CMS-HIG-17-006 ; CERN-EP-2017-168 | ||
Search for resonant and nonresonant Higgs boson pair production in the $\mathrm{ b \bar{b} } \ell\nu \ell\nu$ final state in proton-proton collisions at $ \sqrt{s} = $ 13 TeV | ||
CMS Collaboration | ||
14 August 2017 | ||
JHEP 01 (2018) 054 | ||
Abstract: Searches for resonant and nonresonant pair-produced Higgs bosons (HH) decaying respectively into $\ell\nu \ell\nu$, through either W or Z bosons, and $\mathrm{ b \bar{b} }$ are presented. The analyses are based on a sample of proton-proton collisions at $ \sqrt{s} = $ 13 TeV, collected by the CMS experiment at the LHC, corresponding to an integrated luminosity of 35.9 fb$^{-1}$. Data and predictions from the standard model are in agreement within uncertainties. For the standard model HH hypothesis, the data exclude at 95% confidence level a product of the production cross section and branching fraction larger than 72 fb, corresponding to 79 times the prediction, consistent with expectations. Constraints are placed on different scenarios considering anomalous couplings, which could affect the rate and kinematics of HH production. Upper limits at 95% confidence level are set on the production cross section of narrow-width spin-0 and spin-2 particles decaying to Higgs boson pairs, the latter produced with minimal gravity-like coupling. | ||
Links: e-print arXiv:1708.04188 [hep-ex] (PDF) ; CDS record ; inSPIRE record ; HepData record ; CADI line (restricted) ; |
Figures | |
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Figure 1:
Feynman diagrams for Higgs boson pair production via gluon fusion in the SM. The coupling modifiers for the Higgs boson self-coupling and the top quark Yukawa coupling are denoted by $\kappa _{\lambda }$ and $\kappa _\mathrm{ t } $, respectively. |
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Figure 1-a:
Feynman diagram for Higgs boson pair production via gluon fusion in the SM. The coupling modifiers for the Higgs boson self-coupling and the top quark Yukawa coupling are denoted by $\kappa _{\lambda }$ and $\kappa _\mathrm{ t } $, respectively. |
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Figure 1-b:
Feynman diagram for Higgs boson pair production via gluon fusion in the SM. The coupling modifier for the top quark Yukawa coupling is denoted by $\kappa _\mathrm{ t } $. |
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Figure 2:
The dijet $ {p_{\mathrm {T}}} $ distributions in data and simulated events after requiring two leptons, two b-tagged jets, and 12 $ < {m_{\ell \ell }} < m_{\mathrm{ Z } } - $ 15 GeV, for $\mathrm{ e }^{+} \mathrm{ e }^{-} $ (top left), $\mathrm{ e }^{\mp} {\mu ^\mp } $ (top right), and $\mu^{+} \mu^{-} $ (bottom) events. The various signal hypotheses displayed have been scaled to a cross section of 5 pb for display purposes. Error bars indicate statistical uncertainties, while shaded bands show post-fit systematic uncertainties. |
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Figure 2-a:
The dijet $ {p_{\mathrm {T}}} $ distributions in data and simulated events after requiring two leptons, two b-tagged jets, and 12 $ < {m_{\ell \ell }} < m_{\mathrm{ Z } } - $ 15 GeV, for $\mathrm{ e }^{+} \mathrm{ e }^{-} $ events. The various signal hypotheses displayed have been scaled to a cross section of 5 pb for display purposes. Error bars indicate statistical uncertainties, while shaded bands show post-fit systematic uncertainties. |
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Figure 2-b:
The dijet $ {p_{\mathrm {T}}} $ distributions in data and simulated events after requiring two leptons, two b-tagged jets, and 12 $ < {m_{\ell \ell }} < m_{\mathrm{ Z } } - $ 15 GeV, for $\mathrm{ e }^{\mp} {\mu ^\mp } $ events. The various signal hypotheses displayed have been scaled to a cross section of 5 pb for display purposes. Error bars indicate statistical uncertainties, while shaded bands show post-fit systematic uncertainties. |
