Measurement of the ratio of inclusive cross sections<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:mi>σ</mml:mi><mml:mo stretchy="false">(</mml:mo><mml:mi>p</mml:mi><mml:mover accent="true"><mml:mrow><mml:mi>p</mml:mi></mml:mrow><mml:mrow><mml:mo accent="true" stretchy="false">¯</mml:mo></mml:mrow></mml:mover><mml:mo stretchy="false">→</mml:mo><mml:mi>Z</mml:mi><mml:mo>+</mml:mo><mml:mn>2</mml:mn><mml:mi>b</mml:mi><mml:mtext> </mml:mtext><mml:mi>jets</mml:mi><mml:mtext> </mml:mtext><mml:mo>/</mml:mo><mml:mi>σ</mml:mi><mml:mo stretchy="false">(</mml:mo><mml:mi>p</mml:mi><mml:mover accent="true"><mml:mrow><mml:mi>p</mml:mi></mml:mrow><mml:mrow><mml:mo accent="true" stretchy="false">¯</mml:mo></mml:mrow></mml:mover><mml:mo stretchy="false">→</mml:mo><mml:mi>Z</mml:mi><mml:mo>+</mml:mo><mml:mn>2</mml:mn><mml:mtext> </mml:mtext><mml:mi>jets</mml:mi><mml:mo stretchy="false">)</mml:mo></mml:mrow></mml:math>in<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mi>p</mml:mi><mml:mover accent="true"><mml:mi>p</mml:mi><mml:mo accent="true" stretchy="false">¯</mml:mo></mml:mover></mml:math>collisions at<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:msqrt><mml:mrow><mml:mi>s</mml:mi></mml:mrow></mml:msqrt><mml:mo>=</mml:mo><mml:mn>1.96</mml:mn><mml:mtext> </mml:mtext><mml:mtext> </mml:mtext><mml:mi>TeV</mml:mi></mml:mrow></mml:math>
V. M. Abazov(Joint Institute for Nuclear Research), M. Buehler(Fermi National Accelerator Laboratory), C. Ávila(Universidad de Los Andes), X. B. Bu(Fermi National Accelerator Laboratory), D. Brown, I. A. Bertram(Lancaster University), B. S. Acharya(The Abdus Salam International Centre for Theoretical Physics (ICTP)), M. Borysova(Taras Shevchenko National University of Kyiv), A. Boehnlein(Fermi National Accelerator Laboratory), R. Beuselinck(Imperial College London), O. Brandt(University of Göttingen), S. Bhatia(University of Mississippi), A. Bross, A. Brandt(Bundesministerium für Forschung, Technologie und Raumfahrt), U. Bassler(Commissariat à l'Énergie Atomique et aux Énergies Alternatives), G. Borissov(Lancaster University), J. P. Agnew(University of Manchester), T. Adams(Centre National de la Recherche Scientifique), S. Blessing(Florida State University), Andrew Askew(Florida State University), V. Bhatnagar(Panjab University), P. Baringer(University of Kansas), A. Bean, V. Bazterra(University of Illinois Chicago), E. E. Boos(Lomonosov Moscow State University), R. Bernhard(University of Freiburg), F. Badaud(Centre National de la Recherche Scientifique), J. F. Bartlett(Fermi National Accelerator Laboratory), P. C. Bhat(Fermi National Accelerator Laboratory), G. Bernardi(Centre National de la Recherche Scientifique), K. Augsten(Czech Technical University in Prague), G. Alkhazov(Petersburg Nuclear Physics Institute), M. Begalli(Universidade do Estado do Rio de Janeiro), S. B. Beri(Panjab University), D. V. Bandurin(Florida State University), L. Bagby(Centre National de la Recherche Scientifique), M. Besançon(Commissariat à l'Énergie Atomique et aux Énergies Alternatives), E. Barberis(Northeastern University), L. Bellantoni(Fermi National Accelerator Laboratory), K. Bloom(Invicro (United States)), S. Banerjee(University of Victoria), G. D. Alexeev(Joint Institute for Nuclear Research), M. Adams(University of Illinois Chicago), R. Brock(Michigan State University), D. Boline(State University of New York), S. Atkins(Louisiana Tech University), B. Abbott(University of Oklahoma), B. Baldin(Fermi National Accelerator Laboratory), G. Blazey(Northern Illinois University)
Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields
March 17, 2015
Cited by 6
Related Papers
Measurements of the Higgs boson production and decay rates and constraints on its couplings from a combined ATLAS and CMS analysis of the LHC pp collision data at s = 7 $$ \sqrt{s}=7 $$ and 8 TeV
|Journal of High Energy Physics|2016|1.1k
Performance of the ATLAS trigger system in 2015
|The European Physical Journal C|2017|1k
The Electromagnetic Counterpart of the Binary Neutron Star Merger LIGO/Virgo GW170817. II. UV, Optical, and Near-infrared Light Curves and Comparison to Kilonova Models
|The Astrophysical Journal Letters|2017|1k