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Aspects of North Swedish intonational phonology.

The present contribution discusses features of North Swedish intonational phonology. One characteristic feature is final element stress in compounds occurring particularly in dialects of North Botnia. The idea proposed here is that the accentual pattern (HL) of a compound has a different alignment in these dialects compared to East Standard Swedish. Another characteristic feature is related to a s

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There are several characters with a brief appearance in the history of the drama, thus having an apparent minor significance in designing the play. They seem to be mere “working tools” for the playwright. However when relating them to the major issues of the literary product and if integrating them in a larger vision of the whole creation of the author their significance and role can be outlined i

Den nya svenska arbetarklassen : rasifierade arbetares kamp inom facket

Vilken bild har LO av invandrare och invandrararbetare? Diana Mulinari och Anders Neergaard har forskat om nätverket FAI — Fackligt Aktiva Invandrare — och erfarenheter av kamp inom facket. Hur kan man jobba fackligt om man inte betraktas som ”en riktig arbetare”? Hur skapas medvetanden som samtidigt spänner över klass, kön och etnicitet? Med hjälp av begreppen rasifiering och kulturrasism analyse

Algorithm and Hardware Aspects of Pre-coding in Massive MIMO Systems

Massive Multiple-Input Multiple-Output (MIMO) systems have been shown to improve both spectral and energy efficiency one or more orders of magnitude by efficiently exploiting the spatial domain. Low-cost RF chains can be employed to reduce the Base Station (BS) cost, however this may require additional baseband processing to handle induced distortions due to the hardware impairments. In this artic

The Nature of the Metal-Rich Thick Disk

We have traced the Galactic thick disk to its, to date, highest metallicities. Based on high-resolution spectroscopic observations of 187 F and G dwarf stars that kinematically can be associated either with the thin disk (60 stars) or with the thick disk (127 stars), we find that the thick disk stars reach at least solar metallicities, and maybe even higher. This finding is independent of the U_LS