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Non-destructive evaluation of a city roadway for pavement rehabilitation: A case study

International Journal of Pavement Research and technology 2017年第7期11卷 667-678页

作者： Chao, Chien-Chiao Lin, deng-Fong Luo, Huan-Lin Wang, Yu-Kai Lo, Wei Ph. D. Program in Engineering Science and Technology College of Engineering National Kaohsiung First University of Science and Technology Kaohsiung City Taiwan Department of Civil and Ecological Engineering I-Shou University Kaohsiung City Taiwan Department of Construction Engineering National Kaohsiung First University of Science and Technology Kaohsiung City Taiwan

In this study, a pavement evaluation was carried out on a corridor that carried heavy truck traffic, connecting a harbor, a major high-way, an airport, and industries. The pavement of the corridor was distressed frequently, requiring constant maintenance. With tight maintenance budget and intention to minimize the effects on traffic, full reconstruction or major rehabilitation of the corridor was not practical. To develop proper pavement rehabilitation design within the practical constrains, pavement evaluation was performed in this study using non-destructive techniques, such as visual condition survey, falling weight deflectometer (FWd), ground penetrating radar (GPR), and dynamic cone penetrometer (dCP), and pavement coring. It is demonstrated that appropriate pavement rehabilitation design can be developed to offer practical solution to the repair/maintenance for city streets. © 2017 Chinese Society of Pavement engineering.

关键词： Ground penetrating radar systems

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Hyperspectral imaging and analysis of swirling flames issued from two and four slots circumferential burners

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IOP Conference Series: Materials science and engineering 2019年第1期610卷

作者： A. A. Saad A. M. Abdulnaim M. M. Ibrahim A. A. Emara H. A. Moneib H. S. Ayoub Ashraf F. El-Sherif Ph.D. student Department of Mechanical Power Engineering Faculty of Engineering at El-Mataria Helwan University Cairo Egypt. Demonstrator Department of Mechanical Power Engineering Faculty of Engineering at El-Mataria Helwan University Cairo Egypt. Demonstrator Department of Mechanical Power Engineering Faculty of Engineering at El-Mataria Helwan University Cairo Egypt Assistant Professor of Combustion and Heat Engines - Helwan University and Energy Engineering and Renewable Energies (ENR) Program Coordinator Department of Mechanical Engineering Faculty of Engineering Bader University in Cairo (BUC) Cairo Egypt Professor of Combustion Department of Mechanical Power Engineering Faculty of Engineering at El-Mataria Helwan University Cairo Egypt Physics Department Faculty of Science Cairo University Egypt Engineering Physics Department Military Technical College Egypt

A spectroscopy and visual investigation for turbulent swirling flames formed by four-circumferential swirling turbojet EV in comparison with a two-circumferential swirling air entries configuration burner using hyper spectral camera. The special design of the EV-burner guarantees flame stabilization at the burner exit by a recirculation of hot gases and entrained fresh reactance mixture. A recirculation zone (vortex breakdown) can be generated when a sufficient strong swirling flow exist. The main parameter of combustion diagnostics based on optical devices is the flame itself, whose spectrum is closely related to the process state, as a fingerprint of the instantaneous operational condition, in terms of energetic yield, fuel consumption and pollutants emissions. The hyperspectral imaging technique in the aspect of flame analysis to give a complete description for the flame zones behavior and distribution of reactions through the whole flame. The spectral peaks for issued flames have been studied to give complete vision for the effect of changing the equivalence ratio and different burner arrangement four and two circumferential swirling entries.

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Early Release science of the exoplanet WASP-39b with JWST NIRCam

arXiv

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arXiv 2022年

作者： Ahrer, Eva-Maria Stevenson, Kevin B. Mansfield, Megan Moran, Sarah E. Brande, Jonathan Morello, Giuseppe Murray, Catriona A. Nikolov, Nikolay K. Petit dit de la Roche, dominique J.M. Schlawin, Everett Wheatley, Peter J. Zieba, Sebastian Batalha, Natasha E. damiano, Mario Goyal, Jayesh M. Lendl, Monika Lothringer, Joshua d. Mukherjee, Sagnick Ohno, Kazumasa Batalha, Natalie M. Battley, Matthew P. Bean, Jacob L. Beatty, Thomas G. Benneke, Björn Berta-Thompson, Zachory K. Carter, Aarynn L. Cubillos, Patricio E. daylan, Tansu Espinoza, Néstor Gao, Peter Gibson, Neale P. Gill, Samuel Harrington, Joseph Hu, Renyu Kreidberg, Laura Lewis, Nikole K. Line, Michael R. López-Morales, Mercedes Parmentier, Vivien Powell, diana K. Sing, david K. Tsai, Shang-Min Wakeford, Hannah R. Welbanks, Luis Alam, Munazza K. Alderson, Lili Allen, Natalie H. Anderson, david R. Barstow, Joanna K. Bayliss, daniel Bell, Taylor J. Blecic, Jasmina Bryant, Edward M. Burleigh, Matthew R. Carone, Ludmila Casewell, S.L. Changeat, Quentin Chubb, Katy L. Crossfield, Ian J.M. Crouzet, Nicolas decin, Leen désert, Jean-Michel Feinstein, Adina d. Flagg, Laura Fortney, Jonathan J. Gizis, John E. Heng, Kevin Iro, Nicolas Kempton, Eliza M.-R. Kendrew, Sarah Kirk, James Knutson, Heather A. Komacek, Thaddeus d. Lagage, Pierre-Olivier Leconte, Jérémy Lustig-Yaeger, Jacob Macdonald, Ryan J. Mancini, Luigi May, E.M. Mayne, N.J. Miguel, Yamila Mikal-Evans, Thomas Molaverdikhani, Karan Palle, Enric Piaulet, Caroline Rackham, Benjamin V. Redfield, Seth Rogers, Laura K. Roy, Pierre-Alexis Rustamkulov, Zafar Shkolnik, Evgenya L. Sotzen, Kristin S. Taylor, Jake Tremblin, P. Tucker, Gregory S. Turner, Jake d. de Val-Borro, Miguel Venot, Olivia Zhang, Xi Centre for Exoplanets and Habitability University of Warwick Coventry United Kingdom Department of Physics University of Warwick Coventry United Kingdom Johns Hopkins APL LaurelMD United States Steward Observatory University of Arizona TucsonAZ United States NHFP Sagan Fellow United States Lunar and Planetary Laboratory University of Arizona TucsonAZ United States Department of Physics & Astronomy University of Kansas LawrenceKS United States Tenerife Spain Tenerife Spain INAF- Palermo Astronomical Observatory Piazza del Parlamento Palermo Italy Department of Astrophysical and Planetary Sciences University of Colorado BoulderCO United States Space Telescope Science Institute BaltimoreMD United States Département d'Astronomie Université de Genève Sauverny Switzerland Max Planck Institute for Astronomy Heidelberg Germany Leiden Observatory University of Leiden Leiden Netherlands NASA Ames Research Center Moffett Field CA United States Jet Propulsion Laboratory PasadenaCA United States HBNI Odisha India Department of Physics Utah Valley University OremUT United States Department of Astronomy & Astrophysics University of California Santa Cruz Santa CruzCA United States Astrobiology Program UC Santa Cruz Santa CruzCA United States Department of Astronomy & Astrophysics University of Chicago ChicagoIL United States Department of Astronomy University of Wisconsin-Madison MadisonWI United States Department of Physics Institute for Research on Exoplanets Université de Montréal MontrealQC Canada Space Research Institute Austrian Academy of Sciences Graz Austria INAF Osservatorio Astrofisico di Torino Pino Torinese Italy Department of Astrophysical Sciences Princeton University PrincetonNJ United States LSSTC Catalyst Fellow Department of Physics & Astronomy Johns Hopkins University BaltimoreMD United States Earth and Planets Laboratory Carnegie Institution for Science WashingtonDC United States School of Physics Trinity Col