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Figure 2-c:
The dijet $ {p_{\mathrm {T}}} $ distributions in data and simulated events after requiring two leptons, two b-tagged jets, and 12 $ < {m_{\ell \ell }} < m_{\mathrm{ Z } } - $ 15 GeV, for $\mu^{+} \mu^{-} $ events. The various signal hypotheses displayed have been scaled to a cross section of 5 pb for display purposes. Error bars indicate statistical uncertainties, while shaded bands show post-fit systematic uncertainties. |
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Figure 3:
Performance of the parameterised DNN for the resonant search, shown as the selection efficiency for the $ {m_{\text {X}}} =$ 650 GeV signal as a function of the selection efficiency for the background (ROC curve), for the combined $ {\mathrm {e}^+} {\mathrm {e}^-}$, $ {\mu ^+} {\mu ^-} $ and $ {\mathrm {e}^\pm} {\mu ^\mp} $ channels. The dashed line corresponds to the DNN used in the analysis, trained on all available signal samples, and evaluated at $ {m_{\text {X}}} =$ 650 GeV. The dotted line shows an alternative DNN trained using all signal samples except for $ {m_{\text {X}}} =$ 650 GeV, and evaluated at $ {m_{\text {X}}} =$ 650 GeV. Both curves overlap, indicating that the parameterised DNN is able to generalise to cases not seen during the training phase by interpolating the signal behaviour from nearby $ {m_{\text {X}}} $ points. |
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Figure 3-a:
Performance of the parameterised DNN for the resonant search, shown as the selection efficiency for the $ {m_{\text {X}}} =$ 650 GeV signal as a function of the selection efficiency for the background (ROC curve), for the combined $ {\mathrm {e}^+} {\mathrm {e}^-}$, $ {\mu ^+} {\mu ^-} $ and $ {\mathrm {e}^\pm} {\mu ^\mp} $ channels. The dashed line corresponds to the DNN used in the analysis, trained on all available signal samples, and evaluated at $ {m_{\text {X}}} =$ 650 GeV. The dotted line shows an alternative DNN trained using all signal samples except for $ {m_{\text {X}}} =$ 650 GeV, and evaluated at $ {m_{\text {X}}} =$ 650 GeV. Both curves overlap, indicating that the parameterised DNN is able to generalise to cases not seen during the training phase by interpolating the signal behaviour from nearby $ {m_{\text {X}}} $ points. |
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Figure 3-b:
Performance of the parameterised DNN for the resonant search, shown as the selection efficiency for the $ {m_{\text {X}}} =$ 650 GeV signal as a function of the selection efficiency for the background (ROC curve), for the combined $ {\mathrm {e}^+} {\mathrm {e}^-}$, $ {\mu ^+} {\mu ^-} $ and $ {\mathrm {e}^\pm} {\mu ^\mp} $ channels. The dashed line corresponds to the DNN used in the analysis, trained on all available signal samples, and evaluated at $ {m_{\text {X}}} =$ 650 GeV. The dotted line shows an alternative DNN trained using all signal samples except for $ {m_{\text {X}}} =$ 650 GeV, and evaluated at $ {m_{\text {X}}} =$ 650 GeV. Both curves overlap, indicating that the parameterised DNN is able to generalise to cases not seen during the training phase by interpolating the signal behaviour from nearby $ {m_{\text {X}}} $ points. |
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Figure 3-c:
Performance of the parameterised DNN for the resonant search, shown as the selection efficiency for the $ {m_{\text {X}}} =$ 650 GeV signal as a function of the selection efficiency for the background (ROC curve), for the combined $ {\mathrm {e}^+} {\mathrm {e}^-}$, $ {\mu ^+} {\mu ^-} $ and $ {\mathrm {e}^\pm} {\mu ^\mp} $ channels. The dashed line corresponds to the DNN used in the analysis, trained on all available signal samples, and evaluated at $ {m_{\text {X}}} =$ 650 GeV. The dotted line shows an alternative DNN trained using all signal samples except for $ {m_{\text {X}}} =$ 650 GeV, and evaluated at $ {m_{\text {X}}} =$ 650 GeV. Both curves overlap, indicating that the parameterised DNN is able to generalise to cases not seen during the training phase by interpolating the signal behaviour from nearby $ {m_{\text {X}}} $ points. |
