# Enhancing Sensitivity to Non-Standard Neutrino Interactions at INO   combining muon and hadron information

**Authors:** Amina Khatun, Sabya Sachi Chatterjee, Tarak Thakore, Sanjib Kumar, Agarwalla

arXiv: 1907.02027 · 2020-07-15

## TL;DR

This paper investigates how the ICAL detector at INO can improve sensitivity to non-standard neutrino interactions, especially the flavor-violating parameter _{}, by analyzing atmospheric neutrino oscillations and emphasizing the importance of charge identification.

## Contribution

It demonstrates for the first time that the charge identification capability of ICAL significantly enhances constraints on _{} and assesses the impact on mass hierarchy sensitivity.

## Key findings

- Most optimistic bound on _{} is .01 to .01 at 90% C.L.
- Charge identification is crucial for stringent _{} constraints.
- Mass hierarchy sensitivity decreases by 10-20% when marginalizing over _{}.

## Abstract

The neutral current non-standard interactions (NSI's) of neutrino with matter fermions while propagating through long distances inside the Earth matter can give rise to the extra matter potentials apart from the standard MSW potential due to the $W$-mediated interactions in matter. In this paper, we explore the impact of flavor violating neutral current NSI parameter $\varepsilon_{\mu\tau}$ in the oscillation of atmospheric neutrino and antineutrino using the 50 kt magnetized ICAL detector at INO. We find that due to non-zero $\varepsilon_{\mu\tau}$, $\nu_\mu\rightarrow\nu_\mu$ and $\bar\nu_\mu\rightarrow\bar\nu_\mu$ transition probabilities get modified substantially at higher energies and longer baselines, where vacuum oscillation dominates. We estimate the sensitivity of the ICAL detector for various choices of binning schemes and observables. The most optimistic bound on $\varepsilon_{\mu\tau}$ that we obtain is $-0.01 < \varepsilon_{\mu\tau} < 0.01 $ at 90$\%$ C.L. using 500 kt$\cdot$yr exposure and considering $E_\mu,\, \cos\theta_\mu,\,E'_{\rm had}$ as observables in their ranges [1, 21] GeV, [-1, 1], and [0, 25] GeV respectively. For the first time we show that the charge identification capability of the ICAL detector is crucial to set stringent constraints on $\varepsilon_{\mu\tau}$. We also show that when we marginalize over $\varepsilon_{\mu\tau}$ in fit in its range of -0.1 to 0.1, the mass hierarchy sensitivity deteriorates by 10$\%$ to 20$\%$ depending on the analysis mode, and the precision measurements of atmospheric parameters remain quite robust at the ICAL detector.

## Full text

_Full body text omitted from this summary view._ Fetch the complete paper as Markdown: https://tomesphere.com/paper/1907.02027/full.md

## Figures

39 figures with captions in the complete paper: https://tomesphere.com/paper/1907.02027/full.md

## References

77 references — full list in the complete paper: https://tomesphere.com/paper/1907.02027/full.md

---
Source: https://tomesphere.com/paper/1907.02027