rpms/starlab/devel starlab-4.4.3-freeze.patch,NONE,1.1

[Lubomir Rintel]

Author: lkundrak

Update of /cvs/pkgs/rpms/starlab/devel
In directory cvs1.fedora.phx.redhat.com:/tmp/cvs-serv28917

Added Files:
	starlab-4.4.3-freeze.patch 
Log Message:
Add missing patch

starlab-4.4.3-freeze.patch:

--- NEW FILE starlab-4.4.3-freeze.patch ---
Rename freeze: https://bugzilla.redhat.com/show_bug.cgi?id=472616

diff -urp starlab-4.4.3.freeze/doc/Primer.tex starlab-4.4.3/doc/Primer.tex
--- starlab-4.4.3.freeze/doc/Primer.tex	1999-06-12 21:19:21.000000000 +0200
+++ starlab-4.4.3/doc/Primer.tex	2009-04-30 16:40:02.000000000 +0200
@@ -159,13 +159,13 @@ running small test simulations.  For exa
 effects in a cold collapse could be done as follows:
 
 {\codes
-\quad mkplummer -n 100 | freeze | leapfrog -t 2 -a 0.02 -e 0.05 | lagrad
+\quad mkplummer -n 100 | sl-freeze | leapfrog -t 2 -a 0.02 -e 0.05 | lagrad
 }
 \medskip
 
 Here {\tt \ mkplummer\ } creates initial conditions for a 100-body
 system, according to a Plummer model distribution.  The resulting data
-are piped into the next module, {\tt \ freeze}, which simply sets all
+are piped into the next module, {\tt \ sl-freeze}, which simply sets all
 velocities to zero, while preserving the positions.  Following that,
 the data are read in by the leapfrog integrator, which is asked to
 evolve the system for a period of 2 time units, with a (constant) step
diff -urp starlab-4.4.3.freeze/etc/papers/Preview.tex starlab-4.4.3/etc/papers/Preview.tex
--- starlab-4.4.3.freeze/etc/papers/Preview.tex	1999-06-12 21:19:23.000000000 +0200
+++ starlab-4.4.3/etc/papers/Preview.tex	2009-04-30 16:40:29.000000000 +0200
@@ -826,13 +826,13 @@ of relaxation effects in a cold collapse
 }
 
 {\codes
-mkplummer -n 100 | freeze | leapfrog -t 2 -d 0.02 -e 0.05 | lagrad
+mkplummer -n 100 | sl-freeze | leapfrog -t 2 -d 0.02 -e 0.05 | lagrad
 }
 \medskip
 
 Here {\tt \ mkplummer\ } creates initial conditions for a 100-body system,
 according to a Plummer model distribution.  The resulting data are
-piped into the next module, {\tt \ freeze\ }, which simply sets all
+piped into the next module, {\tt \ sl-freeze\ }, which simply sets all
 velocities to zero, while preserving the positions.  Following that,
 the data are read in by the leapfrog integrator, which is asked to
 evolve the system for a period of 2 time units, with a stepsize of
diff -urp starlab-4.4.3.freeze/src/node/dyn/hdyn/xutil/Demo.csh starlab-4.4.3/src/node/dyn/hdyn/xutil/Demo.csh
--- starlab-4.4.3.freeze/src/node/dyn/hdyn/xutil/Demo.csh	2000-09-18 03:33:01.000000000 +0200
+++ starlab-4.4.3/src/node/dyn/hdyn/xutil/Demo.csh	2009-04-30 16:40:51.000000000 +0200
@@ -1,13 +1,13 @@
 #!/bin/tcsh -f
 
-# Usage:  Demo.csh  N [10]  fb [0.1]  freeze [no]  dt [2^-5]
+# Usage:  Demo.csh  N [10]  fb [0.1]  sl-freeze [no]  dt [2^-5]
 
 set N = 10
 if ($#argv > 0) set N = $1
 set f = 0
 if ($#argv > 1) set f = $2
 alias FREEZE cat
-if ($#argv > 2) alias FREEZE freeze
+if ($#argv > 2) alias FREEZE sl-freeze
 set D = -5
 if ($#argv > 3) set D = $4
 
diff -urp starlab-4.4.3.freeze/TOOLS starlab-4.4.3/TOOLS
--- starlab-4.4.3.freeze/TOOLS	2009-04-30 16:27:18.000000000 +0200
+++ starlab-4.4.3/TOOLS	2009-04-30 16:39:43.000000000 +0200
@@ -81,7 +81,7 @@ Note:  Most tools are just simple interf
     extract_snap     find and print the last snapshot, or the first
                         snapshot following a specified time
     flatten          flatten a dyn tree to a single-level linked list
-    freeze           set all velocities to zero, leaving positions
+    sl-freeze        set all velocities to zero, leaving positions
                         unchanged 
     lagrad           compute Lagrangian (mass) radii for an N-body
                         system