Chapter 6 - Mathematical and Physical Sciences


Programs in the Mathematical and Physical Sciences (MPS) Directorate are designed with the following goals:

The operational activities of MPS are organized around divisional and disciplinary lines that cover astronomical sciences, chemistry, materials research, mathematical sciences, and physics. However, MPS recognizes that "Nature knows no boundaries." Therefore, MPS emphasizes communication among the divisions and across directorate boundaries to ensure effective support of research and education projects in emerging fields that cut across those lines. Potential proposers can gain information and access to a full range of opportunities that are open to them by contacting the division and/or program in MPS that is related to their work.

MPS is an active participant in a number of inter- and intraagency programs that focus on interdisciplinary areas of importance to the national interest. These include advanced materials and processing; biotechnology; environment and global change; high performance computing and communications; advanced manufacturing technologies; civil infrastructure systems; and science, mathematics, engineering, and technology education. Researchers and educators interested in exploring opportunities in these areas should contact the program most closely related to their own interests to learn more about submitting proposals.

Multidisciplinary Activities

Established in 1995, the Office of Multidisciplinary Activities (OMA) supports activities that cut across the MPS disciplines and/or bridge these disciplines with other areas of science from other NSF directorates. OMA works to intensify the directorate's support for multidisciplinary research and human infrastructure and takes advantage of new opportunities. Each year a few areas of emphasis will be targeted for high priority funding consideration. Current examples are optical science and engineering, environmental science and technology, and the Grant Opportunities for Academic Liaison with Industry (GOALI) initiative.

For More Information

For further information, contact the Head, Office of Multidisciplinary Activities, Mathematical and Physical Sciences Directorate, National Science Foundation, 4201 Wilson Boulevard, Room 1005, Arlington, Virginia 22230, (703) 306-1800.


Astronomical Sciences

The overall objective of the Astronomical Sciences (AST) Division is to increase our knowledge of the universe. Support is given for research aimed at determining the composition, structure, and evolution of planets, stars, and galaxies, including our Sun and the Milky Way.

AST supports the development and operation of three National Astronomy Centers. These centers are equipped with radio, optical, infrared, and special telescopes that are made available to the scientific community on a competitive basis. Resident staff at the centers give technical assistance to visiting scientists, conduct studies of their own, and develop advanced instrumentation. The division also supports the Center for Particle Astrophysics, an NSF Science and Technology (S&T) Center. The S&T centers are designed to meet national needs for research in specific areas of science that require facilities, equipment, staffing, and operational support that could not appropriately be offered by a single institution.

Astronomy Projects

The Astronomy and Astrophysics Research Projects Program provides a broad base for support of fundamental research aimed at an understanding of the states of matter and physical processes in the solar system and our Milky Way galaxy, and the origin and evolution of the present universe. Proposals to support searches for extraterrestrial intelligence are not funded in the program.

Areas of Research

Target Dates

Proposals for research that will take place in fiscal year 1996 (after October 1, 1995) had the following target dates:

Target dates for fiscal year 1997 will be announced in the NSF Bulletin, a monthly publication produced by the Office of Legislative and Public Affairs (OLPA).

The Advanced Technologies and Instrumentation Program does not have a target date. Proposers are urged to contact a program officer in advance of submitting a proposal to any of the Astronomy programs.

For More Information

For further information, contact the Division of Astronomical Sciences, National Science Foundation, 4201 Wilson Boulevard, Room 1045, Arlington, Virginia 22230, (703) 306- 1820.

National Astronomy and Ionosphere Center

NSF supports the National Astronomy and Ionosphere Center (NAIC), a visitor-oriented national research center devoted to researching radio and radar astronomy and atmospheric sciences. NAIC's headquarters are in Ithaca, New York, where it is operated and managed for NSF by Cornell University, and its principal observing facilities are 19 kilometers south of the city of Arecibo, Puerto Rico.

NAIC provides telescope users with a wide range of research and observing instrumentation including receivers, transmitters, movable line feeds, and digital data acquisition and processing equipment. The center has a permanent staff of scientists, engineers, and technicians who are available to help visiting investigators with their observing programs.

