{"title":"Simulation of the process e+e−→W+W− with the heavy right-handed neutrino exchange at 1 TeV future lepton colliders","authors":"A. Drutskoy, E. Vasenin","doi":"10.1103/physrevd.111.015025","DOIUrl":null,"url":null,"abstract":"We study potential contribution of the heavy right-handed neutrino exchange in the process e</a:mi>+</a:mo></a:msup>e</a:mi>−</a:mo></a:msup>→</a:mo>W</a:mi>+</a:mo></a:msup>W</a:mi>−</a:mo></a:msup></a:math>. This process is sensitive to heavy neutrinos with masses larger than <d:math xmlns:d=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"><d:msqrt><d:mi>s</d:mi></d:msqrt></d:math>. The Monte Carlo simulation of the studied process is performed assuming the seesaw type-I model, where heavy right-handed neutrinos (heavy neutral leptons, HNLs) are introduced in the leptonic sector. Within the Standard Model (SM), the process has a large cross section described by diagrams with <f:math xmlns:f=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"><f:mi>s</f:mi></f:math>-channel <h:math xmlns:h=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"><h:mi>Z</h:mi><h:mo>/</h:mo><h:mi>γ</h:mi></h:math> exchange and <j:math xmlns:j=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"><j:mi>t</j:mi></j:math>-channel active neutrino exchange. Respectively, the <l:math xmlns:l=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"><l:mi>t</l:mi></l:math>-channel right-handed neutrino exchange amplitude will interfere with these SM amplitudes. However, the angular distributions of the <n:math xmlns:n=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"><n:mi>W</n:mi></n:math> boson production and decay are different for the right-handed neutrino and SM amplitudes. That can be used to evaluate potential HNL contribution using the extended likelihood method. The simulation of the <p:math xmlns:p=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"><p:msup><p:mi>e</p:mi><p:mo>+</p:mo></p:msup><p:msup><p:mi>e</p:mi><p:mo>−</p:mo></p:msup><p:mo stretchy=\"false\">→</p:mo><p:msup><p:mi>W</p:mi><p:mo>+</p:mo></p:msup><p:msup><p:mi>W</p:mi><p:mo>−</p:mo></p:msup></p:math> process is performed at the 1 TeV center-of-mass energy and polarization <s:math xmlns:s=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"><s:msub><s:mi mathvariant=\"script\">P</s:mi><s:mrow><s:msup><s:mi>e</s:mi><s:mo>+</s:mo></s:msup><s:msup><s:mi>e</s:mi><s:mo>−</s:mo></s:msup></s:mrow></s:msub></s:math> of (20%, <v:math xmlns:v=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"><v:mo>−</v:mo><v:mn>80</v:mn><v:mo>%</v:mo></v:math>), which is a standard option for the future linear <x:math xmlns:x=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"><x:msup><x:mi>e</x:mi><x:mo>+</x:mo></x:msup><x:msup><x:mi>e</x:mi><x:mo>−</x:mo></x:msup></x:math> International Linear Collider. Both <z:math xmlns:z=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"><z:mi>W</z:mi></z:math> bosons are reconstructed from two hadronic jets. Simulation of the SM background processes is also done. The beam-induced backgrounds and the initial state radiation effects are taken into account. The majority of background processes are effectively suppressed by the cuts on the invariant masses of two and four jets. Finally, we obtain upper limits on the mixing parameter <bb:math xmlns:bb=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"><bb:mo stretchy=\"false\">|</bb:mo><bb:msub><bb:mi>V</bb:mi><bb:mrow><bb:mi>e</bb:mi><bb:mi>N</bb:mi></bb:mrow></bb:msub><bb:msup><bb:mo stretchy=\"false\">|</bb:mo><bb:mn>2</bb:mn></bb:msup></bb:math> as a function of <fb:math xmlns:fb=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"><fb:mi>M</fb:mi><fb:mo stretchy=\"false\">(</fb:mo><fb:mi>N</fb:mi><fb:mo stretchy=\"false\">)</fb:mo></fb:math>. <jats:supplementary-material> <jats:copyright-statement>Published by the American Physical Society</jats:copyright-statement> <jats:copyright-year>2025</jats:copyright-year> </jats:permissions> </jats:supplementary-material>","PeriodicalId":20167,"journal":{"name":"Physical Review D","volume":"30 1","pages":""},"PeriodicalIF":5.0000,"publicationDate":"2025-01-24","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"Physical Review D","FirstCategoryId":"101","ListUrlMain":"https://doi.org/10.1103/physrevd.111.015025","RegionNum":2,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q1","JCRName":"Physics and Astronomy","Score":null,"Total":0}
引用次数: 0
Abstract
We study potential contribution of the heavy right-handed neutrino exchange in the process e+e−→W+W−. This process is sensitive to heavy neutrinos with masses larger than s. The Monte Carlo simulation of the studied process is performed assuming the seesaw type-I model, where heavy right-handed neutrinos (heavy neutral leptons, HNLs) are introduced in the leptonic sector. Within the Standard Model (SM), the process has a large cross section described by diagrams with s-channel Z/γ exchange and t-channel active neutrino exchange. Respectively, the t-channel right-handed neutrino exchange amplitude will interfere with these SM amplitudes. However, the angular distributions of the W boson production and decay are different for the right-handed neutrino and SM amplitudes. That can be used to evaluate potential HNL contribution using the extended likelihood method. The simulation of the e+e−→W+W− process is performed at the 1 TeV center-of-mass energy and polarization Pe+e− of (20%, −80%), which is a standard option for the future linear e+e− International Linear Collider. Both W bosons are reconstructed from two hadronic jets. Simulation of the SM background processes is also done. The beam-induced backgrounds and the initial state radiation effects are taken into account. The majority of background processes are effectively suppressed by the cuts on the invariant masses of two and four jets. Finally, we obtain upper limits on the mixing parameter |VeN|2 as a function of M(N). Published by the American Physical Society2025
期刊介绍:
Physical Review D (PRD) is a leading journal in elementary particle physics, field theory, gravitation, and cosmology and is one of the top-cited journals in high-energy physics.
PRD covers experimental and theoretical results in all aspects of particle physics, field theory, gravitation and cosmology, including:
Particle physics experiments,
Electroweak interactions,
Strong interactions,
Lattice field theories, lattice QCD,
Beyond the standard model physics,
Phenomenological aspects of field theory, general methods,
Gravity, cosmology, cosmic rays,
Astrophysics and astroparticle physics,
General relativity,
Formal aspects of field theory, field theory in curved space,
String theory, quantum gravity, gauge/gravity duality.