共查询到20条相似文献,搜索用时 31 毫秒
1.
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 μ ν4×10 −10μ B (Bohr magneton). The most restrictive limits remain those from the plasmon decay in globular-cluster stars of eν2×10 −14e and μ ν3×10 −12μ B. 相似文献
2.
Starting point is the hypothesis that the observed Z→e +e −γ decays are mediated by a (composite) spin 0 boson X with 40 mX50 GeV. The consequences for e +e−→e +e−, e +e −→γγ and e +e−→ hadrons at PETRA are explored. PETRA experiments turn out to be sensitive up to masses mX50 GeV; the best indicator for mX 48 GeV is the angular distribution of Bhabha scattering. 相似文献
3.
The reaction γ p → π °γ′ p has been measured with the TAPS BaF 2 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 μ Δ+ = (2.7 +1.0−1.3( stat) ± 1.5( syst) ± ( theor)) π N has been extracted. 相似文献
4.
The time-dependence of the decay rate of initially pure K 0 into the final state (π +π −π 0) has been studied in search for the decay k S0→π +π −π 0. No evidence is found in a sample of 384 observed events. The ratio of the CP -violating K S0 amplitude and the K L0 amplitude is η +−0 = (0.13 −0.20+0.17) + i(0.17 −0.26+0.27); the ratio of the CP-conserving K S0 amplitude and the K L0 amplitude is < 0.4. The energy dependence of the K 0→π +π −π 0 matrix element is found to be a+−0 = −0.31 ± 0.03. 相似文献
5.
The theoretical mechanisms for the decays ψ′ → ψπ 0 and ψ′ → ψη, which violate SU 2 and SU 3, respectively discussed. It is argued that symmetry breaking in the decay amplitudes may be as important as π 0 −η −η′ mixing. The π 0 −η mechanism ψ′ → ψν → ψπ 0 leads to Γ(ψ′ → ψπ 0) = (3.3±1.0) × 10 −3 Γ(ψ′ → ψν), but this number may be enhanced by a factor as large as 12 by π 0−η′ mixing and isospin violation in the decay amplitude. The related decays ψ → ηγ and ψ → η′γ are also discussed. 相似文献
6.
We analyze the supersymmetric contributions to direct– CP–violating observables in K→ππγ decays induced by gluino–mediated magnetic–penguin operators. We find that ε′ +−γ and the differential width asymmetry of K±→π ±π 0γ decays could be substantially enhanced with respect to their Standard Model values, especially in the scenario where ε′/ε is dominated by supersymmetric contributions. These observables could therefore provide a useful tool to search for New Physics effects in |Δ S|=1 transitions, complementary to ε′/ε and rare decays. 相似文献
7.
In terms of a quark model an explanation is given of charged pion photoproduction ratios, at small momentum transfer, in the processes γN → π ±N, γN → π ±Δ. The model is also shown to be consistent with π 0 photoproduction data. 相似文献
8.
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 φ e and φ μ, and an extended e ↔ μ permutation invariance. After symmetry-breaking, a multiplicatively conserved “permutation parity” π = ± 1 for all particles naturally emerges, with π μ = −π e = 1. The model forbids μ → eγ but predicts e −e − → μ −μ − mediated by π = −1 Higgs bosons at 10 −11 times the rate of typical weak cross sections. 相似文献
9.
We study the ρ 0 and φ decays into π +π −γ, π 0π 0γ and φ into π 0ηγ using a chiral unitary approach to deal with the final state interaction of the MM system. The final state interaction modifies only moderately the large momenta tail of the photon spectrum of the ρ 0→π +π −γ decay. In the case of φ decay the contribution to π +π −γ and π 0π 0γ decay proceeds via kaonic loops and gives a distribution of ππ invariant masses in which the f0(980) resonance shows up with a very distinct peak. The spectrum found for φ→π 0π 0γ decay agrees with the recent experimental results obtained at Novosibirsk. The branching ratio for φ→π 0ηγ, dominated by the a0(980), is also in agreement with recent Novosibirsk results. 相似文献
10.
Limits for the neutrino decay ν H→ν L+γ, where ν H and ν L are assumed to be massive neutrinos with mVH> 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>3.3×10 14 s/eV for a thermal spectrum at a temperature
. 相似文献
11.
