scholarly journals First results of baryon interactions from lattice QCD with physical masses (2) -- S=-3 and S=-4 sectors ($\Xi\Xi, \Xi\Sigma, \Xi\Lambda-\Xi\Sigma$ channels) --

2016 ◽  
Author(s):  
Noriyoshi Ishii
Keyword(s):  
Lattice Qcd ◽  
First Results

scholarly journals First results for theΔI = 12 amplitude in K decays with quenched lattice QCD and Wilson fermions

1988 ◽  
Vol 211 (1-2) ◽  
pp. 139-145 ◽  
Author(s):  
M.B. Gavela ◽  
L. Maiani ◽  
S. Petrarca ◽  
G. Martnelli ◽  
O. Pène
Keyword(s):  
Lattice Qcd ◽  
First Results ◽  
Wilson Fermions

scholarly journals NONPERTURBATIVE HQET AT ORDER 1/m

2010 ◽  
Vol 19 (08n10) ◽  
pp. 1661-1666
Author(s):  
B. BLOSSIER ◽  
G. VON HIPPEL ◽  
N. GARRON ◽  
T. MENDES
Keyword(s):  
Lattice Qcd ◽  
Heavy Quark ◽  
Effective Theory ◽  
Heavy Quark Effective Theory ◽  
Vector Mesons ◽  
Decay Constants ◽  
First Results ◽  
Pseudo Scalar

We summarize the first results for masses and decay constants of bottom-strange (pseudo-scalar and vector) mesons from nonperturbatively renormalized heavy-quark effective theory (HQET), using lattice-QCD simulations in the quenched approximation.

scholarly journals First results of baryon interactions from lattice QCD with physical masses (1) -- General overview and two-nucleon forces --

2016 ◽  
Author(s):  
Takumi Doi ◽  
Sinya Aoki ◽  
Shinya Gongyo ◽  
Tetsuo Hatsuda ◽  
Yoichi Ikeda ◽  
...  
Keyword(s):  
Lattice Qcd ◽  
General Overview ◽  
First Results

Discussion of the Oblique Rotator Model Cases Of 108 Aqr and x Serp.

1976 ◽  
Vol 32 ◽  
pp. 577-588
Author(s):  
C. Mégessier ◽  
V. Khokhlova ◽  
T. Ryabchikova
Keyword(s):  
Mathematical Formulation ◽  
The Other ◽  
Rotator Model ◽  
Oblique Rotator ◽  
First Results

My talk will be on the oblique rotator model which was first proposed by Stibbs (1950), and since received success and further developments. I shall present two different attempts at describing a star according to this model and the first results obtained in the framework of a Russian-French collaboration in order to test the precision of the two methods. The aim is to give the best possible representation of the element distributions on the Ap stellar surfaces. The first method is the mathematical formulation proposed by Deutsch (1958-1970) and applied by Deutsch (1958) to HD 125248, by Pyper (1969) to α2CVn and by Mégessier (1975) to 108 Aqr. The other one was proposed by Khokhlova (1974) and used by her group.

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