Results 31 to 40 of about 983 (58)
Amplitude-Based IR-Improvement in Precision LHC/FCC Physics [PDF]
Proceedings of 42nd International Conference on High Energy Physics — PoS(ICHEP2024)We present recent results based on the IR-improvement of unintegrable singularities in the infrared regime via amplitude-based resummation in $QED \times QCD \subset SU(2)_L \times U_1 \times SU(3)_c$.B. Ward, S. Jadach, W. Płaczek, M. Skrzypek, Z. Was, S. A. Y. B. University, Waco, Tx, Usa, Institute of Nuclear Physics, Kraków, Pl, Institute of Computer Science, J. University, The Citadel, Charleston, Sc +16 moresemanticscholar +1 more sourceJ-PLUS: The Javalambre Photometric Local Universe Survey [PDF]
Astronomy & Astrophysics, 2015 The Javalambre Photometric Local Universe Survey (J-PLUS ) is an ongoing 12-band photometric optical survey, observing thousands of square degrees of the Northern Hemisphere from the dedicated JAST/T80 telescope at the Observatorio Astrofísico de ...A. Cenarro, M. Molés, D. Crist'obal-Hornillos, A. Marín-Franch, A. Ederoclite, J. Varela, C. López-Sanjuan, C. Hernandez-Monteagudo, R. Angulo, H. V. Rami'o, K. Viironen, S. Bonoli, Á. Orsi, G. Hurier, I. S. Roman, N. Greisel, G. Vilella-Rojo, L. A. Diaz-Garcia, R. Logroño-García, S. Gurung-López, D. Spinoso, D. Izquierdo-Villalba, J. Aguerri, C. A. Prieto, C. Bonatto, J. Carvano, A. Chies-Santos, S. Daflon, R. Dupke, J. Falcón-Barroso, D. R. Gonçcalves, Y. Jim'enez-Teja, A. Molino, V. Placco, E. Solano, D. D. Whitten, J. Abril, J. Antón, R. Bello, S. Toledo, J. Castillo-Ramirez, S. Chueca, T. Civera, M. C. Díaz-Martín, M. Domínguez-Martínez, J. Garzarán-Calderaro, J. Hernández-Fuertes, R. Iglesias-Marzoa, C. Iñiguez, J. M. J. Ruiz, K. Kruuse, J. L. Lamadrid, N. Lasso-Cabrera, G. López-Alegre, Á. López-Sainz, N. Maícas, A. Moreno-Signes, D. Muniesa, S. Rodríguez-Llano, F. Rueda-Teruel, S. Rueda-Teruel, I. Soriano-Laguía, V. Tilve, L. Valdivielso, A. Yanes-Diaz, J. Alcaniz, C. M. D. Oliveira, L. Sodré, P. Coelho, R. D. Oliveira, A. Tamm, H. S. Xavier, L. Abramo, S. Akras, E. Alfaro, A. Alvarez-Candal, B. Ascaso, M. Beasley, T. Beers, M. B. Fernandes, G. Bruzual, M. L. Buzzo, J. M. Carrasco, J. Cepa, A. Cortesi, M. Costa-Duarte, M. D. Pr'a, G. Favole, A. Galarza, L. Galbany, K. Garcia, R. M. G. Delgado, J. Gonzalez-serrano, L. A. Guti'errez-Soto, J. A. Hernandez-Jimenez, A. Kanaan, H. Kuncarayakti, R. Landim, J. Laur, J. Licandro, G. B. L. Neto, J. Lyman, J. M. Apell'aniz, J. Miralda-Escudé, D. Morate, J. P. Nogueira-Cavalcante, P. Novais, M. Oncins, I. Oteo, R. Overzier, C. Pereira, A. Rebassa-Mansergas, R. Reis, F. Roig, M. Sako, N. Salvador-Rusiñol, L. Sampedro, P. Sánchez-Blázquez, W. Santos, L. Schmidtobreick, B. B. Siffert, E. T. C. D. E. D. F. D. C. D. Csic, Plaza San Juan, E-44001, Teruel, Spain., Centro de Estudios de F'isica del Cosmos de Arag'on, Instituto de Astrof'isica de Canarias, V'ia L'actea sn. E-38205, La Laguna, Tenerife, D. Astrof'isica, Universidad de La Laguna . E-38206, D. D. Astronomia, Universidade Federal do Rio Grande do Sul, Av. Bento Gonccalves, 9500 Porto Alegre 91501-970, Rs, Brazil, Observatório Nacional do Rio de Janeiro, 77 RuaGal.Jos'eCristino, Sao Crist'ovao 20921-400 Rio de Janeiro, Rj, U. Michigan, D. Astronomy, 1085 S. University Ann Arbor, Michigan 48109, Usa, U. Alabama, Dept. of Phys.Astronomy, Gallalee Hall, Tuscaloosa, AL 35401, Observat'orio do Valongo, U. F. R. D. Janeiro, 43 LadeiraPedroAntonio, 20080-090 Rio de Janeiro, I. D. Astronomía, Geof'isica e Ciencias Atmosf'ericas, U. S. Paulo, Rua do Matao 1226, C. Universit'aria, São Paulo, 05508-090, Department of Astronomy Physics, Jina Center for the Evolution of the