Probing the Wave Function of a Surface State in Ag(111): A New Approach

1985 ◽  
Vol 55 (22) ◽  
pp. 2483-2486 ◽  
Author(s):  
T. C. Hsieh ◽  
T. Miller ◽  
T. -C. Chiang
1996 ◽  
Vol 11 (20) ◽  
pp. 1611-1626 ◽  
Author(s):  
A.P. BAKULEV ◽  
S.V. MIKHAILOV

In a recent paper1 we have proposed a new approach for extracting the wave function of the π-meson φπ(x) and the masses and wave functions of its first resonances from the new QCD sum rules for nondiagonal correlators obtained in Ref. 2. Here, we test our approach using an exactly solvable toy model as illustration. We demonstrate the validity of the method and suggest a pure algebraic procedure for extracting the masses and wave functions relating to the case under investigation. We also explore the stability of the procedure under perturbations of the theoretical part of the sum rule. In application to the pion case, this results not only in the mass and wave function of the first resonance (π′), but also in the estimation of π″-mass.


1988 ◽  
Vol 02 (05) ◽  
pp. 1037-1042
Author(s):  
I. G. GOCHEV ◽  
N. B. IVANOV ◽  
P. Kh. IVANOV

A new method for calculation the energy of S = 1/2 Heisenberg antiferromagnet /AFM/ in Gutzwiller state is developed. The method is analogous to low-temperature expansion /LTE/ in statistical physics


2001 ◽  
Vol 482-485 ◽  
pp. 764-769 ◽  
Author(s):  
J.E Ortega ◽  
A Mugarza ◽  
A Närmann ◽  
A Rubio ◽  
S Speller ◽  
...  

1991 ◽  
Vol 06 (24) ◽  
pp. 4341-4358 ◽  
Author(s):  
I. YA. AREF’EVA ◽  
B. DRAGOVICH ◽  
P.H. FRAMPTON ◽  
I.V. VOLOVICH

A new approach to the wave function of the universe is suggested. The key idea is to take into account fluctuating number fields and present the wave function in the form of a Euler product. For this purpose we define a p-adic generalization of both classical and quantum gravitational theory. Elements of p-adic differential geometry are described. The action and gravitation field equations over the p-adic number field are investigated. p-adic analogs of some known solutions to the Einstein equations are presented. It follows that in quantum cosmology one should consider summation only over algebraic manifolds. The correspondence principle with the standard approach is considered.


2015 ◽  
Vol 56 (5) ◽  
pp. 052102
Author(s):  
L. D. Blokhintsev ◽  
A. S. Kadyrov ◽  
A. M. Mukhamedzhanov ◽  
D. A. Savin

2016 ◽  
Vol 31 (35) ◽  
pp. 1650189 ◽  
Author(s):  
Tapashi Das ◽  
D. K. Choudhury ◽  
K. K. Pathak

Considering the Cornell potential [Formula: see text], we have revisited the Dalgarno’s method of perturbation by incorporating two scales [Formula: see text] and [Formula: see text] as integration limit so that the perturbative procedure can be improved in a potential model. With the improved version of the wave function the ground state masses of the heavy–light mesons [Formula: see text], [Formula: see text], [Formula: see text], [Formula: see text] and [Formula: see text] are computed. The slopes and curvatures of the form factors of semileptonic decays of heavy–light mesons in both HQET limit and finite mass limit are calculated and compared with the available data.


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