Measuring the metallicity and carbon-to-oxygen (C/O) ratio in exoplanet atmospheres is a fundamental step towards constraining the dominant chemical processes at work and, if in equilibrium, revealing planet formation histories. Transmission spectroscopye.g., 1,2 provides the necessary means by constraining the abundances of oxygen- and carbon-bearing species;however, this requires broad wavelength coverage, moderate spectral resolution, and high precision that, together, are not achievable with previous observatories. Now that JWST has commenced science operations, we are able to observe exoplanets at previously uncharted wavelengths and spectral resolutions. Here we report time-series observations of the transiting exoplanet WASP-39b using JWST’s Near InfraRed Camera (NIRCam). The long-wavelength spectroscopic and short-wavelength photometric light curves span 2.0 – 4.0 µm, exhibit minimal systematics, and reveal well-defined molecular absorption features in the planet’s spectrum. Specifically, we detect gaseous H2O in the atmosphere and place an upper limit on the abundance of CH4. The otherwise prominent CO2 feature at 2.8 µm is largely masked by H2O. The best-fit chemical equilibrium models favour an atmospheric metallicity of 1–100× solar (i.e., an enrichment of elements heavier than helium relative to the Sun) and a sub-stellar carbon-to-oxygen (C/O) ratio. The inferred high metallicity and low C/O ratio may indicate significant accretion of solid materials during planet formatione.g., 3,4 or disequilibrium processes in the upper atmospheree.g., 5,6 © 2022, CC BY.

关键词： Spectral resolution

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Root microbiota regulates tiller number in rice

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Cell 2025年第12期188卷 3152-3166.e16页

作者： Zhang, Jingying Wang, Bing Xu, Haoran Liu, Weidong Yu, Jingwei Wang, Qiuxia Yu, Hong Wei, Jin-Wei dai, Rui Zhou, Jinghang He, Yuhang Zou, di Yang, Jinhua Ban, Xinwei Hu, Qingliang Meng, Xiangbing Liu, Yong-Xin Wang, Binglei Hu, Bin Wang, Mingyu Xin, Peiyong Chu, Jinfang Li, Changsheng Garrido-Oter, Ruben Yu, Peng van dijk, Aalt dirk Jan dong, Lemeng Bouwmeester, Harro Gao, Song Huang, Ancheng Chu, Chengcai Li, Jiayang Bai, Yang Institute of Genetics and Developmental Biology Chinese Academy of Sciences Beijing 100101 China Peking-Tsinghua Center for Life Sciences State Key Laboratory of Gene Function and Modulation Research Peking-Tsinghua-NIBS Graduate Program School of Life Sciences Peking University Beijing 100871 China CAS-JIC Centre of Excellence for Plant and Microbial Science Institute of Genetics and Developmental Biology Chinese Academy of Sciences Beijing 100101 China College of Advanced Agricultural Sciences University of Chinese Academy of Sciences Beijing 100101 China Shenzhen Key Laboratory of Plant Genetic Engineering and Molecular Design Institute of Plant and Food Science School of Life Sciences Southern University of Science and Technology Shenzhen 518055 China State Key Laboratory of Oncology in South China Collaborative Innovation Center for Cancer Medicine Integrated Traditional Chinese and Western Medicine Research Center Sun Yat-sen University Cancer Center Guangzhou 510060 China Yazhouwan National Laboratory Sanya 572024 China School of Life Sciences Yunnan University Kunming 650504 China Guangdong Basic Research Center of Excellence for Precise Breeding of Future Crops and Guangdong Laboratory for Lingnan Modern Agriculture South China Agricultural University Guangzhou 510642 China Key Laboratory for Enhancing Resource Use Efficiency of Crops in South China Ministry of Agriculture and Rural Affairs South China Agricultural University Guangzhou 510642 China State Key Laboratory of Chemo/Biosensing and Chemometrics College of Biology Hunan University Changsha 410082 China Department of Plant-Microbe Interactions Max Planck Institute for Plant Breeding Research Cologne 50829 Germany Cluster of Excellence on Plant Sciences (CEPLAS) Düsseldorf 40225 Germany Plant Genetics TUM School of Life Sciences Technical University of Munich Freising 85354 Germany Swammerdam Institute for Life Sciences University of Amsterdam Amsterdam 1098 XH Netherlands

