Search for the supersymmetric partner of the top quark in dilepton events from pp̄ collisions at √s = 1.8 TeV

Physical Review Letters 90:25 I (2003) 2518011-2518017

Authors:

D Acosta, T Affolder, H Akimoto, MG Albrow, D Ambrose, D Amidei, K Anikeev, J Antos, G Apollinari, T Arisawa, A Artikov, T Asakawa, W Ashmanskas, F Azfar, P Azzi-Bacchetta, N Bacchetta, H Bachacou, W Badgett, S Bailey, P de Barbaro, A Barbaro-Galtieri, VE Barnes, BA Barnett, S Baroiant, M Barone, G Bauer, F Bedeschi, S Behari, S Belforte, WH Bell, G Bellettini, J Bellinger, D Benjamin, J Bensinger, A Beretvas, J Berryhill, A Bhatti, M Binkley, D Bisello, M Bishai, RE Blair, C Blocker, K Bloom, B Blumenfeld, SR Blusk, A Bocci, A Bodek, G Bolla, A Bolshov, Y Bonushkin, D Bortoletto, J Boudreau, A Brandl, C Bromberg, M Brozovic, E Brubaker, N Bruner, J Budagov, HS Budd, K Burkett, G Busetto, KL Byrum, S Cabrera, P Calafiura, M Campbell, W Carithers, J Carlson, D Carlsmith, W Caskey, A Castro, D Cauz, A Cerri, L Cerrito, AW Chan, PS Chang, PT Chang, J Chapman, C Chen, YC Chen, MT Cheng, M Chertok, G Chiarelli, I Chirikov-Zorin, G Chlachidze, F Chlebana, L Christofek, ML Chu, JY Chung, WH Chung, YS Chung, CI Ciobanu, AG Clark, M Coca, AP Colijn, A Connolly, M Convery, J Conway, M Cordelli, J Cranshaw, R Culbertson

Abstract:

The article discussed about the supersymmetric particles of the top quark in Dilepton events. The Collider Detector at Fermilab was used to gather supersymmetry particles. Due to the high mass, stop decays into the top quark were found kinematically inaccessible. The choice of the renormalization and factorization scale was considered as the source of uncertainty on the number of expected stop events.

Adapting SAM for CDF

ArXiv cs/0306112 (2003)

Authors:

D Bonham, G Garzoglio, R Herber, J Kowalkowski, D Litvintsev, L Lueking, M Paterno, D Petravick, L Piccoli, R Pordes, N Stanfield, I Terekhov, J Trumbo, J Tseng, S Veseli, M Votava, V White, T Huffman, S Stonjek, K Waltkins, P Crosby, D Waters, R St Denis

Abstract:

The CDF and D0 experiments probe the high-energy frontier and as they do so have accumulated hundreds of Terabytes of data on the way to petabytes of data over the next two years. The experiments have made a commitment to use the developing Grid based on the SAM system to handle these data. The D0 SAM has been extended for use in CDF as common patterns of design emerged to meet the similar requirements of these experiments. The process by which the merger was achieved is explained with particular emphasis on lessons learned concerning the database design patterns plus realization of the use cases.

Erratum: Measurement of the tt̄ production cross in pp̄ collisions at √s= 1.8 Tev (Physical Review D (2001) 64 (32002))

Physical Review D Particles Fields Gravitation and Cosmology 67:11 (2003) 1199011-1199012

Authors:

