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Institution

Roma Tre University

EducationRome, Lazio, Italy
About: Roma Tre University is a education organization based out in Rome, Lazio, Italy. It is known for research contribution in the topics: Large Hadron Collider & Galaxy. The organization has 4434 authors who have published 15352 publications receiving 374888 citations. The organization is also known as: Universita degli Studi Roma Tre & RomaTre.


Papers
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Journal ArticleDOI
Morad Aaboud, Georges Aad1, Brad Abbott2, Jalal Abdallah3  +2829 moreInstitutions (197)
TL;DR: In this paper, the mass of the $W$ boson was measured based on proton-proton collision data recorded in 2011 at a centre-of-mass energy of 7 TeV with the ATLAS detector at the LHC.
Abstract: A measurement of the mass of the $W$ boson is presented based on proton-proton collision data recorded in 2011 at a centre-of-mass energy of 7 TeV with the ATLAS detector at the LHC, and corresponding to 4.6 fb$^{-1}$ of integrated luminosity. The selected data sample consists of $7.8 \times 10^6$ candidates in the $W\rightarrow \mu u$ channel and $5.9 \times 10^6$ candidates in the $W\rightarrow e u$ channel. The $W$-boson mass is obtained from template fits to the reconstructed distributions of the charged lepton transverse momentum and of the $W$ boson transverse mass in the electron and muon decay channels, yielding \begin{eqnarray} m_W &=& 80370 \pm 7 \, (\textrm{stat.}) \pm 11 \, (\textrm{exp. syst.}) \pm 14 \, (\textrm{mod. syst.}) \, \textrm{MeV} &=& 80370 \pm 19 \, \textrm{MeV}, \end{eqnarray} where the first uncertainty is statistical, the second corresponds to the experimental systematic uncertainty, and the third to the physics-modelling systematic uncertainty. A measurement of the mass difference between the $W^+$ and $W^-$ bosons yields $m_{W^+}-m_{W^-} = -29 \pm 28$ MeV.

195 citations

Journal ArticleDOI
TL;DR: In this paper, the authors provide an overview of the different certification procedures employed in several countries all over the world, considering also which Green Building Rating System (GBRS) is only applied in its own country and which one is developed in other countries by means of proper adaptations.
Abstract: Building performances play a fundamental role in the worldwide energy scenario. In the last years, many countries have developed certification procedures in order to rate the environmental sustainability of buildings, aiming at reducing energy consumptions and environmental impacts during the construction, management and operational phases of a building. This study firstly provides an overview of the different certification procedures employed in several countries all over the world, considering also which Green Building Rating System (GBRS) is only applied in its own country and which one is developed in other countries by means of proper adaptations. Five widespread and well known green building rating systems (CASBEE, Green Star, BREEAM, LEED and ITACA) are then analyzed in detail and differences and similarities among them are highlighted. To this aim, six new macro-areas (site, water, energy, comfort and safety, materials and outdoor quality) are defined and a normalization procedure is implemented, in order to provide significant information about the sustainability aspects taken into account in the different rating tools and aiming at comparing them. This comparison allows to identify the main features of the five tools and to highlight qualitative and quantitative differences. The analysis shows that the certification tools are not homogeneous from both points of view. The aim of this work is to understand which issues have more influence on the final performance rate of each system and to give to final users a deeper knowledge of the aspects included in these tools.

195 citations

Journal ArticleDOI
TL;DR: A tripartite ATP-binding cassette efflux transporter, here named PvdRT-OpmQ, is identified, which translocates PVD from the periplasmic space to the extracellular milieu and is shown to be responsible for recycling of PVD upon internalization by the cognate outer-membrane receptor FpvA, thus making PVD virtually available for new cycles of iron uptake.
Abstract: The siderophore pyoverdine (PVD) is a primary virulence factor of the human pathogenic bacterium Pseudomonas aeruginosa, acting as both an iron carrier and a virulence-related signal molecule. By exploring a number of P. aeruginosa candidate systems for PVD secretion, we identified a tripartite ATP-binding cassette efflux transporter, here named PvdRT-OpmQ, which translocates PVD from the periplasmic space to the extracellular milieu. We show this system to be responsible for recycling of PVD upon internalization by the cognate outer-membrane receptor FpvA, thus making PVD virtually available for new cycles of iron uptake. Our data exclude the involvement of PvdRT-OpmQ in secretion of de novo synthesized PVD, indicating alternative pathways for PVD export and recycling. The PvdRT-OpmQ transporter is one of the few secretion systems for which substrate recognition and extrusion occur in the periplasm. Homologs of the PvdRT-OpmQ system are present in genomes of all fluorescent pseudomonads sequenced so far, suggesting that PVD recycling represents a general energy-saving strategy adopted by natural Pseudomonas populations.

