DiRAC SMP Facility: The Structure of the Universe
Lead Research Organisation:
University of Cambridge
Department Name: Applied Maths and Theoretical Physics
Abstract
This proposal aims to address key questions about the fundamental structure of the Universe and the origin and nature of the galaxies, stars and planets within it. This proposal is to enhance the STFC DiRAC Facility which provides the primary computational platform for UK particle physicists, cosmologists and astrophysicists. The proposal will fund a flexible shared-memory (SMP) node with 16TB. This proposal will advance our understanding in 3 key scientific areas:
A. Science exploitation of the CMB and Large-scale Structure surveys:
The cosmic microwave background (CMB) remains the premier source for cosmological information. Planck satellite data dramatically supersedes the previous WMAP data and we will use it to constrain fundamental cosmology. With Planck data releases scheduled for 2013 and 2014, this upgrade will leverage the proprietary data, maximizing science exploitation by COSMOS members. Work on large-scale structure encompasses using surveys to constrain the properties of the Universe and understanding the hierarchical formation of galaxies.
B. Observational consequences of the Early Universe.
The consortium has pioneered the use of lattice simulations to understand the physics of non-linear phenomena in the early universe. This is expected in most cosmological models, including those with phase transitions, cosmic defects and extra dimensions. The challenge using the new SMP node will be to calculate the observable consequences of these theories, which can range from signatures in the CMB or large-scale structure through to the production of dark matter or primordial gravitational waves.
C. Extra-solar planets and their atmospheres.
The SMP node will also support key UK research in extra-solar planets. This is concerned with the observation and characterisation of exoplanets and their atmospheres, developing key numerical codes which are vital to this international endeavour. The new SMP system will allow much more information to be extracted from spectroscopic data from exoplanet environments. This will help us answer some of the oldest questions in science such as: Are there worlds beyond our solar system? Are they numerous or rare? How many of them have the right conditions for life?
A. Science exploitation of the CMB and Large-scale Structure surveys:
The cosmic microwave background (CMB) remains the premier source for cosmological information. Planck satellite data dramatically supersedes the previous WMAP data and we will use it to constrain fundamental cosmology. With Planck data releases scheduled for 2013 and 2014, this upgrade will leverage the proprietary data, maximizing science exploitation by COSMOS members. Work on large-scale structure encompasses using surveys to constrain the properties of the Universe and understanding the hierarchical formation of galaxies.
B. Observational consequences of the Early Universe.
The consortium has pioneered the use of lattice simulations to understand the physics of non-linear phenomena in the early universe. This is expected in most cosmological models, including those with phase transitions, cosmic defects and extra dimensions. The challenge using the new SMP node will be to calculate the observable consequences of these theories, which can range from signatures in the CMB or large-scale structure through to the production of dark matter or primordial gravitational waves.
C. Extra-solar planets and their atmospheres.
The SMP node will also support key UK research in extra-solar planets. This is concerned with the observation and characterisation of exoplanets and their atmospheres, developing key numerical codes which are vital to this international endeavour. The new SMP system will allow much more information to be extracted from spectroscopic data from exoplanet environments. This will help us answer some of the oldest questions in science such as: Are there worlds beyond our solar system? Are they numerous or rare? How many of them have the right conditions for life?
Planned Impact
The primary goal of the COSMOS consortium is to enable UK researchers to maintain international leadership as they advance the confrontation between fundamental and observational cosmology. COSMOS work has a significant economic impact through (I) training in high performance computing and (II) collaboration and interaction with HPC technology developers and we have collaborations with SGI and Intel. In June 2014, COSMOS@DiRAC became an Intel Parallel Computing Centre, representing a formal link with Intel. SGI also co-fund programmer support.
The COSMOS consortium has the largest user base of the STFC HPC consortia (mainly PDRAs and graduate students) and maintains a special emphasis on user accessibility and education, ensuring maximum benefit to UK science and subsequent employers. Significant numbers of graduate students and postdoctoral fellows have been and continue to be trained and given transferable skills, including analysis and problem-solving, software engineering and numerical simulation and techniques for massively parallel programming. The computational techniques employed involve a constant interplay between HPC codes and intuition on systems of huge inherent complexity. This sort of activity is highly regarded in the business world and in high-tech industries, providing an important platform for future employment.
