Probing the low mass pseudoscalar in flipped Two Higgs Doublet Model
Dilip Kumar Ghosh, Biswarup Mukhopadhyaya, Sirshendu Samanta, Ritesh K. Singh
TL;DR
This work investigates the viability of a light pseudoscalar $A$ in the flipped 2HDM (with $m_A$ in the 20–60 GeV range) and proposes a collider search in the channel $pp\to h\to AZ(Z^*)\to bb\ell^+\ell^-$. Using MCMC scans to identify phenomenologically allowed regions and representative benchmarks, the study demonstrates that the signal can be probed despite dominant $A\to bb$ decays by exploiting the leptonic $Z$ tag and the Higgs-mediated production. Cut-based analyses at the HL-LHC show strong potential, particularly around $m_A \approx 30$ GeV, with significances up to ~15σ (10% systematics); a BDT approach further enhances sensitivity, extending reach to higher $m_A$ and improving discovery prospects. The results indicate that dedicated searches in this channel could reveal or constrain flipped 2HDM scenarios in the low-mass pseudoscalar regime, with some regions already accessible in Run II.
Abstract
The phenomenology of the flipped two-Higgs-doublet model (2HDM) is relatively less explored so far, as compared to the other, commonly discussed, types. It is found that this scenario, like several others, admits of a light neutral pseudoscalar $A$ in the mass range 20 - 60 GeV, consistently with all current experimental data and theoretical constraints. However, the fact that such a pseudoscalar decays overwhelmingly into a $b\bar{b}$ pair makes its identification at the Large Hadron Collider (LHC) a challenging task. After identifying the region of the flipped 2HDM parameter space yielding a light pseudoscalar, we identify a useful search channel in the process $pp \rightarrow A Z(Z^{*}) \rightarrow b\bar{b} \ell^+ \ell^-$. A cut-based analysis, followed by one based on Boosted Decision Trees, shows that the light-$A$ scenario in flipped 2HDM should be detectable with rather high statistical significance at the high-luminosity LHC run, even after including systematic uncertainties. Furthermore, part of the parameter space, especially around $m_A = 30 - 40$ GeV is amenable to detection at the discovery level within Run-2 itself.
