Why are we fat? Discussions on the socioeconomic dimensions and responses to obesity

This paper draws together contributions to a scientific table discussion on obesity at the European Science Open Forum 2008 which took place in Barcelona, Spain. Socioeconomic dimensions of global obesity, including those factors promoting it, those surrounding the social perceptions of obesity and those related to integral public health solutions, are discussed. It argues that although scientific accounts of obesity point to large-scale changes in dietary and physical environments, media representations of obesity, which context public policy, pre-eminently follow individualistic models of explanation. While the debate at the forum brought together a diversity of views, all the contributors agreed that this was a global issue requiring an equally global response. Furthermore, an integrated ecological model of obesity proposes that to be effective, policy will need to address not only human health but also planetary health, and that therefore, public health and environmental policies coincide.

Kiribilen kosmologia kuantikorako sarrera

Gradu amaierako lan hau kiribilen kosmologia kuantikorako sarrera bat da. Lan honek 4 kapi- tulu ditu. Lehenengoan, sarrera bezala grabitazio kuantikoak izan duen bilakaera historikoa jaso da, halako teoria bat garatzeko motibazioak eta zailtasunak, eta honen garapenean kosmologia kuantikoak duen papera azalduz. Lanean, oro har, grabitazio kuantikoaren teoria bat eraikitzeko formalismo “kanonikoa” jarraitu da, alegia, erlatibitate orokorraren formulazio hamiltondarra era- biliz teoria kuantikoa garatzea. Bigarren kapituluan grabitazioaren teoria klasikoaren formulazio hamiltondarra garatu da, lehenik Arnowitt-Deser-Misner formalismoaren (Einstein-en geometro- dinamika bezala ere ezaguna denaren) bidez eta ondoren Ashtekar-en aldagaiak erabiliz. Bietan hamiltondar guztiz lotua lortzen da, hots, loturen konbinazio lineala den hamiltondarra. Lotu- ren bidezko formulazio hauen kuantizazioaren eta kribilen adierazpenaren oinarrizko aspektuak jaso dira bigarren kapituluan. Hirugarren kapituluan kosmologiaren teoria klasikoa Friedmann- Lemaˆ ıtre-Robertson-Walker metrika laua erabiliz azaltzen da era laburrean lehenik, eta ondoren Wheeler-DeWitt teoria kuantikoa eta kiribilen kosmologia kuantikoa eta hauek erabiliz lorturiko zenbait emaitza aipatzen dira. Azkenik, ondorioen atalarekin amaitzen da lana. Lana euskaraz idatzita dago.

A formalism based on moments for classical and quantum cosmology

Spanish Relativity Meeting (ERE 2014) Valencia, SPAIN, SEP 01-05, 2014