194 citations

Journal ArticleDOI
Stefan Hild1, M. R. Abernathy1, Fausto Acernese2, Pau Amaro-Seoane3, Nils Andersson4, K. G. Arun5, Fabrizio Barone2, B. Barr1, M. Barsuglia, Mark Beker, N. Beveridge1, S. Birindelli6, Suvadeep Bose7, L. Bosi, S. Braccini8, C. Bradaschia8, Tomasz Bulik9, Enrico Calloni10, Giancarlo Cella8, E. Chassande Mottin, S. Chelkowski11, Andrea Chincarini, James S. Clark12, E. Coccia13, C. Colacino8, J. Colas, A. Cumming1, L. Cunningham1, E. Cuoco, S. L. Danilishin14, Karsten Danzmann3, R. De Salvo15, T. Dent12, R. De Rosa10, L. Di Fiore10, A. Di Virgilio8, M. Doets16, V. Fafone13, Paolo Falferi17, R. Flaminio, J. Franc, F. Frasconi8, Andreas Freise11, D. Friedrich18, Paul Fulda11, Jonathan R. Gair19, Gianluca Gemme, E. Genin, A. Gennai11, A. Giazotto8, Kostas Glampedakis20, Christian Gräf3, M. Granata, Hartmut Grote3, G. M. Guidi21, A. Gurkovsky14, G. D. Hammond1, Mark Hannam12, Jan Harms15, D. Heinert22, Martin Hendry1, Ik Siong Heng1, E. Hennes, J. H. Hough, Sascha Husa23, S. H. Huttner1, G. T. Jones12, F. Y. Khalili14, Keiko Kokeyama11, Kostas D. Kokkotas20, Badri Krishnan3, Tjonnie G. F. Li, M. Lorenzini, H. Lück3, Ettore Majorana, Ilya Mandel24, Vuk Mandic25, M. Mantovani8, I. W. Martin1, Christine Michel, Y. Minenkov13, N. Morgado, S. Mosca10, B. Mours26, Helge Müller-Ebhardt18, P. G. Murray1, Ronny Nawrodt1, Ronny Nawrodt22, John Nelson1, Richard O'Shaughnessy27, Christian D. Ott15, C. Palomba, Angela Delli Paoli, G. Parguez, A. Pasqualetti, R. Passaquieti8, R. Passaquieti28, D. Passuello8, Laurent Pinard, Wolfango Plastino29, Rosa Poggiani8, Rosa Poggiani28, P. Popolizio, Mirko Prato, M. Punturo, P. Puppo, D. S. Rabeling16, P. Rapagnani30, Jocelyn Read31, Tania Regimbau6, H. Rehbein3, S. Reid1, F. Ricci30, F. Richard, A. Rocchi, Sheila Rowan1, A. Rüdiger3, Lucía Santamaría15, Benoit Sassolas, Bangalore Suryanarayana Sathyaprakash12, Roman Schnabel3, C. Schwarz22, Paul Seidel22, Alicia M. Sintes23, Kentaro Somiya15, Fiona C. Speirits1, Kenneth A. Strain1, S. E. Strigin14, P. J. Sutton12, S. P. Tarabrin18, Andre Thüring3, J. F. J. van den Brand16, M. van Veggel1, C. Van Den Broeck, Alberto Vecchio11, John Veitch12, F. Vetrano21, A. Viceré21, S. P. Vyatchanin14, Benno Willke3, Graham Woan1, Kazuhiro Yamamoto 
TL;DR: In this article, a special focus is set on evaluating the frequency band below 10Hz where a complex mixture of seismic, gravity gradient, suspension thermal and radiation pressure noise dominates, including the most relevant fundamental noise contributions.
Abstract: Advanced gravitational wave detectors, currently under construction, are expected to directly observe gravitational wave signals of astrophysical origin. The Einstein Telescope, a third-generation gravitational wave detector, has been proposed in order to fully open up the emerging field of gravitational wave astronomy. In this article we describe sensitivity models for the Einstein Telescope and investigate potential limits imposed by fundamental noise sources. A special focus is set on evaluating the frequency band below 10Hz where a complex mixture of seismic, gravity gradient, suspension thermal and radiation pressure noise dominates. We develop the most accurate sensitivity model, referred to as ET-D, for a third-generation detector so far, including the most relevant fundamental noise contributions.

194 citations

Journal ArticleDOI
TL;DR: A fast and accurate method for obtaining the five parameters of the one diode model by starting from the experimental I–V curve of the PV panel by exploiting the adoption of the reduced forms of the original five-parameter model.

194 citations


Authors

Showing all 4598 results

NameH-indexPapersCitations
Andrew White1491494113874
Sw. Banerjee1461906124364
Fuqiang Wang145151895014
Stefano Giagu1391651101569
Silvia Masi13966997618
Filippo Ceradini131101682732
Mattias Ellert131102282637
Francesco Lacava130104279680
Giovanni Organtini129143885866
Georg Zobernig129112583321
Monica Verducci12989676002
Marzio Nessi129104678641
Cristian Stanescu12892276446
Domizia Orestano12898278297
Lashkar Kashif12878274072
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Performance
Metrics
No. of papers from the Institution in previous years
YearPapers
20251
2023121
2022212
20211,137
20201,200
20191,224