Searcharxiv⌕ Search

arXiv subjects

Zubair Ahmad Dar

Publications and source records attributed to Zubair Ahmad Dar.

3 recordsLinked to original sources

Nuclear binding energy and transverse momentum imbalance in neutrino-nucleus reactions

We have measured new observables based on the final state kinematic imbalances in the mesonless production of $ν_μ+A\rightarrowμ^-+p+X$ in the $\text{MINER}ν\text{A}$ tracker. Components of the muon-proton momentum imbalances parallel ($δp_\mathrm{Ty}$) and perpendicular($δp_\mathrm{Tx}$) to the momentum transfer in the transverse plane are found to be sensitive to the nuclear effects such as Fermi motion, binding energy and non-QE contributions. The QE peak location in $δp_\mathrm{Ty}$ is particularly sensitive to the binding energy. Differential cross sections are compared to predictions from different neutrino interaction models. The Fermi gas models presented in this study cannot simultaneously describe features such as QE peak location, width and the non-QE events contributing to the signal process. Correcting the GENIE's binding energy implementation according to theory causes better agreement with data. Hints of proton left-right asymmetry are observed in $δp_\mathrm{Tx}$. Better modeling of the binding energy can reduce bias in neutrino energy reconstruction and these observables can be applied in current and future experiments to better constrain nuclear effects.

hep-ex↗

Independent measurement of Muon neutrino and anti-neutrino oscillations at the INO-ICAL Experiment

The magnetised Iron Calorimeter detector at the India-based Neutrino Observatory (INO) has a unique feature to identify the neutrinos and antineutrinos on an event by event basis. This feature can be harnessed to detect the differences between the oscillation parameters of neutrinos and antineutrinos independently. In this paper, we analysed Charged Current $ν_μ$ and $\overlineν_μ$ events under the influence of earth matter effect using three neutrino flavor oscillation framework. If the atmospheric mass-squared differences and mixing parameters for neutrinos are different from antineutrinos, we present the prospects for the experimental observation of these differences in atmospheric $ν$ and $\overline ν_μ$ oscillations at INO. We estimate the detector sensitivity to confirm a non-zero difference in the mass-squared splittings ($|Δm^{2}_{32}|-|Δ\overline{m^{2}}_{32}|$) for neutrinos and antineutrinos.

hep-ex↗

Search for the differences in Atmospheric Neutrinos and Antineutrinos oscillation parameters at the INO-ICAL Experiment

In this paper, we present a study to measure the differences between the atmospheric neutrino and anti-neutrino oscillations in the Iron-Calorimeter detector at the India-based Neutrino Observatory experiment. Charged Current $ν_μ$ and $\overlineν_μ$ interactions with the detector under the influence of earth matter effect have been simulated for ten years of exposure. The observed $ν_μ$ and $\overlineν_μ$ events spectrum are separately binned into direction and energy bins, and a $χ^{2}$ is minimised with respect to each bin to extract the oscillation parameters for $ν_μ$ and $\overlineν_μ$ separately. We then present the ICAL sensitivity to confirm a non-zero value of the difference in atmospheric mass squared of neutrino and anti-neutrino i.e. $|Δm^{2}_{32}|-|Δ\overline{m^{2}}_{32}|$.

hep-ex↗