scholarly journals Convergence of S-Matrix in Coupled Channel Method of Deuteron Breakup Reactions Based on Totally Antisymmetrized Three-Body Model

1981 ◽  
Vol 65 (6) ◽  
pp. 2051-2055 ◽  
Author(s):  
M. Yahiro ◽  
M. Kamimura
1978 ◽  
Vol 114 (1-2) ◽  
pp. 93-122 ◽  
Author(s):  
N Austern ◽  
C.M Vincent ◽  
J.P Farrell

2009 ◽  
Vol 24 (11n13) ◽  
pp. 895-900 ◽  
Author(s):  
T. SATO ◽  
Y. IKEDA

The three-body resonance of [Formula: see text] system is investigated by using the [Formula: see text] coupled channels Faddeev equation. The resonance energy is determined from the pole of S -matrix on the unphysical sheet. It is found that the pole positions of the predicted amplitudes are significantly modified when the three-body dynamics is approximately treated by introducing the effective [Formula: see text] two-body interaction.


2014 ◽  
Vol 26 ◽  
pp. 1460054 ◽  
Author(s):  
MICHAEL DÖRING

General properties of the S-matrix, such as constraints from two- and three-body unitarity as well as gauge invariance, are discussed and illustrated for the example of a dynamical coupled channel approach. The Jülich model has been updated to analyze πN, ηN, and KY production as well as pion photoproduction. Partial wave amplitudes and resonance properties are determined.


1976 ◽  
Vol 96 (2) ◽  
pp. 333-381 ◽  
Author(s):  
J.P Farrell ◽  
C.M Vincent ◽  
N Austern

2021 ◽  
Vol 2021 (2) ◽  
Author(s):  
Gustav Mogull ◽  
Jan Plefka ◽  
Jan Steinhoff

Abstract A precise link is derived between scalar-graviton S-matrix elements and expectation values of operators in a worldline quantum field theory (WQFT), both used to describe classical scattering of black holes. The link is formally provided by a worldline path integral representation of the graviton-dressed scalar propagator, which may be inserted into a traditional definition of the S-matrix in terms of time-ordered correlators. To calculate expectation values in the WQFT a new set of Feynman rules is introduced which treats the gravitational field hμν(x) and position $$ {x}_i^{\mu}\left({\tau}_i\right) $$ x i μ τ i of each black hole on equal footing. Using these both the 3PM three-body gravitational radiation 〈hμv(k)〉 and 2PM two-body deflection $$ \Delta {p}_i^{\mu } $$ Δ p i μ from classical black hole scattering events are obtained. The latter can also be obtained from the eikonal phase of a 2 → 2 scalar S-matrix, which we show corresponds to the free energy of the WQFT.


2013 ◽  
Vol 54 (7-10) ◽  
pp. 1381-1384
Author(s):  
N. Kurihara ◽  
Y. Kikuchi ◽  
K. Katō
Keyword(s):  

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