36 citations · 326 across the 26 of their papers we have counts for
26 papers
Confronting electroweak MSSM through one-loop renormalized neutralino-Higgs interactions for dark matter direct detection and muon
Subhadip Bisal, Arindam Chatterjee, Debottam Das +1
We compute the next-to-leading order (NLO) corrections to the vertices where a pair of the lightest neutralino couples to CP-even (light or heavy) Higgs scalars. In particular, the…
Radiative Corrections to Aid the Direct Detection of the Higgsino-like Neutralino Dark Matter: Spin-Independent Interactions
Subhadip Bisal, Arindam Chatterjee, Debottam Das +1
The lightest neutralino () is a good Dark Matter (DM) candidate in the R-parity conserving Minimal Supersymmetric Standard Model (MSSM). In this work, we consider the…
Prospects of a Strong first-order Electroweak Phase Transition in the -NMSSM
Arindam Chatterjee, AseshK Datta, Subhojit Roy
We have studied the viability and possible patterns of a strong first-order electroweak phase transition (SFOEWPT) within the -symmetric Next-to-Minimal Supersymmetric Standar…
Electroweak Phase Transition in the -invariant NMSSM: Implications of LHC and Dark matter searches and prospects of detecting the gravitational waves
Arindam Chatterjee, AseshKrishna Datta, Subhojit Roy
We study in detail the viability and the patterns of a strong first-order electroweak phase transition as a prerequisite to electroweak baryogenesis in the framework of -invar…
Optical and Thermodynamic Properties of a Rotating Dyonic Black Hole Spacetime in gauged supergravity
Prateek Sharma, Hemwati Nandan, Uma Papnoi +1
The null geodesics and the distance of closest approach for photon around a rotating dyonic black hole in gauged supergravity is studied. The phenomenon o…
Shedding Light on Dark Matter and Neutrino Interactions from Cosmology
Arnab Paul, Arindam Chatterjee, Anish Ghoshal +1
In CDM cosmology, Dark Matter (DM) and neutrinos are assumed to be non-interacting. However, it is possible to have scenarios, where DM-neutrino interaction may be present, l…