scholarly journals Renormalization of the Three-Body System with Short-Range Interactions

1999 ◽  
Vol 82 (3) ◽  
pp. 463-467 ◽  
Author(s):  
P. F. Bedaque ◽  
H.-W. Hammer ◽  
U. van Kolck
Keyword(s):  
2001 ◽  
Vol 690 (4) ◽  
pp. 535-546 ◽  
Author(s):  
H.-W. Hammer ◽  
Thomas Mehen
Keyword(s):  

2001 ◽  
Vol 680 (1-4) ◽  
pp. 304-307 ◽  
Author(s):  
J. Gegelia
Keyword(s):  

1972 ◽  
Vol 39 (5) ◽  
pp. 594-598 ◽  
Author(s):  
E. Hadjimichael ◽  
S.N. Yang ◽  
G.E. Brown

1993 ◽  
Vol 87 (3) ◽  
pp. 195-213 ◽  
Author(s):  
Vladimir M. Azriel ◽  
Lev Yu. Rusin ◽  
Mikhail B. Sevryuk

2021 ◽  
Author(s):  
Yuji Naruse

<div> <p>Cyclic orbital interaction, in which a series of orbitals interact with each other so as to make a monocyclic system, affords stabilization if the requirements of orbital phase continuity are satisfied. Initially, these requirements were derived from the consideration of a three-body system. Here I propose that these requirements can be easily derived by considering FMO theory. </p> </div>


Author(s):  
Jaume Carbonell ◽  
Emiko Hiyama ◽  
Rimantas Lazauskas ◽  
Francisco Miguel Marqués

We consider the evolution of the neutron-nucleus scattering length for the lightest nuclei. We show that, when increasing the number of neutrons in the target nucleus, the strong Pauli repulsion is weakened and the balance with the attractive nucleon-nucleon interaction results into a resonant virtual state in ^{18}18B. We describe ^{19}19B in terms of a ^{17}17B-nn-nn three-body system where the two-body subsystems ^{17}17B-nn and nn-nn are unbound (virtual) states close to the unitary limit. The energy of ^{19}19B ground state is well reproduced and two low-lying resonances are predicted. Their eventual link with the Efimov physics is discussed. This model can be extended to describe the recently discovered resonant states in ^{20,21}20,21B.


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