Spectral-shift and scattering-equivalent Hamiltonians on a coarse momentum grid

The solution of the scattering problem based on the Lippmann-Schwinger equation requires in many cases a discretization of the spectrum in the continuum which does not respect the unitary equivalence of the S-matrix on the finite grid. We present a new prescription for the calculation of phase shift...

Full description

Bibliographic Details
Main Authors: María Gómez-Rocha, Enrique Ruiz Arriola
Format: Article
Language:English
Published: Elsevier 2020-01-01
Series:Physics Letters B
Online Access:http://www.sciencedirect.com/science/article/pii/S0370269319308299
id doaj-4cded4be1603464fa0f3d4a62d96a20b
record_format Article
spelling doaj-4cded4be1603464fa0f3d4a62d96a20b2020-11-25T01:31:51ZengElsevierPhysics Letters B0370-26932020-01-01800Spectral-shift and scattering-equivalent Hamiltonians on a coarse momentum gridMaría Gómez-Rocha0Enrique Ruiz Arriola1Corresponding author.; Departamento de Física Atómica, Molecular y Nuclear and Instituto Carlos I de Física Teórica y Computacional, Universidad de Granada, E-18071 Granada, SpainDepartamento de Física Atómica, Molecular y Nuclear and Instituto Carlos I de Física Teórica y Computacional, Universidad de Granada, E-18071 Granada, SpainThe solution of the scattering problem based on the Lippmann-Schwinger equation requires in many cases a discretization of the spectrum in the continuum which does not respect the unitary equivalence of the S-matrix on the finite grid. We present a new prescription for the calculation of phase shifts based on the shift that is produced in the spectrum of a Chebyshev-angle variable. This is analogous to the energy shift that is produced in the energy levels of a scattering process in a box, when an interaction is introduced. Our formulation holds for any momentum grid and preserves the unitary equivalence of the scattering problem on the finite momentum grid. We illustrate this procedure numerically considering the non-relativistic NN case for S01 and S13 channels. Our spectral shift formula provides much more accurate results than the previous ones and turns out to be at least as competitive as the standard procedures for calculating phase shifts. Keywords: Lippmann-Schwinger equation, Phase shifts, Scattering, Momentum grid, Equivalent hamiltonianhttp://www.sciencedirect.com/science/article/pii/S0370269319308299
collection DOAJ
language English
format Article
sources DOAJ
author María Gómez-Rocha
Enrique Ruiz Arriola
spellingShingle María Gómez-Rocha
Enrique Ruiz Arriola
Spectral-shift and scattering-equivalent Hamiltonians on a coarse momentum grid
Physics Letters B
author_facet María Gómez-Rocha
Enrique Ruiz Arriola
author_sort María Gómez-Rocha
title Spectral-shift and scattering-equivalent Hamiltonians on a coarse momentum grid
title_short Spectral-shift and scattering-equivalent Hamiltonians on a coarse momentum grid
title_full Spectral-shift and scattering-equivalent Hamiltonians on a coarse momentum grid
title_fullStr Spectral-shift and scattering-equivalent Hamiltonians on a coarse momentum grid
title_full_unstemmed Spectral-shift and scattering-equivalent Hamiltonians on a coarse momentum grid
title_sort spectral-shift and scattering-equivalent hamiltonians on a coarse momentum grid
publisher Elsevier
series Physics Letters B
issn 0370-2693
publishDate 2020-01-01
description The solution of the scattering problem based on the Lippmann-Schwinger equation requires in many cases a discretization of the spectrum in the continuum which does not respect the unitary equivalence of the S-matrix on the finite grid. We present a new prescription for the calculation of phase shifts based on the shift that is produced in the spectrum of a Chebyshev-angle variable. This is analogous to the energy shift that is produced in the energy levels of a scattering process in a box, when an interaction is introduced. Our formulation holds for any momentum grid and preserves the unitary equivalence of the scattering problem on the finite momentum grid. We illustrate this procedure numerically considering the non-relativistic NN case for S01 and S13 channels. Our spectral shift formula provides much more accurate results than the previous ones and turns out to be at least as competitive as the standard procedures for calculating phase shifts. Keywords: Lippmann-Schwinger equation, Phase shifts, Scattering, Momentum grid, Equivalent hamiltonian
url http://www.sciencedirect.com/science/article/pii/S0370269319308299
work_keys_str_mv AT mariagomezrocha spectralshiftandscatteringequivalenthamiltoniansonacoarsemomentumgrid
AT enriqueruizarriola spectralshiftandscatteringequivalenthamiltoniansonacoarsemomentumgrid
_version_ 1725084927588827136