NAIC's principal astronomical research instrument is a 305-meter fixed spherical radio/radar telescope--the world's largest single radio reflector. Its frequency capabilities range from 50 megahertz to 5 gigahertz. Transmitters include an S-band (2,380-megahertz) radar system for planetary studies and a 430-megahertz radar system for aeronomy studies. A second observing site is located 9.6 kilometers from the main site and has a 30.5-meter steerable parabolic antenna that is paired with the main antenna to provide an effective interferometric S-band radar mapping system. This antenna pair is also available for radio astronomy interferometry at a wavelength of 12 centimeters.

The S-Band Planetary Radar System is now available for high-spatial resolution studies of stratospheric dynamics. A high-power ionospheric heating facility provides researchers with a unique capability to investigate nonlinear plasma phenomena in the ionosphere.

A major three-phase upgrade of NAIC's main antenna facility is presently underway. The first phase will be to erect a large reflecting screen around the periphery of the 305-meter reflector to reduce the effect of scattered ground radiation on the observations. The second phase involves the installation of a pair of wide-band aberration-correcting reflectors to replace the line feeds above 250 megahertz. The final phase involves doubling the power of the S-band radar system. The upgrade is expected to be completed in 1996.

Eligibility

NAIC facilities and instrumentation are available--on a competitive basis--to qualified scientists from all over the world. Telescope time is assigned after judgment of research proposals on the basis of scientific merit, the capability of the instruments to do the work, and the availability of the telescope during the requested time period.

For More Information

For further information, contact the Director, National Astronomy and Ionosphere Center, Cornell University, Ithaca, New York 14853.

Gemini 8-Meter Telescopes

The Gemini 8-Meter Telescopes Project is an international undertaking that will provide astronomers from the partnership countries--the United States, the United Kingdom, Canada, Chile, Brazil, and Argentina--with 8-meter telescopes in the Northern Hemisphere on Mauna Kea, Hawaii, and in the Southern Hemisphere on Cerro Pachon, in Chile. The Mauna Kea telescope will be infrared optimized and have superb image quality. The Chilean telescope will be its near twin. NSF acts as the executive agency for the partnership, and the Association of Universities for Research in Astronomy, Inc. (AURA)--a consortium of 20 major universities-- is managing the construction of the telescopes.

When operational, these telescopes will provide astronomers from the partnership countries with world-class observing facilities. Observing time will be assigned on the basis of scientific merit. Completion is expected in 1998 on Mauna Kea and in 2000 in Chile.

National Optical Astronomy Observatories

NSF supports the National Optical Astronomy Observatories (NOAO), a national center for research in ground-based optical and infrared astronomy and solar physics. Large optical telescopes, observing instrumentation, and data analysis equipment are made available to qualified visiting scientists. The NOAO staff of astronomers, engineers, and various support personnel are available to assist visiting scientists in their use of the facilities.

NOAO is operated and managed by AURA with headquarters located in Tucson, Arizona. NOAO has three observatories:

Eligibility

The NOAO facilities and instrumentation are available on a competitive basis to all qualified U.S. scientists and occasionally to foreign visitors. Telescope time is assigned on the basis of scientific merit, the capability of the instruments to do the work, and the availability of the telescope during the requested time period.

For More Information

For further information, contact the Director, National Optical Astronomy Observatories, P.O. Box 26732, Tucson, Arizona 85726.

National Radio Astronomy Observatory

NSF supports the National Radio Astronomy Observatory (NRAO), which makes radio astronomy facilities available to qualified scientists. The NRAO staff help visiting scientists use the large radio antennas, receivers, and other equipment needed to detect, measure, and identify radio waves from astronomical objects.

The headquarters of NRAO are located in Charlottesville, Virginia. Observing sites are located in Green Bank, West Virginia; Kitt Peak near Tucson, Arizona; a site 80 kilometers west of Socorro, New Mexico; and 10 sites in the continental United States and on the islands of Hawaii and St. Croix, on the latter of which individual antennas of the Very-Long-Baseline Array (VLBA) are located. NRAO is supported under the terms of a cooperative agreement between NSF and Associated Universities, Inc. (AUI), the organization responsible for the operation and management of the observatory.

