Effect of flexibility on liquid-vapor coexistence and surface properties of tangent linear vibrating square well chains in two and three dimensions

2013 ◽  
Vol 138 (22) ◽  
pp. 224509 ◽  
Author(s):  
Gustavo A. Chapela ◽  
Enrique Díaz-Herrera ◽  
Julio C. Armas-Pérez ◽  
Jacqueline Quintana-H
2020 ◽  
Vol 35 (20) ◽  
pp. 2050106
Author(s):  
Marco Maceda ◽  
Jairo Villafuerte-Lara

We analyze a modified Dirac equation based on a noncommutative structure in phase space originating from a generalized uncertainty principle with a minimum length. The noncommutative structure induces generalized momenta and contributions to the energy levels of the standard Dirac equation. Applying techniques of perturbation theory, we find the lowest-order corrections to the energy levels and eigenfunctions of the Dirac equation in three dimensions for a spherically symmetric linear potential and for a square-well times triangular potential along one spatial dimension. We find that the corrections due to the noncommutative contributions may be of the same order as the relativistic ones, leading to an upper bound on the parameter fixing the minimum length induced by the generalized uncertainty principle.


1968 ◽  
Vol 46 (15) ◽  
pp. 1725-1727 ◽  
Author(s):  
W. R. Smith ◽  
D. Henderson ◽  
J. A. Barker

The integrals which appear in the first-order term and the local compressibility approximation to the second-order term in the Barker–Henderson perturbation theory of fluids are evaluated analytically for the square-well potential in one and three dimensions and are compared with exact calculations.


2004 ◽  
Vol 120 (24) ◽  
pp. 11754-11764 ◽  
Author(s):  
Pedro Orea ◽  
Yurko Duda ◽  
Volker C. Weiss ◽  
Wolffram Schröer ◽  
José Alejandre

2009 ◽  
Vol 107 (4-6) ◽  
pp. 555-562 ◽  
Author(s):  
Achille Giacometti ◽  
Giorgio Pastore ◽  
Fred Lado
Keyword(s):  

Paradoxically, in beta decay, for instance, the final-state Coulomb forces pulling the electron inwards accelerate the emission. Quantum mechanics (q. m. ) makes the rate proportional to α ≡ ρ 0 / ρ ∞ ; ρ 0, ∞ (and v 0, ∞ ) are the particle densities (and speeds) at r = 0 and far upstream in the scattering state which describes the electron. Hence, as regards the effects of finalstate interactions, one must base one’s physical intuition on this ratio α . It is shown that according to (non-relativistic) classical mechanics, if the origin is accessible, then any central potential U(r) where v 0 < ∞ (i. e. where U (0) > -∞) gives in 1, 2 and 3 dimensions, α 1 = v ∞ / v 0 , α 2 = 1, α 3 = v 0 / v ∞ ; the remaining course of U(r) is irrelevant to α . The same results hold also in q. m. in the semiclassical regime, i. e. in the W. K. B. approximation which for such potentials becomes valid at high wavenumbers; in 2D it needs rather careful formulation, and in 3D one must avoid the Langer modification. (The W. K. B. results apply even if d U / d r diverges at r = 0, provided U (0) remains finite; these cases are covered by a simple extension of the argument. ) The square-well and exponential potentials are discussed as examples. Potentials which diverge at the origin are treated in the following paper.


1979 ◽  
Vol 67 (2-3) ◽  
pp. 397-398 ◽  
Author(s):  
P.K. Chakrabarti ◽  
T. Nammalvar ◽  
R.C. Sastri

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