Challenges
Datasets
Workspaces
Papers
Discussions
Leaderboard
Log inSign up
Challenges
Datasets
Workspaces
Papers
Discussions
Leaderboard
Blog
Job Board
Q3AS

© 2026 Aqora Quantum S.A.S.

TermsPrivacyLegal Notice

Elastic scattering theory

Kenichi Konishi, Giampiero Paffuti

Published Mar 5, 2009• 0 citations
Publisher

Abstract

Abstract In this chapter we shall discuss in an elementary fashion the problem of elastic scattering in quantum mechanics. Several approximation methods specific to scattering problems are discussed. Some of the issues have been discussed in connection with particular approximation schemes (perturbation theory, the semi-classcal approximation, and metastable states) in more specific terms: here we limit ourselves to the general features of the scattering problems.

DOI
10.1093/oso/9780199560264.003.0016

Related papers

Approximation methods

Giampiero V. M. Esposito, Giuseppe Marmo, Gennaro Miele +1 more

Since in both classical and quantum mechanics we are rarely dealing with explicitly solvable equations, this chapter is devoted to an elementary introduction to perturbation theory, Jeffreys–Wentzel–Kramers–Brillouin (hereafter JWKB) method and scattering theory, which are approximation methods that play a key role in all applications of quantum mechanics to atomic and nuclear physics.

Cambridge University Press eBooks•Oct 31, 2014•1 citation

Perturbations and approximation methods

Gennaro Auletta, Mauro Fortunato, Giorgio Parisi A

In this chapter, we present some fundamental issues about approximation methods that are often used when a quantum-mechanical system is perturbed and about the relationship between classical and quantum mechanics. In Sec. 10.1 we introduce the stationary perturbation theory, while Sec. 10.2 is devoted to time-dependent perturbations. In Sec. 10.3 we briefly examine the adiabatic theorem. In Sec. 10.4 we introduce the variation method, an approximation method that is not based on perturbation theory. In Sec. 10.5 we discuss the classical limit of the quantum-mechanical equations, whereas in Sec. 10.6 we deal with the semiclassical approximation, in particular the WKB method. On the basis of the previous approximation methods in Sec. 10.7 we present scattering theory. Finally, in Sec. 10.8 we treat a method that has a wide range of applications: the path-integral method. Stationary perturbation theory Perturbation theory is a rather general approximation method that may be applied when a small additional force (the perturbation) acts on a system (the unperturbed system), whose quantum dynamics is fully known. If the disturbance is small, it modifies both the energy levels and the stationary states. This allows us to make an expansion in power series of a perturbation parameter, which is assumed to be small. Perturbation theory may be applied both to the case where the additional force is time-independent (in which case a stationary treatment suffices – the subject of the present section) as well as to the case where it explicitly depends on time.

Cambridge University Press eBooks•Apr 16, 2009•0 citations

The semi-classical approximation

Kenichi Konishi, Giampiero Paffuti

Abstract In this chapter we study the limit ħ → 0 of quantum mechanics. The passage from quantum mechanics to classical mechanics involves precisely this limit, and the approximation schemes developed for small ħ are known as the semi-classical approximation. The semi-classical approximation has a predecessor: the so-called old quantum theory. Many of the questions concerning the connection between the quantum and classical mechanics were already raised during the years of foundation of quantum mechanics, 1900–1927, but satisfactory answers have not always been obtained.

•Mar 5, 2009•3 citations

Elastic Scattering Theory

Ana Marı́a Cetto, Luis de la Peña

Chapter 18 is entirely devoted to the quantum theory of scattering, which is normally covered in more detail in a course on quantum field theory. We introduce the main concepts, including scattering amplitude, differential and total cross sections, and form factors, and derive the main formulas for elastic scattering, in a nonrelativistic framework; this allows us to appreciate how the information obtained from scattering experiments is used to explore the intricacies of quantum particles that are otherwise inaccessible. The Born approximation is studied and applied to scattering by a periodic potential, a weak potential, and Rutherford scattering. The partial wave expansion is derived and applied to obtain the optical theorem. The chapter concludes with a complementary section on resonant scattering.

Cambridge University Press eBooks•Dec 18, 2025•0 citations

Quantum mechanics. Volume 2. Mecanique quantique

Claude N. Cohen-Tannoudji, Bernard Diu, Franck Laloë

After an introduction to the elementary notions on potential scattering in quantum theory, the spin of electron, the composition of kinetic momenta, the theory of the stationnary perturbations, the approximation methods in time-dependent problems and the systems of identical particles are presented.