Rice tillering is an important agronomic trait regulated by plant genetic and environmental factors. However, the role and mechanism of the root microbiota in modulating rice tillering have not been explored. Here, we examined the root microbiota composition and tiller numbers of 182 genome-sequenced rice varieties grown under field conditions and uncovered a significant correlation between root microbiota composition and rice tiller number. Using cultivated bacterial isolates, we demonstrated that various members of the root microbiota can regulate rice tillering in both laboratory and field conditions. Genetic, biochemical, and structural analyses revealed that cyclo(Leu-Pro), produced by the tiller-inhibiting bacterium Exiguobacterium R2567, activates the rice strigolactone (SL) signaling pathway by binding to the SL receptor Osd14, thus regulating tillering. The present work provides insight into how the root microbiota regulates key agronomic traits and offers a promising strategy for optimizing crop growth by harnessing the root microbiota in sustainable agriculture. © 2025 The Authors

关键词： cyclo(Leu-Pro) dipeptide field trial microbial cultivation rice root microbiome root microbiota strigolactone pathway tiller number

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All-sky, all-frequency directional search for persistent gravitational waves from Advanced LIGO’s and Advanced Virgo’s first three observing runs

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physical Review d 2022年第12期105卷 122001-122001页

作者： R. Abbott T. d. Abbott F. Acernese K. Ackley C. Adams N. Adhikari R. X. Adhikari V. B. Adya C. Affeldt d. Agarwal M. Agathos K. Agatsuma N. Aggarwal O. d. Aguiar L. Aiello A. Ain P. Ajith T. Akutsu S. Albanesi A. Allocca P. A. Altin A. Amato C. Anand S. Anand A. Ananyeva S. B. Anderson W. G. Anderson M. Ando T. Andrade N. Andres T. Andrić S. V. Angelova S. Ansoldi J. M. Antelis S. Antier S. Appert Koji Arai Koya Arai Y. Arai S. Araki A. Araya M. C. Araya J. S. Areeda M. Arène N. Aritomi N. Arnaud S. M. Aronson K. G. Arun H. Asada Y. Asali G. Ashton Y. Aso M. Assiduo S. M. Aston P. Astone F. Aubin C. Austin S. Babak F. Badaracco M. K. M. Bader C. Badger S. Bae Y. Bae A. M. Baer S. Bagnasco Y. Bai L. Baiotti J. Baird R. Bajpai M. Ball G. Ballardin S. W. Ballmer A. Balsamo G. Baltus S. Banagiri d. Bankar J. C. Barayoga C. Barbieri B. C. Barish d. Barker P. Barneo F. Barone B. Barr L. Barsotti M. Barsuglia d. Barta J. Bartlett M. A. Barton I. Bartos R. Bassiri A. Basti M. Bawaj J. C. Bayley A. C. Baylor M. Bazzan B. Bécsy V. M. Bedakihale M. Bejger I. Belahcene V. Benedetto d. Beniwal T. F. Bennett J. d. Bentley M. BenYaala F. Bergamin B. K. Berger S. Bernuzzi d. Bersanetti A. Bertolini J. Betzwieser d. Beveridge R. Bhandare U. Bhardwaj d. Bhattacharjee S. Bhaumik I. A. Bilenko G. Billingsley S. Bini R. Birney O. Birnholtz S. Biscans M. Bischi S. Biscoveanu A. Bisht B. Biswas M. Bitossi M.-A. Bizouard J. K. Blackburn C. d. Blair d. G. Blair R. M. Blair F. Bobba N. Bode M. Boer G. Bogaert M. Boldrini L. d. Bonavena F. Bondu E. Bonilla R. Bonnand P. Booker B. A. Boom R. Bork V. Boschi N. Bose S. Bose V. Bossilkov V. Boudart Y. Bouffanais A. Bozzi C. Bradaschia P. R. Brady A. Bramley A. Branch M. Branchesi J. E. Brau M. Breschi T. Briant J. H. Briggs A. Brillet M. Brinkmann P. Brockill A. F. Brooks J. Brooks d. d. Brown S. Brunett G. Bruno R. Bruntz J. Bryant T. Bulik H. J. Bulten A. Buonanno R. Buscicchio d. Buskulic C. Buy R. L. Byer L. Cadonati G. Cagnoli C. Cahillane J. Calderón Bustillo J. d. Callaghan T. A. Callis LIGO Laboratory California Institute of Technology Pasadena California 91125 USA Louisiana State University Baton Rouge Louisiana 70803 USA Dipartimento di Farmacia Università di Salerno I-84084 Fisciano Salerno Italy INFN Sezione di Napoli Complesso Universitario di Monte S. Angelo I-80126 Napoli Italy OzGrav School of Physics & Astronomy Monash University Clayton 3800 Victoria Australia LIGO Livingston Observatory Livingston Louisiana 70754 USA University of Wisconsin-Milwaukee Milwaukee Wisconsin 53201 USA OzGrav Australian National University Canberra Australian Capital Territory 0200 Australia Max Planck Institute for Gravitational Physics (Albert Einstein Institute) D-30167 Hannover Germany Leibniz Universität Hannover D-30167 Hannover Germany Inter-University Centre for Astronomy and Astrophysics Pune 411007 India University of Cambridge Cambridge CB2 1TN United Kingdom Theoretisch-Physikalisches Institut Friedrich-Schiller-Universität Jena D-07743 Jena Germany University of Birmingham Birmingham B15 2TT United Kingdom Center for Interdisciplinary Exploration & Research in Astrophysics (CIERA) Northwestern University Evanston Illinois 60208 USA Instituto Nacional de Pesquisas Espaciais 12227-010 São José dos Campos São Paulo Brazil Gravity Exploration Institute Cardiff University Cardiff CF24 3AA United Kingdom INFN Sezione di Pisa I-56127 Pisa Italy International Centre for Theoretical Sciences Tata Institute of Fundamental Research Bengaluru 560089 India Gravitational Wave Science Project National Astronomical Observatory of Japan (NAOJ) Mitaka City Tokyo 181-8588 Japan Advanced Technology Center National Astronomical Observatory of Japan (NAOJ) Mitaka City Tokyo 181-8588 Japan INFN Sezione di Torino I-10125 Torino Italy Università di Napoli “Federico II” Complesso Universitario di Monte S. Angelo I-80126 Napoli Italy Université de Lyon Université Claude Bernard Lyon 1 CNRS Institut Lumière Matière F-69622 Villeurbanne France De