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Figure 4:
The ${m_{ {\mathrm {j}} {\mathrm {j}} }}$ distribution in data and simulated events after requiring all selection criteria in the $\mathrm{ e }^{+} \mathrm{ e }^{-} $ (top left), $\mathrm{ e }^{\mp} {\mu ^\mp } $ (top right), and $\mu^{+} \mu^{-} $ (bottom) channels. The various signal hypotheses displayed have been scaled to a cross section of 5 pb for display purposes. Error bars indicate statistical uncertainties, while shaded bands show post-fit systematic uncertainties. |
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Figure 4-a:
The ${m_{ {\mathrm {j}} {\mathrm {j}} }}$ distribution in data and simulated events after requiring all selection criteria in the $\mathrm{ e }^{+} \mathrm{ e }^{-} $ channel. The various signal hypotheses displayed have been scaled to a cross section of 5 pb for display purposes. Error bars indicate statistical uncertainties, while shaded bands show post-fit systematic uncertainties. |
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Figure 4-b:
The ${m_{ {\mathrm {j}} {\mathrm {j}} }}$ distribution in data and simulated events after requiring all selection criteria in the $\mathrm{ e }^{\mp} {\mu ^\mp } $ channel. The various signal hypotheses displayed have been scaled to a cross section of 5 pb for display purposes. Error bars indicate statistical uncertainties, while shaded bands show post-fit systematic uncertainties. |
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Figure 4-c:
The ${m_{ {\mathrm {j}} {\mathrm {j}} }}$ distribution in data and simulated events after requiring all selection criteria in the $\mu^{+} \mu^{-} $ channel. The various signal hypotheses displayed have been scaled to a cross section of 5 pb for display purposes. Error bars indicate statistical uncertainties, while shaded bands show post-fit systematic uncertainties. |
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Figure 5:
The DNN output distributions in data and simulated events after requiring all selection criteria, in the $ {\mathrm {e}^+} {\mathrm {e}^-}$ (top), $ {\mathrm {e}^\pm} {} {\mu ^\mp} $ (middle), and $ {\mu ^+} {\mu ^-} $ (bottom) channels. Output values towards 0 are background-like, while output values towards 1 are signal-like. The parameterised resonant DNN output (left) is evaluated at $ {m_{\text {X}}} = $ 400 GeV and the parameterised nonresonant DNN output (right) is evaluated at $\kappa _{\lambda} =1$, $\kappa _{{\mathrm {t}}} =$ 1. The two signal hypotheses displayed have been scaled to a cross section of 5 pb for display purposes. Error bars indicate statistical uncertainties, while shaded bands show post-fit systematic uncertainties. |
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Figure 5-a:
The DNN output distributions in data and simulated events after requiring all selection criteria, in the $ {\mathrm {e}^+} {\mathrm {e}^-}$ channel. Output values towards 0 are background-like, while output values towards 1 are signal-like. The parameterised resonant DNN output is evaluated at $ {m_{\text {X}}} = $ 400 GeV. The signal hypothesis has been scaled to a cross section of 5 pb for display purposes. Error bars indicate statistical uncertainties, while shaded bands show post-fit systematic uncertainties. |
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Figure 5-b:
The DNN output distributions in data and simulated events after requiring all selection criteria, in the $ {\mathrm {e}^+} {\mathrm {e}^-}$ channel. Output values towards 0 are background-like, while output values towards 1 are signal-like. The parameterised nonresonant DNN output is evaluated at $\kappa _{\lambda} =1$, $\kappa _{{\mathrm {t}}} =$ 1. The signal hypothesis has been scaled to a cross section of 5 pb for display purposes. Error bars indicate statistical uncertainties, while shaded bands show post-fit systematic uncertainties. |
