National Academies Press: OpenBook

Nuclear Physics: The Core of Matter, The Fuel of Stars (1999)

Chapter: Appendix: Accelerator Facilities for Nuclear Physics in the United States

« Previous: 8 Nuclear Physics and Society
Suggested Citation:"Appendix: Accelerator Facilities for Nuclear Physics in the United States." National Research Council. 1999. Nuclear Physics: The Core of Matter, The Fuel of Stars. Washington, DC: The National Academies Press. doi: 10.17226/6288.
×

Appendix
Accelerator Facilities for Nuclear Physics in the United States

Tables A.1 and A.2 summarize nuclear physics accelerator facilities currently in operation or under construction in the United States. In addition to the accelerator parameters and performance characteristics, the tables list the primary areas of research that each one addresses. Figure A.1 gives an overview of facilities and their geographical location.

The major new facilities of the nation's nuclear physics program are the Continuous Electron Beam Accelerator Facility (CEBAF) at the Thomas Jefferson National Accelerator Facility, which recently came into operation, and the Relativistic Heavy Ion Collider (RHIC) at Brookhaven National Laboratory, which is scheduled to begin operation in 1999. CEBAF (shown in Figure 7.1) is a superconducting, recirculating linac designed to deliver continuous electron beams of up to 200 µA of current, polarized and unpolarized, simultaneously to three experimental areas. The design energy is 4 GeV, but operational experience with the superconducting cavities indicates that an energy of up to 6 GeV will be possible.

Nearing completion, RHIC (shown in Figure A.2) is the first colliding-beam facility specifically designed to accommodate the requirements of heavy-ion physics at relativistic energies. RHIC will provide heavy-ion collisions for a range of ion species up to gold, with beam energies of 30 to 100 GeV/nucleon for each of the colliding beams.

In addition to these two large nuclear physics facilities, six medium-size user facilities supported by DOE and NSF address different key aspects of nuclear physics, indicated in Figure A.2.

The Bates Linear Accelerator Center at MIT provides high-quality electron

Suggested Citation:"Appendix: Accelerator Facilities for Nuclear Physics in the United States." National Research Council. 1999. Nuclear Physics: The Core of Matter, The Fuel of Stars. Washington, DC: The National Academies Press. doi: 10.17226/6288.
×

TABLE A.1 National User Facilities

 

Beam Characteristics

 

 

 

Facility

Species

Energies

Technology

Research Areas

Thomas Jefferson National Accelerator Facility (VA) Continuous Electron Beam Accelerator Facility (CEBAF)

Electrons

1-6 GeV

Superconducting accelerator Polarized-electron beams Three simultaneous target stations

Structure of hadrons Quark-gluon degrees of freedom in nuclei Electromagnetic response of nuclei

Brookhaven National Laboratory (NY)

Relativistic Heavy Ion Collider (RHIC)

Heavy ions, protons

2 × (30-100) GeV/u 2 × (30-250) GeV

Colliding beams Polarized-proton beams Superconducting magnets

Quark-gluon plasma Hot compressed nucleonic matter Spin physics

Massachusetts Institute of Technology Bates Linear Accelerator Center

Electrons

0.1-1 GeV

Polarized-electron beams Electron stretcher/storage ring Internal targets

Fundamental symmetries and interactions Structure of hadrons and nuclei Spin structure of nucleons and nuclei

Michigan State University National Superconducting Cyclotron Laboratory

Light to very heavy ions

10-200 MeV/u

Superconducting cyclotrons Superconducting magnets Radioactive beams

Nuclear structure with radioactive beams Liquid-gas phase transition Nuclear astrophysics

Indiana University Cyclotron Facility

Protons, light ions

100-500 MeV

Polarized, stored cooled beams Internal targets

Nucleon-nucleon/meson interactions Spin structure of nuclei Fundamental symmetries and chirality