Only one telescope is currently operated at the Green Bank site. It is a 43-meter aperture instrument that permits the study of spectral lines at centimeter wave lengths and is an integral part of the Very-Long-Baseline-Interferometer network. This network studies quasars and is involved in the high-resolution mapping of galactic objects based on simultaneous observations by combinations of telescopes over transcontinental and intercontinental distances. Currently under construction at Green Bank is a 100-meter telescope that is expected to be fully operational in 1996, at which time the 43-meter telescope will be retired.

A 12-meter millimeter-wavelength telescope is located on Kitt Peak to take advantage of the high altitude and dry climate necessary for short radio wavelengths. This telescope is capable of both continuum and spectral-line studies at wavelengths from 1 centimeter to as short as 1 millimeter.

The Very Large Array (VLA) telescope located west of Socorro, New Mexico, consists of 27 antennas and is available for use in an interferometric mode for aperture synthesis observations of faint radio sources. Both continuum and spectral-line observations at wavelengths of 1.3, 2, 6, and 20 centimeters can be made. The VLBA operates on the basis of the same physical principles as the VLA, but because of the much larger distances between antennas, the data are recorded at each site and compared later at Socorro, New Mexico. Because of its larger antenna separation, the VLBA is capable of resolving much smaller details in astronomical sources than is the VLA.

Eligibility

NRAO makes observing time on each instrument available for all qualified U.S. scientists and occasionally foreign visitors. Telescope time is assigned after judgment of research proposals on the basis of scientific merit, the capability of the instruments to do the work, and the availability of the telescope during the requested time period.

For More Information

For further information, contact the Director, National Radio Astronomy Observatory, Edgemont Road, Charlottesville, Virginia 22903.


Mathematical Sciences

The Division of Mathematical Sciences (DMS) supports a wide range of projects aimed at developing and exploring the properties and applications of mathematical structures. Most of these projects represent the research programs of single investigators or small groups of investigators working with graduate students and postdoctoral researchers. The Mathematical Sciences Infrastructure Program and the Special Projects Program handle a variety of different activities falling outside this mode.

The following activities cut across all disciplinary programs.

Target Dates

The division will continue to have two target dates for proposals submitted to the following programs.

October 11, 1995:
Algebra and Number Theory
Applied Mathematics (except Mathematical Biology)
Classical Analysis
Modern Analysis

November 9, 1995:
Computational Mathematics
Geometric Analysis
Statistics and Probability
Topology and Foundations
Mathematical Biology

The above dates do not apply to the activities of the Mathematical Sciences Infrastructure Program or the Special Projects Program, since most of these activities have specified target or deadline dates.

For More Information

The following program descriptions are necessarily brief. Program officers assign proposals to the appropriate program, and the programs cooperate in reviewing proposals of mutual interest.

For further information, contact the Division of Mathematical Sciences, National Science Foundation, 4201 Wilson Boulevard, Room 1025, Arlington, Virginia 22230, (703) 306- 1870.

  • Mathematical Sciences Infrastructure Program--Supports activities different from the usual research project such as the work of research institutes. Activities include

    1. Regional Conferences. Operated by the Conference Board of the Mathematical Sciences, these conferences feature a principal speaker who gives 10 one-hour talks on a particular subject during a week-long session. The deadline for proposal submission is April 1, 1996.

    2. Scientific Computing Research Environments in the Mathematical Sciences. Offers moderate grants for computing equipment that will benefit groups of researchers of outstanding quality who are highly productive but whose work has been seriously impeded by the lack of computing facilities. The deadline for proposal submission is the first Monday in December.

    3. Undergraduate Activities. Awards are made in conjunction with NSF-wide undergraduate efforts including Research Experiences for Undergraduates, cooperative activities with the Directorate for Education and Human Resources, and other related activities. See the chapters "Education and Human Resources" and "Other Research Activities" for more on NSF's undergraduate efforts.

