Rubin-LSST

Research group

Research theme

Sub department

About

Γ(1S) → γf2′(1525); f2′(1525) → KS0KS0 decays

PHYSICAL REVIEW D 83:3 (2011) ARTN 037101

Authors:

D Besson, DP Hogan, TK Pedlar, D Cronin-Hennessy, J Hietala, P Zweber, S Dobbs, Z Metreveli, KK Seth, A Tomaradze, T Xiao, S Brisbane, L Martin, A Powell, P Spradlin, G Wilkinson, H Mendez, JY Ge, DH Miller, IPJ Shipsey, B Xin, GS Adams, D Hu, B Moziak, J Napolitano, KM Ecklund, J Insler, H Muramatsu, CS Park, LJ Pearson, EH Thorndike, F Yang, S Ricciardi, C Thomas, M Artuso, S Blusk, R Mountain, T Skwarnicki, S Stone, JC Wang, LM Zhang, G Bonvicini, D Cinabro, A Lincoln, MJ Smith, P Zhou, J Zhu, P Naik, J Rademacker, DM Asner, KW Edwards, K Randrianarivony, G Tatishvili, RA Briere, H Vogel, PUE Onyisi, JL Rosner, JP Alexander, DG Cassel, S Das, R Ehrlich, L Fields, L Gibbons, SW Gray, DL Hartill, BK Heltsley, DL Kreinick, VE Kuznetsov, JR Patterson, D Peterson, D Riley, A Ryd, AJ Sadoff, X Shi, WM Sun, J Yelton, P Rubin, N Lowrey, S Mehrabyan, M Selen, J Wiss, J Libby, M Kornicer, RE Mitchell, CM Tarbert
More details from the publisher
Details from ArXiV

Boosted objects: a probe of beyond the Standard Model physics

(2010)

Authors:

A Abdesselam, E Bergeaas Kuutmann, U Bitenc, G Brooijmans, J Butterworth, P Bruckman de Renstrom, D Buarque Franzosi, R Buckingham, B Chapleau, M Dasgupta, A Davison, J Dolen, S Ellis, F Fassi, J Ferrando MT Frandsen, J Frost, T Gadfort, N Glover, A Haas, E Halkiadakis, K Hamilton, C Hays, C Hill, J Jackson, C Issever, M Karagoz, A Katz, L Kreczko, D Krohn, A Lewis, S Livermore, P Loch, P Maksimovic, J March-Russell, A Martin, N McCubbin, D Newbold, J Ott, G Perez, A Policchio, S Rappoccio, AR Raklev, P Richardson, GP Salam, F Sannino, J Santiago, A Schwartzman, C Shepherd-Themistocleous, P Sinervo, J Sjoelin, M Son, M Spannowsky, E Strauss, M Takeuchi, J Tseng, B Tweedie, C Vermilion, J Voigt, M Vos, J Wacker, J Wagner-Kuhr, MG Wilson
More details from the publisher

Boosted objects: a probe of beyond the Standard Model physics

ArXiv 1012.5412 (2010)

Authors:

A Abdesselam, E Bergeaas Kuutmann, U Bitenc, G Brooijmans, J Butterworth, P Bruckman de Renstrom, D Buarque Franzosi, R Buckingham, B Chapleau, M Dasgupta, A Davison, J Dolen, S Ellis, F Fassi, J Ferrando MT Frandsen, J Frost, T Gadfort, N Glover, A Haas, E Halkiadakis, K Hamilton, C Hays, C Hill, J Jackson, C Issever, M Karagoz, A Katz, L Kreczko, D Krohn, A Lewis, S Livermore, P Loch, P Maksimovic, J March-Russell, A Martin, N McCubbin, D Newbold, J Ott, G Perez, A Policchio, S Rappoccio, AR Raklev, P Richardson, GP Salam, F Sannino, J Santiago, A Schwartzman, C Shepherd-Themistocleous, P Sinervo, J Sjoelin, M Son, M Spannowsky, E Strauss, M Takeuchi, J Tseng, B Tweedie, C Vermilion, J Voigt, M Vos, J Wacker, J Wagner-Kuhr, MG Wilson

Abstract:

We present the report of the hadronic working group of the BOOST2010 workshop held at the University of Oxford in June 2010. The first part contains a review of the potential of hadronic decays of highly boosted particles as an aid for discovery at the LHC and a discussion of the status of tools developed to meet the challenge of reconstructing and isolating these topologies. In the second part, we present new results comparing the performance of jet grooming techniques and top tagging algorithms on a common set of benchmark channels. We also study the sensitivity of jet substructure observables to the uncertainties in Monte Carlo predictions.
More details from the publisher
More details
Details from ArXiV