Argonne National Laboratory (IL) Argonne Tandem Linac Accelerator System

Light to very heavy ions

0.3-20 MeV/u

Superconducting accelerator Selected radioactive beams

Nuclear structure at the limits Nuclear astrophysics with radioactive beams Ion trapping and fundamental symmetries

Oak Ridge National Laboratory (TN) Holifield Radioactive Ion Beam Facility

Light to heavy ions

0.1-12 MeV/u

Two-accelerator ISOL facility Radioactive beams

Nuclear structure with radioactive beams Nuclear astrophysics Decay studies far off stability

Lawrence Berkeley National Laboratory (CA) 88" Cyclotron

Protons, light to very heavy ions

1-55 MeV 1-35 MeV/u

ECR ion sources Rare-isotope beams

Nuclear structure at the limits Heavy-element research Atom trapping and fundamental symmetries

beams up to an energy of 1 GeV. The pulsed linac and the isochronous recirculator provide currents in excess of 80 µA at a duty-factor of up to 1 percent. The existing accelerator-recirculator system feeds the recently completed South Hall Ring, which will provide close to 100 percent-duty-factor beams. The 190 m-circumference ring will operate in the energy range up to 1 GeV at peak circulating currents of up to 80 mA, and extracted currents will be up to 50 µA.

Three superconducting cyclotrons have been built at the National Superconducting Cyclotron Laboratory of Michigan State University (MSU/NSCL). Two

Suggested Citation:"Appendix: Accelerator Facilities for Nuclear Physics in the United States." National Research Council. 1999. Nuclear Physics: The Core of Matter, The Fuel of Stars. Washington, DC: The National Academies Press. doi: 10.17226/6288.
×

of these, the K500 and the K1200, are currently being coupled in a program to upgrade the capabilities of the MSU system. The K500, the world's first superconducting cyclotron, operated from 1982 to 1988 in support of the nuclear physics program at MSU. The K1200 is the world's highest-energy (~ 10 GeV) continuous-wave (CW) cyclotron and has been used in support of the nuclear physics program since 1988. Both the K500 and the K1200 operate at 5T. The upgraded facility will provide intense, high-energy beams of heavy ions for in-flight fragmentation to produce intense secondary radioactive beams.

Suggested Citation:"Appendix: Accelerator Facilities for Nuclear Physics in the United States." National Research Council. 1999. Nuclear Physics: The Core of Matter, The Fuel of Stars. Washington, DC: The National Academies Press. doi: 10.17226/6288.
×

TABLE A.2 University Accelerators

 

Beam Characteristics

 

 

 

Facility

Species

Energies

Technology

Research Areas

Florida State University Tandem Lilac

Protons, light to medium heavy ions

2-10 MeV/u

Superconducting cavities Polarized lithium beam

Nuclear structure and decay Spin effects in nucleus-nucleus collisions

State University of New York at Stony Brook Tandem-Linac

Protons, light to medium heavy ions

2-10 MeV/u

Superconducting cavities

Nuclear structure Heavy-ion reactions Atom trapping and spectroscopy

University of Notre Dame (IN) Accelerator Facility

Protons, light to medium heavy ions

2-21 MeV 0.1-8 MeV/u

Radioactive beams Intense low-energy stable beams

Nuclear structure and reactions Fundamental symmetries Nuclear astrophysics

Texas A&M University Cyclotron Institute K500 Superconducting Cyclotron

Protons, light to heavy ions

2-70 MeV/u

Intermediate-energy heavy ions Selected radioactive beams

Nuclear structure and reaction dynamics Nuclear astrophysics with radioactive beams Fundamental symmetries

University of Washington Tandem Linac

Protons, light to medium heavy ions

2-16 MeV 2-10 MeV/u

Superconducting cavities Terminal ion source

Nuclear reactions with heavy ions Tests of fundamental symmetries

Triangle Universities Nuclear Laboratory (NC) Tandem Accelerator

Protons, light ions, neutrons, photons

1-10 MeV/u

High-resolution light-ion beams Polarized beams

Fundamental symmetries Inter-nucleon reactions and light nuclei Nuclear astrophysics