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Figure 5-c:
The DNN output distributions in data and simulated events after requiring all selection criteria, in the $ {\mathrm {e}^\pm} {} {\mu ^\mp} $ channel. Output values towards 0 are background-like, while output values towards 1 are signal-like. The parameterised resonant DNN output is evaluated at $ {m_{\text {X}}} = $ 400 GeV. The signal hypothesis has been scaled to a cross section of 5 pb for display purposes. Error bars indicate statistical uncertainties, while shaded bands show post-fit systematic uncertainties. |
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Figure 5-d:
The DNN output distributions in data and simulated events after requiring all selection criteria, in the $ {\mathrm {e}^\pm} {} {\mu ^\mp} $ channel. Output values towards 0 are background-like, while output values towards 1 are signal-like. The parameterised nonresonant DNN output is evaluated at $\kappa _{\lambda} =1$, $\kappa _{{\mathrm {t}}} =$ 1. The signal hypothesis has been scaled to a cross section of 5 pb for display purposes. Error bars indicate statistical uncertainties, while shaded bands show post-fit systematic uncertainties. |
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Figure 5-e:
The DNN output distributions in data and simulated events after requiring all selection criteria, in the $ {\mu ^+} {\mu ^-} $ channel. Output values towards 0 are background-like, while output values towards 1 are signal-like. The parameterised resonant DNN output is evaluated at $ {m_{\text {X}}} = $ 400 GeV. The signal hypothesis has been scaled to a cross section of 5 pb for display purposes. Error bars indicate statistical uncertainties, while shaded bands show post-fit systematic uncertainties. |
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Figure 5-f:
The DNN output distributions in data and simulated events after requiring all selection criteria, in the $ {\mu ^+} {\mu ^-} $ channel. Output values towards 0 are background-like, while output values towards 1 are signal-like. The parameterised nonresonant DNN output is evaluated at $\kappa _{\lambda} =1$, $\kappa _{{\mathrm {t}}} =$ 1. The signal hypothesis has been scaled to a cross section of 5 pb for display purposes. Error bars indicate statistical uncertainties, while shaded bands show post-fit systematic uncertainties. |
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Figure 6:
The DNN output distributions in data and simulated events, for the $ {\mathrm {e}^+} {\mathrm {e}^-}$ (top), $ {\mathrm {e}^\pm} {} {\mu ^\mp} $ (middle), and $ {\mu ^+} {\mu ^-} $ (bottom) channels, in three different ${m_{{\mathrm {j}} {\mathrm {j}}}}$ regions: $ {m_{{\mathrm {j}} {\mathrm {j}}}} < $ 75 GeV, $ {m_{{\mathrm {j}} {\mathrm {j}}}} \in $ [75,140] GeV, and $ {m_{{\mathrm {j}} {\mathrm {j}}}} \geq $ 140 GeV. The parameterised resonant DNN output (left) is evaluated at $ {m_{\text {X}}} = $ 400 GeV and the parameterised nonresonant DNN output (right) is evaluated at $\kappa _{\lambda} = $ 1, $\kappa _{{\mathrm {t}}} = $ 1. The two signal hypotheses displayed have been scaled to a cross section of 5 pb for display purposes. Error bars indicate statistical uncertainties, while shaded bands show post-fit systematic uncertainties. |
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Figure 6-a:
The DNN output distributions in data and simulated events, for the $ {\mathrm {e}^+} {\mathrm {e}^-}$ channel, in three different ${m_{{\mathrm {j}} {\mathrm {j}}}}$ regions: $ {m_{{\mathrm {j}} {\mathrm {j}}}} < $ 75 GeV, $ {m_{{\mathrm {j}} {\mathrm {j}}}} \in $ [75,140] GeV, and $ {m_{{\mathrm {j}} {\mathrm {j}}}} \geq $ 140 GeV. The parameterised resonant DNN output (left) is evaluated at $ {m_{\text {X}}} = $ 400 GeV. The signal hypothesis has been scaled to a cross section of 5 pb for display purposes. Error bars indicate statistical uncertainties, while shaded bands show post-fit systematic uncertainties. |