We present the first results from an all-sky all-frequency (ASAF) search for an anisotropic stochastic gravitational-wave background using the data from the first three observing runs of the Advanced LIGO and Advanced Virgo detectors. Upper limit maps on broadband anisotropies of a persistent stochastic background were published for all observing runs of the LIGO-Virgo detectors. However, a broadband analysis is likely to miss narrowband signals as the signal-to-noise ratio of a narrowband signal can be significantly reduced when combined with detector output from other frequencies. data folding and the computationally efficient analysis pipeline, PyStoch, enable us to perform the radiometer map-making at every frequency bin. We perform the search at 3072 HEALPix equal area pixels uniformly tiling the sky and in every frequency bin of width 1/32 Hz in the range 20–1726 Hz, except for bins that are likely to contain instrumental artefacts and hence are notched. We do not find any statistically significant evidence for the existence of narrowband gravitational-wave signals in the analyzed frequency bins. Therefore, we place 95% confidence upper limits on the gravitational-wave strain for each pixel-frequency pair, the limits are in the range (0.030−9.6)×10−24. In addition, we outline a method to identify candidate pixel-frequency pairs that could be followed up by a more sensitive (and potentially computationally expensive) search, e.g., a matched-filtering-based analysis, to look for fainter nearly monochromatic coherent signals. The ASAF analysis is inherently independent of models describing any spectral or spatial distribution of power. We demonstrate that the ASAF results can be appropriately combined over frequencies and sky directions to successfully recover the broadband directional and isotropic results.

关键词： Gravitational wave detection Gravitational waves

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Constraints on dark photon dark matter using data from LIGO’s and Virgo’s third observing run

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physical Review d 2022年第6期105卷 063030-063030页

作者： R. Abbott T. d. Abbott F. Acernese K. Ackley C. Adams N. Adhikari R. X. Adhikari V. B. Adya C. Affeldt d. Agarwal M. Agathos K. Agatsuma N. Aggarwal O. d. Aguiar L. Aiello A. Ain P. Ajith T. Akutsu S. Albanesi A. Allocca P. A. Altin A. Amato C. Anand S. Anand A. Ananyeva S. B. Anderson W. G. Anderson M. Ando T. Andrade N. Andres T. Andrić S. V. Angelova S. Ansoldi J. M. Antelis S. Antier S. Appert Koji Arai Koya Arai Y. Arai S. Araki A. Araya M. C. Araya J. S. Areeda M. Arène N. Aritomi N. Arnaud S. M. Aronson K. G. Arun H. Asada Y. Asali G. Ashton Y. Aso M. Assiduo S. M. Aston P. Astone F. Aubin C. Austin S. Babak F. Badaracco M. K. M. Bader C. Badger S. Bae Y. Bae A. M. Baer S. Bagnasco Y. Bai L. Baiotti J. Baird R. Bajpai M. Ball G. Ballardin S. W. Ballmer A. Balsamo G. Baltus S. Banagiri d. Bankar J. C. Barayoga C. Barbieri B. C. Barish d. Barker P. Barneo F. Barone B. Barr L. Barsotti M. Barsuglia d. Barta J. Bartlett M. A. Barton I. Bartos R. Bassiri A. Basti M. Bawaj J. C. Bayley A. C. Baylor M. Bazzan B. Bécsy V. M. Bedakihale M. Bejger I. Belahcene V. Benedetto d. Beniwal T. F. Bennett J. d. Bentley M. BenYaala F. Bergamin B. K. Berger S. Bernuzzi d. Bersanetti A. Bertolini J. Betzwieser d. Beveridge R. Bhandare U. Bhardwaj d. Bhattacharjee S. Bhaumik I. A. Bilenko G. Billingsley S. Bini R. Birney O. Birnholtz S. Biscans M. Bischi S. Biscoveanu A. Bisht B. Biswas M. Bitossi M.-A. Bizouard J. K. Blackburn C. d. Blair d. G. Blair R. M. Blair F. Bobba N. Bode M. Boer G. Bogaert M. Boldrini L. d. Bonavena F. Bondu E. Bonilla R. Bonnand P. Booker B. A. Boom R. Bork V. Boschi N. Bose S. Bose V. Bossilkov V. Boudart Y. Bouffanais A. Bozzi C. Bradaschia P. R. Brady A. Bramley A. Branch M. Branchesi J. E. Brau M. Breschi T. Briant J. H. Briggs A. Brillet M. Brinkmann P. Brockill A. F. Brooks J. Brooks d. d. Brown S. Brunett G. Bruno R. Bruntz J. Bryant T. Bulik H. J. Bulten A. Buonanno R. Buscicchio d. Buskulic C. Buy R. L. Byer L. Cadonati G. Cagnoli C. Cahillane J. Calderón Bustillo J. d. Callaghan T. A. Callis LIGO Laboratory California Institute of Technology Pasadena California 91125 USA Louisiana State University Baton Rouge Louisiana 70803 USA Dipartimento di Farmacia Università di Salerno I-84084 Fisciano Salerno Italy INFN Sezione di Napoli Complesso Universitario di Monte S. Angelo I-80126 Napoli Italy OzGrav School of Physics and Astronomy Monash University Clayton 3800 Victoria Australia LIGO Livingston Observatory Livingston Louisiana 70754 USA University of Wisconsin-Milwaukee Milwaukee Wisconsin 53201 USA OzGrav Australian National University Canberra Australian Capital Territory 0200 Australia Max Planck Institute for Gravitational Physics (Albert Einstein Institute) D-30167 Hannover Germany Leibniz Universität Hannover D-30167 Hannover Germany Inter-University Centre for Astronomy and Astrophysics Pune 411007 India University of Cambridge Cambridge CB2 1TN United Kingdom Theoretisch-Physikalisches Institut Friedrich-Schiller-Universität Jena D-07743 Jena Germany University of Birmingham Birmingham B15 2TT United Kingdom Center for Interdisciplinary Exploration and Research in Astrophysics (CIERA) Northwestern University Evanston Illinois 60208 USA Instituto Nacional de Pesquisas Espaciais 12227-010 São José dos Campos São Paulo Brazil Gravity Exploration Institute Cardiff University Cardiff CF24 3AA United Kingdom INFN Sezione di Pisa I-56127 Pisa Italy International Centre for Theoretical Sciences Tata Institute of Fundamental Research Bengaluru 560089 India Gravitational Wave Science Project National Astronomical Observatory of Japan (NAOJ) Mitaka City Tokyo 181-8588 Japan Advanced Technology Center National Astronomical Observatory of Japan (NAOJ) Mitaka City Tokyo 181-8588 Japan INFN Sezione di Torino I-10125 Torino Italy Università di Napoli “Federico II” Complesso Universitario di Monte S. Angelo I-80126 Napoli Italy Université de Lyon Université Claude Bernard Lyon 1 CNRS Institut Lumière Matière F-69622 Villeurbanne Franc

