scholarly journals Quark-model based study of the triton binding energy

2002 ◽  
Vol 65 (3) ◽  
Author(s):  
B. Juliá-Díaz ◽  
J. Haidenbauer ◽  
A. Valcarce ◽  
F. Fernández
2005 ◽  
Vol 20 (08n09) ◽  
pp. 1797-1802 ◽  
Author(s):  
FL. STANCU

Light and heavy pentaquarks are described within a constituent quark model based on a spin-flavor hyperfine interaction. In this model the lowest state acquires positive parity. The masses of the light antidecuplet members are calculated dynamically using a variational method. It is shown that the octet and antidecuplet states with the same quantum numbers mix ideally due to SU (3)F breaking. Masses of the charmed antisextet pentaquarks are predicted within the same model.


1984 ◽  
Vol 30 (4) ◽  
pp. 1366-1369 ◽  
Author(s):  
S. A. Coon ◽  
M. T. Peña ◽  
R. G. Ellis

1988 ◽  
Vol 38 (3) ◽  
pp. 1397-1402 ◽  
Author(s):  
R. A. Brandenburg ◽  
G. S. Chulick ◽  
R. Machleidt ◽  
A. Picklesimer ◽  
R. M. Thaler

2005 ◽  
Vol 20 (08n09) ◽  
pp. 1963-1966
Author(s):  
T. GOLDMAN

A model for nuclei described directly in terms of quarks has been developed in both relativistic and non-relativistic forms. It describes nuclear binding energy and structure for small nuclei (A=3,4) systematically correctly, including the EMC effect. With one free parameter each for strange and for nonstrange states, it also well describes low energy baryon-nucleon scattering, phase shifts and potentials. It predicts low mass, narrow dibaryon and pentaquark states. To be consistent with reported states, new physics may be required that is not included in any quark model to date.


1993 ◽  
Vol 71 (13) ◽  
pp. 1982-1985 ◽  
Author(s):  
W. S. Wilburn ◽  
C. R. Gould ◽  
D. G. Haase ◽  
P. R. Huffman ◽  
C. D. Keith ◽  
...  

2009 ◽  
Vol 24 (11n13) ◽  
pp. 804-809 ◽  
Author(s):  
H. KAMADA ◽  
W. GLÖCKLE ◽  
H. WITAŁA ◽  
J. GOLAK ◽  
R. SKIBIŃSKI ◽  
...  

The phase equivalent relativistic NN potential, which is related by a nonlinear equation to the original nonrelativistic potential, is used to construct the mass operator (rest Hamiltonian) of the 3-nucleon system. Employing the CD Bonn NN potential, the solution of the relativistic 3N Faddeev equation for 3 H shows slightly less binding energy than the corresponding nonrelativistic result. The effect of the Wigner spin rotation on the binding is very small.


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