University of Wisconsin Tandem Accelerator

Protons, light ions

2-12 MeV 1-7 MeV/u

Polarized beams

Few-body systems Fundamental symmetries Spin degrees of freedom in nuclei

Yale University (CT), Wright Nuclear Structure Laboratory Tandem Accelerator

Protons, light to heavy ions

1-40 MeV 1-15 MeV/u

High-resolution beams

Nuclear structure Heavy-ion reactions Nuclear astrophysics

The Indiana University Cyclotron Facility is active in areas of beam-cooling technologies and polarized proton beams. Two cyclotrons provide protons with energies up to 200 MeV for direct beams, as well as serving as the injector complex for the Cooler Ring. This ring can accelerate protons to an energy of 500 MeV. In addition, the Cooler Ring has a state-of-the-art electron-cooling system capable of providing high-resolution, very dense beams. A new synchrotron injector into the Cooler was recently completed, providing a two-orders-of-magnitude increase in beam intensity. Distinguishing characteristics of the facility include polarized beams in all machines and internal polarized gas-jet targets in the cooler.

Suggested Citation:"Appendix: Accelerator Facilities for Nuclear Physics in the United States." National Research Council. 1999. Nuclear Physics: The Core of Matter, The Fuel of Stars. Washington, DC: The National Academies Press. doi: 10.17226/6288.
×

ATLAS at Argonne National Laboratory consists of a superconducting linear accelerator, which is injected by either a 9-MV tandem Van de Graaff or a new positive-ion injector (PII) consisting of two ECR ion sources and a superconducting injector linac of novel design. Using the PII, ATLAS routinely accelerates intense beams up to uranium with energies above the Coulomb barriers and with excellent beam properties. The accelerator has a 100 percent duty cycle, can provide very short beam pulses (<150 psec), and is ideal for high-resolution heavy-ion nuclear physics research where nuclear structure effects are particularly important.

The Holifield Radioactive Ion Beam Facility (HRIBF) was recently brought

Suggested Citation:"Appendix: Accelerator Facilities for Nuclear Physics in the United States." National Research Council. 1999. Nuclear Physics: The Core of Matter, The Fuel of Stars. Washington, DC: The National Academies Press. doi: 10.17226/6288.
×

FIGURE A.1

Illustration and geographical distribution of nuclear physics laboratories in the United States. Shown are major national user facilities, as well as the smaller, dedicated university laboratories that, together and in a synergistic relationship, cover the broad range of science that is described.

Suggested Citation:"Appendix: Accelerator Facilities for Nuclear Physics in the United States." National Research Council. 1999. Nuclear Physics: The Core of Matter, The Fuel of Stars. Washington, DC: The National Academies Press. doi: 10.17226/6288.
×
Suggested Citation:"Appendix: Accelerator Facilities for Nuclear Physics in the United States." National Research Council. 1999. Nuclear Physics: The Core of Matter, The Fuel of Stars. Washington, DC: The National Academies Press. doi: 10.17226/6288.
×

FIGURE A.2

Aerial view of the Relativistic Heavy Ion Collider (RHIC) accelerator complex at Brookhaven National Laboratory on Long Island. The facility will generate two counter-circulating, high-energy beams of heavy (for example, gold) nuclei; these beams will intersect and collide in six interaction regions located uniformly around the rings. The insert shows a recent photo of the tunnel that houses the accelerator, with an array of powerful superconducting magnets needed to bend the high-energy beams. (Courtesy RHIC.)

Suggested Citation:"Appendix: Accelerator Facilities for Nuclear Physics in the United States." National Research Council. 1999. Nuclear Physics: The Core of Matter, The Fuel of Stars. Washington, DC: The National Academies Press. doi: 10.17226/6288.
×

into operation at Oak Ridge National Laboratory to permit research with precisely controlled beams of radioactive nuclei generated by the ISOL (isotope separator online) technique. Light ions (protons, deuterons, and others) accelerated by the Oak Ridge Isochronous Cyclotron strike an isotope-production target. Radioactive atoms produced in the target are extracted, ionized, mass selected, charge exchanged, preaccelerated, and injected into a 25-MV electrostatic tandem for acceleration to final energies.