We present a search for dark photon dark matter that could couple to gravitational-wave interferometers using data from Advanced LIGO and Virgo’s third observing run. To perform this analysis, we use two methods, one based on cross-correlation of the strain channels in the two nearly aligned LIGO detectors, and one that looks for excess power in the strain channels of the LIGO and Virgo detectors. The excess power method optimizes the Fourier transform coherence time as a function of frequency, to account for the expected signal width due to doppler modulations. We do not find any evidence of dark photon dark matter with a mass between mA∼10−14–10−11 eV/c2, which corresponds to frequencies between 10–2000 Hz, and therefore provide upper limits on the square of the minimum coupling of dark photons to baryons, i.e., U(1)B dark matter. For the cross-correlation method, the best median constraint on the squared coupling is ∼1.31×10−47 at mA∼4.2×10−13 eV/c2; for the other analysis, the best constraint is ∼2.4×10−47 at mA∼5.7×10−13 eV/c2. These limits improve upon those obtained in direct dark matter detection experiments by a factor of ∼100 for mA∼[2–4]×10−13 eV/c2, and are, in absolute terms, the most stringent constraint so far in a large mass range mA∼2×10−13–8×10−12 eV/c2.

关键词： dark matter Gravitational wave detectors

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Jet modification via π0-hadron correlations in Au+Au collisions at sNN=200 GeV

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physical Review C 2024年第4期110卷 044901页

作者： N. J. Abdulameer U. Acharya A. Adare S. Afanasiev C. Aidala N. N. Ajitanand Y. Akiba H. Al-Bataineh J. Alexander M. Alfred K. Aoki N. Apadula L. Aphecetche J. Asai H. Asano E. T. Atomssa R. Averbeck T. C. Awes B. Azmoun V. Babintsev M. Bai G. Baksay L. Baksay A. Baldisseri N. S. Bandara B. Bannier K. N. Barish P. d. Barnes B. Bassalleck A. T. Basye S. Bathe S. Batsouli V. Baublis C. Baumann A. Bazilevsky M. Beaumier S. Beckman S. Belikov R. Belmont R. Bennett A. Berdnikov Y. Berdnikov L. Bichon A. A. Bickley B. Blankenship d. S. Blau J. G. Boissevain J. S. Bok H. Borel V. Borisov K. Boyle M. L. Brooks J. Bryslawskyj H. Buesching V. Bumazhnov G. Bunce S. Butsyk C. M. Camacho S. Campbell B. S. Chang W. C. Chang J. L. Charvet C.-H. Chen d. Chen S. Chernichenko M. Chiu C. Y. Chi I. J. Choi J. B. Choi R. K. Choudhury T. Chujo P. Chung A. Churyn V. Cianciolo Z. Citron B. A. Cole M. Connors P. Constantin R. Corliss M. Csanád T. Csörgő d. d'Enterria T. dahms S. dairaku T. W. danley K. das A. datta M. S. daugherity G. david K. deBlasio K. dehmelt A. denisov A. deshpande E. J. desmond O. dietzsch A. dion P. B. diss M. donadelli V. doomra J. H. do O. drapier A. drees K. A. drees A. K. dubey J. M. durham A. durum d. dutta V. dzhordzhadze Y. V. Efremenko F. Ellinghaus H. En'yo T. Engelmore A. Enokizono R. Esha K. O. Eyser B. Fadem N. Feege d. E. Fields M. Finger, Jr. M. Finger d. Firak d. Fitzgerald F. Fleuret S. L. Fokin Z. Fraenkel J. E. Frantz A. Franz A. d. Frawley K. Fujiwara Y. Fukao T. Fusayasu P. Gallus C. Gal P. Garg I. Garishvili H. Ge F. Giordano A. Glenn H. Gong M. Gonin J. Gosset Y. Goto R. Granier de Cassagnac N. Grau S. V. Greene M. Grosse Perdekamp T. Gunji T. Guo H.-Å. Gustafsson T. Hachiya A. Hadj Henni J. S. Haggerty K. I. Hahn H. Hamagaki H. F. Hamilton J. Hanks R. Han S. Y. Han E. P. Hartouni K. Haruna S. Hasegawa T. O. S. Haseler K. Hashimoto E. Haslum R. Hayano M. Heffner T. K. Hemmick T. Hester X. He J. C. Hill A. Hodges M. Hohlmann R. S. Hollis W. Holzmann K. Homma B. Hong T. Horaguchi d. Hornback T. Debrecen University H-4010 Debrecen Egyetem tér 1 Hungary HUN-REN ATOMKI H-4026 Debrecen Bem tér 18/c Hungary Atlanta Georgia 30303 USA University of Colorado Boulder Colorado 80309 USA Joint Institute for Nuclear Research 141980 Dubna Moscow Region Russia Department of Physics University of Massachusetts Amherst Massachusetts 01003-9337 USA Department of Physics University of Michigan Ann Arbor Michigan 48109-1040 USA Chemistry Department Stony Brook University SUNY Stony Brook New York 11794-3400 USA RIKEN Nishina Center for Accelerator-Based Science Wako Saitama 351-0198 Japan RIKEN BNL Research Center New Mexico State University Las Cruces New Mexico 88003 USA Department of Physics and Astronomy Howard University Washington DC 20059 USA KEK High Energy Accelerator Research Organization Tsukuba Ibaraki 305-0801 Japan Kyoto University Kyoto 606-8502 Japan Iowa State University Ames Iowa 50011 USA Department of Physics and Astronomy Stony Brook University SUNY Stony Brook New York 11794-3800 USA SUBATECH (Ecole des Mines de Nantes CNRS-IN2P3 Université de Nantes) BP 20722-44307 Nantes France Laboratoire Leprince-Ringuet Ecole Polytechnique CNRS-IN2P3 Route de Saclay F-91128 Palaiseau France Oak Ridge National Laboratory Oak Ridge Tennessee 37831 USA Physics Department IHEP Protvino State Research Center of Russian Federation Institute for High Energy Physics Protvino 142281 Russia Collider-Accelerator Department Florida Institute of Technology Melbourne Florida 32901 USA Dapnia CEA Saclay F-91191 Gif-sur-Yvette France University of California-Riverside Riverside California 92521 USA Los Alamos National Laboratory Los Alamos New Mexico 87545 USA University of New Mexico Albuquerque New Mexico 87131 USA Abilene Christian University Abilene Texas 79699 USA Baruch College City University of New York New York New York 10010 USA PNPI Petersburg Nuclear Physics Institute Gatchina Leningrad region 188300 Russia Institut für

