125590731
ALEPH: technical report 1983
122204997
First measurement of the quark-to-photon fragmentation function
Earlier measurements at LEP of isolated hard photons in hadronic Z decays, attributed to radiation from primary quark pairs, have been extended in the ALEPH experiment to include hard photon productioninside hadron jets. Events are selected where all particles combine democratically to form hadron jets, one of which contains a photon with a fractional energyz≥0.7. After statistical subtraction of non-prompt photons, the quark-to-photon fragmentation function,D(z), is extracted directly from the measured 2-jet rate. By taking into account the perturbative contributions toD(z) obtained from anO(ααs) QCD calculation, the unknown non-perturbative component ofD(z) is then determined at highz. Provided due account is taken of hadronization effects nearz=1, a good description of the other event topologies is then found.
122041721
Production of excited beauty states inZ decays
AbstractA data sample of about 3.0 million hadronicZ decays collected by the ALEPH experiment at LEP in the years 1991 through 1994 is used to make an inclusive selection of B hadron events. In this event sample 4227±140±252B* mesons in the decayB*→Bγ and 1944±108±161B**u,d mesons decaying into a B meson and a charged pion are reconstructed. Here and in the followingB**u,d denotes the eightL=1(bū) and (bd) states and their charge conjugate.For the well establishedB* meson the following quantities are obtained:ΔM=MB*−MB=(45.30±0.35±0.87) MeV/c2 andNB*/(NB+NB*)=(77.1±2.6±7.0)%. The angular distribution of the photons in theB* rest frame is used to measure the relative contribution of longitudinalB* polarization states to beσL/(σL+σT)=(33±6±5)%.In theM(Bπ)−M(B) mass difference resonance structure is observed at (424±4±10) MeV/c2, for which the shape and position is consistent with the expectation forB**u,d states decaying intoB(*)π±. The relative production rate is determined to be
$$\begin{gathered} \frac{{BR(Z \to b \to B_{u,d}^{ * * } )}}{{BR(Z \to b \to B_{u,d} )}} \hfill \\ = [27.9 \pm 1.6(stat) \pm 5.9(syst) {}_{ - 5.6}^{ + 3.9} (model)]\% \hfill \\ \end{gathered} $$
 where the third error reflects the uncertainty due to different production and decay models for the broadB**u,d states.
122230572
A measurement of the ratio of longitudinal and transverse structure functions in neutrino interactions between 30 and 200 GeV
Abstract A new measurement of the ratio R = σ L / σ T of longitudinal and transverse structure functions in neutrino interactions on iron between 30 and 190 GeV neutrino energy is reported. The result is given as a function of the scale parameter x and the inelasticity ν of the interaction. The average value is R = 0.10 ± 0.07 around ν ≈ 50 GeV and is in accordance with a prediction from the QCD theory.
26322213
A study of Bose-Einstein correlations ine+e− annihilation at 91 GeV
This paper describes a study of Bose-Einstein correlations made using the ALEPH detector at LEP. The correlations are found to enhance the two particle differential cross section for pairs of identical pions by a factor which can be roughly parametrized byR(Q)=1+λ exp(-Q2σ2), whereQ is the difference in the 3-momenta of the two pions in their centre of mass frame, λ=0.51±0.04±0.11 and σ=3.3±0.2±0.8 GeV−1, which corresponds to a source size of 0.65±0.04±0.16 fm. The large systematic errors on these results reflect their strong dependence on the choice of the reference sample used in the analysis. This problem is believed to occur primarily because of uncertainties in the rates of resonance production and a lack of knowledge about the pion-pion strong interaction. No significant correlations are seen amongst like-charged pion-kaon pairs.
122188618
Charged particle pair production associated with a lepton pair in Z decays. indication of an excess in the tau channel
In a sample of 200 000 Z decays, events with two leptons and an additional pair of charged particles are studied. The 35 events found show a possible excess in the tau channel compared with the expectation from electroweak processes. The features of the events are consistent with radiation of virtual photons.
