RenormalizedπNN coupling constant and theP-wave phase shifts in the cloudy bag model

1986 ◽  
Vol 34 (3) ◽  
pp. 991-1003 ◽  
Author(s):  
B. C. Pearce ◽  
I. R. Afnan
1964 ◽  
Vol 133 (1B) ◽  
pp. B191-B195 ◽  
Author(s):  
Archibald W. Hendry ◽  
Berthold Stech

1995 ◽  
Vol 589 (4) ◽  
pp. 585-600 ◽  
Author(s):  
B. Silvestre-Brac ◽  
J. Leandri ◽  
J. Labarsouque

1961 ◽  
Vol 25 (3) ◽  
pp. 427-435 ◽  
Author(s):  
Shoichiro Otsuki ◽  
Mituo Taketani ◽  
Ryozo Tamagaki ◽  
Wataro Watari

2005 ◽  
Vol 19 ◽  
pp. 48-55 ◽  
Author(s):  
Alexander D Cronin ◽  
John D Perreault

1976 ◽  
Vol 54 (3) ◽  
pp. 322-332
Author(s):  
A. Z. Capri ◽  
D. Menon ◽  
R. Teshima

The two-nucleon interaction, via the exchange of scalar mesons, is examined in a nonperturbative manner. 'Schrödinger' equations are derived, and nonlocal potentials arise naturally. Both scattering and bound states are examined. A half-off-shell T matrix is obtained, and corresponding phase shifts are evaluated. In the bound state, a variational calculation is employed to determine the coupling constant.


1982 ◽  
Vol 60 (4) ◽  
pp. 577-580 ◽  
Author(s):  
M. A. Abdel-Raouf

New variational techniques in which the functional [Formula: see text] is minimized are used to calculate the S-wave phase shifts of e+–H elastic scattering. The convergence of these phases, as n increases, is precisely investigated.


2009 ◽  
Vol 5 (H15) ◽  
pp. 349-350
Author(s):  
Paul S. Cally

AbstractIt has been known for two decades that sunspots both absorb and advance the phase of solar f and p-modes. More recently, Time-Distance and other local helioseismic techniques have been used to probe active regions by exploring phase shifts which are interpreted as travel-time perturbations. Although absorption is an intrinsically magnetic effect, phase shifts may be produced by both thermal and magnetic effects (and of course flows, though these can be factored out by averaging travel times in opposite directions). We will show how these two effects alter wave phase, and conclude that phase shifts in umbrae are predominantly thermal, whilst those in highly inclined field characteristic of penumbrae are essentially magnetic. The two effects are generally not additive.


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