Award Abstract # 2020295
AI Institute: Planning: Physics of the Future

NSF Org: PHY
Division Of Physics
Recipient: CARNEGIE MELLON UNIVERSITY
Initial Amendment Date: August 25, 2020
Latest Amendment Date: August 5, 2022
Award Number: 2020295
Award Instrument: Standard Grant
Program Manager: Kaushik De
kde@nsf.gov
 (703)292-7480
PHY
 Division Of Physics
MPS
 Directorate for Mathematical and Physical Sciences
Start Date: September 1, 2020
End Date: November 30, 2023 (Estimated)
Total Intended Award Amount: $500,000.00
Total Awarded Amount to Date: $750,000.00
Funds Obligated to Date: FY 2020 = $500,000.00
FY 2022 = $250,000.00
History of Investigator:
  • Scott Dodelson (Principal Investigator)
    sdodelso@uchicago.edu
Recipient Sponsored Research Office: Carnegie-Mellon University
5000 FORBES AVE
PITTSBURGH
PA  US  15213-3815
(412)268-8746
Sponsor Congressional District: 12
Primary Place of Performance: Carnegie-Mellon University
5000 Forbes St
Pittsburgh
PA  US  15213-3890
Primary Place of Performance
Congressional District:
12
Unique Entity Identifier (UEI): U3NKNFLNQ613
Parent UEI: U3NKNFLNQ613
NSF Program(s): HEP-High Energy Physics,
OFFICE OF MULTIDISCIPLINARY AC,
AI Research Institutes
Primary Program Source: 01002223DB NSF RESEARCH & RELATED ACTIVIT
01002021DB NSF RESEARCH & RELATED ACTIVIT
Program Reference Code(s): 075Z, 7483
Program Element Code(s): 122100, 125300, 132Y00
Award Agency Code: 4900
Fund Agency Code: 4900
Assistance Listing Number(s): 47.049

ABSTRACT

Physics applications of Artificial Intelligence (AI) have led to some of the most exciting recent breakthroughs, from astrophysics to regulatory genomics and cellular imaging. Scientists at Carnegie-Mellon University (CMU) in Machine Learning, Statistics, and other departments actively collaborate with colleagues in the Department of Physics because of the opportunity for each field to spur development in the other. This award will allow planning of a joint Physics/AI Institute that will bring cutting edge methods from AI into a broad range of physics areas, propagate successful methods from one field of Physics to another, and facilitate back-transfer from the data-rich sub-fields of physics to AI development. This planning phase focuses on areas where CMU scientists are already leaders, with existing strong collaborations, and where rapid advances are being made: astrophysics, subatomic physics, and biophysics. AI has obvious benefits to society in general, so this project includes education, public outreach and promotion of diversity, empowering a wide range of audiences to use AI on a broad array of data.

Applying AI will lead to significant advances in the areas of dark energy and galaxy formation; new ways of extracting information about the Higgs bosons and anomalies in gluon physics; and enhanced understanding of biological networks and predictions for cancerous tissues. Benefits in the other direction are clear as well: physics provides complex use cases and profound problems that motivate AI researchers to advance foundational AI. Planning activities include weekly interdisciplinary, interactive seminars; a visitor program; topical conferences; planning conferences; a graduate student summer program; postdoc mentoring; and an extensive outreach program. Help in planning to scale up to the Institute level will come from partners at universities, national laboratories, and corporations, and by employing a consultant to survey and quantitatively assess the success of different programs.

This award reflects NSF's statutory mission and has been deemed worthy of support through evaluation using the Foundation's intellectual merit and broader impacts review criteria.