111052021
SUPERCONDUCTING ACCELERATOR MODULES FOR STORAGE RINGS AND SYNCHROTRONS
We report on the production status of 6 superconducting 500 MHz accelerating modules (2 for Cornell University for upgrading CESR, 2 for the Taiwan Light Source and two for the Canadian Light Source). We focus on the test results on cavities and RF windows. The superconducting 500 MHz cavities fully prepared and assembled at ACCEL reached 12 MV/m accelerating gradient during cold vertical RF test on a regular basis. The assembly of the first module is almost completed. The cold RF test of this first module at Cornell is scheduled for June this year.[1]
8322223
Flux trapping in niobium cavities during breakdown events ∗
We report on the discovery of increased residual losses in niobium cavities following rapid quenches, in particular after thermal breakdown and multipacting. Increases of the residual resistance in the breakdown affected region by more than a factor of 10 have been recorded in some instances. It is believed that magnetic flux, generated by thermocurrents during breakdown, is trapped as the cavity reverts to the superconducting state, resulting in the enhanced losses. A thermal cycle to above the critical temperature of niobium is required to restore the initial low-loss state.
123667389
Trapped magnetic flux in superconducting niobium samples
Trapped magnetic flux is known to be one cause of residual losses in bulk niobium superconducting radio frequency cavities. In the Meissner state an ambient magnetic field should be expelled from the material. Disturbances such as lattice defects or impurities have the ability to inhibit the expulsion of an external field during the superconducting transition so that the field is trapped. We have investigated the effect the treatment history of bulk niobium has on the trapped flux and which treatment leads to minimal flux trapping. For that purpose, we measured the fraction of trapped magnetic flux in niobium samples representing cavities with different typical treatment histories. The differences between single crystal and polycrystalline material as well as the influence of spatial temperature gradients and different cooling rates were investigated. In addition, the progression of the release of a trapped field during warm-up was studied. We found that heat treatment reduces trapped flux considerably and that single crystal samples trap less flux than polycrystalline niobium. As a consequence, the single crystal sample with $1200\ifmmode^\circ\else\textdegree\fi{}\mathrm{C}$ baking trapped the smallest amount of field which is about 42%. Moreover, the release of the trapped field during warm-up was observed to progress over a broad temperature range for the baked single crystal samples.
32138968
Performance of Tesla Cavities after Fabrication and Preparation in Industry
In order to demonstrate cw operation of TESLA cavities in a linear accelerator driven FEL application, two TESLA cavities were manufactured for BESSY. After production, both cavities were prepared for vertical test at ACCEL’s premises using state of the art chemical polishing and high pressure water rinsing techniques. The cavities were tested in DESY’s vertical RF test installation. Accelerating gradients close to 25 MV/m were reached. One cavity was completed with helium vessel modified for cw operation, prepared with chemical polishing and high pressure water rinsing and assembled with the required high power coupler at ACCEL. The fully dressed cavity was then shipped under vacuum to BESSY and is currently under test in the horizontal cryostat HoBiCaT.
15393287
Explosive field emitter processing in superconducting rf cavities
Superconducting niobium radiofrequency cavities for e + e accelerators presently are limited to accelerating gradients of 25 MV/m — far less than their theoretical capability of 50 MV/m. Field emission presents the main impediment to higher gradients. In many cases, in situ high-pulsed-power processing is used to explode emission sites (rf processing), thereby improving the cavity performance. Thermometric and microscopic results summarized here are used to develop a qualitative theory of the events leading up to rf processing. It is demonstrated that the ionization of gases from the emitter is crucial to the initiation of the explosion, similar to past observations made with dc emitters. This fact is underscored by the examination of emitters processed with intentionally administered helium gas in the cavity (helium processing). Numerical simulations of rf processing, including the ionization of gases by the field emission current, illustrate the conditions required for emitter explosion, and they confirm the importance of a plasma during such events. Most importantly, the calculations demonstrate that the positive space charge of the ions enhances the field emission current, and that the production of ions is a self amplifying process. A runaway situation can ensue, which explains the submicrosecond rf processing times observed experimentally. The rapid release of monolayer surface adsorbates at the emission site, in particular, can play a critical role in initiating voltage breakdown.