    4. Mathematical Sciences Postdoctoral Research Fellowships. These fellowships will be awarded to between 30 and 40 new fellows in fiscal year 1996. Tenure provides a research instructorship option. These fellowships will be offered only to persons who

      1. are citizens, nationals, or lawfully admitted permanent resident aliens of the United States as of January 1, 1996;

      2. will have earned by the beginning of their fellowship tenure a doctoral degree in one of the mathematical sciences listed above or have had research training and experience equivalent to that represented by a Ph.D. in one of those fields;

      3. will have held the doctorate for no more than five years as of January 1, 1996; and

      4. will not previously have held any other NSF postdoctoral fellowship.

      Each applicant will be required to submit a research plan for the tenure period requested. The fellowships are not intended to support the preparation of prior research results for publication or the writing of textbooks. Anticipated deadline for submission is October 17, 1995.

    5. University/Industry Cooperative Research Programs in the Mathematical Sciences. Technical innovations flourish through a symbiotic relationship between academia and industry. The mathematical sciences provide a foundation for the scientific progress that generates technical innovations. It is important to provide more opportunities to conduct research and training in an industrial environment and for industrial scientists to return periodically to academia. In order to facilitate both research and training, the division provides Mathematical Sciences University/Industry Postdoctoral Research Fellowships, Mathematical Sciences University/Industry Senior Research Fellowships, and Industry-Based Graduate Research Assistantships and Cooperative Fellowships in the Mathematical Sciences.

      The deadline date for submission of proposals is expected to be November 13, 1995. Contact the division for further details.

      For More Information

      For further information, contact the Program Officer, Infrastructure Program, Mathematical Sciences Division, National Science Foundation, 4201 Wilson Boulevard, Room 1025, Arlington, Virginia 22230, (703) 306-1870.


    Physics

    The Physics (PHY) Division supports a wide range of programs, many of which for the most part, support individual investigators and small groups. The division operates a few large-scale facilities including the Cornell Electron Storage Ring (CESR), the Indiana University Cyclotron Facility (IUCF), and the Michigan State University National Superconducting Cyclotron Laboratory (NSCL). The PHY Division is supervising the construction of the Laser Interferometer Gravity Wave Observatory (LIGO) and also operates several smaller centers specializing in optical physics and various aspects of theoretical physics. Programs in Elementary Particle Physics and Nuclear Physics benefit greatly from the use of the large accelerator facilities that are constructed by the Department of Energy.

    The division, in cooperation with other MPS divisions, has begun small-scale initiatives in Biological Physics and in Particle Astrophysics.

    The research activities in PHY are inextricably linked to education. PHY supports about 1,000 graduate students who are fully engaged in research programs. Some of these programs also involve substantial numbers of undergraduate students, especially in the summer activities that are centered around the Research Experiences for Undergraduates Program. Research activities at four-year colleges are supported through the Research at Undergraduate Institutions Program. In addition, PHY's support of about 500 postdoctoral fellowships represents a significant training opportunity for young people.


    Chemistry

    The Chemistry (CHE) Division supports research activities and research infrastructure development in most of the principal subdisciplines of the chemical sciences. However, support is also available from the Divisions of Atmospheric Sciences (atmospheric chemistry); Molecular and Cellular Biosciences (biochemistry, biophysics); Chemical and Transport Systems (chemical engineering); Earth Sciences (geochemistry); and Materials Research (solid- state and polymer science).

    CHE supports research activities in emerging areas of national interest that cut across "traditional" subdisciplines. These areas include biological chemistry and biotechnology; the chemistry of advanced materials; environmental chemistry including research in greenhouse gas dynamics, an activity in the Environmentally Benign Chemical Synthesis and Processing Program (see program announcement NSF 92-13) that is jointly supported with the Engineering Directorate and the program in Environmental Geochemistry and Biogeochemistry (see program announcement NSF 95-49); high performance computing and communications; and advanced manufacturing including fundamental research underpinning chemical and pharmaceutical manufacture. Many of these activities are part of research programs that are coordinated through the National Science and Technology Council.

