NSF award 2509269 · Princeton University

Collaborative Research: A New Model of AGN Accretion Disks Dominated by Strong Magnetic Fields

Final report due

29 December 2028

in 803 days · The award ends on 31 August 2028.

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award ending 2028-08-31 · Research.gov
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Extension request17 Jul 2028in 638 days
award ending 2028-08-31 · Research.gov
PAPPG 24-1: “at least 45 days prior to the end date”
No-cost extension notice21 Aug 2028in 673 days
award ending 2028-08-31 · Research.gov
PAPPG 24-1: “at least ten calendar days prior to the end date”
Final report due29 Dec 2028in 803 days
award ending 2028-08-31 · Research.gov
PAPPG 24-1: “no later than 120-days following the end date of the award”
Project outcomes report due29 Dec 2028in 803 days
award ending 2028-08-31 · Research.gov
PAPPG 24-1: “no later than 120 days following the end date”
Award is closed out29 Dec 2028in 803 days
award ending 2028-08-31 · Research.gov
PAPPG 24-1: “financially closed out 120 days after their expiration date”

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NSF lists this award's end date as 31 August 2028.
NSF rules say the final report is due no later than 120 days after that.
So the final report is due by 29 December 2028.

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Award card

Award number: 2509269
Period of support: 1 Sep 2025 – 31 Aug 2028
Amount: $277,023
Awardee: Princeton University, Princeton, NJ
Program: EXTRAGALACTIC ASTRON & COSMOLO
Directorate: MPS

Abstract

Black holes swallowing gas produce the brightest, most powerful sources of radiation in the Universe. That energy can dramatically change everything around the black hole, fundamentally reshaping how stars and galaxies form. This project will develop a new generation of models for gas inflow into black holes, with strong magnetic fields that can completely change how these systems behave. Black holes are one of the…

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