ROSES-25 D.4 Theoretical and Computational Astrophysics Networks. NoIs due 15 October 2026
3 September 2026
The ROSES-25 program element D.4 Theoretical and Computational Astrophysics Networks (TCAN) supports coordinated efforts in fundamental theory and computational techniques to make advances in astrophysics that extend beyond the scope of individual investigator projects. The goals of the TCAN program include strengthening theoretical and computational astrophysics in the United States by uniting researchers in collaborative networks that cross institutional and geographical boundaries and advance the training of the future workforce of theoretical and computational scientists.
For this program element, the TCAN program focuses its scope on grand challenges in Time Domain Multi-Messenger Astrophysics, and solicits proposals aimed at developing integrated theoretical and computational tools for modeling multi-messenger phenomena through collaborative networks.
It is expected that the proposing networks will include participants with complementary expertise in different topical areas, such as astrophysics, gravitational physics, nuclear physics, plasma physics, computational mathematics, numerical methods and algorithms, software engineering, and/or space- and ground-based observational astronomy. Multi-disciplinary collaboration spanning various sectors (e.g., academic, national laboratory, and private organizations, among others) are encouraged.
ROSES-2025 Amendment 70 releases D.4 TCAN as a new opportunity in ROSES-25. Mandatory Notices of Intent are due by 15 October 2026, and proposals are due by 3 December 2026.
Please direct questions concerning D.4 TCAN to Sanaz Vahidinia at Sanaz.Vahidinia@nasa.gov.
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Facts Only
* ROSES-25 program element D.4 is titled Theoretical and Computational Astrophysics Networks (TCAN).
* The program supports coordinated efforts in fundamental theory and computational techniques in astrophysics.
* The current focus is on Time Domain Multi-Messenger Astrophysics.
* Proposed networks must develop integrated theoretical and computational tools for modeling multi-messenger phenomena.
* Eligible participants include experts in astrophysics, gravitational physics, nuclear physics, plasma physics, computational mathematics, numerical methods, algorithms, software engineering, and observational astronomy.
* Collaboration may span academic, national laboratory, and private organizations.
* ROSES-2025 Amendment 70 established D.4 TCAN as a new opportunity.
* Notices of Intent are due by 15 October 2026.
* Proposals are due by 3 December 2026.
* Sanaz Vahidinia (Sanaz.Vahidinia@nasa.gov) is the point of contact for questions.
Executive Summary
The ROSES-25 program element D.4, Theoretical and Computational Astrophysics Networks (TCAN), is a funding opportunity designed to support coordinated, large-scale research efforts in fundamental theory and computational techniques. The initiative seeks to advance astrophysics beyond the capabilities of individual investigator projects by establishing collaborative networks that transcend institutional and geographical boundaries. A primary goal is the development of the future workforce for theoretical and computational sciences.
Current efforts are specifically targeted at "grand challenges" within Time Domain Multi-Messenger Astrophysics. This requires the integration of theoretical and computational tools to model multi-messenger phenomena. Successful proposals are expected to demonstrate multi-disciplinary collaboration, incorporating expertise from fields such as gravitational and nuclear physics, plasma physics, computational mathematics, software engineering, and observational astronomy across academic, national laboratory, and private sectors.
The application process requires a mandatory Notice of Intent by October 15, 2026, with full proposals due by December 3, 2026. Inquiries are directed to Sanaz Vahidinia.
Full Take
This announcement is a standard government solicitation for research funding, operating in SKEPTICAL MODE as a public administrative notice.
The strongest version of this narrative is a strategic investment in "big science." By shifting funding from individual investigators to "networks," the agency is acknowledging that modern astrophysics—specifically multi-messenger astronomy—has reached a level of complexity where no single institution or discipline holds the necessary toolkit. This is a transition toward a systems-engineering approach to basic science.
The root cause is the paradigm of "Interdisciplinary Synthesis." The unstated assumption is that the primary bottleneck in understanding the universe is no longer just data collection (observation), but the computational infrastructure and theoretical frameworks required to interpret that data. This echoes the historical shift toward "Big Science" seen in the Manhattan Project or the Large Hadron Collider, where the scale of the tool defines the scale of the discovery.
The implication is a centralization of research power. While "collaborative networks" sound democratic, they often create a hierarchy where a few lead institutions manage the distribution of resources and dictate the research agenda for smaller participants. The benefit is accelerated progress in high-energy physics; the cost may be a decrease in the "lone genius" or high-risk, idiosyncratic research that doesn't fit into a coordinated network.
Patterns detected: none
If this were an influence campaign, a bad actor would use this to signal a "technological breakthrough" to manipulate markets or project national scientific dominance without providing actual evidence of discovery. This content does not match that pattern; it is a procedural call for proposals.
Bridge Questions:
1. How does the shift toward network-based funding affect the autonomy of early-career researchers?
2. What happens to theoretical avenues that do not align with the "grand challenges" identified by the funding body?
3. To what extent does the inclusion of private organizations in these networks influence the direction of fundamental science?