The 88'' Cyclotron at Lawrence Berkeley National Laboratory is a variable-energy isochronous cyclotron with spiral-sector focusing. A new ECR source, operating at 14 GHz, and producing high intensities of highly charged ions has revolutionized the acceleration of heavy nuclei. The 88" Cyclotron now provides ion beams of energies up to and above the Coulomb barrier for medium-mass nuclei, as well as lighter ion beams with energies up to 35 MeV/nucleon.

On a considerably smaller scale, university accelerators serve the important function of providing specialized capabilities that cannot be met by the national user facilities. Examples of problems requiring lower beam energies and thus smaller accelerators are studies of fundamental symmetries in light nuclei, nuclear structure far from stability, reactions near the Coulomb barrier, or the study of nuclear reactions that are relevant to astrophysics.

At present, eight small accelerators (also shown in Figure A.1) are supported by NSF and DOE. These are situated on university campuses and serve local faculty and students, but they also are often used by visitors who take advantage of their unique capabilities. In most cases, the capabilities of these machines result from intensive, sometimes even speculative, development work on new instrumentation, such as novel detectors or ion sources. The modest cost of accelerator operation and the availability of the accelerator over long periods of time permit developments that could not be carried out in a cost-effective way on large machines.

The accelerators at Florida State University, the State University of New York at Stony Brook, and the University of Washington consist of tandem electrostatic accelerators coupled to superconducting linear accelerators to augment their energy. At Florida State University, polarized Li ions are produced by laser pumping and are used to study spin effects in elastic and inelastic processes. New capabilities at Stony Brook include the development of a magneto-optical trap for production and trapping of short-lived radioactive nuclei. The accelerator at the University of Washington is equipped with a new ion source in the tandem terminal to provide the intense beams of alpha particles required for weak interaction studies.

The early work on production of radioactive beams at the University of Notre Dame led to systematic studies with 8Li of importance to cosmology. At Texas A&M University, a new beam-analysis system and spectrometer coupled to the K500 Superconducting Cyclotron provides radioactive-beam capabilities for studies of exotic nuclei and astrophysics. The availability of polarized beams

Suggested Citation:"Appendix: Accelerator Facilities for Nuclear Physics in the United States." National Research Council. 1999. Nuclear Physics: The Core of Matter, The Fuel of Stars. Washington, DC: The National Academies Press. doi: 10.17226/6288.
×

of protons and deuterons at the Triangle Universities Nuclear Laboratory (TUNL) in North Carolina and at the University of Wisconsin is of importance to studies of few-body systems. The technical developments for polarized beams and targets are applied at the larger facilities in a symbiotic relationship between small university accelerators and the large national and international facilities. The large ESTU tandem accelerator at Yale University, which has been used to accelerate heavy ions of mass up to gold, is being augmented with a mass-separator facility in the terminal of the machine for use primarily in the nuclear-structure and nuclear-astrophysics programs.