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Figure 6-b:
The DNN output distributions in data and simulated events, for the $ {\mathrm {e}^+} {\mathrm {e}^-}$ channel, in three different ${m_{{\mathrm {j}} {\mathrm {j}}}}$ regions: $ {m_{{\mathrm {j}} {\mathrm {j}}}} < $ 75 GeV, $ {m_{{\mathrm {j}} {\mathrm {j}}}} \in $ [75,140] GeV, and $ {m_{{\mathrm {j}} {\mathrm {j}}}} \geq $ 140 GeV. The parameterised nonresonant DNN output is evaluated at $\kappa _{\lambda} = $ 1, $\kappa _{{\mathrm {t}}} = $ 1. The signal hypothesis has been scaled to a cross section of 5 pb for display purposes. Error bars indicate statistical uncertainties, while shaded bands show post-fit systematic uncertainties. |
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Figure 6-c:
The DNN output distributions in data and simulated events, for the $ {\mathrm {e}^\pm} {} {\mu ^\mp} $ channel, in three different ${m_{{\mathrm {j}} {\mathrm {j}}}}$ regions: $ {m_{{\mathrm {j}} {\mathrm {j}}}} < $ 75 GeV, $ {m_{{\mathrm {j}} {\mathrm {j}}}} \in $ [75,140] GeV, and $ {m_{{\mathrm {j}} {\mathrm {j}}}} \geq $ 140 GeV. The parameterised resonant DNN output (left) is evaluated at $ {m_{\text {X}}} = $ 400 GeV. The signal hypothesis has been scaled to a cross section of 5 pb for display purposes. Error bars indicate statistical uncertainties, while shaded bands show post-fit systematic uncertainties. |
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Figure 6-d:
The DNN output distributions in data and simulated events, for the $ {\mathrm {e}^\pm} {} {\mu ^\mp} $ channel, in three different ${m_{{\mathrm {j}} {\mathrm {j}}}}$ regions: $ {m_{{\mathrm {j}} {\mathrm {j}}}} < $ 75 GeV, $ {m_{{\mathrm {j}} {\mathrm {j}}}} \in $ [75,140] GeV, and $ {m_{{\mathrm {j}} {\mathrm {j}}}} \geq $ 140 GeV. The parameterised nonresonant DNN output is evaluated at $\kappa _{\lambda} = $ 1, $\kappa _{{\mathrm {t}}} = $ 1. The signal hypothesis has been scaled to a cross section of 5 pb for display purposes. Error bars indicate statistical uncertainties, while shaded bands show post-fit systematic uncertainties. |
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Figure 6-e:
The DNN output distributions in data and simulated events, for the $ {\mu ^+} {\mu ^-} $ channel, in three different ${m_{{\mathrm {j}} {\mathrm {j}}}}$ regions: $ {m_{{\mathrm {j}} {\mathrm {j}}}} < $ 75 GeV, $ {m_{{\mathrm {j}} {\mathrm {j}}}} \in $ [75,140] GeV, and $ {m_{{\mathrm {j}} {\mathrm {j}}}} \geq $ 140 GeV. The parameterised resonant DNN output (left) is evaluated at $ {m_{\text {X}}} = $ 400 GeV. The signal hypothesis has been scaled to a cross section of 5 pb for display purposes. Error bars indicate statistical uncertainties, while shaded bands show post-fit systematic uncertainties. |
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Figure 6-f:
The DNN output distributions in data and simulated events, for the $ {\mu ^+} {\mu ^-} $ channel, in three different ${m_{{\mathrm {j}} {\mathrm {j}}}}$ regions: $ {m_{{\mathrm {j}} {\mathrm {j}}}} < $ 75 GeV, $ {m_{{\mathrm {j}} {\mathrm {j}}}} \in $ [75,140] GeV, and $ {m_{{\mathrm {j}} {\mathrm {j}}}} \geq $ 140 GeV. The parameterised nonresonant DNN output is evaluated at $\kappa _{\lambda} = $ 1, $\kappa _{{\mathrm {t}}} = $ 1. The signal hypothesis has been scaled to a cross section of 5 pb for display purposes. Error bars indicate statistical uncertainties, while shaded bands show post-fit systematic uncertainties. |
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Figure 7:
