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Insertion of STC into TRT at the Department of Physics, Oxford
Credit: CERN

Professor Dr.rer.nat. Dipl.Phys. Alfons Weber FInstP, MA Ox

Visiting Professor

Research theme

  • Fundamental particles and interactions

Sub department

  • Particle Physics

Research groups

  • Accelerator Neutrinos
Alfons.Weber@physics.ox.ac.uk
Telephone: +49 (6131) 39 24175
Denys Wilkinson Building
AlfonsWeber@JGUMainz
  • About
  • Research
  • Teaching
  • Committees
  • Publications

Observation of muon neutrino disappearance with the MINOS detectors and the NuMI neutrino beam

ArXiv hep-ex/0607088 (2006)
Details from ArXiV

Observation of muon neutrino disappearance with the MINOS Detectors in the NuMI Neutrino Beam

Physical Review Letters 97 (2006) 191801 4pp

Authors:

AJ Weber, D.G. Michael, J. Thomas, D. Petyt
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First observations of separated atmospheric νμ and ν̄μ events in the MINOS detector

Physical Review D - Particles, Fields, Gravitation and Cosmology 73:7 (2006)

Authors:

P Adamson, T Alexopoulos, WWM Allison, GJ Alner, K Anderson, C Andreopoulos, M Andrews, R Andrews, C Arroyo, S Avvakumov, DS Ayres, B Baller, B Barish, MA Barker, PD Barnes, G Barr, WL Barrett, E Beall, BR Becker, A Belias, T Bergfeld, RH Bernstein, D Bhattacharya, M Bishai, A Blake, V Bocean, B Bock, GJ Bock, J Boehm, DJ Boehnlein, D Bogert, PM Border, C Bower, S Boyd, E Buckley-Geer, A Byon-Wagner, A Cabrera, JD Chapman, TR Chase, SK Chernichenko, S Childress, BC Choudhary, JH Cobb, JD Cossairt, H Courant, DA Crane, AJ Culling, JW Dawson, DM DeMuth, A De Santo, M Dierckxsens, MV Diwan, M Dorman, G Drake, R Ducar, T Durkin, AR Erwin, CO Escobar, J Evans, OD Fackler, EF Harris, GJ Feldman, N Felt, TH Fields, R Ford, MV Frohne, HR Gallagher, M Gebhard, A Godley, J Gogos, MC Goodman, Y Gornushkin, P Gouffon, E Grashorn, N Grossman, JJ Grudzinski, K Grzelak, V Guarino, A Habig, R Halsall, J Hanson, D Harris, PG Harris, J Hartnell, EP Hartouni, R Hatcher, K Heller, N Hill, Y Ho, C Howcroft, J Hylen, M Ignatenko, D Indurthy, GM Irwin, C James, L Jenner, D Jensen, T Joffe-Minor, T Kafka, HJ Kang

Abstract:

The complete 5.4 kton MINOS far detector has been taking data since the beginning of August 2003 at a depth of 2070 meters water-equivalent in the Soudan mine, Minnesota. This paper presents the first MINOS observations of νμ and ν̄μ charged-current atmospheric neutrino interactions based on an exposure of 418 days. The ratio of upward- to downward-going events in the data is compared to the Monte Carlo expectation in the absence of neutrino oscillations, giving Rup/downdata/Rup/downMC=0.62-0.14+0.19(stat.) ±0.02(sys.). An extended maximum likelihood analysis of the observed L/E distributions excludes the null hypothesis of no neutrino oscillations at the 98% confidence level. Using the curvature of the observed muons in the 1.3 T MINOS magnetic field νμ and ν̄μ interactions are separated. The ratio of ν̄μ to νμ events in the data is compared to the Monte Carlo expectation assuming neutrinos and antineutrinos oscillate in the same manner, giving Rν̄μ/νμdata/Rν̄μ/νμMC=0.96-0. 27+0.38(stat.)±0.15(sys.), where the errors are the statistical and systematic uncertainties. Although the statistics are limited, this is the first direct observation of atmospheric neutrino interactions separately for νμ and ν̄μ. © 2006 The American Physical Society.
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Precision electroweak measurements on the Z resonance