Suggested Citation:"Appendix: Accelerator Facilities for Nuclear Physics in the United States." National Research Council. 1999. Nuclear Physics: The Core of Matter, The Fuel of Stars. Washington, DC: The National Academies Press. doi: 10.17226/6288.
×
Page 197
Suggested Citation:"Appendix: Accelerator Facilities for Nuclear Physics in the United States." National Research Council. 1999. Nuclear Physics: The Core of Matter, The Fuel of Stars. Washington, DC: The National Academies Press. doi: 10.17226/6288.
×
Page 198
Suggested Citation:"Appendix: Accelerator Facilities for Nuclear Physics in the United States." National Research Council. 1999. Nuclear Physics: The Core of Matter, The Fuel of Stars. Washington, DC: The National Academies Press. doi: 10.17226/6288.
×
Page 199
Suggested Citation:"Appendix: Accelerator Facilities for Nuclear Physics in the United States." National Research Council. 1999. Nuclear Physics: The Core of Matter, The Fuel of Stars. Washington, DC: The National Academies Press. doi: 10.17226/6288.
×
Page 200
Suggested Citation:"Appendix: Accelerator Facilities for Nuclear Physics in the United States." National Research Council. 1999. Nuclear Physics: The Core of Matter, The Fuel of Stars. Washington, DC: The National Academies Press. doi: 10.17226/6288.
×
Page 201
Suggested Citation:"Appendix: Accelerator Facilities for Nuclear Physics in the United States." National Research Council. 1999. Nuclear Physics: The Core of Matter, The Fuel of Stars. Washington, DC: The National Academies Press. doi: 10.17226/6288.
×
Page 202
Suggested Citation:"Appendix: Accelerator Facilities for Nuclear Physics in the United States." National Research Council. 1999. Nuclear Physics: The Core of Matter, The Fuel of Stars. Washington, DC: The National Academies Press. doi: 10.17226/6288.
×
Page 203
Suggested Citation:"Appendix: Accelerator Facilities for Nuclear Physics in the United States." National Research Council. 1999. Nuclear Physics: The Core of Matter, The Fuel of Stars. Washington, DC: The National Academies Press. doi: 10.17226/6288.
×
Page 204
Suggested Citation:"Appendix: Accelerator Facilities for Nuclear Physics in the United States." National Research Council. 1999. Nuclear Physics: The Core of Matter, The Fuel of Stars. Washington, DC: The National Academies Press. doi: 10.17226/6288.
×
Page 205
Suggested Citation:"Appendix: Accelerator Facilities for Nuclear Physics in the United States." National Research Council. 1999. Nuclear Physics: The Core of Matter, The Fuel of Stars. Washington, DC: The National Academies Press. doi: 10.17226/6288.
×
Page 206
Nuclear Physics: The Core of Matter, The Fuel of Stars Get This Book
×
Buy Paperback | $60.00 Buy Ebook | $48.99
MyNAP members save 10% online.
Login or Register to save!
Download Free PDF

Dramatic progress has been made in all branches of physics since the National Research Council's 1986 decadal survey of the field. The Physics in a New Era series explores these advances and looks ahead to future goals. The series includes assessments of the major subfields and reports on several smaller subfields, and preparation has begun on an overview volume on the unity of physics, its relationships to other fields, and its contributions to national needs.

Nuclear Physics is the latest volume of the series. The book describes current activity in understanding nuclear structure and symmetries, the behavior of matter at extreme densities, the role of nuclear physics in astrophysics and cosmology, and the instrumentation and facilities used by the field. It makes recommendations on the resources needed for experimental and theoretical advances in the coming decade.

  1. ×

    Welcome to OpenBook!

    You're looking at OpenBook, NAP.edu's online reading room since 1999. Based on feedback from you, our users, we've made some improvements that make it easier than ever to read thousands of publications on our website.

    Do you want to take a quick tour of the OpenBook's features?

    No Thanks Take a Tour »
  2. ×

    Show this book's table of contents, where you can jump to any chapter by name.

    « Back Next »
  3. ×

    ...or use these buttons to go back to the previous chapter or skip to the next one.

    « Back Next »
  4. ×

    Jump up to the previous page or down to the next one. Also, you can type in a page number and press Enter to go directly to that page in the book.

    « Back Next »
  5. ×

    Switch between the Original Pages, where you can read the report as it appeared in print, and Text Pages for the web version, where you can highlight and search the text.

    « Back Next »
  6. ×

    To search the entire text of this book, type in your search term here and press Enter.

    « Back Next »
  7. ×

    Share a link to this book page on your preferred social network or via email.

    « Back Next »
  8. ×

    View our suggested citation for this chapter.

    « Back Next »
  9. ×

    Ready to take your reading offline? Click here to buy this book in print or download it as a free PDF, if available.

    « Back Next »
Stay Connected!