Astrophysics at RIA (ARIA) Working Group

Journal Article · Wed Jul 12 00:00:00 EDT 2006 · AIP Conference Proceedings

DOI:https://doi.org/10.1063/1.2234461· OSTI ID:20877468

Smith, Michael S ^[1]; Schatz, Hendrik ^[2]; Timmes, Frank X ^[3]; Wiescher, Michael ^[4]; Greife, Uwe ^[5]

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1. Physics Division, Oak Ridge National Laboratory, Oak Ridge, TN, 37831-6354 (United States)
2. National Superconducting Cyclotron Laboratory, Michigan State Univ., 1 Cyclotron Laboratory, East Lansing, MI, 48824-1321 (United States)
3. Theoretical Division, MS B227, Los Alamos National Laboratory, Los Alamos, NM, 87545 (United States)
4. Dept. of Physics, Univ. Notre Dame, 225 Nieuwland Hall, Notre Dame, IN 46556-5670 (United States)
5. Dept. of Physics, Colorado School of Mines, 1523 Illinois St., Golden, CO, 80401 (United States)

The Astrophysics at RIA (ARIA) Working Group has been established to develop and promote the nuclear astrophysics research anticipated at the Rare Isotope Accelerator (RIA). RIA is a proposed next-generation nuclear science facility in the U.S. that will enable significant progress in studies of core collapse supernovae, thermonuclear supernovae, X-ray bursts, novae, and other astrophysical sites. Many of the topics addressed by the Working Group are relevant for the RIKEN RI Beam Factory, the planned GSI-Fair facility, and other advanced radioactive beam facilities.

• OSTI ID: 20877468
• Journal Information: AIP Conference Proceedings, Vol. 847, Issue 1; Conference: International symposium on origin of matter and evolution of galaxies 2005: New horizon of nuclear astrophysics and cosmology, Tokyo (Japan), 8-11 Nov 2005; Other Information: DOI: 10.1063/1.2234461; (c) 2006 American Institute of Physics; Country of input: International Atomic Energy Agency (IAEA); ISSN 0094-243X
• Country of Publication: United States
• Language: English

Related Subjects

72 PHYSICS OF ELEMENTARY PARTICLES AND FIELDS
ASTROPHYSICS
IPCR CYCLOTRON
ISOTOPES
NOVAE
NUCLEAR FACILITIES
RADIOACTIVE ION BEAMS
SUPERNOVAE