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Bharti Rawat

Publications and source records attributed to Bharti Rawat.

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ILC sensitivity for leptophilic scalar dark matter

We explore the viability of detecting a leptophilic scalar dark matter at the ILC in a simplified model approach. We present the constraints on the couplings of scalar dark matter with the standard model fermions ensuing from the relic density bounds deduced from the 2018 Planck data. We, then, present the reach of the ILC in terms of $Λ$, the scale of the effective theory, by performing a detailed analysis for the $Z$ associated DM pair production (i.e., $ e^+ e^- \rightarrow 2 $ jets + $\not \!\! E_T$, $ e^+ e^- \rightarrow μ^+ μ^-$ + $\not \!\! E_T$ and $ e^+ e^- \rightarrow e^+ e^-$ + $\not \!\! E_T$). We present the results for various run scenarios as 3-$σ$ contours in the $m_ϕ-Λ$ plane. We also analyze the effect of beam polarization on the sensitivity of this search. We find that for the process with two hadronic jets in the final state, ILC can probe $Λ$ up to 1.76 TeV for $\sqrt{s}= 1$ TeV that can further enhance to 1.99 TeV, after the inclusion of polarization effects.

hep-ph

Signals of Leptophilic Dark Matter at the ILC

Adopting a model independent approach, we constrain the various effective interactions of leptophilic DM particle with the visible world from the WMAP and Planck data. The thermally averaged indirect DM annihilation cross-section and the DM-electron direct-detection cross-section for such a DM candidate are observed to be consistent with the respective experimental data. We study the production of cosmologically allowed leptophilic DM in association with $Z\, (Z\to f\bar f)$, $f\equiv q,\,e^-,\, μ^-$ at the ILC. We perform the $χ^2$ analysis and compute the 99\% C.L. acceptance contours in the $m_χ$ and $Λ$ plane from the two dimensional differential distributions of various kinematic observables obtained after employing parton showering and hadronization to the simulated data. We observe that the dominant hadronic channel provides the best kinematic reach of 2.62 TeV ($m_χ$ = 25 GeV), which further improves to 3.13 TeV for polarized beams at $\sqrt{s} = 1$ TeV and an integrated luminosity of 1 ab$^{-1}$.

hep-ph