<?xml version="1.0" encoding="UTF-8"?><?xml-stylesheet type="text/xsl" href="static/style.xsl"?><OAI-PMH xmlns="http://www.openarchives.org/OAI/2.0/" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xsi:schemaLocation="http://www.openarchives.org/OAI/2.0/ http://www.openarchives.org/OAI/2.0/OAI-PMH.xsd"><responseDate>2026-04-13T15:00:04Z</responseDate><request verb="GetRecord" identifier="oai:www.recercat.cat:2117/16422" metadataPrefix="qdc">https://recercat.cat/oai/request</request><GetRecord><record><header><identifier>oai:recercat.cat:2117/16422</identifier><datestamp>2026-01-30T08:05:49Z</datestamp><setSpec>com_2072_1033</setSpec><setSpec>col_2072_452950</setSpec></header><metadata><qdc:qualifieddc xmlns:qdc="http://dspace.org/qualifieddc/" xmlns:dc="http://purl.org/dc/elements/1.1/" xmlns:dcterms="http://purl.org/dc/terms/" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xmlns:doc="http://www.lyncode.com/xoai" xsi:schemaLocation="http://purl.org/dc/elements/1.1/ http://dublincore.org/schemas/xmls/qdc/2006/01/06/dc.xsd http://purl.org/dc/terms/ http://dublincore.org/schemas/xmls/qdc/2006/01/06/dcterms.xsd http://dspace.org/qualifieddc/ http://www.ukoln.ac.uk/metadata/dcmi/xmlschema/qualifieddc.xsd">
   <dc:title>Ferromagnetic transition of a two-component Fermi gas of hard spheres</dc:title>
   <dc:creator>Arias de Saavedra, F.</dc:creator>
   <dc:creator>Mazzanti Castrillejo, Fernando Pablo</dc:creator>
   <dc:creator>Boronat Medico, Jordi</dc:creator>
   <dc:creator>Polls, A.</dc:creator>
   <dc:subject>Àrees temàtiques de la UPC::Física</dc:subject>
   <dc:subject>Ferromagnetism</dc:subject>
   <dc:subject>Electron gas</dc:subject>
   <dc:subject>GROUND-STATE</dc:subject>
   <dc:subject>LIQUID-HE-3</dc:subject>
   <dc:subject>HELIUM</dc:subject>
   <dc:subject>ENERGY</dc:subject>
   <dc:subject>Ferromagnetisme</dc:subject>
   <dc:subject>Electrons--Distribució</dc:subject>
   <dcterms:abstract>We use microscopic many-body theory to analyze the problem of itinerant ferromagnetism in a repulsive atomic Fermi gas of hard spheres. Using simple arguments we show that the available theoretical predictions for the onset of the ferromagnetic transition predict a transition point at a density (kF a ∼ 1) that is too large to be compatible with the universal low-density expansion of the energy. We present variational calculations for the hard-sphere Fermi gas, in the framework of Fermi hypernetted chain theory, that shift the transition to higher densities (kF a ∼ 1.8). Backflow correlations, which are mainly active in the unpolarized system, are essential for this shift.</dcterms:abstract>
   <dcterms:abstract>Postprint (published version)</dcterms:abstract>
   <dcterms:issued>2012-03-12</dcterms:issued>
   <dc:type>Article</dc:type>
   <dc:relation>http://pra.aps.org/abstract/PRA/v85/i3/e033615</dc:relation>
   <dc:rights>http://creativecommons.org/licenses/by-nc-nd/3.0/es/</dc:rights>
   <dc:rights>Open Access</dc:rights>
   <dc:rights>Attribution-NonCommercial-NoDerivs 3.0 Spain</dc:rights>
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