activity
19952022
most citedPhysics Potential of the ICAL detector at the India-based Neutrino Observatory (INO)

178 citations · 1.4k across the 70 of their papers we have counts for

collaborators

71 papers

hep-ph2022★ 6 cited

Constraints on the Doublet Left-Right Symmetric Model from Higgs data

Siddhartha Karmakar, Jai More, Akhila Kumar Pradhan +1

We study the constraints on the doublet left-right symmetric model (DLRSM) arising due to the Higgs data. The symmetry of this model is broken by three vacuum expectation…

hep-ph2022

Neutrino mass and charged lepton flavor violation in an extended left-right symmetric model

Chayan Majumdar, Supriya Senapati, S. Uma Sankar +1

We consider an extended left-right symmetric gauge theory where the neutrino masses are generated through inverse seesaw mechanism. In this model the muon …

hep-ph2022★ 6 cited

violation due to a Majorana phase in two flavor neutrino oscillations with decays

Khushboo Dixit, Akhila Kumar Pradhan, S. Uma Sankar

We study the conditions under which the Majorana phase of the two flavor neutrino mixing matrix appears in the oscillation probabilities and causes violation. We find that the…

hep-ph2022★ 15 cited

A review of the tension between the T2K and NOA appearance data and hints to new physics

Ushak Rahaman, Soebur Razzaque, S. Uma Sankar

In this article, we review the status of the tension between the long-baseline accelerator neutrino experiments T2K and NOA. The tension arises mostly due to the mismatch in the…

astro-ph.GA2022★ 14 cited

Probing the physicochemical properties of the Leo Ring and the Leo I group

Sameer, Jane Charlton, Glenn Kacprzak +6

We present an absorption line study of the physical and chemical properties of the Leo HI Ring and the Leo I Group as traced by 11 quasar sightlines spread over a 600 kpc X 800 kpc…

hep-ph2021★ 1 cited

Neutrino Oscillation parameter determination at INO-ICAL using track and hit information from GEANT

Jaydeep Datta, Bana Singh, S. Uma Sankar

We study the capability of INO-ICAL to determine the atmospheric neutrino oscillation parameters and . We do not use any generator level information. I…