2009
DOI: 10.1002/pssc.200982114
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Positron annihilation studies on the nature and thermal behaviour of irradiation induced defects in tungsten

Abstract: The similarity to crown ethers is apparent when the arrangement of the oxygen atoms of the carbonyl groups of the protein backbone in the structure of the potassium channel (see schematic drawing of a section of the structure) found in the bacterium Streptomyces lividans is considered. This particular part of the channel pore acts as the selectivity filter, with the permeability of the channel for K+ being as much as 10 000 times greater than for the Na+ ion. In fact, in this area of the structure two K+ ions … Show more

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Cited by 51 publications
(35 citation statements)
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“…• [253,256,259], and Fe and ferritic-martensitic steels [257,260,262]. For this area, nuclear reaction analysis reveals itself to be a very powerful tool because specific reactions exist for almost every isotope 2 H(D), 3 H(T) and 3 He namely: (1) D(d, p0) 3 He or D( 3 He, p0) 4 He, (2) T(d, n) 4 He, and (3) 3 He(d, p0) 4 He.…”
Section: Discussionmentioning
confidence: 99%
“…• [253,256,259], and Fe and ferritic-martensitic steels [257,260,262]. For this area, nuclear reaction analysis reveals itself to be a very powerful tool because specific reactions exist for almost every isotope 2 H(D), 3 H(T) and 3 He namely: (1) D(d, p0) 3 He or D( 3 He, p0) 4 He, (2) T(d, n) 4 He, and (3) 3 He(d, p0) 4 He.…”
Section: Discussionmentioning
confidence: 99%
“…Before moving on to the investigation of vacancies in W-Ta and W-V alloys, we evaluate the energies of formation of small vacancy clusters in bcc-W, which are important for modeling kinetics of nucleation and growth of voids in tungsten under irradiation. [57][58][59] Table III shows the calculated formation and binding energies of small clusters of vacancies (N v = 2-6) calculated for pure tungsten using the PBE-GGA exchange-correlation functional 43 with semicore electrons included in the PAW potential implemented within the VASP code. The calculated formation energies for the first-nearestneighbor and second-nearest-neighbor divacancies are 6.624 and 6.989 eV, respectively, in agreement with values found previously (6.71 and 6.93 eV) using the PLATO code and atomiclike orbital basis sets.…”
Section: Point Defect Propertiesmentioning
confidence: 99%
“…In order to better understand its swelling and embrittlement observed in special irradiation conditions, we use PAS to study the vacancy defects properties in this material. We have first shown the migration and agglomeration of single vacancy in the temperature range from 473 to 600K [9] and its interaction with helium [10]. More recently we have observed the formation of vacancy clusters in self ion irradiated W and the effect of the temperature on the size of these clusters.…”
mentioning
confidence: 97%