Abstract
The new particle X recently discovered by the ATLAS and CMS Collaborations in searches for the Higgs boson has been observed to decay into γγ, ZZ ∗ and WW ∗, but its spin and parity, J P, remain a mystery, with J P=0+ and 2+ being open possibilities. We use PYTHIA and Delphes to simulate an analysis of the angular distribution of gg→X→γγ decays in a full 2012 data set, including realistic background levels. We show that this angular distribution should provide strong discrimination between the possibilities of spin zero and spin two with graviton-like couplings: ∼3σ if a conservative symmetric interpretation of the log-likelihood ratio (LLR) test statistic is used, and ∼6σ if a less conservative asymmetric interpretation is used. The WW and ZZ couplings of the Standard Model Higgs boson and of a 2+ particle with graviton-like couplings are both expected to exhibit custodial symmetry. We simulate the present ATLAS and CMS search strategies for X→WW ∗ using PYTHIA and Delphes, and show that their efficiencies in the case of a spin-2 particle with graviton-like couplings are a factor ≃1.9 smaller than in the spin-0 case. On the other hand, the ratio of \(X_{2^{+}} \to W W^{\ast}\) and ZZ ∗ branching ratios is larger than that in the 0+ case by a factor ≃1.3. We find that the current ATLAS and CMS results for X→WW ∗ and X→ZZ ∗ decays are compatible with custodial symmetry under both the spin-0 and -2 hypotheses, and that the data expected to become available during 2012 are unlikely to discriminate significantly between these possibilities.
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Notes
We note that in flat extra dimensions one typically finds conservation of a Kaluza–Klein parity that would forbid the coupling of the massive graviton to two light Standard Model particles.
To the extent that these other production mechanisms are suppressed relative to gg→X, their inclusion or omission is not important. We have checked that their inclusion in our simulation does not affect significantly the angular distributions from gg→X alone.
We define \(p_{Tt} \equiv|\vec{p}_{T}^{\gamma \gamma} \times\vec{t}|\), where the thrust vector is defined as \(\vec{t} \equiv(\vec{p}_{T}^{\gamma_{1}}-\vec{p}_{T}^{\gamma_{1}})/|\vec {p}_{T}^{\gamma_{1}}+\vec{p}_{T}^{\gamma_{1}}|\).
For a discussion of the relative merits of the LLR and the asymmetry variable, see [77].
This is the one-sided definition most commonly used in the literature, as opposed to the two-sided convention sometimes seen, which generally yields a higher number of standard deviations for the same p-value.
Adding a 1 % error in N tot does not affect the results.
We implement the relevant quality and isolation criteria at the level of the Delphes simulation.
We cannot use for this purpose the value of λ WZ quoted in [84], because this incorporates information from a combination of channels including X→γγ, which supplies information on a W that does not apply to the spin-2 case.
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Acknowledgements
We thank Oliver Buchmüller, Ben Gripaios, Rakhi Mahbubani, Eduard Massó, and Pierre Savard for valuable discussions. The work of J.E. was supported partly by the London Centre for Terauniverse Studies (LCTS), using funding from the European Research Council via the Advanced Investigator Grant 267352. The work of D.S.H. was supported partly by the Korea Foundation for International Cooperation of Science & Technology (KICOS) and the Basic Science Research Programme of the National Research Foundation of Korea (2012-0002959). The work of T.Y. was supported by a Graduate Teaching Assistantship from King’s College London. J.E., D.S.H. and V.S. thank CERN for kind hospitality, and T.Y. thanks Prof. T. Kobayashi and the Bilateral International Exchange Program of Kyoto University for kind hospitality.
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Ellis, J., Fok, R., Hwang, D.S. et al. Distinguishing ‘Higgs’ spin hypotheses using γγ and WW ∗ decays. Eur. Phys. J. C 73, 2488 (2013). https://doi.org/10.1140/epjc/s10052-013-2488-5
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DOI: https://doi.org/10.1140/epjc/s10052-013-2488-5