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Ushak Rahaman

Publications and source records attributed to Ushak Rahaman.

At least 19 recordsLinked to original sources

Diagnosing Unmodeled Neutrino Physics via DUNE and T2HK Complementarity

Unmodeled beyond Standard Model (BSM) physics in neutrino propagation can masquerade as parameter degeneracies in future precision measurements. Because the upcoming DUNE and T2HK experiments will operate at substantially different baselines, interpreting their data under the standard three-flavor framework provides a powerful diagnostic tool: any propagation BSM effect can manifest as an artificial tension between their extracted parameters. We demonstrate this principle using the complex non-standard interactions (NSI) currently favored to resolve the $\sim2σ$ tension between NO$ν$A and T2K. If these NSI solutions are realized, the NSI-induced interference term $\propto\sin(δ_{\rm CP}+ϕ)$ systematically distorts the DUNE appearance rates, leading to a correlated misidentification of the atmospheric mixing octant and the CP phase $δ_{\rm CP}$. Specifically, for $\varepsilon_{eμ}$ ($\varepsilon_{eτ}$) NSI, the DUNE fit shifts toward CP-conserving values (the opposite CP half-plane) along with a preference for the wrong octant. In contrast, the shorter-baseline T2HK experiment remains largely insensitive to this effect. The resulting $\sim3σ$ incompatibility between the DUNE and T2HK standard-fit results (after 6 years of data collection for each experiment)can provide a powerful experimental diagnostic for propagation NSI, illustrating how baseline complementarity can be a valuable tool to uncover new physics in the precision era.

hep-ph

Enhancing the sensitivity to neutrino oscillation parameters using synergy between T2K, NO$ν$A and JUNO

We study the impact of combining the present NO$ν$A and T2K data with simulated data from the JUNO experiment on the determination of the leptonic CP phase and the neutrino mass hierarchy. The current NO$ν$A data exhibit a hierarchy--$δ_{\rm CP}$ degeneracy, admitting both normal hierarchy (NH) with $δ_{\rm CP} \in [0,180^\circ]$, and inverted hierarchy (IH) with $δ_{\rm CP} \in [180^\circ,360^\circ]$ solutions at comparable significance, while T2K prefers $δ_{\rm CP}\simeq 270^\circ$ for both hierarchies, leading to a $2σ$ tension between the two experiments for normal hierarchy. Using detailed GLoBES simulations, we show that future JUNO data with excellent hierarchy sensitivity, can lift the hierarchy--$δ_{\rm CP}$ degeneracy in NO$ν$A and strengthen the hierarchy reach of T2K in spite of having no $δ_{\rm CP}$ sensitivity. Allowing the hierarchy to be a free parameter in the fit, if the true ordering is IH, JUNO aligns the NO$ν$A and T2K allowed regions and resolves their present tension; if NH is true, the tension continues to persist. We also show that JUNO's precise measurement of $|Δ_{31}|$ leads to improved constraints on $\sin^2θ_{23}$ and $δ_{\rm CP}$ for normal mass hierarchy in NO$ν$A even though JUNO itself is insensitive to these parameters. Finally, updated solar parameter measurements from JUNO's first data release further enhance the combined precision. Our results demonstrate that JUNO plays a crucial synergistic role in the global neutrino oscillation programme, enabling a more robust determination of the mass ordering and improving the sensitivity to the CP phase when combined with long-baseline data.

hep-ph

Quantum Simulation of Collective Neutrino Oscillations using Dicke States

In dense neutrino gases, which exist for instance in supernovae, the flavour states of different neutrinos may become entangled with one another. The theoretical description of such systems may therefore call for simulations on a quantum computer. Existing quantum simulations of simple toy systems are not optimal in the sense that they do not fully exploit the symmetries of the system. Here, we propose a new class of qubit-efficient algorithms based on Dicke states and the $su(2)$ spin algebra. We demonstrate the excellent performance of these algorithms both on classical and on quantum hardware.

quant-ph

Update on non-unitary mixing in the recent NO$ν$A and T2K data

In this paper, we have tested the non-unitary mixing hypothesis with the latest data from NO$ν$A and T2K experiments. We have also analysed their combined data. We have provided the best-fit values of the standard and non standard parameters after the analysis. $90\%$ limits on the non-unitary mixing parameters have also been provided. The constraints on unitary violation is stronger, compared to the constraints obtained from previous data from NO$ν$A and T2K. The tension between NO$ν$A and T2K at the $1\,σ$ for normal mass hierarchy can be reduced for non-unitary mixing due to $α_{10}$, albeit for a value of $|α_{10}|$ larger than the present global $90\%$ limit. Additionally a study of the future sensitivity of NO$ν$A, T2K and DUNE has been provided.

