Award Abstract # 1626251
MRI: Acquisition of High Performance Hybrid Computing Cluster to Advance Cyber-Enabled Science and Education at Penn State

NSF Org: OAC
Office of Advanced Cyberinfrastructure (OAC)
Recipient: THE PENNSYLVANIA STATE UNIVERSITY
Initial Amendment Date: August 5, 2016
Latest Amendment Date: August 5, 2016
Award Number: 1626251
Award Instrument: Standard Grant
Program Manager: Alejandro Suarez
alsuarez@nsf.gov
 (703)292-7092
OAC
 Office of Advanced Cyberinfrastructure (OAC)
CSE
 Directorate for Computer and Information Science and Engineering
Start Date: October 1, 2016
End Date: September 30, 2019 (Estimated)
Total Intended Award Amount: $920,688.00
Total Awarded Amount to Date: $920,688.00
Funds Obligated to Date: FY 2016 = $920,688.00
History of Investigator:
  • Cindy Gulis (Principal Investigator)
  • Douglas Cowen (Co-Principal Investigator)
  • Mahmut Kandemir (Co-Principal Investigator)
  • Adri van Duin (Co-Principal Investigator)
  • Eric Ford (Co-Principal Investigator)
Recipient Sponsored Research Office: Pennsylvania State Univ University Park
201 OLD MAIN
UNIVERSITY PARK
PA  US  16802-1503
(814)865-1372
Sponsor Congressional District: 15
Primary Place of Performance: Pennsylvania State Univ University Park
110 Technology Center Building
University Park
PA  US  16802-7000
Primary Place of Performance
Congressional District:
Unique Entity Identifier (UEI): NPM2J7MSCF61
Parent UEI:
NSF Program(s): Major Research Instrumentation,
Information Technology Researc
Primary Program Source: 01001617DB NSF RESEARCH & RELATED ACTIVIT
Program Reference Code(s): 1189
Program Element Code(s): 118900, 164000
Award Agency Code: 4900
Fund Agency Code: 4900
Assistance Listing Number(s): 47.070

ABSTRACT

Computers are now becoming the driving forces for ground-breaking discoveries and are transforming the science and education in this new data-driven era. The Cyber-Laboratory for Astronomy, Materials and Physics (CyberLAMP) at Penn State will put together a cutting-edge supercomputer cluster that includes both traditional central processing units (CPUs) and the latest hardware accelerators, such as graphics processing units (GPUs), to advance interdisciplinary research and education in cyberscience. Astronomers and physicists will use this high-performance hybrid computer to analyze data from revolutionary surveys and experiments and to perform state-of-the-art simulations to unravel of the origin of our Universe. Material scientists will run realistic, atomistic-scale, simulations to guide the design and development of next-generation complex materials. Computer scientists will analyze these science applications to inform the design of future computer architectures. These advances in both data analysis and simulations will enable the CyberLAMP members to shed new light on topics prioritized by national strategic plans, such as National Research Council's 2010 Decadal Survey for astronomy and astrophysics to search for habitable planets and to understand the fundamental physics of the cosmos and the White House's Materials Genome Initiative to expedite development of new materials. Furthermore, the CyberLAMP team will employ this cluster to enhance a wide range of outreach programs including: computational education to numerous students at The Pennsylvania State University, including its Commonwealth campuses; summer workshops for researchers and high-school teachers; and partnerships with industry to advance materials research and the co-design of future hardware-software systems.

By expediting exploratory data analysis and simulations and catalyzing cross-disciplinary collaboration in developing and prototyping algorithms, the new hybrid cluster will enable the CyberLAMP team to deliver transformative breakthroughs in a number of key research areas. This includes state-of-the-art astrostatistics and astroinformatics for data analysis for world-leading surveys in cosmology and exoplanets, as well as sophisticated simulations to directly address the nature of dark matter and dark energy, and the formation of planetary systems; an order-of-magnitude increase of speed for reconstruction algorithms for the most ambitious astrophysical experiments probing fundamental physics, which will enlarge the discovery space for cosmic sources of neutrinos, gravity waves, and multi-messenger emitters, as well as heighten sensitivity to the neutrino mass hierarchy; dramatic advances in nanosecond-scale fully reactive molecular dynamics simulations for the development of next-generation complex materials; and novel insights for designing the next-generation of hardware accelerators in hybrid systems, highly parallel algorithms and software interfaces which could revolutionize the way hardware accelerators are used by data-intensive applications.