Physics Reports 427:5-6 (2006) 257-454

Authors:

JA Bagger, M Grünewald, S Schael, R Barate, R Brunelière, D Buskulic, I De Bonis, D Decamp, P Ghez, C Goy, S Jézéquel, JP Lees, A Lucotte, F Martin, E Merle, MN Minard, JY Nief, P Odier, B Pietrzyk, B Trocmé, S Bravo, MP Casado, M Chmeissani, P Comas, JM Crespo, E Fernandez, M Fernandez-Bosman, L Garrido, E Grauges, A Juste, M Martinez, G Merino, R Miquel, LM Mir, S Orteu, A Pacheco, IC Park, J Perlas, I Riu, H Ruiz, F Sanchez, A Colaleo, D Creanza, N De Filippis, M De Palma, G Iaselli, G Maggi, M Maggi, S Nuzzo, A Ranieri, G Raso, F Ruggieri, G Selvaggi, L Silvestris, P Tempesta, A Tricomi, G Zito, X Huang, J Lin, Q Ouyang, T Wang, Y Xie, R Xu, S Xue, J Zhang, L Zhang, W Zhao, D Abbaneo, A Bazarko, U Becker, G Boix, F Bird, E Blucher, B Bonvicini, P Bright-Thomas, T Barklow, O Buchmüller, M Cattaneo, F Cerutti, V Ciulli, B Clerbaux, H Drevermann, RW Forty, M Frank, TC Greening, R Hagelberg, AW Halley, F Gianotti, M Girone, JB Hansen, J Harvey, R Jacobsen, DE Hutchcroft, P Janot, B Jost, J Knobloch, M Kado, I Lehraus, P Lazeyras, P Maley

Abstract:

We report on the final electroweak measurements performed with data taken at the Z resonance by the experiments operating at the electron-positron colliders SLC and LEP. The data consist of 17 million Z decays accumulated by the ALEPH, DELPHI, L3 and OPAL experiments at LEP, and 600 thousand Z decays by the SLD experiment using a polarised beam at SLC. The measurements include cross-sections, forward-backward asymmetries and polarised asymmetries. The mass and width of the Z boson, mZ and ΓZ, and its couplings to fermions, for example the ρ parameter and the effective electroweak mixing angle for leptons, are precisely measured: mZ = 91.1875 ± 0.0021 GeV, ΓZ = 2.4952 ± 0.0023 GeV, ρl = 1.0050 ± 0.0010, sin2 θlepteff = 0.23153 ± 0.00016. The number of light neutrino species is determined to be 2.9840 ± 0.0082, in agreement with the three observed generations of fundamental fermions. The results are compared to the predictions of the Standard Model (SM). At the Z-pole, electroweak radiative corrections beyond the running of the QED and QCD coupling constants are observed with a significance of five standard deviations, and in agreement with the Standard Model. Of the many Z-pole measurements, the forward-backward asymmetry in b-quark production shows the largest difference with respect to its SM expectation, at the level of 2.8 standard deviations. Through radiative corrections evaluated in the framework of the Standard Model, the Z-pole data are also used to predict the mass of the top quark, mt = 173+13-10 GeV, and the mass of the W boson, mW = 80.363 ± 0.032 GeV. These indirect constraints are compared to the direct measurements, providing a stringent test of the SM. Using in addition the direct measurements of mt and mW, the mass of the as yet unobserved SM Higgs boson is predicted with a relative uncertainty of about 50% and found to be less than 285 GeV at 95% confidence level.
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First observations of separated atmospheric νμ and (ν)over-barμ events in the MINOS detector

PHYSICAL REVIEW D 73:7 (2006) ARTN 072002

Authors:

P Adamson, T Alexopoulos, WWM Allison, GJ Alner, K Anderson, C Andreopoulos, M Andrews, R Andrews, C Arroyo, S Avvakumov, DS Ayres, B Baller, B Barish, MA Barker, PD Barnes, G Barr, WL Barrett, E Beall, BR Becker, A Belias, T Bergfeld, RH Bernstein, D Bhattacharya, M Bishai, A Blake, V Bocean, B Bock, GJ Bock, J Boehm, DJ Boehnlein, D Bogert, PM Border, C Bower, S Boyd, E Buckley-Geer, A Byon-Wagner, A Cabrera, JD Chapman, TR Chase, SK Chernichenko, S Childress, BC Choudhary, JH Cobb, JD Cossairt, H Courant, DA Crane, AJ Culling, JW Dawson, DM DeMuth, A De Santo, M Dierckxsens, MV Diwan, M Dorman, G Drake, R Ducar, T Durkin, AR Erwin, CO Escobar, J Evans, OD Fackler, EF Harris, GJ Feldman, N Felt, TH Fields, R Ford, MV Frohne, HR Gallagher, M Gebhard, A Godley, J Gogos, MC Goodman, Y Gornushkin, P Gouffon, E Grashorn, N Grossman, JJ Grudzinski, K Grzelak, V Guarino, A Habig, R Halsall, J Hanson, D Harris, PG Harris, J Hartnell, EP Hartouni, R Hatcher, K Heller, N Hill, Y Ho, C Howcroft, J Hylen, M Ignatenko, D Indurthy, GM Irwin, C James, L Jenner, D Jensen, T Joffe-Minor, T Kafka, HJ Kang, SMS Kasahara, J Kilmer, H Kim, G Koizumi, S Kopp, M Kordosky, DJ Koskinen, M Kostin, DA Krakauer, S Kumaratunga, AS Ladran, K Lang, C Laughton, A Lebedev, R Lee, WY Lee, MA Libkind, J Liu, PJ Litchfield, RP Litchfield, NP Longley, P Lucas, W Luebke, S Madani, E Maher, V Makeev, WA Mann, A Marchionni, AD Marino, ML Marshak, JS Marshall, J McDonald, A McGowan, JR Meier, GI Merzon, MD Messier, DG Michael, RH Milburn, JL Miller, WH Miller, SR Mishra, PS Miyagawa, C Moore, J Morfín, R Morse, L Mualem, S Mufson, S Murgia, MJ Murtagh, J Musser, D Naples, C Nelson, JK Nelson, HB Newman, F Nezrick, RJ Nichol, TC Nicholls, JP Ochoa-Ricoux, J Oliver, WP Oliver, VA Onuchin, T Osiecki, R Ospanov, J Paley, V Paolone, A Para, T Patzak, Z Pavlovich, GF Pearce, N Pearson, CW Peck, C Perry, EA Peterson, DA Petyt, H Ping, R Piteira, A Pla-Dalmau, RK Plunkett, LE Price, M Proga, DR Pushka, D Rahman, RA Rameika, TM Raufer, AL Read, B Rebel, DE Reyna, C Rosenfeld, HA Rubin, K Ruddick, VA Ryabov, R Saakyan, MC Sanchez, N Saoulidou, J Schneps, PV Schoessow, P Schreiner, R Schwienhorst, VK Semenov, SM Seun, P Shanahan, PD Shield, W Smart, V Smirnitsky, C Smith, PN Smith, A Sousa, B Speakman, P Stamoulis, A Stefanik, P Sullivan, JM Swan, PA Symes, N Tagg, RL Talaga, E Tetteh-Lartey, J Thomas, J Thompson, MA Thomson, JL Thron, R Trendler, J Trevor, I Trostin, VA Tsarev, G Tzanakos, J Urheim, P Vahle, M Vakili, K Vaziri, C Velissaris, V Verebryusov, B Viren, L Wai, CP Ward, DR Ward, M Watabe, A Weber, RC Webb, A Wehmann, N West, C White, RF White, SG Wojcicki, DM Wright, QK Wu, WG Yan, T Yang, FX Yumiceva, JC Yun, H Zheng, M Zois, R Zwaska
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