hep-ph

Effects of tau-neutrino detection on non-standard interactions at DUNE with a short discussion on the nature of neutrino mixing

In this paper, we investigate the effects of $ν_τ$ and $\barν_τ$ detection at the DUNE far detector on the experiment's sensitivity to Non-Standard Interactions (NSI) in neutrino propagation. We show that the strongest observable NSI effect in the $ν_τ$ and $\barν_τ$ appearance probabilities arises from $ε_{μτ}$. We have studied the hierarchy sensitivity, CP violation sensitivity and octant sensitivity of DUNE from $ν_τ$ and $\barν_τ$ appearance channels in presence of NSI. We have also studied the detection sensitivity of NSI phases and the future constaints on NSI parameters from the tau neutrino appearance channels in DUNE. Additionally, we examine the role of $ν_τ$ detection in constraining the unitary nature of the PMNS matrix. These studies emphasize the importance of incorporating $ν_τ$ detection in long-baseline neutrino experiments such as DUNE.

hep-ph

Dark photon distortions of NO$ν$A and T2K neutrino oscillations

Dark photons coupling to $L_μ-L_τ$ lepton number difference are a highly studied light dark matter candidate, with potential to be discovered through their impact on terrestrial neutrino oscillation experiments. We re-examine this in the light of claimed tensions between the NO$ν$A and T2K long baseline experiments, also taking into account data from the MINOS experiment. We obtain leading limits on the $L_μ-L_τ$ gauge coupling $g'$ versus dark photon mass $m_{A'}$, and find no statistically significant alleviation of the tension from inclusion of the new physics effect.

hep-ph

Effect of non-unitary mixing on the mass hierarchy and CP violation determination at the Protvino to Orca experiment

In this paper, we have estimated the neutrino mass ordering and the CP violation sensitivity of the proposed Protvino to Orca (P2O) experiment after 6 years of data-taking. Both unitary and non-unitary $3\times 3$ neutrino mass mixing have been considered in the simulations. A forecast analysis deriving possible future constraints on non-unitary parameters at P2O have been performed.

hep-ph

On the tension between the latest \nova and T2K data

The latest data from the T2K and \nova experiments show a tension in their preferred values of the oscillation parameters. In this work, we try to identify the source of the tension between the data from these two experiments. An analysis of their data from various channels (individually, and combined) shows that the tension arises primarily from the $ν_e$ appearance data, and is compounded by the $\barν_μ$ disappearance data. We provide an explanation for the tension based on parameter degeneracies. Apart from the analysis with the standard matter effect, we also analyse the data with the vacuum oscillation hypothesis. We find that vacuum oscillations fit the data as well as matter effects do; and also reduce the tension between the two experiments. We have also done a study of the future run of NO$ν$A, T2K and DUNE in the context of resolving this tension.

hep-ph

Non-unitary neutrino mixing in the NO$ν$A near detector data

The $ν_μ\to ν_e$ oscillation probability over short baseline ($\lesssim 1$~km) would be negligible in case the mixing matrix for three active neutrinos is unitary. However, in case of non-unitary mixing of three neutrinos, this probability would be non-negligible due to the so-called "zero distance" effect. Hence, the near detector of the accelerator experiments such as NO$ν$A can provide strong constraints on the parameters of the non-unitary mixing with very large statistics. By analyzing the NO$ν$A near detector data we find that the non-unitary mixing does not improve fits to the $ν_e$ or $ν_μ$ events over the standard unitary mixing. This leads to constraints on the non-unitary parameters: $α_{00}>0.911$, $|α_{10}|<0.020$ and $α_{11}>0.952$ at 90\% C.L. A combined analysis with the near and far detector data does not change these constraints significantly.

hep-ph

A review of the tension between the T2K and NO$ν$A appearance data and hints to new physics