    Research in subdisciplinary areas is also a vital part of the Chemistry Research Project Support investment portfolio. These areas include the following:

    Much of the CHE Division's support for instrumentation and infrastructure is coordinated through the Office of Special Projects. Among these activities is a program of portable Postdoctoral Research Fellowships in Chemistry (see announcement NSF 94-82); a nationwide network of 60 sites for Research Experiences for Undergraduates (see program announcement NSF 93-112); Research Planning Grants for women and minorities; grants for Faculty Early Career Development; and occasional grants for special purposes in education, curriculum development, and graduate training.

    The Chemical Instrumentation and Facilities Program (see program announcement NSF 93- 94) supports infrastructure and instrumentation investments and provides funds to research institutions and consortia thereof for the purchase of multiuser instruments, for major instrumentation development and construction, and for the establishment and support of multiuser research facilities in the chemical sciences. This program is designed to support the following types of academic instrumentation needs:

    1. the purchase or upgrade of shared multiuser instruments (requires a one-third to one-half cost contribution from the grantee institution);
    2. the development plans for multiyear instrument centers in chemistry departments;
    3. instrumentation development including the construction of new prototype instruments; and
    4. the establishment and support of unique national and regional instrumentation facilities.

    This program focuses on shared instruments and facilities. Specialized equipment dedicated for use in particular chemistry research project or projects is funded as part of individual investigator awards, along with personnel and other direct project costs in programs in the CHE Division.


    Materials Research

    The Division of Materials Research (DMR) supports a wide range of programs that address fundamental phenomena in materials, materials synthesis and processing, materials structure and composition, materials properties and performance, and materials education. Formal research program areas are Metals, Ceramics, and Electronic Materials; Materials Theory; Condensed Matter Physics; Solid-State Chemistry and Polymers; and Materials Research Science and Engineering Centers. Investments in research infrastructure in materials science are also made through the National Facilities and Instrumentation Program.

    DMR plays a significant role in various interdisciplinary areas and programs, including the Advanced Materials and Processing Program (AMPP), High Performance Computing and Communications (HPCC), and Advanced Manufacturing Technology (AMT). DMR is also a participant in the Biotechnology, Civil Infrastructure Systems, and Environmental Research Initiatives. DMR's interest in HPCC ranges from computational approaches to real materials and processes to materials for new or advanced computational and communications devices and systems. In AMT, DMR's interests range from the understanding of the fundamental materials science basis of phenomena (e.g., lubrication, adhesion, joining, forming, packaging) that broadly crosscuts strategically significant industrial sectors--to materials for specific manufacturing processes and applications. In addition to the impact of materials on manufacturing, DMR also has an interest in the impact of advanced manufacturing technologies on materials research, such as the cost-effective enhancement of the instrumentation and equipment infrastructure for materials research. In Environmental Research, the division is concerned with the preparation of innovative materials, with new processes that are more environmentally benign, and with novel concepts for reuse or recycling of materials.

    DMR funding modes include support for individual investigators, groups, centers, national facilities, and instrumentation. Individual investigator proposals do not have to be confined or targeted to a specific program. Staff and management work to facilitate the co-funding of highly meritorious proposals across appropriate program, division, or directorate boundaries.

    For More Information

    For further information, contact the following National Facilities:

    Center for High-Resolution Neutron Scattering
    National Institute of Standards and Technology
    Reactor Radiation Division
    Gaithersburg, Maryland 20899
    (301) 975-6242

    Cornell High-Energy Synchrotron Source
    Wilson Laboratory
    Cornell University
    Ithaca, New York 14853
    (607) 255-7163

    National High Magnetic Field Laboratory [operated by Florida State University, the University of Florida, and Los Alamos National Laboratory]
    Florida State University
    1800 E. Paul Dirac Drive
    Tallahassee, Florida 32306-4005
    (904) 644-6257 or (904) 644-4068

    Synchrotron Radiation Center
    University of Wisconsin at Madison
    3731 Schneider Drive
    Stoughton, Wisconsin 53589-2200
    (608) 877-2000

    National Nanofabrication Facility
    Knight Laboratory
    Cornell University
    Ithaca, New York 14853
    (607) 255-2329
    FAX: (607) 255-8601

    Stanford Nanofabrication Facility
    CIS Building
    Stanford University
    Stanford, California 94305-4070
    (415) 725-6266 or (415) 725-NANO
    FAX: (415) 725-6278