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In this paper, we investigate the feasibility of employing the Hyperspherical Adiabatic (HA) basis set to describe continuum states of the Helium trimer molecule. 相似文献
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In this work, the binding energy and wavefunctions of three-nucleon systems are obtained by using hy-perspherical harmonic approach. We have used a mathematical modification method to obtain the eigenvalues and eigenfunctions of Schrdinger equation for three-nucleon systems in calculation. Next, we have used a simple approach to obtain the difference between binding energy of 3H and 3He where gives us mass splitting of three-nucleon systems. We have compared our results with the other works and experimental values. 相似文献
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The adiabatic hyperspherical approach (AHSA) is applied for the numerical investigation of the scattering processes and resonances
in Coulomb three-body mesic atomic systems. The results of the calculations of elastic and inelastic cross sections in low-energy
collisions aμ + b (a, b = p, d,
t), energies, lifetimes and local characteristics of resonant states of mesic molecular ions
n
Heaμ+ (n = 3, 4) are presented.
This revised version was published online in August 2006 with corrections to the Cover Date. 相似文献
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In this work we show results for light nuclear systems and small clusters of helium atoms using the hyperspherical harmonics basis. We use the basis without previous symmetrization or antisymmetrization of the state. After the diagonalization of the Hamiltonian matrix, the eigenvectors have well defined symmetry under particle permutation and the identification of the physical states is possible. We show results for systems composed up to six particles. As an example of a fermionic system, we consider a nucleon system interacting through the Volkov potential, used many times in the literature. For the case of bosons, we consider helium atoms interacting through a potential model which does not present a strong repulsion at short distances. We have used an attractive gaussian potential to reproduce the values of the dimer binding energy, the atom-atom scattering length, and the effective range obtained with one of the most widely used He–He interaction, the LM2M2 potential. In addition, we include a repulsive hypercentral three-body force to reproduce the trimer binding energy. 相似文献
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In this paper we demonstrate the inadequacy of the first order of the Hyperspherical Harmonic Expansion Method, the Lm approximation, for the calculation of the binding energies, charge form factors and charge densities of doubly magic nuclei like 16O and 40Ca. We then extend the Hyperspherical Expansion Method to many-fermion systems, consisting of an arbitrary number of fermions, and develop an exact formalism capable of generating the complete optimal subset of the hyperspherical harmonic basis functions. This optimal subset consists of those hyperspherical harmonic basis functions directly connected to the dominant first term in the expansion, the hyperspherical harmonic of minimal order Lm, through the total interaction between the particles. The required many-body coefficients are given using either the Gogny or Talmi-Moshinsky coefficients for the two-body operators. Using the two-body coefficients the weight function generating the orthogonal polynomials associated with the optimal subset is constructed. 相似文献
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R. Lazauskas 《Few-Body Systems》2009,46(1):37-43
In this article an efficient method to calculate the matrix elements of three-nucleon force is presented. The new method is improved version of partial-wave decomposition of Hüber et al. (Few-Body Syst 22:107, 1997), which simplifies expression to be evaluated as well as permits to reduce computational effort. Proposed method naturally applies to Faddeev-type calculations. 相似文献
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We introduce new values of the strength constants (i.e., a, b, c, and d coefficients) of the Tucson-Melbourne (TM) 2π-exchange three-nucleon potential. The new values come from contemporary dispersion-relation analyses of meson-factory πN-scattering data. We make variational Monte-Carlo calculations of the triton with the original and updated three-body forces to study the effects of this update. We remove a short-range–π-range part of the potential due to the c coefficient and discuss the effect on the triton binding energy. Received September 11, 1999; revised November 2, 1999; accepted February 23, 相似文献
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H. Witała J. Golak R. Skibiński K. Topolnicki H. Kamada E. Epelbaum W. Glöckle H. Krebs W. N. Polyzou A. Nogga 《Few-Body Systems》2013,54(7-10):897-902
Faddeev calculations using the chiral three-nucleon force in next-to-next-to-next-to-leading-order show that this force is too weak to provide an explanation for the low-energy A y puzzle. The large discrepancy between data and theory for the neutron–neutron quasi-free-scattering cross section in low energy neutron–deuteron breakup requires a modification of the ${^{1}S_0}$ neutron–neutron force. We discuss the consequences that a bound ${^{1}S_0}$ state of two neutrons has on neutron–deuteron scattering observables. At higher energies we compare the solutions of the non-relativistic three-nucleon Faddeev equations with three-nucleon force included to the solutions of its Poincaré invariant version. 相似文献
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Four-nucleon states in the continuum are studied through exact microscopic calculations based on the solution of the AGS
equations for four nonrelativistic quantum particles. Our studies include calculations of cross sections and analyzing powers
for all two-body reactions of interest, but here we only show results for n
3He → n
3He. The NN interactions we use are Bonn-CD, Nijmegen II, and Bonn-B. Compared to existing quality data, one finds large discrepancies
and some sensitivity to the choice of NN force model. The calculated n + 3He elastic phase shifts show a very strong inelastic resonance at about 0.3 MeV which is not supported by the total cross-section
data. This result is due to the existence of a 3
P
0 (0−) resonance in isospin I = 0 at this energy and the undesirable coincidence of n + 3He and p + 3H thresholds in our calculation due to lack of Coulomb repulsion between protons. This interpretation is supported by R-matrix analyses of the data on the basis of coincident thresholds. Calculated 0+ and 0− states are compared with modified R-matrix analyses.
Received October 30, 2001; accepted for publication November 7, 2001 相似文献
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J. Golak K. Topolnicki R. Skibiński W. Glöckle H. Kamada A. Nogga 《Few-Body Systems》2013,54(12):2427-2446
Recently a formalism for a direct treatment of the Faddeev equation for the three-nucleon bound state in three dimensions has been proposed. It relies on an operator representation of the Faddeev component in the momentum space and leads to a finite set of coupled equations for scalar functions which depend only on three variables. In this paper we provide further elements of this formalism and show the first numerical results for chiral NNLO nuclear forces. 相似文献
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We include two specific three-nucleon-force terms of pion-range–short-range form in our momentum-space calculations for the
three-nucleon continuum. These two terms are expected by chiral perturbation theory to be non-negligible. We study the effects
of these terms in elastic neutron-deuteron scattering and pay special attention to the neutron vector-analyzing power A
y
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Received September 16, 1999; accepted for publication October 20, 1999 相似文献
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It is shown how a bare three-nucleon force is incorporated into the formalism of the effective interaction approach for hyperspherical harmonics. As a practical example we calculate the ground-state properties of 3H and 3He using the Argonne V18 nucleon-nucleon potential and the Urbana IX three-nucleon force. A very good convergence of binding energies and matter radii is obtained. We also find a very good agreement of our results compared to other high-precision calculations. 相似文献
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Yi-Tian Ding 《International Journal of Theoretical Physics》2014,53(5):1628-1636
In this paper, we deal with the adiabatic approximation of general Hamiltonians by splitting it into two parts, with one part a Hamiltonian that has at least one time-independent eigenstate up to a phase factor. We first develop the method of finding this kind of Hamiltonians. Then the relationship between adiabatic approximation and these Hamiltonians is discussed. Applying this to a general case, we give both a necessary condition and a sufficient condition for adiabatic approximation, followed by a spin-half example to illustrate. 相似文献
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