Improved flux limits for neutrinos with energies above 1022^{22} eV from observations with the Westerbork Synthesis Radio Telescope

Particle cascades initiated by ultra-high energy (UHE) neutrinos in the lunar regolith will emit an electromagnetic pulse with a time duration of the order of nano seconds through a process known as the Askaryan effect. It has been shown that in an observing window around 150 MHz there is a maximum chance for detecting this radiation with radio telescopes commonly used in astronomy. In 50 hours of observation time with the Westerbork Synthesis Radio Telescope array we have set a new limit on the flux of neutrinos, summed over all flavors, with energies in excess of $4\times10^{22}$ eV.Comment: Submitted to Phys. Rev. Let

Consequences of wall stiffness for a beta-soft potential

Modifications of the infinite square well E(5) and X(5) descriptions of transitional nuclear structure are considered. The eigenproblem for a potential with linear sloped walls is solved. The consequences of the introduction of sloped walls and of a quadratic transition operator are investigated.Comment: RevTeX 4, 8 pages, as published in Phys. Rev.

Photoproduction of eta meson within a coupled-channels K-matrix approach

We investigate photoproduction of eta mesons off protons and neutrons within a coupled-channels effective-Lagrangian method which is based on the K-matrix approach. The two-body final channels included are pi-N, eta-N, phi-N, rho-N, gamma-N, K-Lambda, and K-Sigma. Non-resonant meson-baryon interactions are included in the model via nucleon intermediate states in the s- and u-channels, meson exchanges in the t-channel amplitude and the u-channel resonances. The nucleon resonances S_{11}(1535), S_{11}(1650), S_{31}(1620), P_{11}(1440), P_{11}(1710), P_{13}(1720), P_{33}(1232), P_{33}(1600), D_{13}(1520), D_{13}(1700), and D_{33}(1700) are included explicitly in calculations. Our model describes simultaneously the available data as well on total and differential cross sections as on beam and target asymmetries. This holds for the p(gamma,eta)p reaction for photon energies ranging from very close to threshold to up to 3 GeV. The polarization observables show strong sensitivity to resonances that otherwise contribute only weakly to the total cross section. It is found that the pronounced bump-like structure seen in the excitation function of the n(gamma,eta)n cross section at gamma energies around 1 GeV, can be explained by the interference effects of S_{11}, P_{11} and P_{13} resonance contributions.Comment: 36 pages, 14 figures, one new figure added, discussions revised, version to appear in Phys. Rev.

Los bijvoeren van gemalen tarwe bij biggen gespeende

Het vervangen van 25% van het mengvoer door gemalen tarwe is bij gespeende biggen mogelijk met behoud van technische resultaten en gezondheid

Enzymtoevoeging aan biggenvoer

Het toevoegen van de enzymen beta-glucanase en xylanase (Porzyme-8 100e) aan biggenvoer met 30% gerst en 15% tarwe(gries) heeft géén positief effect op de technische resultaten, de uitval en het aantal veterinair behandelde gespeende biggen

Het *STAR-concept in vleesvarkensvoer

Het toevoegen van de structuurrijke componenten tarwekorrel en niet-ontsloten strobrok volgens *STAR-concept aan vleesvarkensvoer verlaagt het aantal varkens met maagslijmvliesaandoeningen. Het effect op de mesterijresultaten is gering

Prospects for GMRT to Observe Radio Waves from UHE Particles Interacting with the Moon

Ultra high energy (UHE) particles of cosmic origin impact the lunar regolith and produce radio signals through Askaryan effect, signals that can be detected by Earth based radio telescopes. We calculate the expected sensitivity for observation of such events at the Giant Metrewave Radio Telescope (GMRT), both for UHE cosmic rays (CR) and UHE neutrino interactions. We find that for 30 days of observation time a significant number of detectable events is expected above $10^{20}$ eV for UHECR or neutrino fluxes close to the current limits. Null detection over a period of 30 days will lower the experimental bounds on UHE particle fluxes by magnitudes competitive to both present and future experiments at the very highest energies.Comment: 21 pages, 9 figure

Voedingsonderzoek met tarwe en perspulp bij vleesvarkens

Begin 1997 starten twee nieuwe voedingsproeven bij vleesvarkens. Het eerste onderzoek richt zich op de vraag of er verschil in technische resultaten ontstaat wanneer 50% tarwe los wordt bijgevoerd of 50% tarwe in het mengvoer wordt geperst. Het tweedeonderzoek richt zich op het voeren van 10% perspulp in brijvoer- én droogvoerrantsoenen