In this article, we review the status of the tension between the long-baseline accelerator neutrino experiments T2K and NO$ν$A. The tension arises mostly due to the mismatch in the appearance data of the two experiments. We explain how this tension arises based on $ν_μ\to ν_e$ and $\barν_μ\to \barν_e$ oscillation probabilities. We define the reference point of vacuum oscillation, maximal $θ_{23}$ and $δ_{CP}=0$ and compute the $ν_e/\barν_e$ appearance events for each experiment. We then study the effects of deviating the unknown parameters from the reference point and the compatibility of any given set of values of unknown parameters with the data from T2K and NO$ν$A. T2K observes a large excess in the $ν_e$ appearance event sample compared to the expected $ν_e$ events at the reference point, whereas \nova observes a moderate excess. The large excess in T2K dictates that $δ_{CP}$ be anchored at $-90^\circ$ and that $θ_{23}>π/4$ with a preference for normal hierarchy. The moderate excess at NO$ν$A leads to two degenerate solutions: A) NH, $0<δ_{CP}<180^\circ$, and $θ_{23}>π/4$; B) IH, $-180^\circ<δ_{CP}<0$, and $θ_{23}>π/4$. This is the main cause of the tension between the two experiments. We have reviewed the status of three beyond standard model (BSM) physics scenarios, (a) non-unitary mixing, (b) Lorentz invariance violation and (c) non-standard neutrino interactions, to resolve the tension.

hep-ph

Looking for Lorentz invariance violation (LIV) in the latest long baseline accelerator neutrino oscillation data

In this paper, we have analysed the latest data from NO$ν$A and T2K with the Lorentz invariance violation along with the standard oscillation hypothesis. We have found that the NO$ν$A data cannot distinguish between the two hypotheses at $1\, σ$ confidence level. T2K data and the combined data analysis excluded standard oscillation at $1\, σ$. All three cases do not have any hierarchy sensitivity when analysed with LIV. There is a mild tension between the two experiments, when analysed with LIV, as $θ_{23}$ at \nova best-fit is at higher octant but the same for T2K is at lower octant. NO$ν$A has a new degeneracy over $\sin^2 θ_{23}$ value, when analysed with LIV.

hep-ph

Searching for non-unitary neutrino oscillations in the present T2K and NO$ν$A data

The mixing of three active neutrino flavors is parameterized by the unitary PMNS matrix. If there are more than three neutrino flavors and if the extra generations are heavy isosinglets, the effective $3\times 3$ mixing matrix for the three active neutrinos will be non-unitary. We have analyzed the latest T2K and \nova data with the hypothesis of non-unitary mixing of the active neutrinos. We found that the 2019 NO$ν$A data slightly (at $\sim 1\, σ$ C.L.) prefer the non-unitary mixing over unitary mixing. In fact, allowing the non-unitary mixing brings the \nova best-fit point in the $\sin^2θ_{23}-δ_{CP}$ plane closer to the T2K best-fit point. The 2019 T2K data, on the other hand, cannot rule out any of the two mixing schemes. A combined analysis of the NO$ν$A and T2K 2019 data prefers the non-unitary mixing at $1\, σ$ C.L.. We derive constraints on the non-unitary mixing parameters using the best-fit to the combined NO$ν$A and T2K data. These constraints are weaker than previously found. The latest 2020 data from both the experiments prefer non-unitarity over unitary mixing at $1\, σ$ C.L. The combined analysis preferes non-unitarity at $2\, σ$ C.L. The stronger tension, which exists between the latest 2020 data of the two experiments, also gets reduced with non-unitary analysis.

hep-ph

Signatures of $A_4$ symmetry in the charged lepton flavour violating decays in a neutrino mass model

We study the charged lepton flavour violation in a popular neutrino mass model with $A_4$ discrete symmetry. This symmetry requires the presence of multiple Higgs doublets in the model and it also dictates the flavour violating Yukawa couplings of the additional neutral scalars of the model. Such couplings lead to the decays of the neutral mesons, the top quark and the $τ$ lepton into charged leptons of different flavours at tree level. The $A_4$ symmetry of the model leads to certain characteristic signatures in these decays. We discuss these signatures and predict the rates for the most favourable charged lepton flavour violating modes.

hep-ph

Matter vs. vacuum oscillations at long baseline accelerator neutrino experiments

The neutrino oscillation probabilities at the long-baseline accelerator neutrino experiments are expected to be modified by matter effects. We search for evidence of such modification in the data of T2K and NO$ν$A, by fitting the data to the hypothesis of (a) matter modified oscillations and (b) vacuum oscillations. We find that vacuum oscillations provide as good a fit to the data as matter modified oscillations. Even extended runs of T2K and NO$ν$A, with 5 years in neutrino mode $(5 ν)$ and five years in anti-neutrino mode $(5 \barν)$, can {\bf not} make a $3~σ$ distinction between vacuum and matter modified oscillations. The proposed experiment DUNE, with neutrino and anti-neutrino runs of 5 years each $(5 ν+ 5 \barν)$, can rule out vacuum oscillations by itself at $5~σ$ if the hierarchy is normal. If the hierarchy is inverted, a $5~σ$ discrimination against vacuum oscillations requires the combination of $(5 ν+ 5 \barν)$ runs of T2K, \nova and DUNE.

