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Sökning: WFRF:(Friedel P.)

  • Resultat 1-6 av 6
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1.
  • Erni, W., et al. (författare)
  • Technical design report for the PANDA (AntiProton Annihilations at Darmstadt) Straw Tube Tracker
  • 2013
  • Ingår i: European Physical Journal A. Hadrons and Nuclei. - : Springer Science and Business Media LLC. - 1434-6001 .- 1434-601X. ; 49:2
  • Tidskriftsartikel (refereegranskat)abstract
    • This document describes the technical layout and the expected performance of the Straw Tube Tracker (STT), the main tracking detector of the PANDA target spectrometer. The STT encloses a Micro-Vertex-Detector (MVD) for the inner tracking and is followed in beam direction by a set of GEM stations. The tasks of the STT are the measurement of the particle momentum from the reconstructed trajectory and the measurement of the specific energy loss for a particle identification. Dedicated simulations with full analysis studies of certain proton-antiproton reactions, identified as being benchmark tests for the whole PANDA scientific program, have been performed to test the STT layout and performance. The results are presented, and the time lines to construct the STT are described.
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2.
  • Trydeman Knudsen, Marie, et al. (författare)
  • Characterization factors for land use impacts on biodiversity in life cycle assessment based on direct measures of plant species richness in European farmland in the ‘Temperate Broadleaf and Mixed Forest`.
  • 2017
  • Ingår i: Science of the Total Environment. - : Elsevier BV. - 0048-9697 .- 1879-1026. ; 580, s. 358-366
  • Tidskriftsartikel (refereegranskat)abstract
    • Life Cycle Assessment (LCA) is a widely used tool to assess environmental sustainability of products. The LCAshould optimally cover themost important environmental impact categories such as climate change, eutrophicationand biodiversity. However, impacts on biodiversity are seldom included in LCAs due tomethodological limitationsand lack of appropriate characterization factors. When assessing organic agricultural products theomission of biodiversity in LCA is problematic, because organic systems are characterized by higher species richnessat field level compared to the conventional systems. Thus, there is a need for characterization factors to estimateland use impacts on biodiversity in life cycle assessment that are able to distinguish between organic andconventional agricultural land use that can be used to supplement and validate the few currently suggested characterization factors. Based on a unique dataset derived fromfield recording of plant species diversity in farmlandacross six European countries, the present study provides newmidpoint occupation Characterization Factors(CF) expressing the Potentially Disappeared Fraction (PDF) to estimate land use impacts on biodiversity in the‘Temperate Broadleaf and Mixed Forest’ biome in Europe. The method is based on calculation of plant specieson randomly selected test sites in the biome and enables the calculation of characterization factors that are sensitiveto particular types ofmanagement.While species richness differs between countries, the calculated CFs areable to distinguish between different land use types (pastures (monocotyledons or mixed), arable land andhedges) and management practices (organic or conventional production systems) across countries. The new occupationCFs can be used to supplement or validate the fewcurrent CF's and can be applied in LCAs of agriculturalproducts to assess land use impacts on species richness in the ‘Temperate Broadleaf and Mixed Forest’ biome.
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6.
  • Webber, K. B., et al. (författare)
  • Chemical Analysis of the Brightest Star of the Cetus II Ultrafaint Dwarf Galaxy Candidate
  • 2023
  • Ingår i: Astrophysical Journal. - 0004-637X .- 1538-4357. ; 959:2
  • Tidskriftsartikel (refereegranskat)abstract
    • We present a detailed chemical abundance analysis of the brightest star in the ultrafaint dwarf (UFD) galaxy candidate Cetus II from high-resolution Magellan/MIKE spectra. For this star, DES J011740.53-173053, abundances or upper limits of 18 elements from carbon to europium are derived. Its chemical abundances generally follow those of other UFD galaxy stars, with a slight enhancement of the alpha-elements (Mg, Si, and Ca) and low neutron-capture element (Sr, Ba, and Eu) abundances supporting the classification of Cetus II as a likely UFD. The star exhibits lower Sc, Ti, and V abundances than Milky Way (MW) halo stars with similar metallicity. This signature is consistent with yields from a supernova originating from a star with a mass of similar to 11.2 M-circle dot. In addition, the star has a potassium abundance of [K/Fe] = 0.81, which is somewhat higher than the K abundances of MW halo stars with similar metallicity, a signature that is also present in a number of UFD galaxies. A comparison including globular clusters and stellar stream stars suggests that high K is a specific characteristic of some UFD galaxy stars and can thus be used to help classify objects as UFD galaxies.
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  • Resultat 1-6 av 6

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