1,824 research outputs found
Analysis of atmospheric neutrino oscillations in three-flavor neutrinos
We analyze the atmospheric neutrino experiments of Super-Kamiokande (830-920
live days) using the three-flavor neutrino framework with the mass hierarchy
m_1 nearly equal m_2 << m_3. We study the sub-GeV, multi- GeV neutrinos and
upward through-going and stopping muons zenith angle distributions taking
account of the Earth matter effects thoroughly. We obtain the allowed regions
of mass and mixing parameters Delm^2_{23}, theta_{13} and theta_{23}.
Delm^2_{23} is restricted to 0.002-0.01eV^2 and theta_{13}<13degrees,
35degrees<theta_{23}<55degrees in 90% C.L. For theta_{12}, there is no
difference between the large angle solar neutrino solution and small one. From
chi^2 fit, the minimum chi^2=55(54DOF) is obtained at
Delm^2_{23}=4x10^(-3)eV^2, theta_{13}=10degrees and theta_{23} =45degrees.Comment: 16 pages, 3 figures, LaTe
Higgs potential in S_3 invariant model for quark/lepton mass and mixing
We analyzed the S_3 invariant Higgs potential with S_3 singlet and doublet
Higgs. We obtained a relation (|v_1|/|v_2|)^2=-sin2phi_2/sin2phi_1 from this
S_3 invariant Higgs potential, where v_1, v_2 and phi_1, phi_2 are vacuum
pectation values and phases of S_3 doublet Higgs, respectively. This relation
could be satisfied exactly by the results |v_1|/ |v_2|=0.207, phi_1=-74.9deg
and phi_2=0.74deg obtained from the previous our work analyzing the
quark/lepton mass and mixing in S_3 invariant Yukawa interaction. Furthermore,
the relation v_S ~ v_D=sqrt{|v_1|^2+|v_2|^2}=174GeV is obtained and then the
coupling strength of Higgs to top quark g_{H_Stt}=m_t/v_S is altered as by a
factor sqrt{2} from the standard value. Introduced the S_3 doublet Higgs, FCNC
are produced in tree level. Predicted branching ratios for rare decays mu^- to
e^-e^+e^-, K^0_L to mu^+\mu^- etc., induced by the FCNC are sufficiently below
the present experimental upper bounds.Comment: 16 pages, 3 figure
Cherenkov Telescope Array: The next-generation ground-based gamma-ray observatory
High energy gamma-ray astronomy is a newly emerging and very successful
branch of astronomy and astrophysics. Exciting results have been obtained by
the current generation Cherenkov telescope systems such as H.E.S.S., MAGIC,
VERITAS and CANGAROO. The H.E.S.S. survey of the galactic plane has revealed a
large number of sources and addresses issues such as the question about the
origin of cosmic rays. The detection of very high energy emission from
extragalactic sources at large distances has provided insights in the star
formation during the history of the universe and in the understanding of active
galactic nuclei. The development of the very large Cherenkov telescope array
system (CTA) with a sensitivity about an order of magnitude better than current
instruments and significantly improved sensitivity is under intense discussion.
This observatory will reveal an order of magnitude more sources and due to its
higher sensitivity and angular resolution it will be able to detect new classes
of objects and phenomena that have not been visible until now. A combination of
different telescope types will provide the sensitivity needed in different
energy ranges.Comment: 4 pages, 3 figures, to appear in the proceedings of the 30th
International Cosmic Ray Conference, Merida, July 200
Flavor Mass and Mixing and S_3 Symmetry -- An S_3 Invariant Model Reasonable to All --
We assume that weak bases of flavors (u, c)_{L,R}, (d,s)_{L,R}, (e, \mu)
_{L,R}, (\nu_e, \nu_\mu)_{L,R} are the S_3 doublet and t_{L,R}, b_{L,R},
\tau_{L,R}, {\nu_\tau}_{L,R} are the S_3 singlet and further there are S_3
doublet Higgs (H_D^1, H_D^2) and S_3 singlet Higgs H_S. We suggest an S_3
invariant Yukawa interaction, in which masses caused from the interaction of
S_3 singlet flavors and Higgs is very large and masses caused from interactions
of S_3 doublet flavors and Higgs are very small, and the vacuum expectation
value _0 is rather small compared to the _0. In this model,
we can explain the quark sector mass hierarchy, flavor mixing V_{CKM} and
measure of CP violation naturally. The leptonic sector mass hierarchy and
flavor mixing described by V_{MNS} having one-maximal and one-large mixing
character can also be explained naturally with no other symmetry restriction.
