Nucleosynthesis occurs in such diverse astrophysical phenomena as ordinary stars, like our own Sun, supernovae, novae, X-ray bursts, and the Big Bang. Large sets of nuclear reaction rates for hundreds of seed isotopes are utilized in simulations of these nucleosynthesis processes. A cross-platform, Java software package called REACLIB aLIVe! has been developed with intuitive graphical interfaces and interactive controls to produce custom one-dimensional plots of reaction rates. The points used for these plots are calculated from exponential fits whose parameters, along with other quantities, make up the REACLIB Nuclear Reaction Rate Library. The software offers nuclear astrophysicists the capability to rapidly display any of 8000 nuclear re...
Nuclear reaction rates are obviously quantities of fundamental importance in nuclear astrophysics. I...
A selected overview of stellar effects and reaction mechanisms with relevance to the prediction of a...
Almost all of the elements heavier than hydrogen that are present in our solar system were produced ...
Nucleosynthesis occurs in such diverse astrophysical phenomena as ordinary stars, like our own Sun, ...
We present results from the JINA REACLIB project, an ongoing effort to maintain a current and accura...
Simulations of nucleosynthesis in astrophysical environments are at the intersection of nuclear phys...
STARLIB is a next-generation, all-purpose nuclear reaction-rate library. For the first time, this li...
Nuclear processes drive stellar evolution and so nuclear physics, stellar models and observations to...
Aims. We present r-Java 2.0, a nucleosynthesis code for open use that performs r-process calculation...
Nuclear reaction rates are quantities of fundamental importance in astrophysics. Substantial efforts...
The majority of nuclear reactions in astrophysics involve unstable nuclei which are not fully access...
Aims. We present r-Java 2.0, a nucleosynthesis code for open use that performs r-process calculation...
Nuclear reaction rates are quantities of fundamental importance in astrophysics. Substantial efforts...
We present r-Java, an r-process code for open use that performs r-process nucleosynthesis calculatio...
Nuclear astrophysics aims to measure nuclear-reaction cross sections of astrophysical interest to be...
Nuclear reaction rates are obviously quantities of fundamental importance in nuclear astrophysics. I...
A selected overview of stellar effects and reaction mechanisms with relevance to the prediction of a...
Almost all of the elements heavier than hydrogen that are present in our solar system were produced ...
Nucleosynthesis occurs in such diverse astrophysical phenomena as ordinary stars, like our own Sun, ...
We present results from the JINA REACLIB project, an ongoing effort to maintain a current and accura...
Simulations of nucleosynthesis in astrophysical environments are at the intersection of nuclear phys...
STARLIB is a next-generation, all-purpose nuclear reaction-rate library. For the first time, this li...
Nuclear processes drive stellar evolution and so nuclear physics, stellar models and observations to...
Aims. We present r-Java 2.0, a nucleosynthesis code for open use that performs r-process calculation...
Nuclear reaction rates are quantities of fundamental importance in astrophysics. Substantial efforts...
The majority of nuclear reactions in astrophysics involve unstable nuclei which are not fully access...
Aims. We present r-Java 2.0, a nucleosynthesis code for open use that performs r-process calculation...
Nuclear reaction rates are quantities of fundamental importance in astrophysics. Substantial efforts...
We present r-Java, an r-process code for open use that performs r-process nucleosynthesis calculatio...
Nuclear astrophysics aims to measure nuclear-reaction cross sections of astrophysical interest to be...
Nuclear reaction rates are obviously quantities of fundamental importance in nuclear astrophysics. I...
A selected overview of stellar effects and reaction mechanisms with relevance to the prediction of a...
Almost all of the elements heavier than hydrogen that are present in our solar system were produced ...