The COSMOS consortium also contributes to the public understanding of science through its high media profile, thereby improving the social acceptability of new technology and attracting young people to consider careers in the sciences. In addition, COSMOS consortium members have had a high public profile and are engaged in outreach. Cosmology remains of major interest to the public. The group contains members who are particularly active in maximizing the impact of our science in the outside world to audiences of all sorts. Hawking is probably the most well known scientist in the world and his lectures, television coverage, and books have very widespread impact that acts as an important standard-bearer for the whole area of the Research Council's scientific work in cosmology and fundamental physics.
The Exomolo consortium will continue and broaden its researchers' current involvement in Knowledge Exchange and Outreach programmes:
(i) Quantemol, a UCL-based 'spin-out' firm related to the Miracle Exomol project
(ii) Providing accurate and complete molecular data to Industry and climate research programmes
(iii) Working with commerce, research design labs and other academic areas to produce new IT (hardware and software) solutions transferrable to Industry and academic areas such as Biomedicine;
(iv) Working with leading IT vendors to test and design new hardware and software solutions which will eventually end up in the marketplace.
There is an extra document attached which describes the impact of the whole DiRAC community.
The COSMOS consortium has the largest user base of the STFC HPC consortia (mainly PDRAs and graduate students) and maintains a special emphasis on user accessibility and education, ensuring maximum benefit to UK science and subsequent employers. Significant numbers of graduate students and postdoctoral fellows have been and continue to be trained and given transferable skills, including analysis and problem-solving, software engineering and numerical simulation and techniques for massively parallel programming. The computational techniques employed involve a constant interplay between HPC codes and intuition on systems of huge inherent complexity. This sort of activity is highly regarded in the business world and in high-tech industries, providing an important platform for future employment.
The COSMOS consortium also contributes to the public understanding of science through its high media profile, thereby improving the social acceptability of new technology and attracting young people to consider careers in the sciences. In addition, COSMOS consortium members have had a high public profile and are engaged in outreach. Cosmology remains of major interest to the public. The group contains members who are particularly active in maximizing the impact of our science in the outside world to audiences of all sorts. Hawking is probably the most well known scientist in the world and his lectures, television coverage, and books have very widespread impact that acts as an important standard-bearer for the whole area of the Research Council's scientific work in cosmology and fundamental physics.
The Exomolo consortium will continue and broaden its researchers' current involvement in Knowledge Exchange and Outreach programmes:
(i) Quantemol, a UCL-based 'spin-out' firm related to the Miracle Exomol project
(ii) Providing accurate and complete molecular data to Industry and climate research programmes
(iii) Working with commerce, research design labs and other academic areas to produce new IT (hardware and software) solutions transferrable to Industry and academic areas such as Biomedicine;
(iv) Working with leading IT vendors to test and design new hardware and software solutions which will eventually end up in the marketplace.
There is an extra document attached which describes the impact of the whole DiRAC community.
Organisations
Publications
Abbott R
(2020)
Direct C P violation and the ? I = 1 / 2 rule in K ? p p decay from the standard model
in Physical Review D
Abidi M
(2018)
Cubic halo bias in Eulerian and Lagrangian space
in Journal of Cosmology and Astroparticle Physics
Achúcarro A
(2019)
Cosmological evolution of semilocal string networks.