In our model, an origin of Cabibbo angle is the ratio \lambda=_0
/_0 and an origin of CP violation is the phase of H_D^1.Comment: 16 page
A chiral qbarqbarqq nonet?
We point out that meson spectrum indicates the existence of a degenerate
chiral nonet in the energy region around 1.4 GeV with a slightly inverted
spectrum with respect to a qq nonet. Based on this observation, the
approximately linear rising of the mass of a hadron with the number of
constituent quarks, and the existence of a cuasidegenerate pseudoscalar nonet,
we conjecture the existence of a tetraquark chiral nonet in this energy region
with chiral symmetry implemented directly. We realize this idea in a chiral
model and take into account the mixing of the tetraquark chiral nonet with a
conventional qq nonet. We find that the mass spectrum of mesons below 1.5 GeV
is consistent with this picture. In general, pseudoscalar states arise as
mainly qq states but scalar states turn out to be strong admixtures of qq and
tetraquark states.Comment: 8 pages, 3 figure
Effects to Scalar Meson Decays of Strong Mixing between Low and High Mass Scalar Mesons
We analyze the mass spectroscopy of low and high mass scalar mesons and get
the result that the coupling strengths of the mixing between low and high mass
scalar mesons are very strong and the strengths of mixing for scalar
mesons and those of I=0 scalar mesons are almost same. Next, we analyze the
decay widths and decay ratios of these mesons and get the results that the
coupling constants for which represents the coupling of high
mass scalar meson -> two pseudoscalar mesons are almost same as the
coupling for the I=0. On the other hand, the coupling constant for
which represents the low mass scalar meson -> are far
from the coupling constant for I=0. We consider a resolution for this
discrepancy. Coupling constant for glueball -> is smaller than
the coupling . is .Comment: 15 pages, 6 figure
Mixing among light scalar mesons and L=1 q\bar{q} scalar mesons
Following the re-establishment of the \sigma(600) and the \kappa(900), the
light scalar mesons a_0(980) and f_0(980) together with the \sigma(600) and the
\kappa(900) are considered as the chiral scalar partner of pseudoscalar nonet
in SU(3) chiral symmetry, and the high mass scalar mesons a_0(1450),
K^*_0(1430), f_0(1370) and f_0(1710) turned out to be considered as the L=1
q\bar{q} scalar mesons. We assume that the high mass of the L=1 q\bar{q} scalar
mesons is caused by the mixing with the light scalar mesons. For the structure
of the light scalar mesons, we adopted the qq\bar{q}\bar{q} model in order to
explain the "scalar meson puzzle". The inter-mixing between the light scalar
nonet and the high mass L=1 q\bar{q} nonet and the intra-mixing among each
nonet are analyzed by including the glueball into the high mass scalar nonet.Comment: 16 pages, 5 figure
A simulation of high energy cosmic ray propagation 1
High energy cosmic ray propagation of the energy region 10 to the 14.5 power - 10 to the 18th power eV is simulated in the inter steller circumstances. In conclusion, the diffusion process by turbulent magnetic fields is classified into several regions by ratio of the gyro-radius and the scale of turbulence. When the ratio becomes larger then 10 to the minus 0.5 power, the analysis with the assumption of point scattering can be applied with the mean free path E sup 2. However, when the ratio is smaller than 10 to the minus 0.5 power, we need a more complicated analysis or simulation. Assuming the turbulence scale of magnetic fields of the Galaxy is 10-30pc and the mean magnetic field strength is 3 micro gauss, the energy of cosmic ray with that gyro-radius is about 10 to the 16.5 power eV
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