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Subhasmita Mishra

Researcher at Indian Institute of Technology, Hyderabad

Publications -  47
Citations -  1137

Subhasmita Mishra is an academic researcher from Indian Institute of Technology, Hyderabad. The author has contributed to research in topics: Neutrino & Neutrino oscillation. The author has an hindex of 13, co-authored 45 publications receiving 855 citations.

Papers
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Long-Baseline Neutrino Facility (LBNF) and Deep Underground Neutrino Experiment (DUNE) : 2: The Physics Program for DUNE at LBNF

R. Acciarri, +800 more
TL;DR: In this paper, the physics program for the Deep Underground Neutrino Experiment (DUNE) at the Fermilab Long-Baseline Neurtrino Facility (LBNF) is described.
ReportDOI

Long-Baseline Neutrino Facility (LBNF) and Deep Underground Neutrino Experiment (DUNE) Conceptual Design Report, Volume 4 The DUNE Detectors at LBNF

R. Acciarri, +796 more
TL;DR: A description of the proposed detector(s) for Dune at LBNF can be found in this paper, along with a description of Dune detector detector detector(S).
Journal ArticleDOI

Search for active-sterile neutrino mixing using neutral-current interactions in NOvA

P. Adamson, +180 more
- 14 Jun 2017 - 
TL;DR: In this article, the first search for sterile neutrinos mixing with active neutrino through a reduction in the rate of neutral-current interactions over a baseline of 810 km between the NOvA detectors was reported.
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Long-baseline neutrino oscillation physics potential of the DUNE experiment

B. Abi, +966 more
TL;DR: The sensitivity of the Deep Underground Neutrino Experiment (DUNE) to neutrino oscillation is determined, based on a full simulation, reconstruction, and event selection of the far detector and full simulation and parameterized analysis of the near detector.
Journal ArticleDOI

Supernova Neutrino Burst Detection with the Deep Underground Neutrino Experiment

B. Abi, +966 more
TL;DR: The Deep Underground Neutrino Experiment (DUNE) as mentioned in this paper is a 40kton underground liquid argon time projection chamber experiment, which is sensitive to the electron-neutrinos flavor component of the burst of neutrinos expected from the next Galactic core-collapse supernova.