Documents/DOEER/5: Explore Nuclear Matter — from Quarks to Stars/5.4: Nuclear Astrophysics

5.4: Nuclear Astrophysics

Investigate nuclear astrophysics.

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Nuclear physics research is essential if we are to solve important problems in astrophysics—the origin of the chemical elements, the behavior of neutron stars, core-collapse supernovae and the associated neutrino physics, and galactic and extragalactic gamma-ray sources. Almost all the chemical elements in the universe were generated by nuclear reactions in stars or in cataclysmic stellar explosions. Given the high temperatures and particle densities in stellar objects and explosions, the relevant nuclear reactions typically occur among radioactive or exotic nuclei. Our strategy includes the following emphases: • Using exotic beams of nuclei that have many neutrons, study interactions in nuclear matter like those that occur in neutron stars and those that create the nuclei of most atomic elements inside stars and supernovae. • Develop computer simulations for the behavior of supernovae, including core collapse and explosion, which incorporate the relevant nuclear reaction dynamics. • Develop a unique nextgeneration facility with forefront experimental instrumentation that will provide new species of exotic beams at unprecedented intensities to advance science at the intersection of nuclear physics and astronomy. This facility is similarly described in section 5.2.

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