نتایج جستجو برای: two jets

تعداد نتایج: 2447634  

Journal: :JOURNAL OF THE FLOW VISUALIZATION SOCIETY OF JAPAN 1987

Journal: :Journal of Physics: Conference Series 2019

Journal: :Transactions of the Society of Instrument and Control Engineers 1978

Journal: :Journal of the Visualization Society of Japan 1996

2008
L. Bellagamba D. Boscherini A. Bruni G. Bruni P. Bruni G. Cara Romeo G. Castellini M. Chiarini L. Cifarelli F. Cindolo A. Contin M. Corradi I. Gialas P. Giusti G. Iacobucci G. Laurenti G. Levi A. Margotti T. Massam R. Nania C. Nemoz F. Palmonari A. Polini

Photoproduction events which have two or more jets have been studied in the Wγp range 135 GeV < Wγp < 280 GeV with the ZEUS detector at HERA. A class of events is observed with little hadronic activity between the jets. The jets are separated by pseudorapidity intervals (∆η) of up to four units and have transverse energies greater than 6 GeV. A gap is defined as the absence between the jets of ...

2016
V. Khachatryan

Measurements are presented of the cross section for the production of at least four jets, of which at least two originate from b quarks, in proton-proton collisions. Data collected with the CMS detector at the LHC at a center-of-mass energy of 7 TeV are used, corresponding to an integrated luminosity of 3 pb−1. The cross section is measured as a function of the jet transverse momentum for pT > ...

2007
Daniel González-Jiménez Manuele Bicego Johan W. H. Tangelder Ben A. M. Schouten Onkar Ambekar José Luis Alba-Castro Enrico Grosso Massimo Tistarelli

Local Gabor features (jets) have been widely used in face recognition systems. Once the sets of jets have been extracted from the two faces to be compared, a proper measure of similarity (or distance) between corresponding features should be chosen. For instance, in the well known Elastic Bunch Graph Matching (EBGM) approach and other Gabor-based face recognition systems, the cosine distance wa...

2008
Assaf Sternberg Noam Soker

We conduct hydrodynamical numerical simulations and find that precessing massive slow jets can inflate fat bubbles, i.e., more or less spherical bubbles, that are attached to the center of clusters of galaxies. To inflate a fat bubble the jet should precess fast. The precessing angle θ should be large, or change over a large range 0 ≤ θ ≤ θmax ∼ 30 − 70 ◦ (depending also on other parameters), w...

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