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  • ASTROPHYSICS  (2)
  • Polymer and Materials Science  (2)
  • 1985-1989  (2)
  • 1975-1979  (2)
  • 1
    Electronic Resource
    Electronic Resource
    Weinheim : Wiley-Blackwell
    Angewandte Makromolekulare Chemie 75 (1979), S. 167-175 
    ISSN: 0003-3146
    Keywords: Chemistry ; Polymer and Materials Science
    Source: Wiley InterScience Backfile Collection 1832-2000
    Topics: Chemistry and Pharmacology , Physics
    Description / Table of Contents: The crazing of two rubber-toughened plastics (ABS, HIPS) is investigated by measuring the small angle x-ray scattering (SAXS) during a tensile deformation. In both systems the onset of crazing is observed near the yield-maximum if the samples are continuously strained. The craze-rate of HIPS is much higher than that of ABS and after unloading HIPS shows a considerable recovery in contrast to ABS. The application of SAXS to the characterization of craze-phenomena is compared with that of other methods.
    Notes: An zwei schlagfesten Mehrphasensystemen (ABS, HIPS) wird das Crazing durch Messung der Röntgenkleinwinkelstreuung bei einer mechanischen Verformung verfolgt. In beiden Systemen setzt bei kontinuierlicher Zugbeanspruchung unmittelbar in der Nähe des Yield-Maximums eine starke Craze-Bildung ein. Beim schlagfesten Polystyrol (HIPS) findet man eine in Vergleich zum ABS wesentlich höhere Craze-Rate und nach Entlastung eine ausgeprägtere Reversibilität des Crazings. Die Aussagemöglichkeiten der Röntgenkleinwinkelstreuung zur Craze-Charakterisierung werden mit denen anderer Methoden verglichen.
    Additional Material: 6 Ill.
    Type of Medium: Electronic Resource
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  • 2
    Electronic Resource
    Electronic Resource
    Weinheim : Wiley-Blackwell
    Materialwissenschaft und Werkstofftechnik 17 (1986), S. 120-126 
    ISSN: 0933-5137
    Keywords: Chemistry ; Polymer and Materials Science
    Source: Wiley InterScience Backfile Collection 1832-2000
    Topics: Mechanical Engineering, Materials Science, Production Engineering, Mining and Metallurgy, Traffic Engineering, Precision Mechanics
    Description / Table of Contents: Investigations on the Creep Behaviour of a X 20 CrMoV 12 1 Bend, Fabricated by an Inductive Pipe Bending MachineA bend with a bend radius of 1700 mm -350 mm outer diameter and 25 mm wall thickness - of a X 20 CrMo V 12 1 steel, fabricated by an inductive pipe bending machine at 1050-900 °C deformation temperature was investigated. Heat treatment after fabrication: air cooling from 1050 °C, following a 2 hour annealing at 770 °C with air cooling. In addition to the usual mechanical and technological tests at ambient temperature and 530 °C, creep tests were conducted at 530 °C with unnotched and notched specimens. For comparison a straight pipe with the same dimensions was proofed, too.
    Notes: Ein Rohrbogen mit einem Biegeradius von 1700 mm - bei einem Rohraußendurchmesser von 350 mm und einer Wanddicke von etwa 25 mm - wurde aus dem warmfesten Röhrenstahl X 20 CrMo V 12 1, W.-Nr. 1.4922, nach dem Induktivbiegeverfahren bei einer Verformungstemperatur von 1050 bis 900 °C hergestellt. Die nachfolgende Wärmebehandlung erfolgte bei 1050 °C/Luft + 770 °C/2 h/Luft.Neben den üblichen mechanischen und mechanisch-technologischen Untersuchungen bei Raumtemperatur und bei 530 °C wurden auch Zeitstandversuche mit glatten und gekerbten Proben bei 530 °C durchgeführt. Zum Vergleich wurde auch ein gerades Rohr mit den gleichen Abmessungen zur Prüfung herangezogen.Alle ermittelten Werte entsprechen den Gewährleistungswerten. Rohrbogen und Rohr weisen auch nach langer Laufzeit noch hohe Werte der Duktilität auf.
    Additional Material: 9 Ill.
    Type of Medium: Electronic Resource
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  • 3
    Publication Date: 2019-06-27
    Description: Variational calculations of the binding energies of iron atoms and condensed matter in strong magnetic fields (greater than 10 to the 12th gauss). These calculations include the electron exchange energy. The cohesive energy of the condensed matter, which is the difference between these two binding energies, is of interest in pulsar theories and in the description of the surfaces of neutron stars. It is found that the cohesive energy ranges from 2.6 keV to 8.0 keV.
    Keywords: ASTROPHYSICS
    Type: Astrophysical Journal; vol. 215
    Format: text
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  • 4
    Publication Date: 2019-07-12
    Description: The evolution of polytropic 1.46-solar-mass 3-Gg/cu cm (4 x 10 to the 8th)-K pure C cores is investigated theoretically by means of model computations starting from the runaway stage. The temperature in central zones is raised to the runaway temperature, and the evolution is followed in a spherical coordinate system. In models of burning without detonation, it is found that the initially spherical burning front is Rayleigh-Taylor unstable, without bipolar jets or equatorial rings; that some C is not burned to Ni; and that the Ni in the 0.8-1.0 solar mass of burned fuel produced can account for observed properties of type I supernovae.
    Keywords: ASTROPHYSICS
    Type: Astrophysical Journal, Part 1 (ISSN 0004-637X); 307; 619-643
    Format: text
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