996 resultados para sum


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We use QCD sum rules (QCDSR) to calculate the width of the radiative decay of the meson X(3872), assumed to be a mixture between charmonium and exotic molecular [c (q) over bar][q (c) over bar] states with J(PC) = 1(++). We find that in a small range for the values of the mixing angle, 5 degrees <= theta <= 13 degrees, we get the branching ratio Gamma(X -> J/psi gamma)/Gamma(X -> J/psi pi(+)pi(-)) = 0.19 +/- 0.13, which is in agreement, with the experimental value. This result is compatible with the analysis of the mass and decay width of the mode J/psi(n pi) performed in the same approach.

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We evaluate the mass of the B(s0) scalar meson and the coupling constant in the B(s0)BK vertex in the framework of QCD sum rules. We consider the B(s0) as a tetraquark state to evaluate its mass. We get m(Bs0) = (5.85 +/- 0.13) GeV, which is in agreement, considering the uncertainties, with predictions supposing it as a b (s) over bar state or a B (K) over bar bound state with J(P) = 0(+). To evaluate the g(Bs0BK) coupling, we use the three-point correlation functions of the vertex, considering B(s0) as a normal b (s) over bar state. The obtained coupling constant is: g(Bs0BK) = (16.3 +/- 3.2) GeV. This number is in agreement with light-cone QCD sum rules calculation. We have also compared the decay width of the B(s0) -> BK process considering the B(s0) to be a b (s) over bar state and a BK molecular state. The width obtained for the BK molecular state is twice as big as the width obtained for the b (s) over bar state. Therefore, we conclude that with the knowledge of the mass and the decay width of the B(s0) meson, one can discriminate between the different theoretical proposals for its structure.

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We use QCD sum rules to test the nature of the meson X(3872), assumed to be a mixture between charmonium and exotic molecular [c (q) over bar][q (c) over bar] states with J(PC) = 1(++). We find that there is only a small range for the values of the mixing angle theta that can provide simultaneously good agreement with the experimental value of the mass and the decay width, and this range is 5(0) <= theta <= 3(0). In this range we get m(X) = (3.77 +/- 0.18) GeV and Gamma(X -> J/psi pi(+)pi(-)) = (9.3 +/- 6.9) MeV, which are compatible, within the errors, with the experimental values. We, therefore, conclude that the X(3872) is approximately 97% a charmonium state with 3% admixture of similar to 88% D(0)D*(0) molecule and similar to 12% D(+)D*(-) molecule.

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We investigate the widths of the recently observed charmonium like resonances X(3872), Z(4430), and Z(2)(4250) using QCD sum rules. Extending previous analyses regarding these states as diquark-antiquark states or molecules of D mesons, we introduce the Breit-Wigner function in the pole term. We find that introducing the width increases the mass at the small Borel window region. Using the operator-product expansion up to dimension 8, we find that the sum rules based on interpolating current with molecular components give a stable Borel curve from which both the masses and widths of these resonances can be well obtained. Thus the QCD sum rule approach strongly favors the molecular description of these states.

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We evaluate the coincidence spectra in the nonmesonic weak decay (NMWD) Lambda N -> nN of Lambda hypernuclei (4)(Lambda)He, (5)(Lambda)He, (12)(Lambda)C, (16)(Lambda)O, and (28)(Lambda)Si, as a function of the sum of kinetic energies E(nN)=E(n)+E(N) for N=n,p. The strangeness-changing transition potential is described by the one-meson-exchange model, with commonly used parametrization. Two versions of the independent-particle shell model (IPSM) are employed to account for the nuclear structure of the final residual nuclei. They are as follows: (a) IPSM-a, where no correlation, except for the Pauli principle, is taken into account and (b) IPSM-b, where the highly excited hole states are considered to be quasistationary and are described by Breit-Wigner distributions, whose widths are estimated from the experimental data. All np and nn spectra exhibit a series of peaks in the energy interval 110 MeV < E(nN)< 170 MeV, one for each occupied shell-model state. Within the IPSM-a, and because of the recoil effect, each peak covers an energy interval proportional to A(-1) , going from congruent to 4 MeV for (28)(Lambda)Si to congruent to 40 MeV for (4)(Lambda)He. Such a description could be pretty fair for the light (4)(Lambda)He and (5)(Lambda)He hypernuclei. For the remaining, heavier, hypernuclei it is very important, however, to consider as well the spreading in strength of the deep-hole states and bring into play the IPSM-b approach. Notwithstanding the nuclear model that is employed the results depend only very weakly on the details of the dynamics involved in the decay process proper. We propose that the IPSM is the appropriate lowest-order approximation for the theoretical calculations of the of kinetic energy sum spectra in the NMWD. It is in comparison to this picture that one should appraise the effects of the final-state interactions and of the two-nucleon-induced decay mode.

