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Institution

Technical University of Dortmund

EducationDortmund, Nordrhein-Westfalen, Germany
About: Technical University of Dortmund is a education organization based out in Dortmund, Nordrhein-Westfalen, Germany. It is known for research contribution in the topics: Large Hadron Collider & Neutrino. The organization has 13028 authors who have published 27666 publications receiving 615557 citations. The organization is also known as: Dortmund University & University of Dortmund.


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Journal ArticleDOI
TL;DR: A suitable modification of the standard Abadie constraint qualification is introduced as well as a corresponding optimality condition, and it is shown that this modified constraint qualification holds under fairly mild assumptions.
Abstract: We consider a difficult class of optimization problems that we call a mathematical program with vanishing constraints. Problems of this kind arise in various applications including optimal topology design problems of mechanical structures. We show that some standard constraint qualifications like LICQ and MFCQ usually do not hold at a local minimum of our program, whereas the Abadie constraint qualification is sometimes satisfied. We also introduce a suitable modification of the standard Abadie constraint qualification as well as a corresponding optimality condition, and show that this modified constraint qualification holds under fairly mild assumptions. We also discuss the relation between our class of optimization problems with vanishing constraints and a mathematical program with equilibrium constraints.

152 citations

Journal ArticleDOI
Roel Aaij, Bernardo Adeva1, Marco Adinolfi2, A. A. Affolder3  +715 moreInstitutions (63)
TL;DR: In this paper, the LHCb observations of the rare decays are presented using data corresponding to an integrated luminosity of 3.0 fb(-1), collected by the LHb experiment at center-of-mass energies of 7 and 8 TeV.
Abstract: First observations of the rare decays B (+) -> K (+)pi (+) pi (-) mu (+) mu (-) and B (+)-> phi K+ mu(+)mu(-) are presented using data corresponding to an integrated luminosity of 3.0 fb(-1), collected by the LHCb experiment at centre-of-mass energies of 7 and 8 TeV. The branching fractions of the decays are B(B (+) -> K (+)pi (+) pi (-) mu (+) mu (-) ) = (4.36 (-0.27) (+0.29) (stat) +/- 0.21 (syst) +/- (norm)) x 10(-7), B(B (+)-> phi K+ mu(+)mu(-)) = (0.82 (+0.19)(-0.17) (stat) (+0.10)(-0.04) (syst) +/- 0.27 (norm)) x 10(-7) where the uncertainties are statistical, systematic, and due to the uncertainty on the branching fractions of the normalisation modes. A measurement of the differential branching fraction in bins of the invariant mass squared of the dimuon system is also presented for the decay B (+) -> K (+)pi (+) pi (-) mu (+) mu (-)

152 citations

Journal ArticleDOI
Justin Albert1, E. Aliu, H. Anderhub2, P. Antoranz3, A. Armada, M. Asensio3, C. Baixeras4, Juan Abel Barrio3, M. Bartelt5, H. Bartko6, Denis Bastieri7, R. Bavikadi8, W. Bednarek, K. Berger1, Ciro Bigongiari7, Adrian Biland2, E. Bisesi8, R. K. Bock6, Thomas Bretz1, I. Britvitch2, M. Camara3, Ashot Chilingarian9, Stefano Ciprini, J. A. Coarasa6, S. Commichau2, Jose Luis Contreras3, Juan Cortina, V. Curtef5, V. Danielyan9, Francesco Dazzi7, A. De Angelis8, R. de los Reyes3, B. De Lotto8, E. Domingo-Santamaría, Daniela Dorner1, Michele Doro7, Manel Errando, Michela Fagiolini10, Daniel Ferenc11, E. Fernandez, R. Firpo, Jose Flix, M. V. Fonseca3, Ll. Font4, Nicola Galante10, M. Garczarczyk6, Markus Gaug, Maria Giller, Florian Goebel6, D. Hakobyan9, Masaaki Hayashida6, T. Hengstebeck12, D. Höhne1, J. Hose6, P. Jacon, O. Kalekin12, D. Kranich11, D. Kranich2, A. Laille11, T. Lenisa8, P. Liebing6, Elina Lindfors, Francesco Longo13, Jorge Andres Lopez Lopez, M. López3, E. Lorenz2, E. Lorenz6, F. Lucarelli3, P. Majumdar6, G. Maneva, K. Mannheim1, Mosè Mariotti7, M. I. Martínez, K. Mase6, Daniel Mazin6, M. Merck1, Mario Meucci10, M. Meyer1, Jose Miguel Miranda3, R. Mirzoyan6, S. Mizobuchi6, Abelardo Moralejo6, K. Nilsson, E. Oña-Wilhelmi, R. Orduña4, N. Otte6, I. Oya3, David Paneque6, Riccardo Paoletti10, M. Pasanen, D. Pascoli7, F. Pauss2, N. Pavel12, R. Pegna10, L. Peruzzo7, A. Piccioli10, Elisa Prandini7, J. Rico, Wolfgang Rhode5, B. Riegel1, M. Rissi2, A. Robert4, S. Rügamer1, A. Saggion7, Alvaro Sanchez4, P. Sartori7, V. Scalzotto7, R. Schmitt1, T. Schweizer12, M. Shayduk12, K. Shinozaki6, S. N. Shore14, N. Sidro, A. Sillanpää, Dorota Sobczyńska, Antonio Stamerra10, A. Stepanian, L. S. Stark2, L. O. Takalo, Petar Temnikov, D. Tescaro, Masahiro Teshima6, N. Tonello6, A. Torres4, Diego F. Torres15, Nicola Turini10, H. Vankov, A. Vardanyan9, V. Vitale8, Robert Wagner6, Tadeusz Wibig, W. Wittek6, J. Zapatero4 
TL;DR: In this paper, MAGIC observations of the Galactic center were used to detect a differential gamma-ray flux consistent with a steady, hard-slope power law, described as dN gamma/(dA dt dE) = (29 +/- 06) x 10(-12) (E/TeV)-22 +/- 02 cm(-2) s(-1) TeV-1 The Gamma-ray source is centered at (RA, decl) p (17(h)45(m)20(s), -29 degrees 2')
Abstract: Recently, the Galactic center has been reported to be a source of very high energy (VHE) gamma-rays by the CANGAROO, VERITAS, and HESS experiments The energy spectra as measured by these experiments show substantial differences In this Letter we present MAGIC observations of the Galactic center, resulting in the detection of a differential gamma-ray flux consistent with a steady, hard-slope power law, described as dN gamma/(dA dt dE) = (29 +/- 06) x 10(-12) (E/TeV)-22 +/- 02 cm(-2) s(-1) TeV-1 The gamma-ray source is centered at (RA, decl) p (17(h)45(m)20(s), -29 degrees 2') This result confirms the previous measurements by the HESS experiment and indicates a steady source of TeV gamma-rays We briefly describe the observational technique used and the procedure implemented for the data analysis, and we discuss the results in the perspective of different models proposed for the acceleration of the VHE gamma-rays