Large scale structure simulations of inhomogeneous Lemaître-Tolman-Bondi void models

Physical Review D American Physical Society 82:12 (2010) ARTN: 123530

Authors:

David Alonso, J García-Bellido, T Haugbølle, J Vicente

Abstract:

We perform numerical simulations of large scale structure evolution in an inhomogeneous Lemaître-Tolman-Bondi (LTB) model of the Universe. We follow the gravitational collapse of a large underdense region (a void) in an otherwise flat matter-dominated Einstein–de Sitter model. We observe how the (background) density contrast at the center of the void grows to be of order one, and show that the density and velocity profiles follow the exact nonlinear LTB solution to the full Einstein equations for all but the most extreme voids. This result seems to contradict previous claims that fully relativistic codes are needed to properly handle the nonlinear evolution of large scale structures, and that local Newtonian dynamics with an explicit expansion term is not adequate. We also find that the (local) matter density contrast grows with the scale factor in a way analogous to that of an open universe with a value of the matter density Ω M ( r ) corresponding to the appropriate location within the void.
More details from the publisher
Details from ORA

Model-independent determination of the strong-phase difference between D0 and D⊃̄0→KS,L0h+h- (h=π, K) and its impact on the measurement of the CKM angle γ/Φ3

Physical Review D - Particles, Fields, Gravitation and Cosmology 82:11 (2010)

Authors:

J Libby, M Kornicer, RE Mitchell, MR Shepherd, CM Tarbert, D Besson, TK Pedlar, J Xavier, D Cronin-Hennessy, J Hietala, P Zweber, S Dobbs, Z Metreveli, KK Seth, A Tomaradze, T Xiao, S Brisbane, S Malde, L Martin, A Powell, P Spradlin, G Wilkinson, H Mendez, JY Ge, DH Miller, IPJ Shipsey, B Xin, GS Adams, D Hu, B Moziak, J Napolitano, KM Ecklund, J Insler, H Muramatsu, CS Park, LJ Pearson, EH Thorndike, F Yang, S Ricciardi, C Thomas, M Artuso, S Blusk, N Horwitz, R Mountain, T Skwarnicki, S Stone, JC Wang, LM Zhang, T Gershon, G Bonvicini, D Cinabro, A Lincoln, MJ Smith, P Zhou, J Zhu, P Naik, J Rademacker, DM Asner, KW Edwards, K Randrianarivony, G Tatishvili, RA Briere, H Vogel, PUE Onyisi, JL Rosner, JP Alexander, DG Cassel, S Das, R Ehrlich, L Fields, L Gibbons, SW Gray, DL Hartill, BK Heltsley, DL Kreinick, VE Kuznetsov, JR Patterson, D Peterson, D Riley, A Ryd, AJ Sadoff, X Shi, WM Sun, J Yelton, P Rubin, N Lowrey, S Mehrabyan, M Selen, J Wiss

Abstract:

We report the first determination of the relative strong-phase difference between D0→KS,L0K+K- and D⊃̄0→KS, L0K+K-. In addition, we present updated measurements of the relative strong-phase difference between D0→KS, L0π+π- and D⊃̄0→KS,L0π +π-. Both measurements exploit the quantum coherence between a pair of D0 and D⊃̄0 mesons produced from ψ(3770) decays. The strong-phase differences measured are important for determining the Cabibbo-Kobayashi-Maskawa angle γ/Φ3 in B -→K-D⊃0 decays, where D⊃0 is a D0 or D⊃̄0 meson decaying to KS0h+h- (h=π, K), in a manner independent of the model assumed to describe the D0→KS0h +h- decay. Using our results, the uncertainty in γ/Φ3 due to the error on the strong-phase difference is expected to be between 1.7° and 3.9° for an analysis using B -→K-D⊃0, D⊃0→KS0π+π - decays, and between 3.2° and 3.9° for an analysis based on B-→K-D⊃0, D⊃0→KS0K+K - decays. A measurement is also presented of the CP-odd fraction, F-, of the decay D0→KS0K+K- in the region of the Φ→K+K- resonance. We find that in a region within 0.01GeV2/c4 of the nominal Φ mass squared F->0.91 at the 90% confidence level. © 2010 The American Physical Society.
More details from the publisher
More details
Details from ArXiV