2. How to select reaction rates other than the default
ones.
2a. First step: go to Individual Reaction.
Type in the requested reaction, and
provide the bibliographic index for the requested rate:
For most reactions, different rates are proposed. These can be selected
with the 'bibliographic index' field, according to the following
rules:
1 = nominal rate from Goriely (1999, Astron. Astrophys. 342, 881;
Table available in electronic form), updating Takahashi
& Yokoi (1987, Atomic Data Nucl. Data Tables 36, 375) table
2 = low rate from Goriely (1999)
3 = high rate from Goriely (1999)
4 = forces the use of Takahashi
& Yokoi (1987, Atomic Data Nucl. Data Tables 36, 375) table
300 = forces the use of Langanke & Martinez (2000, Nucl.Phys. A 673, 481) table
301 = forces the use of Oda et al. (1994,
Atomic Data and Nuclear Data Tables 56, 231) table
For non-NACRE reactions, the list of available rates may be
consulted beforehand at http://www-astro.ulb.ac.be/Netgen/references.html
.
No such list is available for NACRE reactions. However, by setting the
bibliographic index to 11, the log file will return all rates available
before NACRE. In a second step, the bibliographic index may then be set to
either 11, 12, or 13... according to the list provided in the log file.
Click on the button 'Add reaction to network'
Note: If this is not the first time Netgen is run from your current
IP address, it might be necessary to click first on `Clear network'; otherwise,
the selected reaction will be appended to the network generated by the
previous Netgen run.
It is possible to edit the network at this stage
by removing some reactions. Go to the list of reactions at the bottom of the form, and select the reactions to be deleted from the network.
Then click on the button Delete selected reactions. The edited network
will appear in a similar form, and the editing process may be pursued as many times as required.
the log file
listing the bibliographical references of all the
rates available for the reactions included in the considered
network, and the rate provided in the table.
Possible problems in finding or computing the rate are also reported in
this file.
The files are named, respectively:
tmpIP_address.tail
tmpIP_address.rates
tmpIP_address.refs
where IP_address is the IP address of the client, as indicated
here. Example: tmp164.15.125.42.rates
What is to be found in the table of reaction rates?
This table provides the number of reactions
per sec per (cm3mole-1)(N-1),
where N refers to the number of particles in the entrance
channel:
Radiative neutron capture reactions: Maxwellian-average
NAv
< sigma v > [cm3 mole-1 s-1]
NAv < sigma v > is
generally derived from the Maxwellian-averaged cross section <sigma
v>/vT using the formula
NAv < sigma v > = 2.645 104 (kT)(1/2)
<sigma v>/vT, with NAv
< sigma v > expressed in cgs units, kT in keV and <sigma v>/vT in mb
Beta-decays, electron captures, or photodesintegrations:
decays per s [lambda (s-1)]
Some beta-decay rates from Takahashi & Yokoi (1987)
consist of four successive columns, corresponding to electronic number
densities of 1, 3, 10 and 30 x 1026 cm-3 A special
treatment applies to electron captures by 7Be, as indicated in the corresponding
log file
The reaction kind is coded in the header line labelled Type in the following way:
--: two-particle reactions
---: three-particle reactions
----: four-particle reactions
+: photodissociation or beta-decay
++: electron capture
+++: electron capture on Be7
nE+mm: value of the electron number density (in units of electrons/cm3) for beta-decay rates dependent upon electron number density
NaN (`Not a Number`) symbols are given in the table for temperatures
at which no data are available
Reverse reaction rates with no data available for the
direct reaction are set to NaN or to .1000E-98,
although the exact value may possibly be much larger
than .1000E-98 (especially for neutron-capture reactions)!
The energetics (Q = Qrad + Qnu) of the reaction is also
provided in the header.
Q is computed from Audi & Wapstra mass table (Audi
G., Wapstra A.H., 1995, Nucl. Phys. A595, 409), as the difference between
the mass excess in the entrance and exit chanels.
Qrad provides the radiative losses, i.e., Q - Qnu, where
Qnu is the energy possibly carried away by neutrinos.
The neutrino loss Qnu is computed according to Eqs. 1
and 2 of Fowler W.A., Caughlan G.R. & Zimmerman B.A. (1975, ARA&A
13, 69).
A fortran routine
is available to read the table of reaction rates.
Here is an example of reaction rates from Netgen: