Scheme for an accurate solution of Faddeev integral equations in configuration space
Faddeev equations in configuration space for three-atom scattering processes are formulated in integral form allowing for additive and nonadditive forces. The object of the equations are T–functions, that are the product of wave functions times potentials, that decay to zero in all directions. The d...
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Published in: | Nuclear physics. A Vol. 790; no. 1; pp. 282c - 285c |
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Main Authors: | , |
Format: | Journal Article |
Language: | English |
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Elsevier B.V
15-06-2007
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Abstract | Faddeev equations in configuration space for three-atom scattering processes are formulated in integral form allowing for additive and nonadditive forces. The object of the equations are
T–functions, that are the product of wave functions times potentials, that decay to zero in all directions. The driving and coupling terms are based on the two-body
t–matrices, which describe the two-body correlations in each arrangement. However, three-atom forces are also included in the formalism. The solution is based on an accurate numerical spectral expansion method, and steps for a practical implementation are described for a simplified “toy” model, although numerical results are not yet available. This formulation appears to be a valuable alternative to current approaches. |
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AbstractList | Faddeev equations in configuration space for three-atom scattering processes are formulated in integral form allowing for additive and nonadditive forces. The object of the equations are
T–functions, that are the product of wave functions times potentials, that decay to zero in all directions. The driving and coupling terms are based on the two-body
t–matrices, which describe the two-body correlations in each arrangement. However, three-atom forces are also included in the formalism. The solution is based on an accurate numerical spectral expansion method, and steps for a practical implementation are described for a simplified “toy” model, although numerical results are not yet available. This formulation appears to be a valuable alternative to current approaches. |
Author | Rawitscher, G. Glöckle, W. |
Author_xml | – sequence: 1 givenname: W. surname: Glöckle fullname: Glöckle, W. organization: Institut für theoretische Physik II, Ruhr Universitat Bochum, D-44780 Bochum, Germany – sequence: 2 givenname: G. surname: Rawitscher fullname: Rawitscher, G. organization: Physics Department, University of Connecticut, Storrs, CT 06268 |
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CitedBy_id | crossref_primary_10_1007_s00601_008_0301_z crossref_primary_10_1007_s00601_010_0146_0 crossref_primary_10_1103_PhysRevA_77_012707 crossref_primary_10_1103_PhysRevE_85_026701 crossref_primary_10_1103_PhysRevC_86_034004 crossref_primary_10_1119_1_3534837 |
Cites_doi | 10.1016/0003-4916(80)90344-9 10.1103/PhysRevA.65.032725 10.1088/0143-0807/27/5/017 10.1016/0370-1573(95)00085-2 |
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Copyright | 2007 Elsevier B.V. |
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References | Glöckle (bib007) 1983 Gloeckle, Rawitscher (bib004) Rawitscher, Koltracht (bib005) 2005; 7 paper in preparation Papp, Darai, Hu, Hlousek, Kónya, Yakovlev (bib002) 2002; 65 Merkuriev, Faddeev, Merkuriev (bib001) 1980; 130 Rawitscher, Koltracht (bib006) 2006; 27 G. Rawitscher and I. Koltracht Hüber, Kamada, Witala, Glöckle, Glöckle, Witala, Hüber, Kamada, Golak (bib003) 1997; 28 Glöckle (10.1016/j.nuclphysa.2007.03.045_bib007) 1983 Rawitscher (10.1016/j.nuclphysa.2007.03.045_bib005) 2005; 7 Glöckle (10.1016/j.nuclphysa.2007.03.045_bib003_2) 1996; 274 Faddeev (10.1016/j.nuclphysa.2007.03.045_bib001_2) 1993 Merkuriev (10.1016/j.nuclphysa.2007.03.045_bib001_1) 1980; 130 10.1016/j.nuclphysa.2007.03.045_bib008 Rawitscher (10.1016/j.nuclphysa.2007.03.045_bib006) 2006; 27 Papp (10.1016/j.nuclphysa.2007.03.045_bib002) 2002; 65 Gloeckle (10.1016/j.nuclphysa.2007.03.045_bib004) Hüber (10.1016/j.nuclphysa.2007.03.045_bib003_1) 1997; 28 |
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