgeMA02139 United States Kavli Institute for Astrophysics and Space Research Massachusetts Institute of Technology CambridgeMA United States School of Physics & Astronomy University of Birmingham Edgbaston BirminghamB15 2TT United Kingdom LESIA Observatoire de Paris CNRS Université Paris Diderot Université Pierre et Marie Curie 5 place Jules Janssen Meudon92190 France Calle Vía Láctea s/n Tenerife La Laguna38200 Spain Center for Space and Habitability University of Bern Gesellschaftsstrasse 6 BernCH-3012 Switzerland Instituto de Astronomía Universidad Nacional Autónoma de México Ciudad Universitaria Ciudad de México04510 Mexico NASA Johnson Space Center 2101 NASA Parkway HoustonTX77058 United States Departamento de Astrofísica Universidad de La Laguna Astrofísico Francisco Sánchez s/n Tenerife La Laguna38206 Spain Department of Astronomy & Astrophysics University of California San Diego La Jolla San DiegoCA92093 United States NASA Ames Research Center Moffett FieldCA94035 United States Komaba Institute for Science The University of Tokyo 3-8-1 Komaba Meguro Tokyo153-8902 Japan Astrobiology Center 2-21-1 Osawa Mitaka Tokyo181-8588 Japan Institute Université de Liège Allée du 6 Août 19C LiègeB-4000 Belgium Institute of Astronomy KU Leuven Celestijnenlaan 200D Leuven3001 Belgium Center for Computational Astrophysics Flatiron Institute 162 Fifth Avenue New YorkNY10010 United States Department of Astrophysical and Planetary Sciences University of Colorado Boulder BoulderCO80309 United States Glorieta de la Astronomía s/n GranadaE-18008 Spain Centro Astro

Located at the bottom of the main-sequence, ultracool dwarf stars are widespread in the solar neighborhood. Nevertheless, their extremely low luminosity has left their planetary population largely unexplored, and only one of them, TRAPPIST-1, has so far been found to host a transiting planetary system. In this context, we present the SPECULOOS project’s detection of an Earth-sized planet in a 17-hour orbit around an ultracool dwarf of M6.5 spectral type located 16.8 parsecs away. The planet’s high irradiation (16 times that of Earth) combined with the infrared luminosity and Jupiter-like size of its host star make it one of the most promising rocky exoplanets for detailed emission spectroscopy characterization with JWST. Indeed, our sensitivity study shows that just 10 secondary eclipse observations with the Mid-InfraRed Instrument Low-Resolution Spectrometer on board JWST should bring strong constraints on its atmospheric composition and/or surface mineralogy. © 2024, CC BY.

关键词： Emission spectroscopy

来源：评论

学校读者我要写书评

暂无评论

State conversion and resource measures in general quantum resource theories

arXiv

引用

arXiv 2020年

作者： Kuroiwa, Kohdai Yamasaki, Hayata Institute for Quantum Computing Department of Physics and Astronomy University of Waterloo WaterlooONN2L 3G1 Canada Department of Applied Physics Graduate School of Engineering University of Tokyo 7–3–1 Hongo Bunkyo-ku Tokyo113–8656 Japan Photon Science Center Graduate School of Engineering University of Tokyo 7–3–1 Hongo Bunkyo-kuTokyo113–8656 Japan

Quantum resource theories (QRTs) provide a unified theoretical framework for understanding inherent quantum-mechanical properties that serve as resources in quantum information processing, but resources motivated by physics may possess intractable mathematical structure to analyze, such as non-uniqueness of maximally resourceful states, lack of convexity, and infinite dimension. We investigate state conversion and resource measures in general QRTs under minimal assumptions to figure out universal properties of physically motivated quantum resources that may have such intractable mathematical structure. In the general setting, we prove the existence of maximally resourceful states in one-shot state conversion. Also analyzing asymptotic state conversion, we discover catalytic replication of quantum resources, where a resource state is infinitely replicable by free operations. In QRTs without assuming uniqueness of maximally resourceful states, we formulate the tasks of distillation and formation of quantum resources, and introduce distillable resource and resource cost based on the distillation and the formation, respectively. Furthermore, we introduce consistent resource measures that quantify the amount of quantum resources without contradicting the rate of state conversion even in QRTs with non-unique maximally resourceful states. Progressing beyond the previous work showing a uniqueness theorem for additive resource measures, we prove the corresponding uniqueness inequality for the consistent resource measures;that is, consistent resource measures of a quantum state take values between the distillable resource and the resource cost of the state. These formulations and results establish a foundation of QRTs applicable to mathematically intractable but physically motivated quantum resources in a unified way. Copyright © 2020, The Authors. All rights reserved.

关键词： Distillation

来源：评论

学校读者我要写书评

暂无评论

建议与咨询留下您的常用邮箱和电话号码，以便我们向您反馈解决方案和替代方法

时间限定

文献类型

馆藏选择

核心期刊

语言

文献类型

帮助

文字说明：

检索规则说明：

检索范例：

分类表

所选分类

限定检索结果

文献类型

馆藏范围

日期分布

学科分类号

主题

机构

作者

语言

请选择保存的检索档案：

请选择收藏分类：

通借通还

建议与咨询 留下您的常用邮箱和电话号码，以便我们向您反馈解决方案和替代方法

时间限定

文献类型

馆藏选择

核心期刊

语言

文献类型

帮助

文字说明：

检索规则说明：

检索范例：

分类表

所选分类

限定检索结果

文献类型

馆藏范围

日期分布

学科分类号

主题

机构

作者

语言

请选择保存的检索档案： 新增检索档案 确定 取消

请选择收藏分类： 新增自定义分类 确定 取消

通借通还

建议与咨询留下您的常用邮箱和电话号码，以便我们向您反馈解决方案和替代方法

请选择保存的检索档案：

请选择收藏分类：