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1.
In e+e annihilations at SPEAR we have searched for narrow neutral resonances in the eπ and μπ channels for masses between 0.5 GeV/c2 and 1.5 GeV/c2. No evidence for such states has been found. Under standard theoretical assumptions for production cross sections and decay branching ratios of heavy leptons a lower limit of 1.2 GeV/c2 can be set on the mass.  相似文献   

2.
We compute non-perturbative contributions to BXsl+l that are not explicitly suppressed by powers of the b-quark mass. They are proportional to and arise from an interference between the free-quark amplitude and high order terms in the matrix element of the four-quark operator sγμ(1 − γ5)cc−βγμ(1 − γ5)bβ. This correction is found to be small over most of the dalitz plot except near the charm threshold. Unfortunately, the perturbative computation we have performed is invalid near charm threshold and we do not except to see the structure found at lowest order reproduced in the data. We conclude that these non-perturbative contributions do not significantly modify the previous analysis of BXsl+l.  相似文献   

3.
4.
O. Shanker 《Nuclear Physics B》1985,250(1-4):351-368
We describe a scheme to generate light Dirac neutrinos. It uses a heavy symmetry-breaking scale to avoid introducing very small couplings or vacuum expectation values. We show how the scheme can be applied to left-right symmetric and to horizontal gauge models with four generations of fermions. In these models neutrino oscillations occur only between pairs of generations (e.g. νe−ντ oscillations can occur with no νμ−νe or νμ−ντ oscillations).  相似文献   

5.
The similarity between the weak interactions of electron and muon is extended to the principle that all e and μ interactions in gauge models are invariant under e ↔ μ exchange. This necessitates the existence of two Higgs doublets φe and φμ, and an extended e ↔ μ permutation invariance. After symmetry-breaking, a multiplicatively conserved “permutation parity” π = ± 1 for all particles naturally emerges, with πμ = −πe = 1. The model forbids μ → eγ but predicts ee → μμ mediated by π = −1 Higgs bosons at 10−11 times the rate of typical weak cross sections.  相似文献   

6.
We argue that the presence of second-class neutral currents can be tested from the observations of and electron polarisation in η→π0e+e-. Consequences of this model in η→π±eνe±→ηπ±ντ and τ±→ωπ±ντ decays which would establish second-class charged currents are also discussed.  相似文献   

7.
A search is made for a short lived neutral particle, ø, in the decay of the 3.68 MeV (3/2-) state in 13C. No evidence for such a particle with a rest mass in the region of 1.7–2.0 MeV/c2 is found with a limit on the branching ratio Γ øγ7×10 −5. An upper limit of 10−6 is placed for the coupling of such a particle to proton/neutron.  相似文献   

8.
We present a model where an unstable MeV Majorana tau neutrino can naturally reconcile the cold dark matter model (CDM) with cosmological observations of large and small scale density fluctuations and, simultaneously, with data on solar and atmospheric neutrinos. The solar neutrino deficit is explained through long wavelength, so-called just-so oscillations involving conversions of νe into both νμ and a sterile species νs , while atmospheric neutrino data are explained through νμ to νe conversions. Future long baseline neutrino oscillation experiments, as well as some reactor experiments will test this hypothesis. The model is based on the spontaneous violation of a global lepton number symmetry at the weak scale. This symmetry plays a key role in generating the cosmologically required decay of the ντ with lifetime τντ ≈ 102-104 seconds, as well as the masses and oscillations of the three light neutrinos νe, νμ and νs required in order to account for solar and atmospheric neutrino data. It also leads to the invisibly decaying Higgs signature that can be searched at LEP and future particle colliders.  相似文献   

9.
A general approach for construction of quark and lepton mass matrices is formulated. The hierarchy of quarks and charged leptons (“electrons”) is large, it leads using the experimental values of mixing angles to the hierarchical mass matrix slightly deviating from the ones suggested earlier by Stech and including naturally the CP-phase.

The same method based on the rotation of generation numbers in the diagonal mass matrix is used in the electron–neutrino sector of theory, where neutrino mass matrix is determined by the Majorano see-saw approach. The hierarchy of neutrino masses, much smaller than for quarks, was used including all existing (even preliminary) experimental data on neutrino mixing.

The leptonic mass matrix found in this way includes the unknown value of the leptonic CP-phase. It leads to large νμντ oscillations and suppresses the νeντ and also νeνμ oscillations. The explicit expressions for the probabilities of neutrino oscillation were obtained in order to specify the role of leptonic CP-phase. The value of time reversal effect (proportional to sin δ′) was found to be small 1%. However, a dependence of the values of νeνμeντ transition probabilities, averaged over oscillations, on the leptonic CP-phase has found to be not small – of order of ten percent.  相似文献   


10.
The time-dependence of the decay rate of initially pure K0 into the final state (π+ππ0) has been studied in search for the decay kS0→π+ππ0. No evidence is found in a sample of 384 observed events. The ratio of the CP -violating KS0 amplitude and the KL0 amplitude is η+−0 = (0.13−0.20+0.17) + i(0.17−0.26+0.27); the ratio of the CP-conserving KS0 amplitude and the KL0 amplitude is < 0.4. The energy dependence of the K0→π+ππ0 matrix element is found to be a+−0 = −0.31 ± 0.03.  相似文献   

11.
The differential geometry of an imbedded (e.g. string or membrane world sheet) surface in a higher-dimensional background is shown to be conveniently describable (except in the null limit case) in terms of what are designated as its first, second, and third fundamental tensors, which will have the respective symmetry properties ημν = η(μν) as a trivial algebraic identity, Kμνρ = K(μν)ρ as the “generalised Weingarten identity”, which is the (Frobenius type) integrability condition for the imbedding, and Ξλμνρ = Ξ(λμν)ρ as a “generalised Codazzi equation”, which depends on the background geometry being flat or of constant curvature, needing replacement by a more complicated expression for a generic value of the background curvature Bκλμν. The “generalised Gauss equation” expressing the dependence on this background curvature of the internal curvature tensor Rκλμν of the imbedded surface is converted into terms of the first and second fundamental tensors, and it is thereby demonstrated that the vanishing of the (conformally invariant) “conformation tensor”, i.e. the trace free part Cμνρ of the second fundamental tensor Kμvρ, is a sufficient condition for conformal flatness of the imbedded surface (and thus in particular for the vanishing of its (Weyl type) conformal curvature tensor Cκλμν) provided the background is itself conformally flat. In a trio of which the first two members are the generalised Gauss and Codazzi equations, the “third” member is shown to give an expression in terms of Cμνρ for the (trace free, conformally invariant) “outer curvature” tensor Ωκλμν whose vanishing is the condition for feasibility of the natural generalisation of the Walker frame transportation ansatz. The vanishing of Cμνρ is shown to be sufficient in a conformally flat background for the vanishing also of Ωκλμν.  相似文献   

12.
“Rare” annihilation channels for antiprotons stopping on heavy (Ag, Br) nuclei of photoemulsion, have been sought; 4872 stops of antiprotons on photoemulsion nuclei are analysed. Events of formation and decay of the hyperfragment Λ4H, escape of 8He and 8Li nuclei, one-prong stars with the mean range 79.5±5.1 μm of secondary slow “b” particles are found among the annihilation stars at capture on nuclei (Ag, Br). The lower limits for the production probability of Λ4H and 8He, 8Li nuclei per antiproton stopping in the nuclei (Ag, Br) are
WΛ4H2×10−4 and W8He,8Li=(1.3±0.6)×10−3.

The branching ratio for the production of one-prong stars with the secondary “b” particles is at least (1.3±0.6)×10−3. Possible mechanisms for a production of these events in annihilation processes are considered.  相似文献   


13.
The infrared reflection spectrum of p-type SnS single crystals was measured between 2 and 25μ. The observed dispersion was ascribed to the combined effects of lattice vibrations and free holes. An analysis gave for the index of refraction n0 = 3.6 ± 0.1, the dielectric constant = 19.5 ± 2, and the effective charge on the atoms e* = 0.7e0.

The effective mass of holes is isotropic in the plane perpendicular to the c-axis, with m* = 0.20m0; the effective mass parallel to the c-axis is much larger: m* m0.  相似文献   


14.
《Physics letters. [Part B]》2002,550(3-4):147-153
Narrow structures in the range of a few MeV have been searched for in ppπ+ and ppπ invariant mass spectra (Mppπ+ and Mppπ) obtained from exclusive measurements of the ppppπ+π reaction at Tp=725,750 and 775 MeV using the PROMICE/WASA detector at CELSIUS. The selected reaction is particularly well suited for the search for dibaryon resonances decoupled from NN and/or NΔ. In the mass range 2020 MeV/c2<mdibaryon<2085 MeV/c2 no narrow structures could be identified on the 3σ level of statistical significance neither in Mppπ nor in Mppπ+ giving an upper limit (95% C.L.) for dibaryon production in this reaction of σ<20 nb.  相似文献   

15.
Limits on neutrino electromagnetic properties from laboratory experiments and astrophysical arguments are reviewed with an emphasis on the currently favored range of small neutrino masses. We derive a helioseismological limit on the charge and dipole moment for all flavors of eν6×10−14e and μν4×10−10μB (Bohr magneton). The most restrictive limits remain those from the plasmon decay in globular-cluster stars of eν2×10−14e and μν3×10−12μB.  相似文献   

16.
Following recent results from the SNO solar neutrino experiment and the K2K long-baseline neutrino experiment, the combined existing data on neutrino oscillations now point strongly to a specific form for the lepton mixing matrix, with effective bimaximal mixing of νμ and ντ at the atmospheric scale and effective trimaximal mixing for νe with νμ and ντ at the solar scale (hence ‘tri-bimaximal’ mixing). We give simple mass-matrices leading to tri-bimaximal mixing, and discuss its relation to the Fritzsch–Xing democratic ansatz.  相似文献   

17.
Limits for the neutrino decay νH→νL+γ, where νH and νL are assumed to be massive neutrinos withmVH>mVL, are presented using data from the Solar Maximum Mission satellite taken in coincidence with the detected neutrino burst from SN 1987A. These limits are essentially independent of supernova models and are and τ/mνμ,τ>3.3×1014 s/eV for a thermal spectrum at a temperature .  相似文献   

18.
The lifetimes of the Cd+ 52P3/2 and 52P1/2 states have been measured by the Hanle effect. The Cd+ ions are produced in a d.c. discharge in cadmium vapor, with helium as buffer gas. The results are: τ(52P3/2) = (2.60±0.20) ×10−9sec, and τ(52P1/2) = (3.05 ± 0.13) × 10−9sec.

We measured also the cross sections for the destruction of the orientation in the 52P1/2Cd+ state (<5Å2), of the orientation (18±10Å2) and of the alignment (46±10Å2) in the 52P3/2 state due to collisions with the helium atoms.  相似文献   


19.
Let nν be the number if neutrinos much lighter than their charged lepton partners. In the standard electroweak model, using low-energy particle physics data, we prove that nν<137. If moreover the up-type and down type quarks are also highly nondegenerate in mass nν<47. The limits are much tighter for nondegenerate leptonic mass spectra. If the ratio of the lepton masses in two consecutive families is about 10 then there are at most two neutrinos beyond the known νe, νμ and ντ. The same result is obtained for a mass spectrum à la Froggat and Nielsen.  相似文献   

20.
The reaction γp → π°γ′p has been measured with the TAPS BaF2 calorimeter at the Mainz Microtron accelerator facility MAMI for energies between √2 = 1221–1331 MeV. Cross sections differential in angle and energy have been determined for the photon γ′ in three bins of the excitation energy. This reaction channel provides access to the magnetic dipole moment of the Δ+(1232) resonance and, for the first time, a value of μΔ+ = (2.7+1.0−1.3(stat) ± 1.5(syst) ± (theor)) πN has been extracted.  相似文献   

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