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中微子振荡的物质的常规近似公式是从质量平方差的比率扩张Δ=αm 21 2 / m 31 2≥0.03的情况下获得的,首先由Cervera提出, 等。 和Freund证明是加速器中微子实验的准确公式。 最初,它要求中微子的能量远高于太阳共振才能验证膨胀,但是当将公式外推到共振时,发现中微子能量仍然非常准确,这对于T2K实验非常重要。 本文表明,通过消除分支切点的奇异性可以保证精度,并且,这是首次通过解析计算公式的实际误差。 实际错误意味着可以在当前实验中安全删除原始要求。
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JHEP10(2015)090
Published for SISSA by Springer
Received: May 25, 2015
Revised: September 16, 2015
Accepted: September 21, 2015
Published: October 14, 2015
Why is the neutrino oscillation formula expanded in
∆m
2
21
/∆m
2
31
still accurate near the solar resonance in
matter?
Xun-Jie Xu
Max-Planck-Institut f¨ur Kernphysik,
Postfach 103980, D-69029 Heidelberg, Germany
Institute of Modern Physics and Center for High Energy Physics, Tsinghua University,
Beijing 100084, China
E-mail: xunjie.xu@gmail.com
Abstract: The conventional approximate formula for neutrino oscillation in matter which
is obtained from the expansion in terms of the ratio of mass square differences α =
∆m
2
21
/∆m
2
31
≈ 0.03, first proposed by Cervera, et al. and Freund, turns out to be an
accurate formula for accelerator neutrino experiments. Originally it required the neutrino
energy to be well above the solar resonance to validate the expansion but it is found to be
still very accurate when the formula is extrapolated to the resonance, which is practically
important for the T2K experiment. This paper shows that the accuracy is guaranteed by
cancellations of branch cut singularities and also, for the first time, analytically computes
the actual error of the formula. The actual error implies that the original requirement can
be safely removed in current experiments.
Keywords: Neutrino Physics, CP violation, Solar and Atmospheric Neutrinos
ArXiv ePrint: 1502.02503
Open Access,
c
The Authors.
Article funded by SCOAP
3
.
doi:10.1007/JHEP10(2015)090
JHEP10(2015)090
Contents
1 Introduction 1
2 The α-expansion and the accidental accuracy 3
3 Non-differentiabilities, singularities and branch cuts in the oscillating
system 7
4 Solution 9
5 Numerical verification 14
6 Conclusion 15
A Some details of analytic calculations 17
A.1 Simplify the p term and q term 17
A.2 Calculate P
(B)
− P
(A)
18
1 Introduction
In long-baseline(LBL) neutrino experiments, the matter effect [1–3] is usually not negligible.
For current LBL accelerator neutrino experiments such as T2K [4, 5], MINOS [6] and
NOvA [7, 8] where the matter densities are almost constant, there is a useful approximate
formula for the transition probability. Taking the same notations as PDG, the formula
is [9]
P (ν
µ
→ ν
e
) = 4s
2
13
c
2
13
s
2
23
sin
2
(1 − A)∆
(1 − A)
2
+8α
J
CP
s
δ
cos(∆ + δ)
sin A∆
A
sin(1 − A)∆
1 − A
+4α
2
s
2
12
c
2
12
c
2
23
sin
2
A∆
A
2
(1.1)
where
A ≡ 2
√
2G
F
N
e
E/∆m
2
31
, α ≡ ∆m
2
21
/∆m
2
31
≈ 0.03, (1.2)
and ∆ ≡ ∆m
2
31
L/(4E). N
e
is the electron number density in matter, about 1.4cm
−3
N
A
in
the Earth’s crust.
The formula was originally derived in [10, 11] as a series expansion in α. But the prob-
lem is that due to the non-perturbative behavior near the solar resonance, the expansion
is expected to be valid only when the neutrino energy is well above the solar resonance,
E 0.34GeV
∆m
2
21
7.6 × 10
−5
eV
2
1.4cm
−3
N
A
N
e
. (1.3)
– 1 –
JHEP10(2015)090
This was emphasized in ref. [11], because the approximation α/A 1 was used when the
formula was derived. We will reformulate the derivation of the formula in section 2 to show
the problem more explicitly but here we take the solar mixing angle θ
12
as a good example
to show the problem. The effective sin 2θ
12
in matter, denoted as sin 2θ
m
12
, expanded in α
to first order, is [11]
sin 2θ
m
12
∼ α/A. (1.4)
The solar resonance is at A = α cos 2θ
12
≈ 0.4α so near the solar resonance sin 2θ
m
12
is quite
likely to be larger than 1. As will be shown in section 2, sin 2θ
m
12
> 1 does appear in the
expansion when the energy is lower than 0.34GeV, which makes the calculation invalid.
Originally, sin 2θ
m
12
in the calculation was expected not only less than 1 but also small, i.e.
sin 2θ
m
12
1, otherwise the unitarity of the effective mixing matrix will be badly violated,
thereby invalidating the calculation.
