Weak Interaction Rates of sd-Shell Nuclei in Stellar Matter Data by T. Oda, M. Hino, K. Muto, M. Takahara and K. Sato, Rate Tables for the Weak Processes of sd-Shell Nuclei in Stellar Matter; Atomic Data and Nuclear Data Tables, 56, 231-403 (1994).
The data file(1.238Mb) for A=1 and A=17-39 is available at (oda.txt ). Below is the explanation of the table, followed by a sample data set of A = 1.
Symbol | Description |
---|---|
A | Mass number |
Z | Proton number |
N | Neutron number |
M | Ground-state mass, with M(Z,N)-M(Z-1,N+1) given in the table in MeV |
RHOYE | log(rho*Ye)(in g.cm-3), where rho is the baryon density and Ye is the ratio of the electron number to the baryon number |
T9 | Temperature in units of 109 K |
UF | Fermi energy of eleotron and positron, including the rest mass (in MeV) |
E-CAP | Electron capture rate(s-1) |
E+DEC | Positron decay rate(s-1) |
NEUE | Neutrino energy loss rate (MeV.s-1) |
GAMRAY | Gamma-ray heating rate (MeV.s-1), tabulated separately for beta+direction (left) and beta-direction (right) |
E+CAP | Positron capture rate(s-1) |
E-DEC | Electron decay rate(s-1) |
NEUEBAR | Anti-neutrino energy loss rate (MeV.s-1) |