Expected (dashed) and observed (continuous) 95% CL upper limits on the product of the production cross section for $\mathrm{X} $ and branching fraction for $\mathrm{X} \to \mathrm{ H } \mathrm{ H } \to {\mathrm{ b \bar{b} } } {\mathrm {V}} {\mathrm {V}} \to {\mathrm{ b \bar{b} } } \ell \nu \ell \nu $, as a function of $ {m_{\text {X}}} $. The inner (green) band and the outer (yellow) band indicate the regions containing 68 and 95%, respectively, of the distribution of limits expected under the background-only hypothesis. These limits are computed using the asymptotic $\mathrm {CL_s}$ method, combining the $\mathrm{ e }^{+} \mathrm{ e }^{-} $, $ \mu^+ \mu^-$ and $\mathrm{ e } ^{\pm }\mu ^{\mp }$ channels, for spin-0 (left) and spin-2 (right) hypotheses. The solid circles represent fully-simulated mass points. The dashed red lines represent possible cross sections for the production of a radion (left) or a Kaluza-Klein graviton (right), assuming absence of mixing with the Higgs boson [49]. Parameters used to compute these cross sections can be found in the legend. |
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Figure 7-a:
Expected (dashed) and observed (continuous) 95% CL upper limits on the product of the production cross section for $\mathrm{X} $ and branching fraction for $\mathrm{X} \to \mathrm{ H } \mathrm{ H } \to {\mathrm{ b \bar{b} } } {\mathrm {V}} {\mathrm {V}} \to {\mathrm{ b \bar{b} } } \ell \nu \ell \nu $, as a function of $ {m_{\text {X}}} $. The inner (green) band and the outer (yellow) band indicate the regions containing 68 and 95%, respectively, of the distribution of limits expected under the background-only hypothesis. These limits are computed using the asymptotic $\mathrm {CL_s}$ method, combining the $\mathrm{ e }^{+} \mathrm{ e }^{-} $, $ \mu^+ \mu^-$ and $\mathrm{ e } ^{\pm }\mu ^{\mp }$ channels, for the spin-0 hypothesis. The solid circles represent fully-simulated mass points. The dashed red lines represent possible cross sections for the production of a radion, assuming absence of mixing with the Higgs boson [49]. Parameters used to compute these cross sections can be found in the legend. |
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Figure 7-b:
Expected (dashed) and observed (continuous) 95% CL upper limits on the product of the production cross section for $\mathrm{X} $ and branching fraction for $\mathrm{X} \to \mathrm{ H } \mathrm{ H } \to {\mathrm{ b \bar{b} } } {\mathrm {V}} {\mathrm {V}} \to {\mathrm{ b \bar{b} } } \ell \nu \ell \nu $, as a function of $ {m_{\text {X}}} $. The inner (green) band and the outer (yellow) band indicate the regions containing 68 and 95%, respectively, of the distribution of limits expected under the background-only hypothesis. These limits are computed using the asymptotic $\mathrm {CL_s}$ method, combining the $\mathrm{ e }^{+} \mathrm{ e }^{-} $, $ \mu^+ \mu^-$ and $\mathrm{ e } ^{\pm }\mu ^{\mp }$ channels, for the spin-2 hypothesis. The solid circles represent fully-simulated mass points. The dashed red lines represent possible cross sections for the production of a Kaluza-Klein graviton, assuming absence of mixing with the Higgs boson [49]. Parameters used to compute these cross sections can be found in the legend. |
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Figure 8:
Left: expected (dashed) and observed (continuous) 95% CL upper limits on the product of the Higgs boson pair production cross section and branching fraction for $\mathrm{ H } \mathrm{ H } \to {\mathrm{ b \bar{b} } } {\mathrm {V}} {\mathrm {V}} \to {\mathrm{ b \bar{b} } } \ell \nu \ell \nu $ as a function of $\kappa _{\lambda } / \kappa _{\mathrm{ t } }$. The inner (green) band and the outer (yellow) band indicate the regions containing 68 and 95%, respectively, of the distribution of limits expected under the background-only hypothesis. Red lines show the theoretical cross sections, along with their uncertainties, for $\kappa _{\mathrm{ t } } = $ 1 (SM) and $\kappa _{\mathrm{ t } } = $ 2. Right: exclusions in the ($\kappa _{\lambda }$, $\kappa _{\mathrm{ t } }$) plane. The red region corresponds to parameters excluded at 95% CL with the observed data, whereas the dashed black line and the blue areas correspond to the expected exclusions and the 68 and 95% bands (light and dark respectively). Isolines of the product of the theoretical cross section and branching fraction for $\mathrm{ H } \mathrm{ H } \to {\mathrm{ b \bar{b} } } {\mathrm {V}} {\mathrm {V}} \to {\mathrm{ b \bar{b} } } \ell \nu \ell \nu $ are shown as dashed-dotted lines. The diamond marker indicates the prediction of the SM. All theoretical predictions are extracted from Refs. [12,13,14,15,16,17,84]. |
