{ "cells": [ { "cell_type": "markdown", "metadata": {}, "source": [ "\n", "\n", "# One-Boson Exchange Models\n", "\n", " \n", "**Scott Bogner**, [National Superconducting Cyclotron Laboratory](http://www.nscl.msu.edu/) and [Department of Physics and Astronomy](https://www.pa.msu.edu/), [Michigan State University](http://www.msu.edu/), East Lansing, MI 48824, USA \n", "\n", " **Morten Hjorth-Jensen**, [National Superconducting Cyclotron Laboratory](http://www.nscl.msu.edu/) and [Department of Physics and Astronomy](https://www.pa.msu.edu/), [Michigan State University](http://www.msu.edu/), East Lansing, MI 48824, USA\n", "\n", "Date: **2017**\n", "\n", "## A typical form of the nuclear force\n", "Here we display a typical way to parametrize (non-relativistic expression) the nuclear two-body force\n", "in terms of some operators, the central part, the spin-spin part and the central force." ] }, { "cell_type": "markdown", "metadata": {}, "source": [ "0\n", " \n", "<\n", "<\n", "<\n", "!\n", "!\n", "M\n", "A\n", "T\n", "H\n", "_\n", "B\n", "L\n", "O\n", "C\n", "K" ] }, { "cell_type": "markdown", "metadata": {}, "source": [ "$$\n", "\\left. + C_{SL} \\left( {1\\over m_\\alpha r} + {1\\over \\left( m_\\alpha r\\right)^2}\n", "\\right) \\mathbf{L}\\cdot \\mathbf{S}\n", "\\right\\} \\frac{e^{-m_\\alpha r}}{m_\\alpha r}\n", "$$" ] }, { "cell_type": "markdown", "metadata": {}, "source": [ "How do we derive such terms? (Note: no isospin dependence and that the above is an approximation)\n", "\n", "\n", "\n", "\n", "## Nuclear forces\n", "To derive the above famous form of the nuclear force using field theoretical concepts, we will need some \n", "elements from relativistic quantum mechanics. These derivations will be given below. \n", "The material here gives some background to this.\n", "I know that many of you have not taken a course in quantum field theory. I hope however that you can see the basic ideas leading to the famous non-relativistic expressions for the nuclear force. \n", "\n", "**Furthermore, when we analyze nuclear data, we will actually try to explain properties like spectra, single-particle energies etc in terms of the various terms of the nuclear force. Moreover, many of you will hear about these terms at various talks, workshops, seminars etc. Then, it is good to have an idea of what people actually mean!!**\n", "\n", " \n", "\n", "## Dramatis Personae\n", "\n", "
Baryons | Mass (MeV) | Mesons | Mass (MeV) |
---|---|---|---|
$p,n$ | 938.926 | $\\pi$ | 138.03 |
$\\Lambda$ | 1116.0 | $\\eta$ | 548.8 |
$\\Sigma$ | 1197.3 | $\\sigma$ | $\\approx 550.0$ |
$\\Delta$ | 1232.0 | $\\rho$ | 770 |
$\\omega$ | 782.6 | ||
$\\delta$ | 983.0 | ||
$K$ | 495.8 | ||
$K^{\\star}$ | 895.0 |