We study the contribution of Bc mesons to the search for B → τν τ decays. We find that at LEP the contributions from Bu and Bc mesons can be comparable. This observation can have a relevant impact on the extraction of constraints on new physics (such as charged-Higgs contributions) from current LEP limits on B → τν final states. Inclusion of the Bc contribution can reduce the current L3 limit on tan β/ MH from 0.38 GeV −1 (90% CL) down to 0.27 GeV −1 (90% CL). 相似文献
12.
Five dimensional classical unified field theories as well as Yang-Mills theory with gauge group U (1), are described in terms of a Lorentzian five dimensional space V 5 with metric tensor γβ which admits a space-like Killing vector ζ . It is assumed that: (1) V 5 has the topology of V 4 x S 1, S 1 is a circle and V 4 is a four dimensional Lorentzian space that is asymptotically flat and (2) the Einstein tensor Γ β of V5 satisfies Γ β Uυ β 0 where U and υ are future oriented time-like vectors with γ βυ ζ β = 0. The spinor approach of Witten [4], Nester [3] and Moreschi and Sparling [5] is used to show that the conserved five dimensional energymomentum vector P = ifΓ β = 0 then V 5 must admit a time-like Killing vector. Lichnerowicz's results [1] then imply that V 5 must be flat. A lower bound for P 4 (the mass) similar to that found by Gibbons and Hull [6] is obtained. 相似文献
13.
We calculate the corrections to various low-energy theorems concerning the behaviour of the pseudoscalar meson form factors near t=0. In particular we discuss (i) the Ademollo-Gatto theorem, (ii) Sirlin's relation between the Kl3 form factor ƒ +Kπ( t) and the electromagnetic form factors, (iii) the Callan-Treiman relation, and (iv) the Dashen-Weinstein relation, which connects the slope λ 0 of ƒ 0Kπ( t) with the ratio FK/ Fπ. Furthermore, we point out a remarkable isospin breaking effect which is clearly visible in the experimental rates of the decays K +→π 0e +ν, K 0→π −e +ν. 相似文献
14.
We calculate the amplitude of the decays η → π 0π +π − and η → π 0π 0π 0 to first non-leading order in the low-energy expansion. It is shown that the infrared singularities of chiral perturbation theory strongly enhance the perturbation generated by the quark mass term. The corrections of order ms increase the current algebra prediction for the rate by more than a factor of two and remove the well-known discrepancy between the low-energy theorems of current algebra and experiment. 相似文献
15.
A FNAL E799 Collaboration has carried out a search for the lepton-family number violating decay π 0 → μ ±e using π 0's produced from KL → π 0π 0π 0 decays in flight. No events were observed. Assuming that lepton-family number violation is charge independent, the 90% confidence level upper limit on was determined to be 8.6 × 10 −9. 相似文献
17.
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 νeνμ,νeντ 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
18.
The process η → π 0π 0γγ is discussed in Chiral Perturbation Theory (ChPT). Special attention is deveted to one-loop corrections, η-η′ mixing effects and vector-meson dominance of ChPT counter-terms. The less interesting η → π +π −γγ transition is briefly discussed too. 相似文献
19.
We study semileptonic decays B→η (′)lν, taking into account the flavor-singlet contribution ( Fsinglet+) to the B→η (′) form factors, which arises from the two-gluon emission in a decaying B meson. It has been recently pointed out that, in addition to large weak annihilation effects, the unknown value of Fsinglet+ prevents accurate theoretical estimates in the analysis of B→η′ K decays in QCD factorization. We present a certain method to determine Fsinglet+ with a reasonable accuracy, using B→η (′)lν and B→π lν decays. We also investigate the possible effect of Fsinglet+ on the estimated branching ratios (BRs) for B→η (′)lν and find that the BR for B→η′ lν is particularly sensitive to the effect of Fsinglet+. 相似文献
20.
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 ν e into both ν μ and a sterile species ν s , while atmospheric neutrino data are explained through ν μ to ν e 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 ν τ with lifetime τ ντ ≈ 10 2-10 4 seconds, as well as the masses and oscillations of the three light neutrinos ν e, ν μ and ν s 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
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