hep-ph

Tensions between the appearance data of T2K and NOvA

The long baseline neutrino experiments, T2K and NOvA, have taken significant amount of data in each of the four channels: (a) $ν_μ$ disappearance, (b) $\barν_μ$ disappearance (c) $ν_e$ appearance and (d) $\barν_e$ appearance. There is a mild tension between the disappearance and the appearance data sets of T2K. A more serious tension exists between the $ν_e$ appearance data of T2K and the $ν_e / \barν_e$ appearance data of NOvA. This tension is significant enough that T2K rules out the best-fit point of NOvA at $95\%$ confidence level whereas NOvA rules out T2K best-fit point at $90\%$ confidence level. We explain the reason why these tensions arise. We also do a combined fit of T2K and NOvA data and comment on the results of this fit.

hep-ph

Understanding the degeneracies in NO$ν$A data

The combined analysis of $ν_μ$ disappearance and $ν_e$ appearance data of NO$ν$A experiment leads to three nearly degenerate solutions. This degeneracy can be understood in terms of deviations in $ν_e$ appearance signal, caused by unknown effects, with respect to the signal expected for a reference set of oscillations parameters. We define the reference set to be vacuum oscillations in the limit of maximal $θ_{23}$ and no CP-violation. We then calculate the deviations induced in the $ν_e$ appearance signal event rate by three unknown effects: (a) matter effects, due to normal or inverted hierarchy (b) octant effects, due to $θ_{23}$ being in higher or lower octant and (c) CP-violation, whether $δ_{CP} \sim - π/2$ or $δ_{CP} \sim π/2$. We find that the deviation caused by each of these effects is the same for NO$ν$A. The observed number of $ν_e$ events in NO$ν$A is equivalent to the increase caused by one of the effects. Therefore, the observed number of $ν_e$ appearance events of NO$ν$A is the net result of the increase caused by two of the unknown effects and the decrease caused by the third. Thus we get the three degenerate solutions. We also find that further data by NO$ν$A can not distinguish between these degenerate solutions but addition of one year of neutrino run of DUNE can make a distinction between all three solutions. The distinction between the two NH solutions and the IH solution becomes possible because of the larger matter effect in DUNE. The distinction between the two NH solutions with different octants is a result of the synergy between the anti-neutrino data of NO$ν$A and the neutrino data of DUNE.

hep-ph

Mass hierarchy and CP-phase sensitivity of ORCA using Fermilab Neutrino Beam

We explore neutrino mass hierarchy determination and CP-phase measurement using multi-megaton water Cherenkov detector KM3NeT-Oscillation Research with Cosmics in the Abyss (ORCA) in the Mediterranean sea receiving neutrino beam from the Fermilab Long Baseline Neutrino Facility (LBNF) over 6900 km baseline. We find that with the proposed beam luminosity of $1.2\times 10^{21}$ proton-on-target per year, it will be possible to determine mass hierarchy at $\gtrsim 4\,σ$ confidence level within 1 year in the neutrino mode alone. A combined 1 year in neutrino and 1 year in antineutrino mode can determine hierarchy at $\gtrsim 6\,σ$ confidence level. We also find that a non-zero CP-phase can be detected with up to $\sim 1.8\,σ$ significance after 10 years of data taking. We explore degeneracy of neutrino oscillation parameters and uncertainties in detection efficiencies affecting the results.

hep-ph

Hierarchy sensitivity of NO$ν$A in light of T2K $ν_e$ appearance data

The $ν_e$ appearance data of T2K experiment has given a glimpse of the allowed parameters in the hierarchy-$δ_{CP}$ parameter space. In this paper, we explore how this data affects our expectations regarding the hierarchy sensitivity of the NO$ν$A experiment. For the favourable combinations of hierarchy and $δ_{CP}$, the hierarchy sensitivity of NO$ν$A is unaffected by the addition of T2K data. For the unfavourable combinations, NO$ν$A data gives degenerate solutions. Among these degenerate solutions, T2K data prefers IH and $δ_{CP}$ in the lower half plane over NH and $δ_{CP}$ in the upper half plane. Hence, addition of the T2K data to NO$ν$A creates a bias towards IH and $δ_{CP}$ in the lower half plane irrespective of what the true combination is.

hep-ph