<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:msup><mml:mrow><mml:mi>Z</mml:mi></mml:mrow><mml:mrow><mml:mn>0...

Abstract

We present the invariant-mass distributions for the production of ${Z}^{0}$${Z}^{0}$ pairs by ${W}^{+}$${W}^{\mathrm{\ensuremath{-}}}$ and ${Z}^{0}$${Z}^{0}$ fusion at 40 TeV. Results are given for Higgs-boson masses of 0.5 and 1.0 TeV and a rapidity cut ${\ensuremath{\eta}}_{c}$ of 1.5. These calculations, which are performed using the effective-gauge-boson approximation, are compared with the corresponding results for the production of ${W}^{+}$${W}^{\mathrm{\ensuremath{-}}}$ pairs by the same fusion mechanism. A comparison between the approximate calculation and an exact calculation of ${Z}^{0}$${Z}^{0}$ pair production by ${W}^{+}$${W}^{\mathrm{\ensuremath{-}}}$ fusion is also presented.

Keywords

PhysicsPair productionParticle physicsBosonProduction (economics)Higgs bosonRapidityNuclear physicsFusionGauge bosonInvariant massGauge theoryHadron

Affiliated Institutions

Michigan State University US

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Publication Info

Year: 1988
Type: article
Volume: 37
Issue: 9
Pages: 2668-2671
Citations: 14
Access: Closed

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<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:msup><mml:mrow><mml:mi>Z</mml:mi></mml:mrow><mml:mrow><mml:mn>0</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math><mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:msup><mml:mrow><mml:mi>Z</mml:mi></mml:mrow><mml:mrow><mml:mn>0</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math>and<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:msup><mml:mrow><mml:mi>W</mml:mi></mml:mrow><mml:mrow><mml:mo>+</mml:mo></mml:mrow></mml:msup></mml:mrow></mml:math><mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:msup><mml:mrow><mml:mi>W</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">−</mml:mi></mml:mrow></mml:msup></mml:mrow></mml:math>pair production at supercollider energies

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APA Style

                            
                                    A. Abbasabadi, 
                                
                                    Wayne W. Repko
                                
                            (1988). 
                            <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:msup><mml:mrow><mml:mi>Z</mml:mi></mml:mrow><mml:mrow><mml:mn>0</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math><mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:msup><mml:mrow><mml:mi>Z</mml:mi></mml:mrow><mml:mrow><mml:mn>0</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math>and<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:msup><mml:mrow><mml:mi>W</mml:mi></mml:mrow><mml:mrow><mml:mo>+</mml:mo></mml:mrow></mml:msup></mml:mrow></mml:math><mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:msup><mml:mrow><mml:mi>W</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">−</mml:mi></mml:mrow></mml:msup></mml:mrow></mml:math>pair production at supercollider energies. 
                            Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields
                            , 37
                            (9)
                            , 2668-2671.
                            https://doi.org/10.1103/physrevd.37.2668

Identifiers

DOI: 10.1103/physrevd.37.2668