Nuclear reaction rates are quantities of fundamental importance in astrophysics. Substantial efforts have been devoted in the last decades to measuring or calculating them. This paper presents a detailed description of the Brussels nuclear reaction rate library BRUSLIB and of the nuclear network generator NETGEN. BRUSLIB is made of two parts. The first one contains the 1999 NACRE compilation based on experimental data for 86 reactions with (mainly) stable targets up to Si. BRUSLIB provides an electronic link to the published, as well as to a large body of unpublished, NACRE data containing adopted rates, as well as lower and upper limits. The second part of BRUSLIB concerns nuclear reaction rate predictions to complement the experimentally-...
The majority of nuclear reactions in astrophysics involve unstable nuclei which are not fully access...
“Published under licence in Journal of Physics: Conference Series by IOP Publishing Ltd. Content fro...
The first part of the paper discusses nuclear properties relevant to predict compound reactions. The...
Nuclear reaction rates are quantities of fundamental importance in astrophysics. Substantial efforts...
Nuclear reaction rates are quantities of fundamental importance in astrophysics. Substantial efforts...
Nuclear reaction rates are obviously quantities of fundamental importance in nuclear astrophysics. I...
An update of a previous description of the BRUSLIB + NACRE package of nuclear data for astrophysics ...
An update of a previous description of the BRUSLIB + NACRE package of nuclear data for astrophysics ...
Modern computer technology has revolutionized theoretical calculations on stellar structure and stel...
In a previous publication (ATOMIC DATA AND NUCLEAR DATA TABLES 75, 1 (2000)), we gave seven-paramete...
Context. Nuclear reaction rates of astrophysical applications are traditionally determined on the ba...
Nuclear reaction rates determine the abundances of isotopes in stellar burning pro-cesses. A multitu...
Theoretical reaction rates in the temperature range 0.01 x 10(9) less than or equal to T(K) less tha...
The majority of nuclear reactions in astrophysics involve unstable nuclei which are not fully access...
STARLIB is a next-generation, all-purpose nuclear reaction-rate library. For the first time, this li...
The majority of nuclear reactions in astrophysics involve unstable nuclei which are not fully access...
“Published under licence in Journal of Physics: Conference Series by IOP Publishing Ltd. Content fro...
The first part of the paper discusses nuclear properties relevant to predict compound reactions. The...
Nuclear reaction rates are quantities of fundamental importance in astrophysics. Substantial efforts...
Nuclear reaction rates are quantities of fundamental importance in astrophysics. Substantial efforts...
Nuclear reaction rates are obviously quantities of fundamental importance in nuclear astrophysics. I...
An update of a previous description of the BRUSLIB + NACRE package of nuclear data for astrophysics ...
An update of a previous description of the BRUSLIB + NACRE package of nuclear data for astrophysics ...
Modern computer technology has revolutionized theoretical calculations on stellar structure and stel...
In a previous publication (ATOMIC DATA AND NUCLEAR DATA TABLES 75, 1 (2000)), we gave seven-paramete...
Context. Nuclear reaction rates of astrophysical applications are traditionally determined on the ba...
Nuclear reaction rates determine the abundances of isotopes in stellar burning pro-cesses. A multitu...
Theoretical reaction rates in the temperature range 0.01 x 10(9) less than or equal to T(K) less tha...
The majority of nuclear reactions in astrophysics involve unstable nuclei which are not fully access...
STARLIB is a next-generation, all-purpose nuclear reaction-rate library. For the first time, this li...
The majority of nuclear reactions in astrophysics involve unstable nuclei which are not fully access...
“Published under licence in Journal of Physics: Conference Series by IOP Publishing Ltd. Content fro...
The first part of the paper discusses nuclear properties relevant to predict compound reactions. The...