•Jan 1, 1977•5 citations

Scattering theory

Giampiero V. M. Esposito, Giuseppe Marmo, Gennaro Miele +1 more

Aims and problems of quantum scattering theory Scattering theory is the branch of physics concerned with interacting systems on a scale of time and/or distance that is large compared with the scale of the interaction itself, and it provides the most powerful tool for studying the microscopic nature of the world. In quantum mechanics, a typical scattering process involves a beam of particles prepared with a given energy and with a more or less defined linear momentum. One then studies either the collision with a similar wave packet, or the collision of the given wave packet against a fixed target. In particular, for a two-body elastic scattering problem with conservative forces, we work in the centre of mass frame, hence reducing the original problem to the analysis of a particle in an external field of forces. Indeed, in Section 7.2 we already used such a technique in the investigation of the hydrogen atom. The crucial difference with respect to Section 7.2 is that, in scattering problems, the continuous spectrum and its perturbations are studied, whereas the Balmer formula has to do with bound states. In the following section we outline the basic aspects of what is called time-dependent scattering. Time-dependent scattering The physical situation we would like to study is as follows: a beam of particles is prepared in a state that is approximately free and allowed to evolve towards the scatterer. After the collision we detect the scattered beam far away from the interaction region.

Cambridge University Press eBooks•Oct 31, 2014•0 citations
Abstract In this chapter we shall discuss in an elementary fashion the problem of elastic scattering in quantum mechanics. Several approximation methods specific to scattering problems are discussed. Some of the issues have been discussed in connection with particular approximation schemes (perturbation theory, the semi-classcal approximation, and metastable states) in more specific terms: here we limit ourselves to the general features of the scattering problems.
In this chapter, we present some fundamental issues about approximation methods that are often used when a quantum-mechanical system is perturbed and about the relationship between classical and quantum mechanics. In Sec. 10.1 we introduce the stationary perturbation theory, while Sec. 10.2 is devoted to time-dependent perturbations. In Sec. 10.3 we briefly examine the adiabatic theorem. In Sec. 10.4 we introduce the variation method, an approximation method that is not based on perturbation theory. In Sec. 10.5 we discuss the classical limit of the quantum-mechanical equations, whereas in Sec. 10.6 we deal with the semiclassical approximation, in particular the WKB method. On the basis of the previous approximation methods in Sec. 10.7 we present scattering theory. Finally, in Sec. 10.8 we treat a method that has a wide range of applications: the path-integral method. Stationary perturbation theory Perturbation theory is a rather general approximation method that may be applied when a small additional force (the perturbation) acts on a system (the unperturbed system), whose quantum dynamics is fully known. If the disturbance is small, it modifies both the energy levels and the stationary states. This allows us to make an expansion in power series of a perturbation parameter, which is assumed to be small. Perturbation theory may be applied both to the case where the additional force is time-independent (in which case a stationary treatment suffices – the subject of the present section) as well as to the case where it explicitly depends on time.
Abstract In this chapter we study the limit ħ → 0 of quantum mechanics. The passage from quantum mechanics to classical mechanics involves precisely this limit, and the approximation schemes developed for small ħ are known as the semi-classical approximation. The semi-classical approximation has a predecessor: the so-called old quantum theory. Many of the questions concerning the connection between the quantum and classical mechanics were already raised during the years of foundation of quantum mechanics, 1900–1927, but satisfactory answers have not always been obtained.
Chapter 18 is entirely devoted to the quantum theory of scattering, which is normally covered in more detail in a course on quantum field theory. We introduce the main concepts, including scattering amplitude, differential and total cross sections, and form factors, and derive the main formulas for elastic scattering, in a nonrelativistic framework; this allows us to appreciate how the information obtained from scattering experiments is used to explore the intricacies of quantum particles that are otherwise inaccessible. The Born approximation is studied and applied to scattering by a periodic potential, a weak potential, and Rutherford scattering. The partial wave expansion is derived and applied to obtain the optical theorem. The chapter concludes with a complementary section on resonant scattering.
Aims and problems of quantum scattering theory Scattering theory is the branch of physics concerned with interacting systems on a scale of time and/or distance that is large compared with the scale of the interaction itself, and it provides the most powerful tool for studying the microscopic nature of the world. In quantum mechanics, a typical scattering process involves a beam of particles prepared with a given energy and with a more or less defined linear momentum. One then studies either the collision with a similar wave packet, or the collision of the given wave packet against a fixed target. In particular, for a two-body elastic scattering problem with conservative forces, we work in the centre of mass frame, hence reducing the original problem to the analysis of a particle in an external field of forces. Indeed, in Section 7.2 we already used such a technique in the investigation of the hydrogen atom. The crucial difference with respect to Section 7.2 is that, in scattering problems, the continuous spectrum and its perturbations are studied, whereas the Balmer formula has to do with bound states. In the following section we outline the basic aspects of what is called time-dependent scattering. Time-dependent scattering The physical situation we would like to study is as follows: a beam of particles is prepared in a state that is approximately free and allowed to evolve towards the scatterer. After the collision we detect the scattered beam far away from the interaction region.