PUBLICATIONS PRODUCED AS A RESULT OF THIS RESEARCH

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(Showing: 1 - 10 of 49)
Abbott, T.M.C. and Aguena, M. and Alarcon, A. and Allam, S. and Alves, O. and Amon, A. and Andrade-Oliveira, F. and Annis, J. and Avila, S. and Bacon, D. and Baxter, E. and Bechtol, K. and Becker, M. R. and Bernstein, G. M. and Bhargava, S. and Birrer, "Dark Energy Survey Year 3 results: Cosmological constraints from galaxy clustering and weak lensing" Physical Review D , v.105 , 2022 https://doi.org/10.1103/PhysRevD.105.023520 Citation Details
Abbott, T.M.C. and Aguena, M. and Alarcon, A. and Alves, O. and Amon, A. and Andrade-Oliveira, F. and Annis, J. and Ansarinejad, B. and Avila, S. and Bacon, D. and Baxter, E. J. and Bechtol, K. and Becker, M. R. and Benson, B. A. and Bernstein, G. M. an "Joint analysis of Dark Energy Survey Year 3 data and CMB lensing from SPT and Planck . III. Combined cosmological constraints" Physical Review D , v.107 , 2023 https://doi.org/10.1103/PhysRevD.107.023531 Citation Details
Abbott, T.M.C. and Aguena, M. and Alarcon, A. and Alves, O. and Amon, A. and Andrade-Oliveira, F. and Annis, J. and Avila, S. and Bacon, D. and Baxter, E. and Bechtol, K. and Becker, M. R. and Bernstein, G. M. and Birrer, S. and Blazek, J. and Bocquet, "Dark Energy Survey Year 3 results: Constraints on extensions to CDM with weak lensing and galaxy clustering" Physical Review D , v.107 , 2023 https://doi.org/10.1103/PhysRevD.107.083504 Citation Details
Abbott, T.M.C. and Aguena, M. and Alarcon, A. and Alves, O. and Amon, A. and Andrade-Oliveira, F. and Asgari, M. and Avila, S. and Bacon, D. and Bechtol, K. and Becker, M. R. and Bernstein, G. M. and Bertin, E. and Bilicki, M. and Blazek, J. and Bocquet, "DES Y3 + KiDS-1000: Consistent cosmology combining cosmic shear surveys" The Open Journal of Astrophysics , v.6 , 2023 https://doi.org/10.21105/astro.2305.17173 Citation Details
Andrews, M. and Burkle, B. and Chen, Y. and DiCroce, D. and Gleyzer, S. and Heintz, U. and Narain, M. and Paulini, M. and Pervan, N. and Shafi, Y. and Sun, W. and Usai, E. and Yang, K. "End-to-end jet classification of boosted top quarks with the CMS open data" Physical Review D , v.105 , 2022 https://doi.org/10.1103/PhysRevD.105.052008 Citation Details
Banerjee, Shiladitya and Lo, Klevin and Ojkic, Nikola and Stephens, Roisin and Scherer, Norbert F. and Dinner, Aaron R. "Mechanical feedback promotes bacterial adaptation to antibiotics" Nature Physics , 2021 https://doi.org/10.1038/s41567-020-01079-x Citation Details
Campos, A. and Samuroff, S. and Mandelbaum, R. "An empirical approach to model selection: weak lensing and intrinsic alignments" Monthly Notices of the Royal Astronomical Society , v.525 , 2023 https://doi.org/10.1093/mnras/stad2213 Citation Details
Chang, C. and Omori, Y. and Baxter, E. J. and Doux, C. and Choi, A. and Pandey, S. and Alarcon, A. and Alves, O. and Amon, A. and Andrade-Oliveira, F. and Bechtol, K. and Becker, M. R. and Bernstein, G. M. and Bianchini, F. and Blazek, J. and Bleem, L. E. "Joint analysis of Dark Energy Survey Year 3 data and CMB lensing from SPT and Planck . II. Cross-correlation measurements and cosmological constraints" Physical Review D , v.107 , 2023 https://doi.org/10.1103/PhysRevD.107.023530 Citation Details
Chen, A. and Aricò, G. and Huterer, D. and Angulo, R. E. and Weaverdyck, N. and Friedrich, O. and Secco, L. F. and Hernández-Monteagudo, C. and Alarcon, A. and Alves, O. and Amon, A. and Andrade-Oliveira, F. and Baxter, E. and Bechtol, K. and Becker, M. R "Constraining the baryonic feedback with cosmic shear using the DES Year-3 small-scale measurements" Monthly Notices of the Royal Astronomical Society , v.518 , 2022 https://doi.org/10.1093/mnras/stac3213 Citation Details
Cheng, T-Y and Domínguez Sánchez, H. and Vega-Ferrero, J. and Conselice, C. J. and Siudek, M. and Aragón-Salamanca, A. and Bernardi, M. and Cooke, R. and Ferreira, L. and Huertas-Company, M. and Krywult, J. and Palmese, A. and Pieres, A. and Plazas Malagó "Lessons learned from the two largest Galaxy morphological classification catalogues built by convolutional neural networks" Monthly Notices of the Royal Astronomical Society , v.518 , 2022 https://doi.org/10.1093/mnras/stac3228 Citation Details
Chen, Huanqing and Croft, Rupert A. C. and Gnedin, Nickolay Y. "Reconstructing large-scale temperature profiles around z 6 quasars" Monthly Notices of the Royal Astronomical Society , v.519 , 2023 https://doi.org/10.1093/mnras/stad049 Citation Details
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PROJECT OUTCOMES REPORT

