Opportunity Information: Apply for PD 11 1252
Apply for PD 11 1252
- The National Science Foundation in the science and technology and other research and development sector is offering a public funding opportunity titled "Gravitational Theory" and is now available to receive applicants.
- Interested and eligible applicants and submit their applications by referencing the CFDA number(s): 47.049 Mathematical and Physical Sciences.
- This funding opportunity was created on Sep 19, 2013 and posted on May 13, 2011.
- Applicants must submit their applications by Archived. Replaced by PD 13 1252.. (Agency may still review applications by suitable applicants for the remaining/unused allocated funding in 2026.)
- Eligible applicants include: Unrestricted (i.e., open to any type of entity above), subject to any clarification in text field entitled Additional Information on Eligibility.
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Opportunity Summary:
The National Science Foundation (NSF) Gravitational Theory program (Funding Opportunity Number PD 11 1252) was a discretionary grant opportunity in the Mathematical and Physical Sciences area (CFDA 47.049) focused on advancing fundamental research in gravity. Its core purpose was to support work in both classical and quantum gravity theory, with particular emphasis on problems where gravity is strongest or most complex, such as strong-field regimes near compact objects and the theoretical foundations needed to understand gravitational waves and their sources. A key theme of the program was the bridge between gravitation and quantum mechanics, meaning proposals could address the conceptual and mathematical tensions between general relativity and quantum theory, as well as develop frameworks that help connect them.
The scope of supported research was broad and included theoretical, computational, and in some cases experimentally connected efforts. The program encouraged the development of new approaches, methods, and models that probe the fundamental laws of physics and the behavior of physical systems governed by gravity. Typical activities included formulating clear, quantitative hypotheses; analyzing those hypotheses using analytic techniques and numerical or computational tools; and, where applicable, helping interpret experimental or observational results. The mention of gravitational wave source simulations highlights interest in the modeling work needed to predict signals from events like black hole or neutron star mergers, which in turn helps connect theory to data analysis and observation.
Another defining feature of the program was its interdisciplinary character. NSF noted that a considerable number of awards in this area involved crossing traditional boundaries, which in practice can mean links to astrophysics, cosmology, particle physics, mathematics, computational science, or even instrumentation and data methods when theory is being tied to measurements. In addition to direct research grants, the program also supported infrastructure-like activities that strengthen the research community and accelerate progress, such as short- and long-term visitor programs, workshops, and research centers. These activities were intended to bring together external scientists from universities, national laboratories, and industry, and to provide meaningful participation opportunities for graduate students and postdoctoral researchers.
Administratively, this opportunity was posted May 13, 2011, and used a grant funding instrument under the Science and Technology and other Research and Development activity category. The original full proposal target date was October 26, 2011, with the last Wednesday in October identified as an annual target thereafter. The listing indicates no cost sharing or matching requirement and eligibility was described as unrestricted (open to any type of entity), subject to any clarifications in the official text. The opportunity is now archived and was replaced by PD 13 1252, with an archive date of September 19, 2013. The record also lists expected awards and estimated total funding as 0, which is best read as the listing not specifying amounts in this snapshot rather than as a definitive statement about actual NSF funding levels. For access issues, the notice directed applicants to NSF Grants.gov support via grantsgovsupport@nsf.gov.
Frequently Asked Questions (FAQs) - NSF Gravitational Theory Program (PD 11 1252)
What is the NSF Gravitational Theory program (PD 11 1252)?
The NSF Gravitational Theory program (Funding Opportunity Number PD 11 1252) was a discretionary grant opportunity within NSF's Mathematical and Physical Sciences area (CFDA 47.049). It focused on advancing fundamental research in gravitational theory, including both classical and quantum approaches.
What kinds of research did the program aim to support?
The program aimed to support fundamental work in gravity theory, especially research that tackles situations where gravity is strongest or most complicated. This included strong-field regimes near compact objects and theoretical foundations relevant to understanding gravitational waves and their sources.
Did the program support both classical and quantum gravity?
Yes. A core purpose of the program was to support work in both classical gravity theory (including general relativity and related frameworks) and quantum gravity theory, including efforts that explore the relationship between gravitation and quantum mechanics.
What does "bridging gravitation and quantum mechanics" mean in this program's context?
A key theme was research addressing the conceptual and mathematical tensions between general relativity and quantum theory. Proposals could focus on developing frameworks, methods, or models that help connect or reconcile aspects of the two, or otherwise clarify their relationship.
Was the scope limited to purely theoretical work?
No. While the emphasis was on gravitational theory, the supported scope was described as broad and could include theoretical and computational research, and in some cases efforts that were experimentally connected (for example, theory work tied to interpreting observational or experimental results).
What types of activities were considered typical or encouraged?
Typical activities included formulating clear, quantitative hypotheses; analyzing them using analytic approaches and numerical or computational tools; and, where applicable, helping interpret experimental or observational outcomes.
Did the program include gravitational-wave-related research?
Yes. The opportunity specifically highlighted interest in theoretical foundations for understanding gravitational waves and their sources, including modeling and simulation of gravitational wave sources (such as events involving compact objects).
What is meant by "strong-field regimes near compact objects"?
In the program description, this phrase referred to physical settings where gravitational effects are extreme or highly non-linear, such as environments around compact objects (for example, black holes or neutron stars). The program emphasized theory relevant to these regimes.
Did NSF emphasize interdisciplinary work under this program?
Yes. NSF noted that many awards in this area crossed traditional boundaries. Interdisciplinary connections could include links to astrophysics, cosmology, particle physics, mathematics, computational science, or other areas (including instrumentation and data methods when theory is closely tied to measurements).
Besides research grants, what other kinds of support were included?
In addition to direct research awards, the program supported activities intended to strengthen the research community and accelerate progress. Examples listed included short- and long-term visitor programs, workshops, and research centers.
Who were these community and infrastructure activities intended to involve?
These activities were intended to bring together external scientists from universities, national laboratories, and industry. They also aimed to provide meaningful participation opportunities for graduate students and postdoctoral researchers.
What type of funding instrument was used?
The opportunity used a grant funding instrument.
What was the overall activity category for this opportunity?
The listing identified the activity category as "Science and Technology and other Research and Development."
When was the opportunity posted?
The opportunity was posted on May 13, 2011.
What was the full proposal target date?
The original full proposal target date was October 26, 2011.
Was this an annual opportunity?
The notice indicated an annual target date pattern: the last Wednesday in October was identified as the annual target date after the initial 2011 target date.
Was cost sharing or matching required?
No. The listing indicated there was no cost sharing or matching requirement.
Who was eligible to apply?
Eligibility was described as unrestricted (open to any type of entity), subject to any clarifications provided in the official opportunity text.
Is this funding opportunity still open?
No. This opportunity is archived. It was replaced by PD 13 1252, and the archive date for PD 11 1252 was September 19, 2013.
What opportunity replaced PD 11 1252?
The archived opportunity indicates it was replaced by PD 13 1252.
The listing shows expected awards and estimated total funding as 0. Does that mean there was no funding?
Not necessarily. Based on the listing notes, the "0" values are best interpreted as the snapshot not specifying amounts, rather than as a definitive statement about actual NSF funding levels.
Where were applicants directed for access or submission support?
For access issues, the notice directed applicants to NSF Grants.gov support via the email address grantsgovsupport@nsf.gov.
Which NSF area and CFDA number were associated with this program?
The opportunity was in the Mathematical and Physical Sciences area and was associated with CFDA 47.049.
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