This is a Hauser-Feshbach statistical model code. The speciality of
this
code is that it is fully web driven (catchword
cloud computing)
and that even new functions for
certain nuclear properties (e.g. optical potentials) can be introduced
without recompilation. You are not limited by the options below.
There are
further
explanations
available.
For latest news or help, take a look at the
Forum.
For quick access
to the standard (default)
results it is better to use the HTML
database
access (no registration required)! If you just want to compare
to cross sections or rates (for example, from experiments) use this database
and NOT the code below!!!
The standard
results are published in Atomic Data Nuclear
Data Tables 79 (2001) 47 and Atomic
Data Nuclear Data
Tables 88 (2004) 1.
Fits to the reaction rates and additional information can be found in
Atomic Data Nuclear Data Tables 75
(2000) 1.
The NON-SMOKERWEB
code is
different from the previous NON-SMOKER code and may yield different
results!
You need to be registered to use the code
(test account available)!
If you are interested in starting a collaboration using this
code,
please register for access,
stating what you want to use the code for.
Output
What to expect: Cross sections (g.s. target) and
astrophysical reaction
rates (both g.s. and thermally excited target); Maxwellian averaged
cross sections (both g.s. and thermally excited target) when using
neutrons as projectiles; astrophysical S-factors (g.s. target)
when using a charged projectile.
If you need the cross sections or rates at different energies
or
temperatures than provided here, feel free to use
my interpolation program.
Please read the instructions
carefully!
(Secure http is used to transmit the information in this form. If your
browser complains about an untrusted certificate, ignore this warning and
allow the browser to continue and remember the exception. You only have to
do this once.)