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

Wade De La

Emeritus Professor

Sub department

  • Particle Physics
Wade.Allison@physics.ox.ac.uk
Telephone: 01865 (2)82065,01844237602
Denys Wilkinson Building, room 659
  • About
  • Publications

Search for nucleon decay into lepton+K0 final states using Soudan 2

Physical Review D - Particles, Fields, Gravitation and Cosmology 61:7 (2000) 1-16

Authors:

D Wall, WWM Allison, GJ Alner, DS Ayres, WL Barrett, C Bode, PM Border, CB Brooks, JH Cobb, R Cotton, H Courant, DM Demuth, TH Fields, HR Gallagher, C Garcia-Garcia, MC Goodman, R Gran, T Joffe-Minor, T Kafka, SMS Kasahara, W Leeson, PJ Litchfield, NP Longley, WA Mann, ML Marshak, RH Milburn, WH Miller, L Mualem, A Napier, WP Oliver, GF Pearce, EA Peterson, DA Petyt, LE Price, K Ruddick, M Sanchez, J Schneps, MH Schub, R Seidlein, A Stassinakis, H Tom, JL Thron, G Villaume, SP Wakely, N West

Abstract:

A search for nucleon decay into two-body final states containing K0 mesons has been conducted using the 963 metric ton Soudan 2 iron tracking calorimeter. The topologies, ionizations, and kinematics of contained events recorded in a 5.52 kiloton-year total exposure (4.41 kton-year fiducial volume exposure) are examined for compatibility with nucleon decays in an iron medium. For proton decay into the fully visible final states μ+KS0 and e+KS0, zero and one event candidates are observed respectively. The lifetime lower limits (τ/B) thus implied are 1.5×1032 yr and 1.2×1032 yr, respectively. Lifetime lower limits are also reported for proton decay into l+K10, and for neutron decay into vKS0. ©2000 The American Physical Society.
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Observation of a shadow of the Moon in the underground muon flux in the Soudan 2 detector

Physical Review D - Particles, Fields, Gravitation and Cosmology 61:9 (2000)

Authors:

JH Cobb, ML Marshak, WWM Allison, GJ Alner, DS Ayres, WL Barrett, C Bode, PM Border, CB Brooks, RJ Cotton, H Courant, DM Demuth, TH Fields, HR Gallagher, MC Goodman, R Gran, T Joffe-Minor, T Kafka, SMS Kasahara, W Leeson, PJ Litchfield, NP Longley, WA Mann, RH Milburn, WH Miller, C Moon, L Mualem, A Napier, WP Oliver, GF Pearce, EA Peterson, DA Petyt, LE Price, K Ruddick, M Sanchez, P Sankey, J Schneps, MH Schub, R Seidlein, A Stassinakis, JL Thron, V Vassiliev, G Villaume, SP Wakely, N West, D Wall

Abstract:

A shadow of the Moon, with a statistical significance of (Formula presented) has been observed in the underground muon flux at a depth of 2090 mwe using the Soudan 2 detector. The angular resolution of the detector is well described by a Gaussian with a sigma (Formula presented) The position of the shadow confirms that the alignment of the detector is known to better than (Formula presented) and has remained stable during ten years of data taking. © 2000 The American Physical Society.
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The atmospheric neutrino flavor ratio from a 3.9 fiducial kiloton-year exposure of Soudan 2

Physics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics 449:1-2 (1999) 137-144

Authors:

WWM Allison, GJ Alner, DS Ayres, G Barr, WL Barrett, C Bode, PM Border, CB Brooks, JH Cobb, RJ Cotton, H Courant, DM Demuth, TH Fields, HR Gallagher, C Garcia-Garcia, MC Goodman, R Gran, T Joffe-Minor, T Kafka, SMS Kasahara, W Leeson, PJ Litchfield, NP Longley, WA Mann, ML Marshak, RH Milburn, WH Miller, L Mualem, A Napier, WP Oliver, GF Pearce, EA Peterson, DA Petyt, LE Price, K Ruddick, M Sanchez, J Schneps, MH Schub, R Seidlein, A Stassinakis, JL Thron, V Vassiliev, G Villaume, S Wakely, D Wall, N West, UM Wielgosz

Abstract:

We report a measurement of the atmospheric neutrino flavor ratio, R, using a sample of quasi-elastic neutrino interactions occurring in an iron medium. The flavor ratio (tracks/showers) of atmospheric neutrinos in a 3.9 fiducial kiloton-year exposure of Soudan 2 is 0.64 ± 0.11(stat.) ± 0.06(syst.) of that expected. Important aspects of our main analysis have been checked by carrying out two independent, alternative analyses; one is based upon automated scanning, the other uses a multivariate approach for background subtraction. Similar results are found by all three approaches. © 1999 Elsevier Science B.V. All rights reserved.
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Search for the proton decay mode p → ν K+ in Soudan 2

Physics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics 427:1-2 (1998) 217-224

Authors:

WWM Allison, GJ Alner, DS Ayres, G Barr, WL Barrett, C Bode, PM Border, CB Brooks, JH Cobb, R Cotton, H Courant, DM Demuth, TH Fields, HR Gallagher, C Garcia-Garcia, MC Goodman, R Gran, T Joffe-Minor, T Kafka, SMS Kasahara, W Leeson, PJ Litchfield, NP Longley, WA Mann, ML Marshak, RH Milburn, WH Miller, L Mualem, A Napier, WP Oliver, GF Pearce, EA Peterson, DA Petyt, LE Price, K Ruddick, J Schneps, MH Schub, R Seidlein, A Stassinakis, H Tom, JL Thron, V Vassiliev, G Villaume, S Wakeley, D Wall, N West, UM Wielgosz

Abstract:

We have searched for the proton decay mode p → ν K+ using the one-kiloton Soudan 2 high resolution calorimeter. Contained events obtained from a 3.56 kiloton-year fiducial exposure through June 1997 are examined for occurrence of a visible K+ track which decays at rest into μ+ ν or π+ π0. We found one candidate event consistent with background, yielding a limit, τ/B(p → ν K+) > 4.3 × 1031 years at 90% CL with no background subtraction. © 1998 Published by Elsevier Science B.V. All rights reserved.
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Measurement of the atmospheric neutrino flavour composition in Soudan 2

Physics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics 391:3-4 (1997) 491-500

Authors:

WWM Allison, GJ Alner, DS Ayres, WL Barrett, C Bode, PM Border, CB Brooks, JH Cobb, DJA Cockerill, RJ Cotton, H Courant, DM DeMuth, TH Fields, HR Gallagher, C Garcia-Garcia, MC Goodman, RN Gray, K Johns, T Kafka, SMS Kasahara, W Leeson, PJ Litchfield, NP Longley, MJ Lowe, WA Mann, ML Marshak, EN May, RH Milburn, WH Miller, L Mualem, A Napier, W Oliver, GF Pearce, DH Perkins, EA Peterson, DA Petyt, LE Price, DM Roback, K Ruddick, DJ Schmid, J Schneps, MH Schub, RV Seidlein, MA Shupe, A Stassinakis, N Sundaralingam, J Thomas, JL Thron, V Vassiliev, G Villaume, SP Wakely, D Wall, SJ Werkema, N West, UM Wielgosz

Abstract:

The atmospheric neutrino flavour ratio measured using a 1.52 kton-year exposure of Soudan 2 is found to be 0.72 ± 0.19+0.05-0.07 relative to the expected value from a Monte Carlo calculation. The possible background of interactions of neutrons and photons produced in muon interactions in the rock surrounding the detector has been investigated and is shown not to produce low values of the ratio.
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