Jump to content
 







Main menu
   


Navigation  



Main page
Contents
Current events
Random article
About Wikipedia
Contact us
Donate
 




Contribute  



Help
Learn to edit
Community portal
Recent changes
Upload file
 








Search  

































Create account

Log in
 









Create account
 Log in
 




Pages for logged out editors learn more  



Contributions
Talk
 



















Contents

   



(Top)
 


1 Formal definition  





2 Hard-spheres gas  





3 Hard-spheres liquid  





4 The Carnahan-Starling Equation of State  





5 See also  





6 Literature  





7 References  














Hard spheres






Deutsch
Français
Nederlands
Українська
 

Edit links
 









Article
Talk
 

















Read
Edit
View history
 








Tools
   


Actions  



Read
Edit
View history
 




General  



What links here
Related changes
Upload file
Special pages
Permanent link
Page information
Cite this page
Get shortened URL
Download QR code
Wikidata item
 




Print/export  



Download as PDF
Printable version
 
















Appearance
   

 






From Wikipedia, the free encyclopedia
 


Hard spheres are widely used as model particles in the statistical mechanical theory of fluids and solids. They are defined simply as impenetrable spheres that cannot overlap in space. They mimic the extremely strong ("infinitely elastic bouncing") repulsion that atoms and spherical molecules experience at very close distances. Hard spheres systems are studied by analytical means, by molecular dynamics simulations, and by the experimental study of certain colloidal model systems.

Beside being a model of theoretical significance, the hard-sphere system is used as a basis in the formulation of several modern, predictive Equations of State for real fluids through the SAFT approach, and models for transport properties in gases through Chapman-Enskog Theory.

Formal definition[edit]

Hard spheres of diameter are particles with the following pairwise interaction potential:

where and are the positions of the two particles.

Hard-spheres gas[edit]

The first three virial coefficients for hard spheres can be determined analytically

=
=
=

Higher-order ones can be determined numerically using Monte Carlo integration. We list

=
=
=

A table of virial coefficients for up to eight dimensions can be found on the page Hard sphere: virial coefficients.[1]

Phase diagram of hard sphere system (Solid line - stable branch, dashed line - metastable branch): Pressure as a function of the volume fraction (or packing fraction)

The hard sphere system exhibits a fluid-solid phase transition between the volume fractions of freezing and melting . The pressure diverges at random close packing for the metastable liquid branch and at close packing for the stable solid branch.

Hard-spheres liquid[edit]

The static structure factor of the hard-spheres liquid can be calculated using the Percus–Yevick approximation.

The Carnahan-Starling Equation of State[edit]

A simple, yet popular equation of state describing systems of pure hard spheres was developed in 1969 by N. F. Carnahan and K. E. Starling.[2] By expressing the compressibility of a hard-sphere system as a geometric series, the expression

is obtained, where is the packing fraction, given by

where isAvogadros number, is the molar density of the fluid, and is the diameter of the hard-spheres. From this Equation of State, one can obtain the residual Helmholtz energy,[3]

,

which yields the residual chemical potential

.

One can also obtain the value of the radial distribution function, , evaluated at the surface of a sphere,[3]

.

The latter is of significant importance to accurate descriptions of more advanced intermolecular potentials based on perturbation theory, such as SAFT, where a system of hard spheres is taken as a reference system, and the complete pair-potential is described by perturbations to the underlying hard-sphere system. Computation of the transport properties of hard-sphere gases at moderate densities using Revised Enskog Theory also relies on an accurate value for , and the Carnahan-Starling Equation of State has been used for this purpose to large success.[4]

See also[edit]

Literature[edit]

References[edit]

  1. ^ Clisby, Nathan; McCoy, Barry M. (January 2006). "Ninth and Tenth Order Virial Coefficients for Hard Spheres in D Dimensions". Journal of Statistical Physics. 122 (1): 15–57. arXiv:cond-mat/0503525. Bibcode:2006JSP...122...15C. doi:10.1007/s10955-005-8080-0. S2CID 16278678.
  • ^ Carnahan, Norman F.; Starling, Kenneth E. (1969-07-15). "Equation of State for Nonattracting Rigid Spheres". The Journal of Chemical Physics. 51 (2): 635–636. doi:10.1063/1.1672048. ISSN 0021-9606.
  • ^ a b Lee, Lloyd L. (1995-12-01). "An accurate integral equation theory for hard spheres: Role of the zero-separation theorems in the closure relation". The Journal of Chemical Physics. 103 (21): 9388–9396. doi:10.1063/1.469998. ISSN 0021-9606.
  • ^ López de Haro, M.; Cohen, E. G. D.; Kincaid, J. M. (1983-03-01). "The Enskog theory for multicomponent mixtures. I. Linear transport theory". The Journal of Chemical Physics. 78 (5): 2746–2759. doi:10.1063/1.444985. ISSN 0021-9606.

  • Retrieved from "https://en.wikipedia.org/w/index.php?title=Hard_spheres&oldid=1212374469"

    Categories: 
    Statistical mechanics
    Conceptual models
    Hidden categories: 
    Articles with short description
    Short description matches Wikidata
     



    This page was last edited on 7 March 2024, at 14:45 (UTC).

    Text is available under the Creative Commons Attribution-ShareAlike License 4.0; additional terms may apply. By using this site, you agree to the Terms of Use and Privacy Policy. Wikipedia® is a registered trademark of the Wikimedia Foundation, Inc., a non-profit organization.



    Privacy policy

    About Wikipedia

    Disclaimers

    Contact Wikipedia

    Code of Conduct

    Developers

    Statistics

    Cookie statement

    Mobile view



    Wikimedia Foundation
    Powered by MediaWiki