T Affolder, H Akimoto, A Akopian, MG Albrow, P Amaral, SR Amendolia, D Amidei, K Anikeev, J Antos, G Apollinari, T Arisawa, T Asakawa, W Ashmanskas, F Azfar, P Azzi-Bacchetta, N Bacchetta, MW Bailey, S Bailey, P de Barbaro, A Barbaro-Galtieri, VE Barnes, BA Barnett, S Baroiant, M Barone, G Bauer, F Bedeschi, S Belforte, WH Bell, G Bellettini, J Bellinger, D Benjamin, J Bensinger, A Beretvas, JP Berge, J Berryhill, B Bevensee, A Bhatti, M Binkley, D Bisello, M Bishai, RE Blair, C Blocker, K Bloom, B Blumenfeld, SR Blusk, A Bocci, A Bodek, W Bokhari, G Bolla, Y Bonushkin, D Bortoletto, J Boudreau, A Brandl, S van den Brink, C Bromberg, M Brozovic, N Bruner, E Buckley-Geer, J Budagov, HS Budd, K Burkett, G Busetto, A Byon-Wagner, KL Byrum, P Calafiura, M Campbell, W Carithers, J Carlson, D Carlsmith, W Caskey, J Cassada, A Castro, D Cauz, A Cerri, AW Chan, PS Chang, PT Chang, J Chapman, C Chen, YC Chen, MT Cheng, M Chertok, G Chiarelli, I Chirikov-Zorin, G Chlachidze, F Chlebana, L Christofek, ML Chu, YS Chung, CI Ciobanu, AG Clark, A Connolly, J Conway, M Cordelli, J Cranshaw, D Cronin-Hennessy, R Cropp, R Culbertson, D Dagenhart, S D'Auria

A search for correlations of TeV gamma rays with ultra-high-energy cosmic rays

Astrophysical Journal 586:2 I (2003) 1232-1237

Authors:

CW Akerlof, S Biller, P Boyle, J Buckley, DA Carter-Lewis, M Catanese, MF Cawley, V Connaughton, DJ Fegan, J Finley, J Gaidos, AM Hillas, F Krennrich, RC Lamb, R Lessard, J Mcenery, G Mohanty, NA Porter, J Quinn, A Rodgers, HJ Rose, F Samuelson, MS Schubnell, G Sembroski, R Srinivasan, TC Weekes, J Zweerink

Abstract:

A search was conducted for TeV γ-rays emitted from the direction of the ultra-high-energy cosmic ray detected by the Fly's Eye experiment with energy E ∼ 3 × 1020 eV. No enhancement was found at a level of 10-10 cm-2 s-1 for E > 350 GeV. A steady source of ultra-high-energy cosmic ray protons or photons would be expected to produce a γ-ray flux above this level. An upper limit was also set for the flux of TeV γ-rays from 3C 147, the most prominent active galactic nucleus in the error box.

Neutral current and day night measurements from the pure D2O phase of SNO

Nuclear and Particle Physics Proceedings Elsevier 118 (2003) 3-14

Authors:

AL Hallin, EW Beier, SD Biller, MG Boulay, MG Bowler, TJ Bowles, SJ Brice, TV Bullard, J Cameron, YD Chan, X Chen, M Chen, BT Cleveland, GA Cox, X Dai, F Dalnoki-Veress, PJ Doe, G Doucas, MR Dragowsky, CA Duba, FA Duncan, M Dunford, JA Dunmore, ED Earle, SR Elliott, HC Evans, GT Ewan, J Farine, H Fergani, JA Formaggio, MM Fowler, K Frame, W Frati, N Gagnon, K Graham, DR Grant, RL Hahn, ED Hallman, AS Hamer, WB Handler, CK Hargrove, PJ Harvey, R Hazama, KM Heeger, WJ Heintzelman, J Heise, RL Helmer, A Hime, M Howe, P Jagam, NA Jelley, K Kazkaz, PT Keener, JR Klein, T Kutter, CCM Kyba, J Law, IT Lawson, KT Lesko, JR Leslie, I Levine, S Luoma, S Majerus, HB Mak, J Maneira, J Manor, AD Marino, N McCauley, AB McDonald, G McGregor, GG Miller, CW Nally, AJ Noble, EB Norman, CE Okada, JL Orrell, SM Oser, AWP Poon, BC Robertson, RGH Robertson, SSE Rosendahl, VL Rusu, KK Schaffer, MH Schwendener, JJ Simpson, CJ Sims, D Sinclair, P Skensved, MWE Smith, T Spreitzer, N Starinsky, RG Stokstad, LC Stonehill, R Tafirout, N Tagg, R Van Berg, RG Van de Water, CJ Virtue, CE Waltham, DL Wark, N West, JB Wilhelmy, JF Wilkerson, JR Wilson, P Wittich, JM Wouters, M Yeh