Jump to content
Main menu
Main menu
move to sidebar
hide
Navigation
Main page
Recent changes
Random page
Help about MediaWiki
Special pages
Niidae Wiki
Search
Search
Appearance
Create account
Log in
Personal tools
Create account
Log in
Pages for logged out editors
learn more
Contributions
Talk
Editing
Sintering
(section)
Page
Discussion
English
Read
Edit
View history
Tools
Tools
move to sidebar
hide
Actions
Read
Edit
View history
General
What links here
Related changes
Page information
Appearance
move to sidebar
hide
Warning:
You are not logged in. Your IP address will be publicly visible if you make any edits. If you
log in
or
create an account
, your edits will be attributed to your username, along with other benefits.
Anti-spam check. Do
not
fill this in!
==== Grain boundary energy/tension ==== The atoms in the GB are normally in a higher energy state than their equivalent in the bulk material. This is due to their more stretched bonds, which gives rise to a GB tension <math>\sigma_{GB}</math>. This extra energy that the atoms possess is called the grain boundary energy, <math>\gamma_{GB}</math>. The grain will want to minimize this extra energy, thus striving to make the grain boundary area smaller and this change requires energy.<ref name="Fundamentals of Materials Science" /> "Or, in other words, a force has to be applied, in the plane of the grain boundary and acting along a line in the grain-boundary area, in order to extend the grain-boundary area in the direction of the force. The force per unit length, i.e. tension/stress, along the line mentioned is ΟGB. On the basis of this reasoning it would follow that: <math display="block">\sigma_{GB} dA \text{ (work done)} = \gamma_{GB} dA \text{ (energy change)}\,\!</math> with dA as the increase of grain-boundary area per unit length along the line in the grain-boundary area considered."<ref name="Fundamentals of Materials Science" /><sup>[pg 478]</sup> The GB tension can also be thought of as the attractive forces between the atoms at the surface and the tension between these atoms is due to the fact that there is a larger interatomic distance between them at the surface compared to the bulk (i.e. [[surface tension]]). When the surface area becomes bigger the bonds stretch more and the GB tension increases. To counteract this increase in tension there must be a transport of atoms to the surface keeping the GB tension constant. This diffusion of atoms accounts for the constant surface tension in liquids. Then the argument, <math display="block">\sigma_{GB} dA \text{ (work done)} = \gamma_{GB} dA \text{ (energy change)}\,\!</math> holds true. For solids, on the other hand, diffusion of atoms to the surface might not be sufficient and the surface tension can vary with an increase in surface area.<ref name=Sintering>{{cite book|last=Kang|first=Suk-Joong L.|title=Sintering: Densification, Grain Growth, and Microstructure|url=https://archive.org/details/sinteringdensifi00kang_089|url-access=limited|year=2005|publisher=Elsevier Ltd.|isbn=978-0-7506-6385-4|pages=[https://archive.org/details/sinteringdensifi00kang_089/page/n21 9]β18}}</ref> For a solid, one can derive an expression for the change in Gibbs free energy, dG, upon the change of GB area, dA. dG is given by <math display="block">\sigma_{GB} dA \text{ (work done)} = dG \text{ (energy change)} = \gamma_{GB} dA + A d\gamma_{GB}\,\!</math> which gives <math display="block">\sigma_{GB} = \gamma_{GB} + \frac{Ad\gamma_{GB}}{dA}\,\!</math> <math>\sigma_{GB}</math> is normally expressed in units of <math>\frac{N}{m}</math> while <math>\gamma_{GB}</math> is normally expressed in units of <math>\frac{J}{m^2}</math> <math>(J = Nm)</math> since they are different physical properties.<ref name="Fundamentals of Materials Science" />
Summary:
Please note that all contributions to Niidae Wiki may be edited, altered, or removed by other contributors. If you do not want your writing to be edited mercilessly, then do not submit it here.
You are also promising us that you wrote this yourself, or copied it from a public domain or similar free resource (see
Encyclopedia:Copyrights
for details).
Do not submit copyrighted work without permission!
Cancel
Editing help
(opens in new window)
Search
Search
Editing
Sintering
(section)
Add topic