High-momentum two-particle correlations are a useful tool for studying jet-quenching effects in the quark-gluon plasma. Angular correlations between neutral-pion triggers and charged hadrons with transverse momenta in the range 4–12 GeV/c and 0.5–7 GeV/c, respectively, have been measured by the phENIX experiment in 2014 for Au+Au collisions at sNN=200 GeV. Suppression is observed in the yield of high-momentum jet fragments opposite the trigger particle, which indicates jet suppression stemming from in-medium partonic energy loss, while enhancement is observed for low-momentum particles. The ratio and differences between the yield in Au+Au collisions and p+p collisions, IAA and ΔAA, as a function of the trigger-hadron azimuthal separation, Δϕ, are measured for the first time at the BNL Relativistic Heavy Ion Collider. These results better quantify how the yield of low-pT associated hadrons is enhanced at wide angle, which is crucial for studying energy loss as well as medium-response effects.

关键词： Particle correlations & fluctuations Relativistic heavy-ion collisions Hadrons Pions Hadron colliders

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Early Release science of the exoplanet WASP-39b with JWST NIRISS

arXiv

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arXiv 2022年

作者： Feinstein, Adina d. Radica, Michael Welbanks, Luis Murray, Catriona Anne Ohno, Kazumasa Coulombe, Louis-philippe Espinoza, Néstor Bean, Jacob L. Teske, Johanna K. Benneke, Björn Line, Michael R. Rustamkulov, Zafar Saba, Arianna Tsiaras, Angelos Barstow, Joanna K. Fortney, Jonathan J. Gao, Peter Knutson, Heather A. Macdonald, Ryan J. Mikal-Evans, Thomas Rackham, Benjamin V. Taylor, Jake Parmentier, Vivien Batalha, Natalie M. Berta-Thompson, Zachory K. Carter, Aarynn L. Changeat, Quentin dos Santos, Leonardo A. Gibson, Neale P. Goyal, Jayesh M. Kreidberg, Laura López-Morales, Mercedes Lothringer, Joshua d. Miguel, Yamila Molaverdikhani, Karan Moran, Sarah E. Morello, Giuseppe Mukherjee, Sagnick Sing, david K. Stevenson, Kevin B. Wakeford, Hannah R. Ahrer, Eva-Maria Alam, Munazza K. Alderson, Lili Allen, Natalie H. Batalha, Natasha E. Bell, Taylor J. Blecic, Jasmina Brande, Jonathan Caceres, Claudio Casewell, S.L. Chubb, Katy L. Crossfield, Ian J.M. Crouzet, Nicolas Cubillos, Patricio E. decin, Leen désert, Jean-Michel Harrington, Joseph Heng, Kevin Henning, Thomas Iro, Nicolas Kempton, Eliza M.-R. Kendrew, Sarah Kirk, James Krick, Jessica Lagage, Pierre-Olivier Lendl, Monika Mancini, Luigi Mansfield, Megan May, E.M. Mayne, N.J. Nikolov, Nikolay K. Palle, Enric Petit dit de la Roche, dominique J.M. Piaulet, Caroline Powell, diana Redfield, Seth Rogers, Laura K. Roman, Michael T. Roy, Pierre-Alexis Nixon, Matthew C. Schlawin, Everett Tan, Xianyu Tremblin, P. Turner, Jake d. Venot, Olivia Waalkes, William C. Wheatley, Peter J. Zhang, Xi Department of Astronomy & Astrophysics University of Chicago ChicagoIL United States NSF Graduate Research Fellow Department of Physics Institute for Research on Exoplanets Université de Montréal MontrealQC Canada School of Earth and Space Exploration Arizona State University TempeAZ United States NHFP Sagan Fellow Department of Astrophysical and Planetary Sciences University of Colorado BoulderCO United States Department of Astronomy & Astrophysics University of California Santa Cruz Santa CruzCA United States Space Telescope Science Institute BaltimoreMD United States Department of Physics & Astronomy Johns Hopkins University BaltimoreMD United States Earth and Planets Laboratory Carnegie Institution for Science WashingtonDC United States Department of Earth and Planetary Sciences Johns Hopkins University BaltimoreMD United States Department of Physics and Astronomy University College London United Kingdom INAF - Osservatorio Astrofisico di Arcetri Largo E. Fermi 5 Firenze Italy School of Physical Sciences The Open University Milton Keynes United Kingdom Division of Geological and Planetary Sciences California Institute of Technology PasadenaCA United States Department of Astronomy University of Michigan Ann ArborMI United States Department of Astronomy Carl Sagan Institute Cornell University IthacaNY United States Max Planck Institute for Astronomy Heidelberg Germany Department of Earth Atmospheric and Planetary Sciences Massachusetts Institute of Technology CambridgeMA United States Kavli Institute for Astrophysics and Space Research Massachusetts Institute of Technology CambridgeMA United States 51 Pegasi b Fellow Atmospheric Oceanic and Planetary Physics Department of Physics University of Oxford Oxford United Kingdom Université Côte d'Azur Observatoire de la Côte d'Azur CNRS Laboratoire Lagrange France Astrobiology Program UC Santa Cruz Santa CruzCA United States European Space Agency Space Telescope Science Institute Balti