152 citations

Journal ArticleDOI
TL;DR: In this paper, the present status of the determination of parton distribution functions (PDFs) in the light of the precision requirements for the LHC in Run 2 and other future hadron colliders is reviewed.
Abstract: We review the present status of the determination of parton distribution functions (PDFs) in the light of the precision requirements for the LHC in Run 2 and other future hadron colliders. We provide brief reviews of all currently available PDF sets and use them to compute cross sections for a number of benchmark processes, including Higgs boson production in gluon–gluon fusion at the LHC. We show that the differences in the predictions obtained with the various PDFs are due to particular theory assumptions made in the fits of those PDFs. We discuss PDF uncertainties in the kinematic region covered by the LHC and on averaging procedures for PDFs, such as advocated by the PDF4LHC15 sets, and provide recommendations for the usage of PDF sets for theory predictions at the LHC.

152 citations

Journal ArticleDOI
Rasha Abbasi1, Y. Abdou2, T. Abu-Zayyad3, Jenni Adams4  +265 moreInstitutions (35)
TL;DR: In this paper, the results of time-integrated searches for astrophysical neutrino sources in both the northern and southern skies were presented, and limits were set for neutrinos fluxes from astrophysical sources over the entire sky and compared to predictions.
Abstract: We present the results of time-integrated searches for astrophysical neutrino sources in both the northern and southern skies. Data were collected using the partially completed IceCube detector in the 40-string configuration recorded between 2008 April 5 and 2009 May 20, totaling 375.5 days livetime. An unbinned maximum likelihood ratio method is used to search for astrophysical signals. The data sample contains 36,900 events: 14,121 from the northern sky, mostly muons induced by atmospheric neutrinos, and 22,779 from the southern sky, mostly high-energy atmospheric muons. The analysis includes searches for individual point sources and stacked searches for sources in a common class, sometimes including a spatial extent. While this analysis is sensitive to TeV-PeV energy neutrinos in the northern sky, it is primarily sensitive to neutrinos with energy greater than about 1 PeV in the southern sky. No evidence for a signal is found in any of the searches. Limits are set for neutrino fluxes from astrophysical sources over the entire sky and compared to predictions. The sensitivity is at least a factor of two better than previous searches (depending on declination), with 90% confidence level muon neutrino flux upper limits being between E(2)d Phi/dE similar to 2-200 x 10(-12) TeV cm(-2) s(-1) in the northern sky and between 3-700 x 10(-12) TeV cm(-2) s(-1) in the southern sky. The stacked source searches provide the best limits to specific source classes. The full IceCube detector is expected to improve the sensitivity to d Phi/dE proportional to E-2 sources by another factor of two in the first year of operation.

152 citations


Authors

Showing all 13240 results

NameH-indexPapersCitations
Hermann Kolanoski145127996152
Marc Besancon1431799106869
Kerstin Borras133134192173
Emmerich Kneringer129102180898
Achim Geiser129133184136
Valerio Vercesi12993779519
Jens Weingarten12889674667
Giuseppe Mornacchi12789475830
Kevin Kroeninger12683670010
Daniel Muenstermann12688570855
Reiner Klingenberg12673370069
Claus Gössling12677571975
Diane Cinca12682270126
Frank Meier12467764889
Daniel Dobos12467967434
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Performance
Metrics
No. of papers from the Institution in previous years
YearPapers
2023131
2022306
20211,694
20201,773
20191,653
20181,579