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S. Uma Sankar

Researcher at Indian Institute of Technology Bombay

Publications -  104
Citations -  2129

S. Uma Sankar is an academic researcher from Indian Institute of Technology Bombay. The author has contributed to research in topics: Neutrino & Neutrino oscillation. The author has an hindex of 24, co-authored 97 publications receiving 1883 citations. Previous affiliations of S. Uma Sankar include Tata Institute of Fundamental Research & Indian Institutes of Technology.

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Physics Potential of the ICAL detector at the India-based Neutrino Observatory (INO)

Shakeel Ahmed, +90 more
TL;DR: In this paper, the authors presented the physics potential of the ICAL detector as obtained from realistic detector simulations and gave the expected physics reach of the detector with 10 years of runtime.
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Invited review: Physics potential of the ICAL detector at the India-based Neutrino Observatory (INO)

A. Kumar, +120 more
- 26 Apr 2017 - 
TL;DR: In this paper, the authors presented the physics potential of the ICAL detector as obtained from realistic detector simulations and gave the expected physics reach of the detector with 10 years of runtime.
Journal ArticleDOI

D* polarization as a probe to discriminate new physics in B --> D* tau nubar

TL;DR: In this article, the angular observables in the LHCb spectra were used to distinguish between scalar and tensor new physics operators and their coupling strengths, and the polarization fraction was found to be a good discriminant of scalar/tensor operators.
ReportDOI

The Single-Phase ProtoDUNE Technical Design Report

B. Abi, +825 more
TL;DR: ProtoDune-SP is the single-phase Dune Far Detector prototype that is under construction and will be operated at the CERN Neutrino Platform (NP) starting in 2018 as mentioned in this paper.
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Mass hierarchy determination via future atmospheric neutrino detectors

TL;DR: In this paper, the problem of determination of the sign of the neutrino mass hierarchy through observations of atmospheric neutrinos in future detectors has been studied, and two proposed detector types: (a) megaton sized water C\ifmmode \breve{}\else \u{}\fi{}erenkov detectors, which can measure the event rates of ${\ensuremath{ u}}{m}{31}^{2}$, and (b) 100 kton sized magnetized iron detectors, who can detect the event rate of