Transmission spectroscopy provides insight into the atmospheric properties and consequently the formation history, physics, and chemistry of transiting exoplanets1. However, obtaining precise inferences of atmospheric properties from transmission spectra requires simultaneously measuring the strength and shape of multiple spectral absorption features from a wide range of chemical species2–4. This has been challenging given the precision and wavelength coverage of previous observatories5. Here, we present the transmission spectrum of the Saturn-mass exoplanet WASP-39 b obtained using the SOSS mode of the NIRISS instrument on the JWST. This spectrum spans 0.6–2.8 µm in wavelength and reveals multiple water absorption bands, the potassium resonance doublet, as well as signatures of clouds. The precision and broad wavelength coverage of NIRISS-SOSS allows us to break model degeneracies between cloud properties and the atmospheric composition of WASP-39 b, favouring a heavy element enhancement ("metallicity") of ~10 – 30× the solar value, a sub-solar carbon-to-oxygen (C/O) ratio, and a solar-to-super-solar potassium-to-oxygen (K/O) ratio. The observations are also best explained by wavelength-dependent, non-gray clouds with inhomogeneous coverage of the planet’s terminator. © 2022, CC BY.

关键词： Water absorption

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Search for Gravitational Waves Associated with Fast Radio Bursts detected by CHIME/FRB during the LIGO-Virgo Observing Run O3a

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Astrophysical Journal 2023年第2期955卷 155-155页

作者： Abbott, R. Abbott, T.d. Acernese, F. Ackley, K. Adams, C. Adhikari, N. Adhikari, R.X. Adya, V.B. Affeldt, C. Agarwal, d. Agathos, M. Agatsuma, K. Aggarwal, N. Aguiar, O.d. Aiello, L. Ain, A. Ajith, P. Akutsu, T. Albanesi, S. Allocca, A. Altin, P.A. Amato, A. Anand, C. Anand, S. Ananyeva, A. Anderson, S.B. Anderson, W.G. Ando, M. Andrade, T. Andres, N. Andrić, T. Angelova, S.V. Ansoldi, S. Antelis, J.M. Antier, S. Appert, S. Arai, Koya Arai, Y. Araki, S. Araya, A. Araya, M.C. Areeda, J.S. Arène, M. Aritomi, N. Arnaud, N. Aronson, S.M. Arun, K.G. Asada, H. Asali, Y. Ashton, G. Aso, Y. Assiduo, M. Aston, S.M. Astone, P. Aubin, F. Austin, C. Babak, S. Badaracco, F. Bader, M.K.M. Badger, C. Bae, S. Bae, Y. Baer, A.M. Bagnasco, S. Bai, Y. Baiotti, L. Baird, J. Bajpai, R. Ball, M. Ballardin, G. Ballmer, S.W. Balsamo, A. Baltus, G. Banagiri, S. Bankar, d. Barayoga, J.C. Barbieri, C. Barish, B.C. Barker, d. Barneo, P. Barone, F. Barr, B. Barsotti, L. Barsuglia, M. Barta, d. Bartlett, J. Barton, M.A. Bartos, I. Bassiri, R. Basti, A. Bawaj, M. Bayley, J.C. Baylor, A.C. Bazzan, M. Bécsy, B. Bedakihale, V.M. Bejger, M. Belahcene, I. Benedetto, V. Beniwal, d. Bennett, T.F. Bentley, J.d. BenYaala, M. Bergamin, F. Berger, B.K. Bernuzzi, S. Berry, C.P.L. Bersanetti, d. Bertolini, A. Betzwieser, J. Beveridge, d. Bhandare, R. Bhardwaj, U. Bhattacharjee, d. Bhaumik, S. Bilenko, I.A. Billingsley, G. Bini, S. Birney, R. Birnholtz, O. Biscans, S. Bischi, M. Biscoveanu, S. Bisht, A. Biswas, B. Bitossi, M. Bizouard, M.-A. Blackburn, J.K. Blair, C.d. Blair, d.G. Blair, R.M. Bobba, F. Bode, N. Boer, M. Bogaert, G. Boldrini, M. Bonavena, L.d. Bondu, F. Bonilla, E. Bonnand, R. Booker, P. Boom, B.A. Bork, R. Boschi, V. Bose, N. Bose, S. Bossilkov, V. Boudart, V. Bouffanais, Y. Boumerdassi, A. Bozzi, A. Bradaschia, C. Brady, P.R. Bramley, A. Branch, A. Branchesi, M. Brau, J.E. Breschi, M. Briant, T. Briggs, J.H. Brillet, A. Brinkmann, M. Brockill, P. Brooks, A.F. Brooks, J. Brown, d.d. Brunett, S. Bruno, G. Bruntz, R. Bryant, J. Buchanan, J. B LIGO Laboratory California Institute of Technology Pasadena 91125 CA United States Louisiana State University Baton Rouge 70803 LA United States Dipartimento di Farmacia Università di Salerno Fisciano Salerno I-84084 Italy INFN Sezione di Napoli Complesso Universitario di Monte S. Angelo Napoli I-80126 Italy OzGrav School of Physics & Astronomy Monash University Clayton 3800 VIC Australia LIGO Livingston Observatory Livingston 70754 LA United States University of Wisconsin-Milwaukee Milwaukee 53201 WI United States OzGrav Australian National University Canberra 0200 ACT Australia Max Planck Institute for Gravitational Physics (Albert Einstein Institute) Hannover D-30167 Germany Leibniz Universität Hannover Hannover D-30167 Germany Inter-University Centre for Astronomy and Astrophysics Pune 411007 India University of Cambridge Cambridge CB2 1TN United Kingdom Theoretisch-Physikalisches Institut Friedrich-Schiller-Universität Jena Jena D-07743 Germany University of Birmingham Birmingham B15 2TT United Kingdom Center for Interdisciplinary Exploration & Research in Astrophysics (CIERA) Northwestern University Evanston 60208 IL United States Instituto Nacional de Pesquisas Espaciais São Paulo São José dos Campos 12227-010 Brazil Gravity Exploration Institute Cardiff University Cardiff CF24 3AA United Kingdom INFN Sezione di Pisa Pisa I-56127 Italy International Centre for Theoretical Sciences Tata Institute of Fundamental Research Bengaluru 560089 India Gravitational Wave Science Project National Astronomical Observatory of Japan (NAOJ) Mitaka City Tokyo 181-8588 Japan Advanced Technology Center National Astronomical Observatory of Japan (NAOJ) Mitaka City Tokyo 181-8588 Japan INFN Sezione di Torino Torino I-10125 Italy Università di Napoli “Federico II Complesso Universitario di Monte S. Angelo Napoli I-80126 Italy Université de Lyon Université Claude Bernard Lyon 1 CNRS Institut Lumière Matière Villeurbanne F-69622

