Apresentação Seção Especial Motricidades (v. 5, n. 1, seç. esp.)
نویسندگان
چکیده
منابع مشابه
$n$-cocoherent rings, $n$-cosemihereditary rings and $n$-V-rings
Let $R$ be a ring, and let $n, d$ be non-negative integers. A right $R$-module $M$ is called $(n, d)$-projective if $Ext^{d+1}_R(M, A)=0$ for every $n$-copresented right $R$-module $A$. $R$ is called right $n$-cocoherent if every $n$-copresented right $R$-module is $(n+1)$-coprese-nted, it is called a right co-$(n,d)$-ring if every right $R$-module is $(n, d)$-projective. $R$...
متن کامل06 1 v 1 1 5 Ja n 20 01 Quantum Information Theory – an Invitation
This text is part of a volume entitled " Quantum information — an introduction to basic theoretical concepts and experiments " , to be published in Springer Tracts in Modern Physics. Authors will be From the foundations of quantum theory to quantum technology-an introduction Mixed-state entanglement and quantum communication Joint index Joint list of references References to " articles in this ...
متن کامل5 v 1 1 4 N ov 1 99 4 Renormalizing Partial Differential Equations
We explain how to apply Renormalization Group ideas to the analysis of the long-time asymptotics of solutions of partial differential equations. We illustrate the method on several examples of nonlinear parabolic equations. We discuss many applications, including the stability of profiles and fronts in the Ginzburg-Landau equation, anomalous scaling laws in reaction-diffusion equations, and the...
متن کاملv 1 1 5 N ov 1 99 7 Chaotic eigenfunctions in phase space
We study individual eigenstates of quantized area-preserving maps on the 2-torus which are classically chaotic. In order to analyze their semiclassical behavior, we use the Bargmann–Husimi representations for quantum states, as well as their stellar parametrization, which encodes states through a minimal set of points in phase space (the constellation of zeros of the Husimi density). We rigorou...
متن کامل0 v 1 5 N ov 1 99 9 Identification of SH ∆ v = 1 ro - vibrational lines in R And
We report the identification of SH ∆v = 1 ro-vibrational lines in the published high-resolution infrared spectrum of the S-type star, R And. This is the first astronomical detection of this molecule. The lines show inverse P-Cygni profiles, indicating infall motion of the molecular layer due to stellar pulsation. A simple spherical shell model with a constant infall velocity is adopted to deter...
متن کاملذخیره در منابع من
با ذخیره ی این منبع در منابع من، دسترسی به آن را برای استفاده های بعدی آسان تر کنید
ژورنال
عنوان ژورنال: MOTRICIDADES: Revista da Sociedade de Pesquisa Qualitativa em Motricidade Humana
سال: 2021
ISSN: 2594-6463
DOI: 10.29181/2594-6463-2021-v5-n1-secesp-p93-95