S-matrix pole trajectories for separable interactions

1989 ◽  
Vol 67 (1) ◽  
pp. 37-40 ◽  
Author(s):  
L. A. L. Roriz ◽  
A. Delfino

By solving the Lippmann–Schwinger equation in momentum space for a set of two-body separable interactions, we study eir S-matrix pole trajectories. The connection of such a study with the three-body bound-state collapse is also discussed.


1984 ◽  
Vol 29 (4) ◽  
pp. 1450-1460 ◽  
Author(s):  
D. R. Lehman ◽  
A. Eskandarian ◽  
B. F. Gibson ◽  
L. C. Maximon


1995 ◽  
Vol 51 (4) ◽  
pp. 1633-1637 ◽  
Author(s):  
S. Nakaichi-Maeda


1976 ◽  
Vol 15 (5) ◽  
pp. 134-138 ◽  
Author(s):  
W. Glöckle ◽  
R. Offermann


2020 ◽  
Vol 10 (1) ◽  
Author(s):  
M. R. Hadizadeh ◽  
M. Radin ◽  
K. Mohseni


2001 ◽  
Vol 63 (4) ◽  
Author(s):  
G. Pantis ◽  
I. E. Lagaris ◽  
S. A. Sofianos


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.



1989 ◽  
Vol 40 (8) ◽  
pp. 2654-2661 ◽  
Author(s):  
M. Komachiya ◽  
M. Ukita ◽  
R. Fukuda


1936 ◽  
Vol 32 (3) ◽  
pp. 482-485 ◽  
Author(s):  
R. A. Smith

When an electron makes a transition from a continuous state to a bound state, for example in the case of neutralization of a positive ion or formation of a negative ion, its excess energy must be disposed of in some way. It is usually given off as radiation. In the case of neutralization of positive ions the radiation forms the well-known continuous spectrum. No such spectrum due to the direct formation of negative ions has, however, been observed. This process has been fully discussed in a recent paper by Massey and Smith. It is shown that in this case the spectrum would be difficult to observe.



Author(s):  
M. de Leeuw ◽  
B. Eden ◽  
D. le Plat ◽  
T. Meier
Keyword(s):  


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