ترغب بنشر مسار تعليمي؟ اضغط هنا

An Effective Two-Flavor Approximation for Neutrino Survival Probabilities in Matter

104   0   0.0 ( 0 )
 نشر من قبل Hisakazu Minakata
 تاريخ النشر 2017
  مجال البحث
والبحث باللغة English
 تأليف Hisakazu Minakata




اسأل ChatGPT حول البحث

It is known in vacuum that the three-flavor neutrino survival probability can be approximated by the effective two-flavor form to first orders in $epsilon equiv Delta m^2_{21} / Delta m^2_{31}$, with introduction of the effective $Delta m^2_{alpha alpha}$ ($alpha = e, mu, tau$), in regions of neutrino energy $E$ and baseline $L$ such that $Delta m^2_{31} L / 2E sim pi$. Here, we investigate the question of whether the similar effective two-flavor approximation can be formulated for the survival probability in matter. Using a perturbative framework with the expansion parameters $epsilon$ and $s_{13} propto sqrt{epsilon}$, we give an affirmative answer to this question and the resultant two-flavor form of the probability is valid to order $epsilon$. However, we observe a contrived feature of the effective $Delta m^2_{alpha alpha} (a)$ in matter. It ceases to be a combination of the fundamental parameters and has energy dependence, which may be legitimate because it comes from the matter potential. But, it turned out that $Delta m^2_{mu mu} (a)$ becomes $L$-dependent, though $Delta m^2_{ee} (a)$ is not, which casts doubt on adequacy of the concept of effective $Delta m^2$ in matter. We also find that the appearance probability in vacuum admits, to order $epsilon$, the similar effective two-flavor form with a slightly different effective $Delta m^2_{beta alpha}$ from the disappearance channel. A general result is derived to describe suppression of the matter effect in the oscillation probability.



قيم البحث

اقرأ أيضاً

73 - Hisakazu Minakata 2015
We construct a new perturbative framework to describe neutrino oscillation in matter with the unique expansion parameter epsilon, which is defined as Delta m^2_{21} / Delta m^2_{ren} with the renormalized atmospheric Delta m^2_{ren} equiv Delta m^2_{ 31} - s^2_{12} Delta m^2_{21}. It allows us to derive the maximally compact expressions of the oscillation probabilities in matter to order epsilon in the form akin to those in vacuum. This feature allows immediate physical interpretation of the formulas, and facilitates understanding of physics of neutrino oscillations in matter. Moreover, quite recently, we have shown that our three-flavor oscillation probabilities P( u_alpha rightarrow u_beta) in all channels can be expressed in the form of universal functions of L/E. The u_e disappearance oscillation probability P( u_e rightarrow u_e) has a special property that it can be written as the two-flavor form which depends on the single frequency. This talk is based on the collaborating work with Stephen Parke [1].
Motivated by tremendous progress in neutrino oscillation experiments, we derive a new set of simple and compact formulas for three-flavor neutrino oscillation probabilities in matter of a constant density. A useful definition of the $eta$-gauge neutr ino mass-squared difference $Delta^{}_* equiv eta Delta^{}_{31} + (1-eta) Delta^{}_{32}$ is introduced, where $Delta^{}_{ji} equiv m^2_j - m^2_i$ for $ji = 21, 31, 32$ are the ordinary neutrino mass-squared differences and $0 leq eta leq 1$ is a real and positive parameter. Expanding neutrino oscillation probabilities in terms of $alpha equiv Delta^{}_{21}/Delta^{}_*$, we demonstrate that the analytical formulas can be remarkably simplified for $eta = cos^2 theta^{}_{12}$, with $theta_{12}^{}$ being the solar mixing angle. As a by-product, the mapping from neutrino oscillation parameters in vacuum to their counterparts in matter is obtained at the order of ${cal O}(alpha^2)$. Finally, we show that our approximate formulas are not only valid for an arbitrary neutrino energy and any baseline length, but also still maintaining a high level of accuracy.
In neutrino oscillations, a neutrino created with one flavor can be later detected with a different flavor, with some probability. In general, the probability is computed exactly by diagonalizing the Hamiltonian operator that describes the physical s ystem and that drives the oscillations. Here we use an alternative method developed by Ohlsson & Snellman to compute exact oscillation probabilities, that bypasses diagonalization, and that produces expressions for the probabilities that are straightforward to implement. The method employs expansions of quantum operators in terms of SU(2) and SU(3) matrices. We implement the method in the code NuOscProbExact, which we make publicly available. It can be applied to any closed system of two or three neutrino flavors described by an arbitrary time-independent Hamiltonian. This includes, but is not limited to, oscillations in vacuum, in matter of constant density, with non-standard matter interactions, and in a Lorentz-violating background.
The existence of light sterile neutrinos is a long standing question for particle physics. Several experimental ``anomalies could be explained by introducing ~eV mass scaled light sterile neutrinos. Many experiments are actively hunting for such ligh t sterile neutrinos through neutrino oscillation. For long baseline experiments, matter effect needs to be treated carefully for precise neutrino oscillation probability calculation. However, it is usually time-consuming or analytical complexity. In this manuscript we adopt the Jacobi-like method to diagonalize the Hermitian Hamiltonian matrix and derive analytically simplified neutrino oscillation probabilities for 3 (active) + 1 (sterile)-neutrino mixing for a constant matter density. These approximations can reach quite high numerical accuracy while keeping its analytical simplicity and fast computing speed. It would be useful for the current and future long baseline neutrino oscillation experiments.
Expressions for neutrino oscillations contain a high degree of symmetry, but typical forms for the oscillation probabilities mask these symmetries. We elucidate the $2^7=128$ symmetries of the vacuum parameters and draw connections to the choice of d efinitions of the parameters as well as interesting degeneracies. We also show that in the presence of matter an additional set of $2^7=128$ symmetries exist of the matter parameters for a total of $2^{14}=16,384$ symmetries of the vacuum and/or matter parameters in the oscillation probabilities in matter. Due to the complexity of the exact expressions for neutrino oscillations in matter, we show that under certain assumptions, approximate expressions have at most $2^6=64$ additional symmetries of the matter parameters for a total of $2^{13}=8,192$ symmetries. We investigate which of these symmetries apply to numerous approximate expressions in the literature and show that a more careful consideration of symmetries improves the precision of approximations.
التعليقات
جاري جلب التعليقات جاري جلب التعليقات
سجل دخول لتتمكن من متابعة معايير البحث التي قمت باختيارها
mircosoft-partner

هل ترغب بارسال اشعارات عن اخر التحديثات في شمرا-اكاديميا