Disclaimer

This Project Outcomes Report for the General Public is displayed verbatim as submitted by the Principal Investigator (PI) for this award. Any opinions, findings, and conclusions or recommendations expressed in this Report are those of the PI and do not necessarily reflect the views of the National Science Foundation; NSF has not approved or endorsed its content.

The NSF AI Planning Institute brought domain experts in astronomy, high energy physics, biophysics, climate science, and engineering together with experts in AI, statistics, and computer science. The common tools used by all members and visitors served to unify these very disparate topics and move forward research in all areas, so that progress in one area could immediately translate to another without wheel reinvention.

One example of this is super-resolution simulations, developed to simulate small scale structure in the universe. These
simulations are physics-based models of the Universe and its contents.
Even with enormous computational resources there are tradeoffs between
volume and resolution. We developed deep learning methods which
seamlessly extend the dynamic range of these calculations. Generative
neural networks trained on high resolution (HR) models are
conditionally applied to low resolution models, leading to full super
resolution (SR) simulations. We showed how statistical properties at
SR are remarkably consistent with full HR, but can be orders of
magnitude larger and more complex than standard techniques allow.
Deep learning can therefore combine and extend modelling of physics
processes, offering a route to simulation of the Universe beyond
current models of superclusters and galaxies and into the realm of
stars and planets. This work was the subject of press releases which
highlighted the work of the AI Planning Institute, and was picked up
by over fifty different news outlets. We learned
that this technique is used not only by our cosmologists, but also by climate scientists (who call the method "downsampling"), engineers, and biologists. This led to one of 5 well-attended conferences that the Institute hosted.

An interdisciplinary seminar series was formally established, with
speakers covering domain areas that included climate forecasting,
extragalactic astronomy, nuclear fusion power, molecular biology,
hardware security, quantum chemistry, and particle physics. The
unifying themes were those of the Institute, the links between AI and
Physics. The seminars included 40 minutes
of open discussion. Participants included undergraduate and graduate
students, faculty members from five different CMU departments and also
from sixteen other institutions, including Historically Black Colleges
and Universities as well as national labs, and companies
such as Qualcomm and Amazon. Seminars were weekly
throughout the whole academic year and there were 102 unique
participants, with an average attendance per seminar of 31.
The seminar series was linked with a course on AI in Physics, which
provided opportunities for training for the diverse participants.

The Institute hosted a summer REU program starting in 2021. Seven students were accepted, and six of them were from under-repsented groups. Each was embedded in a research group and produced posters at the end of their 7 weeks of research. The Institute housed them and provided them with 5-6 social events so that the program provided students with a well-rounded experience that offered not just access to state-of-art AI research but also the opportunity to interact with peers and become comfortable in a research setting. The success of this program led us to repeat it for all the years of the Planning Institute, and it has now been combined with other summer programs at CMU to become an independent NSF supported REU.

Among the disseminations of results were interactive
demonstrations and presentations of AI techniques in astrohysics to
classes of students at Arsenal Middle School. The school body is
composed of 85% underrepresented minorities and 98% of students
qualify for free/discounted lunches. Lively discussions occurred
during the presentations on the role of AI in modern life and how the
generative models used in Minecraft are different from cosmological
simulations. Similar interactions occurred during a high school teacher training program that we set up that is now in its 3rd year of operation.

We developed a course for undergraduates that was taken by students at CMU as well as other schools such as South Carolina State University and University of Maryland, Baltimore County. 

 

 


 


Last Modified: 05/03/2024
Modified by: Scott Dodelson

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