Elements, U. N. Dame, Notre Dame, IN 46556, C. D. Astrobiolog'ia, CSIC-INTA, Esac campus, camino bajo del castillo sn, E. Canada, Madrid, D. D. F'isica, Universidade Federal do Rio Grande do Norte, 59072-970 Natal, Rn, Rn, Av. Marechal Rondon, sn., 49000-000 Sao Crist'ovao, Se, X-ray Astrophysics Laboratory, Nasa Goddard Space Flight Center, Greenbelt, MD 20771, U. Maryland, Baltimore County, 1000 Hilltop Circle, Baltimore., MD 21250, Tartu Observatory, Tartu University, 1. Observatooriumi, Toravere, 61602 Tartu maakond, Estonia., I. D. F'isica, Rua do Matao 1371, Sp, Inst. de Astrof'isica de Andaluc'ia, Consejo Superior de Investigaciones Cient'ificas, Glorieta de la Astronom'ia, sn., 18008, Granada, Laboratoire Astroparticule et Cosmologie, 10 Rue Alice Domon et L'eonie Duquet, 7. Paris, France, I. D. Astrof'isica, Universidad Nacional Aut'onoma de M'exico, A. C. A. P. 8701, Ex-Hda. San Jos'e de la Huerta, 58341 Morelos, Mich., M'exico., Instituto de Ciencias del Cosmos, U. Barcelona, 1. Mart'iiFranques, 08193 Barcelona, Gran Via de les Corts Catalanes, 585, 08193 Barcelona, E. Centre, 28692 Villanueva de la Canada, Pitt Pacc, Astronomy, U. Pittsburgh, Pittsburgh, PA 15260, Usa, Instituto de F'isica de Cantabria, Avenida de los Castros, 39005 Santander, Cantabria, Campus Reitor Joao David Ferreira Lima, sn - Trindade, SC Florian'opolis-, 88040-900, Finnish Magic Consortium Finnish Centre of Astronomy with Eso, U. Turku, 20 Vaisalantie, 21500 Piikkio, Finland., T. Observatory, U. Warwick, Coventry CV4 7AL, Uk, I. C. D. R. I. E. Avanccats, 23 PasseigLlu'isCompanys, 08010-Barcelona, Institute for Astronomy, U. Edinburgh, R. Observatory, B. Hill, Edinburgh EH9 3HJ, United Kingdom., E. Observatory, 2. Karl-Schwarzschild-Str., 85748 Garching, Germany, D. D. F'isica, Universitat Politècnica de Catalunya, 5. CEsteveTerrades, E-08860, Casteldefells, Institute for Space Studies of Catalonia, cGran Capita 2-4, Edif. Nexus 201, 08193 Barcelona, C. P. 68528, Cep 21941-972, R. Janeiro, U. Pennsylvania, 2. S. 3. St., Philadelphia, PA 19104, U. Madrid, F. Ciencias, Plaza de Ciencias, Ciudad Universitaria, 28040, Alonso de C'ordova 3107, Vitacura, Santiago, Chile., Campus Duque de Caxias, Cep 25245-390 Duque de Caxias +290 moresemanticscholar +1 more sourceVERA monitoring of the radio jet 3C 84 in the period of 2007–2013: Detection of non-linear motion [PDF]
Nippon Tenmon Gakkai obun kenkyu hokoku, 2018 We present a kinematic study of the subparsec-scale radio jet of the radio galaxy 3C 84/NGC 1275 with the VLBI Exploration of Radio Astrometry (VERA) array at 22 GHz for 80 epochs from 2007 October to 2013 December.Koichiro Hiura, H. Nagai, M. Kino, K. Niinuma, K. Sorai, H. Chida, K. Akiyama, F. D’Ammando, G. Giovannini, M. Giroletti, K. Hada, M. Honma, S. Koyama, M. Orienti, G. Orosz, Satoko Sawada-Satoh Department of Cosmosciences, Graduate School of Science, Hokkai-Gakuen University, N. A. O. O. Japan, K. University, Academic Support Center, G. S. O. Sciences, Technology for Innovation, Y. University, D. Physics, Faculty of Computer Science, D. Physics, Faculty of Pure, A. Sciences, U. Tsukuba, Tomonaga Center for the History of the Universe, T. University, National Radio Astronomy Observatory, M. I. O. Technology, H. Observatory, I. D. Radioastronomia, D. Astronomia, U. Bologna, Department of Materials Science, The Graduate University for Advanced Studies, I. O. Astronomy, Astrophysics, A. Sinica, Engineering, Kagoshima University, Xinjiang Astronomical Observatory, Chinese Academy of Sciences +46 moresemanticscholar +1 more sourceA precise and accurate determination of the cosmic microwave background temperature at z = 0.89 [PDF]
