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Three-body systems

Sometimes potential energy surfaces are plotted with skewed axes that is, the Tab 2nd tbc axes meet at an angle less than 90°. This is done so that the relative kinetic energy of the three-body system can be represented by the motion of a single point over the surface. In order to achieve this condition it is necessaiy that the cross-product terms in the kinetic energy drop out. The calculations have been described - Because our use of potential energy surfaces is qualitative,... [Pg.197]

Heibst, E. In Atomic, Molecular, Optical Physics Handbook Drake, G., Ed. AIP Press New Yoik, 1996, p 429 Adams, N. G. In Atomic, Molecular, Optical Physics Handbook Drake, G., Ed. AIP Press New Yoik, 1996, p 441. For three-body systems, a slightly more complex temperature dependence is observed. For saturated systems, more complex treatments are needed —see Gilbert, R. G. Smith, S. C. Theory erf Unimolecular and Recombination Reactions Blackwell Oxford, 1990. [Pg.46]

For a three-body system such as A + BC AB + C, there are 3 x 3 = 9 degrees of freedom in the problem. However, three degrees of freedom can be eliminated by considering the centre of mass coordinates. If we consider... [Pg.229]

The Hamilton s equations for three-body system described by the general dynamical coordinates qp are... [Pg.230]

Kellman, M. E., Amar, F., and Berry, R. S. (1980), Correlation Diagrams for Rigid and Nonrigid Three-Body Systems, J. Chem. Phys. 73, 2387. [Pg.229]

The basis we have chosen is not that which has been used in the majority of the studies of three-body systems. The most-used basis, often called a Hylleraas basis, consists of functions of the form... [Pg.409]

Spectral moments may be computed from expressions such as Eqs. 5.15 or 5.16. Furthermore, the theory of virial expansions of the spectral moments has shown that we may consider two- and three-body systems, without regard to the actual number of atoms contained in a sample if gas densities are not too high. Near the low-density limit, if mixtures of non-polar gases well above the liquefaction point are considered, a nearly pure binary spectrum may be expected (except near zero frequencies, where the intercollisional process generates a relatively sharp absorption dip due to many-body interactions.) In this subsection, we will sketch the computations necessary for the actual evaluation of the binary moments of low order, especially Eqs. 5.19 and 5.25, along with some higher moments. [Pg.206]

Induced dipole autocorrelation functions of three-body systems have not yet been computed from first principles. Such work involves the solution of Schrodinger s equation of three interacting atoms. However, classical and semi-classical methods, especially molecular dynamics calculations, exist which offer some insight into three-body dynamics and interactions. Very useful expressions exist for the three-body spectral moments, with the lowest-order Wigner-Kirkwood quantum corrections which were discussed above. [Pg.229]

Because the orbital angular momentum of the positron-hydrogen system is zero for s-wave scattering, the total wave function is spherically symmetric and depends only on the three internal coordinates which specify the shape of the three-body system. The kinetic energy operator... [Pg.106]

The dipole interaction couples higher sublevel channels too, for which the order of the coefficient matrix on R 2 is larger than for the 2s 2p channel coupling. Numerical values of a and/or (or e () for the decoupled higher sublevel channels are tabulated for some three-body systems [44,53, 66,77-79],... [Pg.208]

By the transformation of the independent-particle coordinates into the hyperspherical coordinates the Hamiltonian for the three-body system changes into the form... [Pg.212]

When the constituent two-body interactions in a three-body system produce an s-wave scattering length a of much larger magnitude a than... [Pg.215]

The three-body systems discussed so far contain two identical particles. Another system of interest, C He1, contains three different particles and can decay into two different arrangement channels... [Pg.222]

C.D. Lin, Hyperspherical coordinate approach to atomic and other Coulombic three-body systems, Phys. Rep. 257 (1995) 1. [Pg.241]

M. Ragni, A.C.P. Bitencourt, V. Aquilanti, Hyperspherical and related types of coordinates for the dynamical treatment of three-body systems, Prog. Theor. Chem. Phys. 16 (2007) Part 1,123. [Pg.243]

V. Efimov, Energy levels arising from resonant two-body forces in a three-body system, Phys. Lett. B 33 (1970) 563. [Pg.244]

Z. Chen, C.D. Lin, Classification of Coulombic three-body systems in hyperspherical coordinates, Phys. Rev. A 42 (1990) 18. [Pg.244]

The effects of plasma environments on the spectral properties of exotic two-and three-body systems have been studied. Influence of the Debye plasma on the stability and spectral properties of spatially confined exotic systems like p+ x and [i+[i was investigated by Sil et al. [217] along the same line as was... [Pg.157]

The calculations have been further extended by Sil et al. [219] for analyzing the stability of exotic systems like ppp, ddp and ttp and also finding the behavior of the hadronic affinity under Debye plasma. An interesting feature emerges from this particular study, namely, a given two-body system becomes unstable at a screening parameter for which the corresponding three-body system is stable. This property depends very much on the... [Pg.158]

Fig. 1. Linear free energy relationships as predicted for simple three-body systems (Bell, 1959b). In (a) the energy of the starting state is assumed to change with changes in AH. In (a ) the energy of the product state is assumed to change. In either case AAE is approximately proportional to AAE°. Fig. 1. Linear free energy relationships as predicted for simple three-body systems (Bell, 1959b). In (a) the energy of the starting state is assumed to change with changes in AH. In (a ) the energy of the product state is assumed to change. In either case AAE is approximately proportional to AAE°.
Docking of a Three-Body System The Recognition of Human Growth Hormone by Its Receptor. [Pg.93]

Helium is not the only three body system under study, but it is likely the most complicated one. The electron-electron interaction is comparable with the electron-nucleus interaction and cannot be considered as a perturbation. The situation is different with helium-like (and lithium-like) ions, where the electron-electron interaction is as small as 1 jZ with respect to the interaction of an electron and the nucleus. [Pg.9]

The p and He2+ are thus regarded as two atomic centers in a diatomic molecule. Because of the dual character as an exotic atom and an exotic molecule Antiprotonic Helium is often called antiprotonic helium atom-molecule, or for short, atomcule. Since the Is electron motion, coupled to a large-(n, l) p orbital, is faster by a factor of 40 than the p motion, the three-body system pHe+ is solved by using the Born-Oppenheimer approximation, as fully discussed by Shimamura [6]. [Pg.249]

Finite-element numerical calculation method Elander and Yarevsky [9] solved the three-body system by employing the finite-element numerical method. The precision achieved in this method is impressively high. [Pg.250]


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See also in sourсe #XX -- [ Pg.102 , Pg.241 ]

See also in sourсe #XX -- [ Pg.131 , Pg.142 , Pg.145 , Pg.146 ]




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Atoms three-bodied systems

Body system

Electrons three-bodied systems

General properties of three-body systems with Hill-type stability

Molecular systems three-bodied

Plasma three body systems

Standard three-body systems

Three body systems, under plasma

Three-body system dynamical treatment

Vectors, three body system

Vectors, three body system calculations

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