Scaling in the BCS to Bose crossover problem in different partial waves

The BCS superconductivity to Bose condensation crossover problem is studied in two dimensions in S, P, and D waves, for a simple anisotropic pairing, with a finite-range separable potential at zero temperature. The gap parameter and the chemical potential as a function of Cooper-pair binding B c exhibit universal scaling. In the BCS limit the results for coherence length ξ and the critical temperature T c are appropriate for highT c cuprate superconductors and also exhibit universal scaling as a function of B c.

On closed Einstein-de Sitter universes

We briefly summarize the idea of cosmological models with compact, flat spatial sections. It has been suggested that, because of the COBE satellite's maps of the microwave background, such models cannot be small in the sense of Ellis, and hence are no longer interesting. Here we use the method of cosmic crystallography by Lehoucq et al. to show that these models are physically meaningful even if the size of the spatial sections is of the same order of magnitude as the radius of the observational horizon. © 1998 Elsevier Science B.V.

One-dimensional superfluid Bose-Fermi mixture: Mixing, demixing, and bright solitons

We study an ultracold and dilute superfluid Bose-Fermi mixture confined in a strictly one-dimensional (1D) atomic waveguide by using a set of coupled nonlinear mean-field equations obtained from the Lieb-Liniger energy density for bosons and the Gaudin-Yang energy density for fermions. We consider a finite Bose-Fermi interatomic strength gbf and both periodic and open boundary conditions. We find that with periodic boundary conditions-i.e., in a quasi-1D ring-a uniform Bose-Fermi mixture is stable only with a large fermionic density. We predict that at small fermionic densities the ground state of the system displays demixing if gbf >0 and may become a localized Bose-Fermi bright soliton for gbf <0. Finally, we show, using variational and numerical solutions of the mean-field equations, that with open boundary conditions-i.e., in a quasi-1D cylinder-the Bose-Fermi bright soliton is the unique ground state of the system with a finite number of particles, which could exhibit a partial mixing-demixing transition. In this case the bright solitons are demonstrated to be dynamically stable. The experimental realization of these Bose-Fermi bright solitons seems possible with present setups. © 2007 The American Physical Society.

Faraday waves in quasi-one-dimensional superfluid Fermi-Bose mixtures

The generation of Faraday waves in superfluid Fermi-Bose mixtures in elongated traps is investigated. The generation of waves is achieved by periodically changing a parameter of the system in time. Two types of modulations of parameters are considered: a variation of the fermion-boson scattering length and the boson-boson scattering length. We predict the properties of the generated Faraday patterns and study the parameter regions where they can be excited. © 2013 American Physical Society.

Equações de estado exóticas na equação de Einstein

Pós-graduação em Física - IFT

Influência da temperatura e do teor de gordura nos parâmetros reológicos do leite condensado e creme de leite

Pós-graduação em Engenharia e Ciência de Alimentos - IBILCE

A trajetória escolar dos alunos(as) do curso de Educação Física: um estudo das Faculdades Integradas Einstein de Limeira

Coordenação de Aperfeiçoamento de Pessoal de Nível Superior (CAPES)

Análise de biografias de Einstein em dois livros de divulgação científica

In this paper we analyzed and compared two Albert Einstein’s biographies. The first one was “Albert Einstein and his inflatable universe”, written by Mike Goldsmith. The second biography was “Einstein – his life and universe”, written by Walter Isaacson. The intention of this comparison was to identify convergent and divergent points between two books, beyond verifying the possible neglected important points of Einstein’s life suppressed by Goldsmith to facilitate the comprehension of the text. Such details are those that we consider important to Albert Einstein’s intellectual development, and may have significantly contributed to the development of his theories. For this, our analysis was grounded in Douglas Allchin’s perspective, whose work presents aspects in the rhetoric of the text that contribute to the Science and scientist mystification.

Albert Einstein y la revolución de la Física al inicio del Siglo XX

Esta charla se enmarca dentro de la celebración de las XX Jornadas Blascabrerianas (de homenaje a y recuerdo de Blas Cabrera Felipe

Untersuchungen zum nichtstörungstheoretischen Renormierungsverhalten der Quanten-Einstein-Gravitation

Deutsche Version: Zunächst wird eine verallgemeinerte Renormierungsgruppengleichung für die effektiveMittelwertwirkung der EuklidischenQuanten-Einstein-Gravitation konstruiert und dann auf zwei unterschiedliche Trunkierungen, dieEinstein-Hilbert-Trunkierung und die$R^2$-Trunkierung, angewendet. Aus den resultierendenDifferentialgleichungen wird jeweils die Fixpunktstrukturbestimmt. Die Einstein-Hilbert-Trunkierung liefert nebeneinem Gaußschen auch einen nicht-Gaußschen Fixpunkt. Diesernicht-Gaußsche Fixpunkt und auch der Fluß in seinemEinzugsbereich werden mit hoher Genauigkeit durch die$R^2$-Trunkierung reproduziert. Weiterhin erweist sichdie Cutoffschema-Abhängigkeit der analysierten universellenGrößen als äußerst schwach. Diese Ergebnisse deuten daraufhin, daß dieser Fixpunkt wahrscheinlich auch in der exaktenTheorie existiert und die vierdimensionaleQuanten-Einstein-Gravitation somit nichtperturbativ renormierbar sein könnte. Anschließend wird gezeigt, daß der ultraviolette Bereich der$R^2$-Trunkierung und somit auch die Analyse des zugehörigenFixpunkts nicht von den Stabilitätsproblemen betroffen sind,die normalerweise durch den konformen Faktor der Metrikverursacht werden. Dadurch motiviert, wird daraufhin einskalares Spielzeugmodell, das den konformen Sektor einer``$-R+R^2$''-Theorie simuliert, hinsichtlich seinerStabilitätseigenschaften im infraroten (IR) Bereichstudiert. Dabei stellt sich heraus, daß sich die Theorieunter Ausbildung einer nichttrivialen Vakuumstruktur auf dynamische Weise stabilisiert. In der Gravitation könnteneventuell nichtlokale Invarianten des Typs $intd^dx,sqrt{g}R (D^2)^{-1} R$ dafür sorgen, daß der konformeSektor auf ähnliche Weise IR-stabil wird.

Einstein e Minkowski sulla relatività ristretta

La tesi è relativa al confronto tra Minkowski e Einstein in merito all'esposizione della teoria della relatività.

Cosmological predictions for a scalar tensor dark energy model by a dedicated Einstein-Boltzmann code

We have extended the Boltzmann code CLASS and studied a specific scalar tensor dark energy model: Induced Gravity