Dergi makalesi Açık Erişim
CERN İşbirliği
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<identifier identifierType="URL">https://aperta.ulakbim.gov.tr/record/274643</identifier>
<creators>
<creator>
<creatorName>CERN İşbirliği</creatorName>
<affiliation>CERN</affiliation>
</creator>
</creators>
<titles>
<title>Search For The Exclusive $W$ Boson Hadronic Decays ${W}^{±}\To {\Pi }^{±}\Gamma $, ${W}^{±}\To {K}^{±}\Gamma $ And ${W}^{±}\To {\Rho }^{±}\Gamma $ With The Atlas Detector</title>
</titles>
<publisher>Aperta</publisher>
<publicationYear>2024</publicationYear>
<dates>
<date dateType="Issued">2024-10-17</date>
</dates>
<resourceType resourceTypeGeneral="Text">Journal article</resourceType>
<alternateIdentifiers>
<alternateIdentifier alternateIdentifierType="url">https://aperta.ulakbim.gov.tr/record/274643</alternateIdentifier>
</alternateIdentifiers>
<relatedIdentifiers>
<relatedIdentifier relatedIdentifierType="DOI" relationType="IsIdenticalTo">10.1103/PhysRevLett.133.161804</relatedIdentifier>
</relatedIdentifiers>
<rightsList>
<rights rightsURI="http://www.opendefinition.org/licenses/cc-by">Creative Commons Attribution</rights>
<rights rightsURI="info:eu-repo/semantics/openAccess">Open Access</rights>
</rightsList>
<descriptions>
<description descriptionType="Abstract"><p>A search for the exclusive hadronic decays ${W}^{±}\to {\pi }^{±}\gamma $, ${W}^{±}\to {K}^{±}\gamma $, and ${W}^{±}\to {\rho }^{±}\gamma $ is performed using up to $140\text{}\text{}{\mathrm{fb}}^{-1}$ of proton-proton collisions recorded with the ATLAS detector at a center-of-mass energy of $\sqrt{s}=13\text{}\text{}\mathrm{TeV}$. If observed, these rare processes would provide a unique test bench for the quantum chromodynamics factorization formalism used to calculate cross sections at colliders. Additionally, at future colliders, these decays could offer a new way to measure the $W$ boson mass through fully reconstructed decay products. The search results in the most stringent upper limits to date on the branching fractions $B\left({W}^{±}\to {\pi }^{±}\gamma \right)&lt;1.9×{10}^{-6}$, $B\left({W}^{±}\to {K}^{±}\gamma \right)&lt;1.7×{10}^{-6}$, $B\left({W}^{±}\to {\rho }^{±}\gamma \right)&lt;5.2×{10}^{-6}$ at 95% confidence level.</p></description>
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