CHAPTER 2 THE RESEARCH METHODOLOGY
2.1 Chapter Introduction
In this section, we study the prospects for detecting NSI in future reactor and superbeam experiments. We define the discovery reach (or discovery potential) of an experiment for some NSI parameter ε as the minimum value the true |ε| must have in order to be distinguishable from the ε = 0 case at a given confidence level. To compute the discovery reach, we simulate the event spectra for different “true” values of ε and then perform fits in which ε is kept fixed at zero. In fig. 4.4, we show the NSI discovery reach of T2K, Double Choozand of a combined analysis of these experiments. We have computed results for all NSI parameters which, according to table 4.2, might potentially be detectable, and we consider scenarios both with and without the constraint (4.17), εsαβ = (εdαβ)∗.
Our first observation is that the discovery reach crucially depends on the values nature has chosen for the complex phases δCP and arg(εs,d,mαβ ).3 For favourable combinations of these phases (light portions of bars), much smaller non-standard effects may be detected than for unfavourable combinations (dark portions of bars).
Reactor
By comparing fig. 4.4 with table 4.2, one can see that our expectations for the relative importance of different NSI parameters are mostly confirmed. In particular, the figure shows that reactor experiments are sensitive only to non-standard CC interactions of neutrinos and electrons, i.e. to the parameters εsee, εseµ, εseτ, εdee, εdµe and εdτ e. As dis-cussed in sec. 4.2.1, the discovery potential for εsee and εdee can never be better than the uncertainty in the reactor neutrino flux and spectrum, which is on the per cent level.
It can, however, be much worse if arg(εs,dee)∼ π/2, 3π/2 because then, the lowest order order contribution to P (¯νes→ ¯νed) vanishes (cf. eq. (C.2)).
The phase dependence that it visible for the parameters εseµ, εseτ, εdµeand εdτ edisappears when the combinations εseµ = (εdµe)∗ and εseτ = (εdτ e)∗ are considered. We interpret this feature with the help of the analytical expression for P (¯νes → ¯νed) from eq. (C.2): In general, the main sensitivity to NSI parameters comes from terms having an energy dependence different from that of the standard oscillation probability. In (C.2), this is the case for terms containing a factor sin(∆m231L/2E). For εseµ= (εdµe)∗and εseτ = (εdτ e)∗, however, all such terms cancel, and therefore, spectral information can no longer be used to disentangle standard and non-standard effects. On the other hand, the second order expansion of the ¯νe survival probability at L = 0, given in eq. (C.3), shows that the near
3The impact of the true δCP is not directly evident from fig. 4.4, which has been computed for fixed δtrueCP = 3π/2. It can, however, be seen from the equations given in appendix C, in which most terms depend on sums or differences of δCPand the non-standard phases.
10-2 10-1 100 101 Εees ΕeΜs ΕeΤs ΕΜes ΕΜΜs ΕΜΤs
Εeed ΕeΜd ΕΜed ΕΜΜd ΕΤed ΕΤΜd
Εees = Εeed * ΕeΜs = Εd *Μe ΕeΤs = ΕΤed * ΕΜes = ΕeΜd * ΕΜΜs = ΕΜΜd * ΕΜΤs = ΕΤΜd *
Εeem ΕeΜm ΕeΤm ΕΜΜm ΕΜΤm ΕΤΤm
ÈΕÈ GLoBES 2008
better
90% C.L. discovery reach D-Chooz bestworst T2K bestworst Combined bestworst Current bounds
Figure 4.4: 90% C.L. NSI discovery reaches of Double Chooz (green bars), T2K (blue bars), and of a combined analysis of these experiments (red bars). Parameter values covered by the dark portions of the bars can be discovered independently of the complex phases, while values covered by the light portions are accessible only if nature has chosen favourable values for the phases.
detector is sensitive to the combinations εseµ= (εdµe)∗ and εseτ = (εdτ e)∗, even though it is insensitive to each parameter on its own. We conclude that the discovery reaches for εseµ, εseτ, εdµeand εdτ e, treated as independent parameters, are dominated by phase-dependent spectral distortions seen in the far detector, while the discovery reaches for εseµ= (εdµe)∗ and εseτ = (εdτ e)∗ come mainly from phase-independent terms in the near detector.
Superbeam
The superbeam has some sensitivity to all shown NSI parameters except εseµand εseτ. For most parameters, however, the discovery potential is competitive with current bounds only for very special values of the complex phases. Unaffected by the phases are only the discovery potentials for εsµe, εdµe, and for the combinations εseµ= (εdµe)∗, εseτ = (εdτ e)∗, εsµe= (εdeµ)∗ and εsµτ = (εdτ µ)∗. In all of these cases, the sensitivity is dominated byO(ε2) effects causing a modified νe or νµ flux in the near detector. Also the relatively good sensitivity to εsee and εdee is due to near detector effects. Of the other discovery reaches, those for εdτ e, εmeµ and εmeτ come from the appearance channel, while those for εsµµ, εsµτ, εdµµ, εdτ τ and εmµτ are dominated by the disappearance channel.
A careful inspection of the superbeam discovery reaches shows that, in several places, our expectations from table 4.2 are contradicted by the simulation. For example, we would have expected the discovery reach for the parameter combination εsµτ = (εdτ µ)∗ to be similar to or better than the discovery reaches for εsµτ and εdτ µtreated as independent parameters. The reason why this is not the case can be deduced from eq. (C.7) or eq. (C.8). These expressions show that, of the terms proportional to εsµτ and εdτ µ, those having a non-standard energy dependence ∼ sin(∆m231L/2E), cancel in the case εsµτ = (εdτ µ)∗.
It is also interesting to observe that the discovery reach of the superbeam for εmeµ is more than an order of magnitude better than the discovery reach for εmeτ even though the corresponding terms in eq. (C.6) are identical up to effects of O(θ23− π/4), and up to signs. It turns out that an intricate interplay of these signs causes the contributions proportional to εmeτ to be always smaller. In sec. 4.3, we will see that, in a neutrino factory experiment, the sensitivities to εmeµand εmeτ are more similar than in the superbeam case.
Combined analysis
Comparing the discovery reaches achievable in T2K and Double Chooz separately to the potential of a combined analysis, we find that for most parameters, the combined analysis is dominated either by the reactor experiment or by the superbeam, and that the contribution from the other experiment is negligible. For εdτ e and εmeτ, however, the discovery prospects in the combined approach are much better than in the single experiment fits. We will see in the next section that this can be explained by the fact that the χ2 of a standard oscillation fit to a single set of experimental data is very small in the presence of εdτ e or εmeτ, but that there is a large discrepancy between the fitted
parameter values obtained in the reactor and superbeam experiments, respectively. It is this discrepancy, which effectively enhances the sensitivity of the combined analysis.
In conclusion, we have seen that reactor and superbeam experiments have some discovery potential for non-standard interactions, but only if the NSI couplings are very large and if, moreover, the complex phases are favourable. Next-generation neutrino oscillation experiments will certainly not be able to probe the parameter region εs,d,mαβ < 0.01, in which new effects might be expected, according to the estimate (4.7), if there is new physics at the TeV scale.