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Let P be a linear partial differential operator with analytic coefficients. We assume that P is of the form ""sum of squares"", satisfying Hormander's bracket condition. Let q be a characteristic point; for P. We assume that q lies on a symplectic Poisson stratum of codimension two. General results of Okaji Show that P is analytic hypoelliptic at q. Hence Okaji has established the validity of Treves' conjecture in the codimension two case. Our goal here is to give a simple, self-contained proof of this fact.

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Given a prime power q, define c (q) as the minimum cardinality of a subset H of F 3 q which satisfies the following property: every vector in this space di ff ers in at most 1 coordinate from a multiple of a vector in H. In this work, we introduce two extremal problems in combinatorial number theory aiming to discuss a known connection between the corresponding coverings and sum-free sets. Also, we provide several bounds on these maps which yield new classes of coverings, improving the previous upper bound on c (q)

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A Work Project, presented as part of the requirements for the Award of a Masters Degree in Finance from the NOVA – School of Business and Economics

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We report experimental results on one-shot two person 3x3 constant sum games played by non-economists without previous experience in the laboratory. Although strategically our games are very similar to previous experiments in which game theory predictions fail dramatically, 80% of actions taken in our experiment coincided with the prediction of the unique Nash equilibrium in pure strategies and 73% of actions were best responses to elicited beliefs. We argue how social preferences, presentation effects and belief elicitation procedures may influence how subjects play in simple but non trivial games and explain the diferences we observe with respect to previous work.

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Foram estudadas correlações lineares simples entre os parâmetros erosividade da chuva e da enxurrada e as perdas de solo provocadas por chuvas erosivas num solo Bruno Não-Cálcico Vértico. Os dados correspondentes aos anos de 1986-1990 foram obtidos na estação experimental de Sumé (PB), pertencente à Universidade Federal da Paraíba-UFPB. Os parâmetros erosividade da chuva e da enxurrada estudados foram: (a) altura total da chuva (P), em mm; (b) intensidades máximas (In), ocorridas nos tempos de 5; 10; 15; 20; 25; 30; 35; 40; 45; 50; 55; 60 e 120 minutos, respectivamente, em mm h-1; (c) energia cinética total, pelo método de Wischmeier e Smith (Ec) e pelo método de Wagner e Massambani (EcW), em MJ ha-1; (d) somatório da energia cinética de intensidades superior a 10 mm h-1 (Ec > 10 e EcW > 10) em MJ ha-1; (e) somatório da energia cinética de intensidades superior a 25 mm h-1 (Ec > 25 e EcW > 25), em MJ ha-1; (f) produtos da energia cinética total pelas intensidades máximas de chuva em intervalos crescentes de tempo (EIn), ou seja: EI5; EI10; EI15; EI20; EI25; EI30; EIW30; EI35; EI40; EI45; EI50; EI55; EI60 e EI120, em MJ mm ha-1 h-1; (g) produtos da altura total da chuva pelas intensidades máximas das chuvas em intervalos crescentes de tempo (PIn), ou seja: PI5; PI10; PI15; PI20; PI25; PI30; PI35; PI40; PI45; PI50; PI55; PI60 e PI120, em mm² h-1, e (h) volume de enxurrada (Vu), em m³. O parâmetro volume de enxurrada (Vu) foi o que melhor estimou (r = 0,812) as perdas de solo em Sumé (PB). Dentre os parâmetros erosividade da chuva, o que melhor se correlacionou com as perdas de solo foi o parâmetro PI25 (r = 0,753). As equações de Wischmeier & Smith e de Wagner & Massambani, utilizadas no cálculo da energia cinética total da chuva, apresentaram o mesmo grau de precisão na estimativa das perdas de solo.

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Foram estudados os efeitos do desmatamento da caatinga sobre as perdas de solo e água provocadas por chuvas erosivas num Luvissolo. Os dados relativos aos anos de 1983-1990 foram obtidos na Estação Experimental de Sumé (PB), pertencente à Universidade Federal da Paraíba - UFPB. Os tratamentos consistiram de duas parcelas desmatadas, uma parcela com caatinga nativa, uma parcela com caatinga nova, duas macroparcelas com caatinga nativa e duas macroparcelas desmatadas. Nas parcelas desmatadas, as perdas de solo foram de 61,7 e 47,7 t ha-1 e as perdas de água de 224,2 e 241,0 mm. A parcela com caatinga nativa, quando comparada com a parcela desmatada, reduziu a perda de solo em cerca de 98% e a perda de água em torno de 73%. Nas macroparcelas desmatadas foram observadas perdas anuais de solo de 31 e 26 t ha-1 e de água de 151,3 e 131,5 mm. Nas macroparcelas com caatinga, houve uma redução de aproximadamente 99% das perdas de solo e 90% das perdas de água, em relação às macroparcelas desmatadas.