, 2012 Context. According to the Big Bang theory and as a consequence of adiabatic expansion of the Universe, the temperature of the cosmic microwave background (CMB) increases linearly with redshift. This relation is, however, poorly explored, and detection of S. Muller, A. Beelen, J. Black, S. Curran, C. Horellou, S. Aalto, F. Combes, M. Guélin, C. O. Earth, S. Sciences, C. U. Technology, O. Observatory, Onsala, Sweden Institut d'Astrophysique Spatiale, U. Paris-sud, Orsay Cédex, France Niels Bohr Institute for Astronomy, S. O. Physics, The University of Sydney, Australia Arc Centre of Excellence for All-sky Astrophysics Paris, Lerma, Cnrs, París, France Institut de Radioastronomie Millim'etrique, S. d’Hères, France Ecole Normale Sup'erieureLERMA, France Max-Planck-Institut fur Radioastonomie, Bonn, Germany Astron. Dept., King Abdulaziz University, Jeddah, S. Arabia +31 moresemanticscholar +1 more sourceVLTI/GRAVITY enables the determination of the first dynamical masses of a classical Be + stripped and bloated pre-subdwarf binary [PDF]
Astronomy & AstrophysicsHR 6819 is the first post-mass transfer binary system composed of a classical Be star and a bloated pre-subdwarf stripped star directly confirmed by interferometry.R. Klement, T. Rivinius, D. Baade, A. Mérand, J. Bodensteiner, A. J. Frost, H. Sana, T. Shenar, D. Gies, P. H. E. O. F. A. R. Hemisphere, Chile, European Organisation for Astronomical Research in the Sout Hemisphere, Germany, Institue of Astronomy KU Leuven, Belgium, Leuven Gravity Institute, K. Leuven, T. Physics, Astronomy, T. University, Israel, C. F. Astronomy, D. Physics, Georgia State University, Usa, A. Institute, Academy of Sciences of the Czech Republic, Czech Republic +27 moresemanticscholar +1 more sourceIntensified training augments cardiac function, but not blood volume, in male youth elite ice hockey team players
Experimental Physiology, Volume 110, Issue 5, Page 755-766, 1 May 2025.Abstract
While it is well‐established that a period of interval training performed at near maximal effort, such as speed endurance training (SET), enhances intense exercise performance in well‐trained individuals, less is known about its effect on cardiac morphology and function as well as blood volume.Mads Fischer, Jan S. Jeppesen, Jeppe F. Vigh‐Larsen, Eric J. Stöhr, Magni Mohr, Kate A. Wickham, Lasse Gliemann, Jens Bangsbo, Ylva Hellsten, Morten Hostrup +9 morewiley +1 more sourcePressure‐Induced Capacity Recovery and Performance Enhancements in LTO/NMC‐LCO Batteries
Advanced Functional Materials, Volume 35, Issue 14, April 3, 2025.This work explores the effects of different pressurization methods on prismatic industrial‐grade high‐power lithium titanate oxide (LTO) batteries, both on pristine and aged cells. Continuously applied pressure of 0.3 MPa reduces capacity loss by 42% compared to unpressurized aged cells.Ahmed Chahbaz, Yucheng Luo, Gereon Stahl, Heinrich Ditler, Tony Jaumann, Martin Glinka, Christian Lingen, Dirk Uwe Sauer, Weihan Li +8 morewiley +1 more sourcePareto‐Optimal Design of Automotive Battery Systems with Tabless Cylindrical Lithium‐Ion Cells: Resolving the Trade‐Off Between Energy, Performance, Weight, and Cost for Variable Vehicle Requirements
Energy Technology, Volume 13, Issue 4, April 2025.Pareto fronts reveal a significant influence of cylindrical cell dimensions and housing materials on the trade‐off between the battery systems key performance indicators of energy, performance, weight, and cost. Introducing extruded aluminum housings is identified as a strong lever to optimize multiple properties at once compared to traditional deep ...Hendrik Pegel, Lukas Jany, Dirk Uwe Sauer +2 morewiley +1 more source