Everything Totally Explained


Ask & we'll explain, totally!
Semi-empirical mass formula
Totally Explained


  NEW! All the latest news in the worlds of computer gaming, entertainment, the environment,  
finance, health, politics, science, stocks & shares, technology and much, much, more.  


View this entry using RSS

Everything about Liquid-drop Model totally explained

In nuclear physics, the semi-empirical mass formula (SEMF), sometimes also called Weizsäcker's formula, is a formula used to approximate the mass and various other properties of an atomic nucleus. As the name suggests, it's partially based on theory and partly on empirical measurements; the theory is based on the liquid drop model, and can account for most of the terms in the formula, and gives a rough estimates for the values of the coefficients. It was first formulated in 1935 by German physicist Carl von Weizsäcker, and although refinements have been made to the coefficients over the years, the form of the formula remains the same today.
   This formula shouldn't be confused with the mass formula of Weizsäcker's student Burkhard Heim.
   The formula gives a good approximation for atomic masses and several other effects, but doesn't explain the appearance of magic numbers.

The liquid drop model and its analysis

The liquid drop model is a model in nuclear physics which treats the nucleus as a drop of incompressible nuclear fluid, first proposed by George Gamow. The fluid is made of nucleons (protons and neutrons), which are held together by the strong nuclear force.
   This is a crude model that doesn't explain all the properties of nuclei, but does explain the spherical shape of most nuclei. It also helps to predict the binding energy of the nucleus.
   Mathematical analysis of the theory delivers an equation which attempts to predict the binding energy of a nucleus in terms of the numbers of protons and neutrons it contains. This equation has five terms on its right hand side. These correspond to the cohesive binding of all the nucleons by the strong nuclear force, the electrostatic mutual repulsion of the protons, a surface energy term, an asymmetry term (derivable from the protons and neutrons occupying independent quantum momentum states) and a pairing term (partly derivable from the protons and neutrons occupying independent quantum spin states).
   If we consider the sum of the following five types of energies, then the picture of a nucleus as a drop of incompressible liquid roughly accounts for the observed variation of binding energy of the nucleus:
Volume energy. When an assembly of nucleons of the same size is packed together into the smallest volume, each interior nucleon has a certain number of other nucleons in contact with it. So, this nuclear energy is proportional to the volume. Surface energy. A nucleon at the surface of a nucleus interacts with fewer other nucleons that one in the interior of the nucleus and hence its binding energy is less. This surface energy term takes that into account and is therefore negative and is proportional to the surface area. Coulomb Energy. The electric repulsion between each pair of protons in a nucleus contributes toward decreasing its binding energy. Asymmetry energy (also called Pauli Energy). An energy associated with the Pauli exclusion principle. If it wasn't for the Coulomb energy, the most stable form of nuclear matter would have N=Z, since unequal values of N and Z imply filling higher energy levels for one type of particle, while leaving lower energy levels vacant for the other type. Pairing energy. An energy which is a correction term that arises from the tendency of proton pairs and neutron pairs to occur. An even number of particles is more stable than an odd number.

The formula

In the following formulae, let A be the total number of nucleons, Z the number of protons, and N the number of neutrons.
   The mass of an atomic nucleus is given by » m = Z m_

This is roughly A/2 for light nuclei, but for heavy nuclei there's an even better agreement with nature.
   By substituting the above value of Z back into B one obtains the binding energy as a function of the atomic weight, B(A). Maximizing B(A)/A with respect to A gives the nucleus which is most strongly bound, for example most stable. The value we get is A=63 (copper), close to the measured values of A=62 (nickel) and A=58 (iron).

Further Information

Get more info on 'Liquid-drop Model'.


External Link Exchanges

Do you know how hard it is to get a link from a large encyclopaedia? Well we're different and will prove it. To get a link from us just add the following HTML to your site on a relevant page:

    <a href="http://semi-empirical_mass_formula.totallyexplained.com">Semi-empirical mass formula Totally Explained</a>

Then simply click through this link from your web page. Our crawlers will verify your link, extract the title of your web page and instantly add a link back to it. If you like you can remove the words Totally Explained and embed the link in article text.
   As long as your link remains in place, we'll keep our link to you right here. Please play fair - our crawlers are watching. Your site must be closely related to this one's topic. Any kind of spamming, dubious practises or removing the link will result in your link from us being dropped and, potentially, your whole site being banned.



Copyright © 2007-8 totallyexplained.com | Licensed under the GNU Free Documentation License | Site Map
This article contains text from the Wikipedia article Semi-empirical mass formula (History) and is released under the GFDL | RSS Version