Number of the records: 1
Search for Higgs boson pair production in the γγWW.sup.∗./sup. channel using pp collision data recorded at √s=13 TeV with the ATLAS detector
- 1.0519484 - FZÚ 2020 RIV DE eng J - Journal Article
Aaboud, M. - Aad, G. - Abbott, B. - Chudoba, Jiří - Hejbal, Jiří - Hladík, Ondřej - Jačka, Petr - Jakoubek, Tomáš - Kepka, Oldřich - Kroll, Jiří - Kupčo, Alexander - Lokajíček, Miloš - Lysák, Roman - Marčišovský, Michal - Mikeštíková, Marcela - Němeček, Stanislav - Penc, Ondřej - Šícho, Petr - Staroba, Pavel - Svatoš, Michal - Taševský, Marek … Total 2915 authors
Search for Higgs boson pair production in the γγWW∗ channel using pp collision data recorded at √s=13 TeV with the ATLAS detector.
European Physical Journal C. Roč. 78, č. 12 (2018), s. 1-26, č. článku 1007. ISSN 1434-6044. E-ISSN 1434-6052
R&D Projects: GA MŠMT LM2015058
Institutional support: RVO:68378271
Keywords : ATLAS * CERN LHC Coll * channel cross section: upper limit * channel cross section: branching ratio: upper limit * mass dependence
OECD category: Particles and field physics
Impact factor: 4.843, year: 2018
Method of publishing: Open access
Searches for non-resonant and resonant Higgs boson pair production are performed in the γγWW∗ channel with the final state of γγℓνjj using 36.1 fb−1 of proton–proton collision data recorded at a centre-of-mass energy of s√= 13 TeV by the ATLAS detector at the Large Hadron Collider. No significant deviation from the Standard Model prediction is observed. A 95% confidence-level observed upper limit of 7.7 pb is set on the cross section for non-resonant production, while the expected limit is 5.4 pb. A search for a narrow-width resonance X decaying to a pair of Standard Model Higgs bosons HH is performed with the same set of data, and the observed upper limits on σ(pp→X)×B(X→HH) range between 40.0 and 6.1 pb for masses of the resonance between 260 and 500 GeV, while the expected limits range between 17.6 and 4.4 pb. When deriving the limits above, the Standard Model branching ratios of the H→γγ and H→WW∗ are assumed.
Permanent Link: http://hdl.handle.net/11104/0304458
File Download Size Commentary Version Access 0519484.pdf 0 2.4 MB CC licence Publisher’s postprint open-access
Number of the records: 1