PUBLICATIONS PRODUCED AS A RESULT OF THIS RESEARCH

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{Kite}, Edwin S. and {Fegley}, Bruce, Jr. and {Schaefer}, Laura and {Ford}, Eric B. "{Superabundance of Exoplanet Sub-Neptunes Explained by Fugacity Crisis}" \apjl , v.887 , 2019 , p.L33 10.3847/2041-8213/ab59d9
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{Aartsen}, M.~G. and {Ackermann}, M. and {Adams}, J. and {Aguilar}, J.~A. and {Ahlers}, M. and {Ahrens}, M. and {Alispach}, C. and {Andeen}, K. and {Anderson}, T. and {Ansseau}, I. and {Anton}, G. and {Arg{\"u}elles}, C. and {Ar "{Neutrino astronomy with the next generation IceCube Neutrino Observatory}" arXiv e-prints , 2019 , p.arXiv:191
{Aartsen}, M.~G. and {Ackermann}, M. and {Adams}, J. and {Aguilar}, J.~A. and {Ahlers}, M. and {Ahrens}, M. and {Alispach}, C. and {Andeen}, K. and {Anderson}, T. and {Ansseau}, I. and {Anton}, G. and {Arg{\"u}elles}, C. and {Au "{A Search for MeV to TeV Neutrinos from Fast Radio Bursts with IceCube}" arXiv e-prints , 2019 , p.arXiv:190
{Aartsen}, M.~G. and {Ackermann}, M. and {Adams}, J. and {Aguilar}, J.~A. and {Ahlers}, M. and {Ahrens}, M. and {Alispach}, C. and {Andeen}, K. and {Anderson}, T. and {Ansseau}, I. and {Anton}, G. and {Arg{\"u}elles}, C. and {Au "{Cosmic ray spectrum and composition from PeV to EeV using 3 years of data from IceTop and IceCube}" \prd , v.100 , 2019 , p.082002 10.1103/PhysRevD.100.082002
{Aartsen}, M.~G. and {Ackermann}, M. and {Adams}, J. and {Aguilar}, J.~A. and {Ahlers}, M. and {Ahrens}, M. and {Alispach}, C. and {Andeen}, K. and {Anderson}, T. and {Ansseau}, I. and {Anton}, G. and {Arg{\"u}elles}, C. and {Au "{Probing the Neutrino Mass Ordering with Atmospheric Neutrinos from Three Years of IceCube DeepCore Data}" arXiv e-prints , 2019 , p.arXiv:190
{Aartsen}, M.~G. and {Ackermann}, M. and {Adams}, J. and {Aguilar}, J.~A. and {Ahlers}, M. and {Ahrens}, M. and {Alispach}, C. and {Andeen}, K. and {Anderson}, T. and {Ansseau}, I. and {Anton}, G. and {Arg{\"u}elles}, C. and {Au "{Search for PeV Gamma-Ray Emission from the Southern Hemisphere with 5 Years of Data from the IceCube Observatory}" arXiv e-prints , 2019 , p.arXiv:190
{Aartsen}, M.~G. and {Ackermann}, M. and {Adams}, J. and {Aguilar}, J.~A. and {Ahlers}, M. and {Ahrens}, M. and {Alispach}, C. and {Andeen}, K. and {Anderson}, T. and {Ansseau}, I. and {Anton}, G. and {Arg{\"u}elles}, C. and {Au "{Search for Sources of Astrophysical Neutrinos Using Seven Years of IceCube Cascade Events}" \apj , v.886 , 2019 , p.12 10.3847/1538-4357/ab4ae2
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