We search for gravitational-wave (GW) transients associated with fast radio bursts (FRBs) detected by the Canadian Hydrogen Intensity Mapping Experiment Fast Radio Burst Project, during the first part of the third observing run of Advanced LIGO and Advanced Virgo (2019 April 1 15:00 UTC-2019 October 1 15:00 UTC). Triggers from 22 FRBs were analyzed with a search that targets both binary neutron star (BNS) and neutron star-black hole (NSBH) mergers. A targeted search for generic GW transients was conducted on 40 FRBs. We find no significant evidence for a GW association in either search. Given the large uncertainties in the distances of our FRB sample, we are unable to exclude the possibility of a GW association. Assessing the volumetric event rates of both FRB and binary mergers, an association is limited to 15% of the FRB population for BNS mergers or 1% for NSBH mergers. We report 90% confidence lower bounds on the distance to each FRB for a range of GW progenitor models and set upper limits on the energy emitted through GWs for a range of emission scenarios. We find values of order 10⁵¹-10⁵⁷ erg for models with central GW frequencies in the range 70-3560 Hz. At the sensitivity of this search, we find these limits to be above the predicted GW emissions for the models considered. We also find no significant coincident detection of GWs with the repeater, FRB 20200120E, which is the closest known extragalactic FRB. © 2023. The Author(s). Published by the American Astronomical Society.

关键词： Gravitational wave astronomy Radio transient sources

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Keep Your Friends Close and Your Colleagues Nearby: The Hidden Ties That Improve STEM Education

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Change 2019年第1期51卷 42页

作者： Mestre, Jose P. Herman, Geoffrey L. Tomkin, Jonathan H. West, Matthew Jose P. Mestre (mestre@illinois.edu). A theoretical nuclear physicist by training Mestre’s research focuses on the learning of physics contributing in areas such as the acquisition and use of knowledge by experts and novices transfer of learning problem solving and instructional design. He has offered Congressional testimony on The Science of Learning has published numerous articles and books and is a Fellow of the American Physical Society.http://***/0000-0003-2110-1954 Geoffrey L. Herman (glherman@illinois.edu). Herman has a Ph.D. in Electrical and Computer Engineering and is a Teaching Assistant Professor in Computer Science and a Research Assistant Professor in the Department of Curriculum & Instruction at the University of Illinois. His research focuses on how students learn engineering and computing concepts and studying processes for creating systemic instructional change in college settings. Previously he was a postdoctoral researcher in Engineering Education at Purdue University.http://***/0000-0002-9501-2295 Jonathan H. Tomkin (tomkin@illinois.edu). Tomkin is a mathematically based geoscientist with two research focus areas: first he uses models and large data sets to determine how climates glaciers tectonics and landscapes interact. Second he explores how new technological and organizational approaches can improve STEM education. He produced the first geoscience MOOC is the editor of an open-source textbook and has published widely in both geoscience and STEM education. Matthew West (mwest@illinois.edu). Matthew West is an Associate Professor of Mechanical Science and Engineering at the University of Illinois with research interests in scientific computing that include time integration of deterministic and stochastic systems distributed computation and particle methods for simulation and estimation. In education he researches computer-based assessment and the development of innovative teaching cultures. Professor West is a University of Illinois Distinguished Teacher-Scholar and Colleg

A science department on the campus of the University of Illinois has received numerous national awards for excellence in undergraduate teaching. The secret to their success? For nearly two decades, they have collaboratively used evidence-based instructional practices (EBIP) in their introductory level courses. despite these successes and efforts to spread their EBIP, no other departments followed this department's lead. Then, suddenly six years ago, many instructors from other departments began adopting EBIP in their classrooms. This article asks what was the catalyst for this change? Why had previous attempts at institutional change failed? The authors answer these questions by analyzing their efforts to transform the teaching practices in large-enrollment science and engineering introductory courses on their campus.

关键词： STEM Education Evidence Based Practice Teaching Methods Undergraduate Study college Faculty Educational Change Communities of Practice Mentors School CultureIllinois

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