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Effective field theories in QCD
These are the proceedings of the workshop on ``Effective Field Theories of QCD'' held at the Physikzentrum Bad Honnef of the Deutsche Physikalische Gesellschaft, Bad Honnef, Germany from November 26 to 30, 2001. The workshop concentrated on Chiral Perturbation Theory in its various settings, its relations with lattice QCD and dispersion theory and the use of effective field theories in systems wit
At bryta in i ledarskap - kvinnor och ledarkarriärer vid Lunds universitet
CREEPER - a new algorithm for sequential decoding
Spontaneous innovation for future deception in a male chimpanzee
Information, Trust and Diffusion of Smallpox Vaccination. The Case of Scania, Sweden 1802-1835
No title
Insecure Attachment and other Relational Qualities predict Depressive Symptoms in Fathers Post-birth
Carbon neutral destinations: a conceptual analysis
Metodstöd habilitering/rehabilitering – En modell för kvalitetsutveckling av projektarbete i praktisk verksamhet.
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German language short article on the 'Risk of Defining Risk', discussing and comparing the pros and cons of different sociological definitions (e.g. by Ulrich Beck and Niklas Luhmann)
Being there: Reaching critical mass in the virtual classroom
Cognitive functional limitations and changes in travel behaviour after stroke.
Nanofluidics in hollow nanowires
On targets
Fabrication and characterisation of high sensitive microcantilever for biosensor application
A new environmental attention technique.
Exploring National – Local Dynamics in the Social Exclusion of immigrant groups: A Swedish Case
Evocations- Mixing Art and Cultural Analysis
A Comparison of Copper Abundances in Globular Cluster and Halo Field Giant Stars
We derive [Cu/Fe] for 117 giant stars in 10 globular clusters (M3, M4, M5, M10, M13, M15, M71, NGC 7006, NCG 288, and NGC 362) and find that globular cluster Cu abundances appear to follow [Cu/Fe] trends found in the field. This result is interesting in light of recent work, which indicates that the globular cluster ω Centauri shows no trend in [Cu/Fe] with [Fe/H] over the abundance range -2.0<[Fe