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Figure 8-a:
Expected (dashed) and observed (continuous) 95% CL upper limits on the product of the Higgs boson pair production cross section and branching fraction for $\mathrm{ H } \mathrm{ H } \to {\mathrm{ b \bar{b} } } {\mathrm {V}} {\mathrm {V}} \to {\mathrm{ b \bar{b} } } \ell \nu \ell \nu $ as a function of $\kappa _{\lambda } / \kappa _{\mathrm{ t } }$. The inner (green) band and the outer (yellow) band indicate the regions containing 68 and 95%, respectively, of the distribution of limits expected under the background-only hypothesis. Red lines show the theoretical cross sections, along with their uncertainties, for $\kappa _{\mathrm{ t } } = $ 1 (SM) and $\kappa _{\mathrm{ t } } = $ 2. |
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Figure 8-b:
Exclusions in the ($\kappa _{\lambda }$, $\kappa _{\mathrm{ t } }$) plane. The red region corresponds to parameters excluded at 95% CL with the observed data, whereas the dashed black line and the blue areas correspond to the expected exclusions and the 68 and 95% bands (light and dark respectively). Isolines of the product of the theoretical cross section and branching fraction for $\mathrm{ H } \mathrm{ H } \to {\mathrm{ b \bar{b} } } {\mathrm {V}} {\mathrm {V}} \to {\mathrm{ b \bar{b} } } \ell \nu \ell \nu $ are shown as dashed-dotted lines. The diamond marker indicates the prediction of the SM. All theoretical predictions are extracted from Refs. [12,13,14,15,16,17,84]. |
Tables | |
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Table 1:
Summary of the systematic uncertainties and their impact on total background yields and on the SM and $ {m_{\text {X}}} = 400$ GeV signal hypotheses in the signal region. |
Summary |
A search for resonant and nonresonant Higgs boson pair production (HH) is presented, where one of the Higgs bosons decays to $\mathrm{ b \bar{b} }$, and the other to $\mathrm{ V }\mathrm{ V } \to \ell\nu \ell\nu$, where V is either a W or a Z boson. The LHC proton-proton collision data at $\sqrt{s}= $ 13 TeV collected by the CMS experiment corresponding to an integrated luminosity of 35.9 fb$^{-1}$ are used. Masses are considered in the range between 260 and 900 GeV for the resonant search, while anomalous Higgs boson self-coupling and coupling to the top quark are considered in addition to the standard model case for the nonresonant search. The results obtained are in agreement, within uncertainties, with the predictions of the standard model. For the resonant search, the data exclude a product of the production cross section and branching fraction of narrow-width spin-0 particles from 430 to 17 fb, in agreement with the expectations of 340$^{+140}_{-100}$ to 14$^{+6}_{-4}$ fb, and narrow-width spin-2 particles produced with minimal gravity-like coupling from 450 to 14 fb, in agreement with the expectations of 360$^{+140}_{-100}$ to 13$^{+6}_{-4}$ fb. For the standard model HH hypothesis, the data exclude a product of the production cross section and branching fraction of 72 fb, corresponding to 79 times the SM cross section. The expected values exclude a product of the production cross section and branching fraction of 81$^{+42}_{-25}$ fb, corresponding to 89$^{+47}_{-28}$ times the SM cross section. |
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Compact Muon Solenoid LHC, CERN |