Despite the claimed bound (1.3) in [11], in practice this formula works well below the
bound (see figures 6, 7 presented later in this paper). For example T2K has used this
formula in their recent publication [12] because eq. (1.1) exhibits excellent accuracy near
the solar resonance.
1
So (1.3) is most likely not the true bound of validity. We would like to know to what
extent the formula is accurate or valid. The main goal of this paper, is to mathematically
demonstrate that there is no lower bound of A for the domain of validity. We will provide
explicit errors of the formula, among which the main error related to the matter effect is
only O(s
2
13
αA∆
2
). This implies that the formula is still accurate when A is close to α and
one may apply (1.1) below the bound.
Note that a higher order calculation in the original perturbative approach will not work
since the series in α/A can not converge at the resonance if the branch cut singularity is
not treated carefully. Actually a higher order correction to the formula (1.1) is computed
in ref. [13] but the correction blows up when taking the vacuum limit A → 0. Thus it can
not give a correct estimation when A is small. This is due to a lack of careful treatment of
the branch cut singularity related to the solar resonance.
Branch cuts in the oscillation system with the matter effect are essentially related
to level crossings [14, 15], but less noticed before. Note that the three eigenvalues of the
oscillation system come from the same cubic equation but they are different. The difference
originates from the different branches in the square roots and cubic roots in the general
solutions of a cubic equation. At a level crossing two of the eigenvalues are very close
to each other which makes the problem quite non-perturbative and this just corresponds
to the starting point of the branch cuts, which are called branch cut singularities. The
branch cut singularities are essentially origins of all non-perturbativities in the oscillation
system. In this paper, we will remove the singularity corresponding to the solar resonance
in our analytic calculation by transformation of the eigenvalues to some singularity-free
variables and compute the S-matrix using the Cayley-Hamilton theorem. In this way the
1
Note that for T2K, the energy range is 0.1-1.2 GeV and the spectrum peaks at 0.6 GeV [5]. A part of
the current measured range 0.1-0.34 GeV is below the bound (1.3) which would lead to sin 2θ
m
12
> 1 in the
expansion.
– 2 –
JHEP10(2015)090
conventional formula will be proven to be accurate below the bound (1.3). The relation
between the branch cut singularities and level crossings will be discussed in detail and thus
improve our understanding of the matter effect in neutrino oscillation [16–29].
As a byproduct of our analysis, a new approximate formula is derived in this paper,
with better accuracy. Though the exact form is a little more complicated than (1.1), for
practical use in neutrino simulation, it is useful and covers most aspects. This is important
considering that simulation of LBL experiments and performing χ
2
-fits require a fast and
simple method to compute a large number of oscillation probabilities. Therefore even
though the numerical calculation is always viable, there are still many studies on analytic
approximation formulae for neutrino oscillation in matter [13, 30–41].
This paper is organized as follows. In section 2, we reformulate the original derivation
of the formula (1.1) and numerically show the accuracy of the α-expansion in the case of
T2K. We will see that the α-expansion for some effective parameters is actually invalid
below 0.34GeV in T2K while the final result of the probability is very accurate. Then in
section 3 from the viewpoint of singularities, we show that non-differentiable singularities in
many parameters originate from the branch cut and result in the failure of the α-expansion.
In section 4 we solve the problem rigorously and then compute the analytical error of (1.1).
Based on the calculation in section 4, we also propose an alternative to the conventional
formula. Their accuracies are numerically verified, which will be shown in section 5. Finally
we conclude in section 6.
2 The α-expansion and the accidental accuracy
In this section, we first introduce analytic diagonalization of the 3 × 3 effective Hamilto-
nian, which has early been done by Zaglauer and Schwarzer [42] without any approximation.
Then we show the α-expansion of the result from Freund’s calculation [11] and compare
the approximate result with the exact result (though complicated but numerically pro-
grammable) to see how much it deviates from the exact result. We will show that the
α-expansion result of effective neutrino parameters are quite inaccurate and even invalid
near the solar resonance but the final result (i.e. the assembled oscillation probability) from
these parameters is very accurate.
Neutrino oscillation in matter is subjected to the Schr¨odinger equation in the flavor
space,
i
d
dL
|ν(L)i = H|ν(L)i, (2.1)
where |ν(L)i denotes the flavor state of the evolving neutrino at a distance of L from the
source and H is the Hamiltonian represented by the 3 ×3 matrix in the standard neutrino
oscillation framework,
H =
1
2E
U.
m
2
1
m
2
2
m
2
3
.U
†
+
√
2G
F
N
e
1
0
0
. (2.2)
Here U and m
i
’s are neutrino mixing matrix and masses in vacuum respectively. The second
term in eq. (2.2) comes from the matter effect. Without the second term (i.e. N
e
= 0), the
– 3 –
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