0000000001034720

AUTHOR

T. M. Sprouse

showing 3 related works from this author

Horizons: Nuclear Astrophysics in the 2020s and Beyond

2022

Nuclear astrophysics is a field at the intersection of nuclear physics and astrophysics, which seeks to understand the nuclear engines of astronomical objects and the origin of the chemical elements. This white paper summarizes progress and status of the field, the new open questions that have emerged, and the tremendous scientific opportunities that have opened up with major advances in capabilities across an ever growing number of disciplines and subfields that need to be integrated.We take a holistic view of the field discussing the unique challenges and opportunities in nuclear astrophysics in regards to science, diversity, education, and the interdisciplinarity and breadth of the field…

High Energy Astrophysical Phenomena (astro-ph.HE)Nuclear and High Energy PhysicsNuclear TheoryComputingMethodologies_SIMULATIONANDMODELINGastrofysiikkaStarke Wechselwirkung und exotische Kerne – Abteilung BlaumWhite PaperFOS: Physical sciencesReviewtutkimustoimintatutkimuskohteet530Nuclear Theory (nucl-th)Astrophysics - Solar and Stellar AstrophysicsNuclear astrophysicsddc:530Nuclear Experiment (nucl-ex)ydinfysiikkaAstrophysics - High Energy Astrophysical PhenomenaNuclear ExperimenttiedeyhteisötSolar and Stellar Astrophysics (astro-ph.SR)
researchProduct

FRIB and the GW170817 Kilonova

2018

In July 2018 an FRIB Theory Alliance program was held on the implications of GW170817 and its associated kilonova for r-process nucleosynthesis. Topics of discussion included the astrophysical and nuclear physics uncertainties in the interpretation of the GW170817 kilonova, what we can learn about the astrophysical site or sites of the r process from this event, and the advances in nuclear experiment and theory most crucial to pursue in light of the new data. Here we compile a selection of scientific contributions to the workshop, broadly representative of progress in r-process studies since the GW170817 event.

High Energy Astrophysical Phenomena (astro-ph.HE)Nuclear Theory (nucl-th)Astrophysics - Solar and Stellar AstrophysicsNuclear TheoryFOS: Physical sciencesAstrophysics - High Energy Astrophysical PhenomenaSolar and Stellar Astrophysics (astro-ph.SR)
researchProduct

FRIB and the GW170817 Kilonova

2018

In July 2018 an FRIB Theory Alliance program was held on the implications of GW170817 and its associated kilonova for r-process nucleosynthesis. Topics of discussion included the astrophysical and nuclear physics uncertainties in the interpretation of the GW170817 kilonova, what we can learn about the astrophysical site or sites of the r process from this event, and the advances in nuclear experiment and theory most crucial to pursue in light of the new data. Here we compile a selection of scientific contributions to the workshop, broadly representative of progress in r-process studies since the GW170817 event.

High Energy Astrophysical Phenomena (astro-ph.HE)Nuclear Theory (nucl-th)FOS: Physical sciencesSolar and Stellar Astrophysics (astro-ph.SR)
researchProduct