git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@8028 f3b2605a-c512-4ea7-a41b-209d697bcdaa

This commit is contained in:
sjplimp 2012-04-20 14:26:22 +00:00
parent 0a85b18a46
commit 0534908c8a
2 changed files with 10 additions and 4 deletions

View File

@ -112,11 +112,14 @@ phi(r) array are listed for all i,j element pairs in the same format
as other arrays. Since these interactions are symmetric (i,j = j,i)
only phi arrays with i >= j are listed, in the following order: i,j =
(1,1), (2,1), (2,2), (3,1), (3,2), (3,3), (4,1), ..., (Nelements,
Nelements).
Nelements). The tabulated values for each phi function are listed as
r*phi (in units of eV-Angstroms), since they are for atom pairs, the
same as for <A HREF = "pair_eam.html">other EAM files</A>.
</P>
<P>After the phi(r) arrays, each of the u(r) arrays are listed in the
same order with the same assumptions of symmetry. Directly following
the u(r), the w(r) arrays are listed.
the u(r), the w(r) arrays are listed. Note that phi(r) is the only
array tabulated with a scaling by r.
</P>
<HR>

View File

@ -108,11 +108,14 @@ phi(r) array are listed for all i,j element pairs in the same format
as other arrays. Since these interactions are symmetric (i,j = j,i)
only phi arrays with i >= j are listed, in the following order: i,j =
(1,1), (2,1), (2,2), (3,1), (3,2), (3,3), (4,1), ..., (Nelements,
Nelements).
Nelements). The tabulated values for each phi function are listed as
r*phi (in units of eV-Angstroms), since they are for atom pairs, the
same as for "other EAM files"_pair_eam.html.
After the phi(r) arrays, each of the u(r) arrays are listed in the
same order with the same assumptions of symmetry. Directly following
the u(r), the w(r) arrays are listed.
the u(r), the w(r) arrays are listed. Note that phi(r) is the only
array tabulated with a scaling by r.
:line