in Philosophical transactions. Series A, Mathematical, physical, and engineering sciences
Acuto A
(2021)
The BAHAMAS project: evaluating the accuracy of the halo model in predicting the non-linear matter power spectrum
in Monthly Notices of the Royal Astronomical Society
Adamek J
(2020)
Numerical solutions to Einstein's equations in a shearing-dust universe: a code comparison
in Classical and Quantum Gravity
Agudelo Rueda J
(2022)
Energy Transport during 3D Small-scale Reconnection Driven by Anisotropic Plasma Turbulence
in The Astrophysical Journal
Agudelo Rueda J
(2021)
Three-dimensional magnetic reconnection in particle-in-cell simulations of anisotropic plasma turbulence
in Journal of Plasma Physics
Ahad S
(2021)
The stellar mass function and evolution of the density profile of galaxy clusters from the Hydrangea simulations at 0 < z < 1.5
in Monthly Notices of the Royal Astronomical Society
Al-Refaie A
(2021)
TauREx 3: A Fast, Dynamic, and Extendable Framework for Retrievals
in The Astrophysical Journal
Description | High energy grazing collisions of black holes |
Amount | $48,207 (USD) |
Funding ID | NSF-XSEDE Grant No. PHY-090003 |
Organisation | National Science Foundation (NSF) |
Sector | Public |
Country | United States |
Start | 01/2017 |
End | 12/2017 |
Description | Probing fundamental physics with gravity |
Amount | € 1 (EUR) |
Funding ID | RACE grant Tier-0 PPFPWG |
Organisation | European Commission |
Sector | Public |
Country | European Union (EU) |
Start | 12/2016 |
End | 11/2017 |
Description | 2nd Institute of Space Sciences Summer School |
Form Of Engagement Activity | A talk or presentation |
Part Of Official Scheme? | No |
Geographic Reach | International |
Primary Audience | Postgraduate students |
Results and Impact | In July 2018, Dr Ulrich Sperhake gave a talk entitled "Gravitational Waves Source Modeling" as part of the 2nd Institute of Space Sciences Summer School in Barcelona. |
Year(s) Of Engagement Activity | 2018 |
URL | https://www.ice.csic.es/indico/event/9/ |
Description | 6th form talk (Chelmsford) |
Form Of Engagement Activity | A talk or presentation |
Part Of Official Scheme? | No |
Geographic Reach | Local |
Primary Audience | Schools |
Results and Impact | October 2017: Ulrich Sperhake gave a talk to a 6th form college in Chelmsford. Subject: The direct detection of gravitational waves by LIGO and the insights already obtained from this new window on the Universe as well as the enormous potential for our search for answers to the most profound questions in astrophysics and fundamental physics. |
Year(s) Of Engagement Activity | 2017 |
Description | Discovery programme |
Form Of Engagement Activity | A broadcast e.g. TV/radio/film/podcast (other than news/press) |
Part Of Official Scheme? | No |
Geographic Reach | International |
Primary Audience | Public/other audiences |
Results and Impact | Stephen Hawking was one of the best-known scientists of his generation. In addition to his visionary contributions to our understanding of black holes and the early universe, he reached millions of people, communicating his research through public lectures, books, TV and film, social media and digital applications - stimulating public interest and understanding of fundamental scientific research. In 2017 the CTC held a public symposium to mark Stephen Hawking's 75th birthday. The public lecture he gave was livestreamed by Discovery Science on its YouTube and Facebook pages and reached over five million people worldwide. In the lecture, Professor Hawking reflected on his life and career, weaving together his personal stories and scientific discoveries. The symposium also featured talks by Brian Cox, Gabriela González and Martin Rees. https://www.youtube.com/watch?v=hotwr3uUUD4 The enormous success of the event inspired CTC and Discovery to collaborate on a new project, producing science content for Discovery Channel youth initiatives and social media websites. The project has since grown considerably in breadth and ambition - thanks partly to generous funding from the Kavli Foundation for science editorial and technical support - to include an extended video documentary series consisting of 26 short episodes to be made available via Discovery's new video on demand (VOD) streaming service. It is an exciting opportunity for CTC researchers to share their work with a global audience. The filming has taken place (undertaken by the production team Navada Studios) in locations within the Centre for Mathematical Sciences (home of the CTC), the Kavli Institute and the Institute of Astronomy, and we were pleased that it was possible to film some footage of the KICC 10th Anniversary Symposium. The series is split into two halves: gravity and cosmology. The gravity episodes cover general relativity, modified theories of gravity, black holes, gravitational waves, cosmic strings, as well as Stephen Hawking's work on black holes, Hawking radiation and the information paradox. The contributors for these episodes were Ulrich Sperhake, Harvey Reall, Michalis Agathos, Amelia Drew, Jorge Santos, Miren Radia and Felicity Eperon. The cosmology episodes cover the expanding universe and the Big Bang, the CMB, inflation and the seeds of structure, dark matter and the ingredients of the universe, quantum gravity, B-modes in the CMB and non-Gaussianity. The contributors for these episodes are Blake Sherwin, Enrico Pajer, Fran Day, Sadra Jazayeri, Cora Uhlemann, Omar Darwish and James Fergusson. The final episode of the series will feature interviews with Paul Shellard and Roberto Maiolini to recap material and highlight the vision of the CTC and KICC. The release date is yet to be confirmed by Discovery but we hope that the initial episodes in the series will be available within the next few months. |
Year(s) Of Engagement Activity | 2020 |
Description | IOP Engineering Society (Chelmsford) |
Form Of Engagement Activity | A talk or presentation |
Part Of Official Scheme? | No |
Geographic Reach | Regional |
Primary Audience | Professional Practitioners |
Results and Impact | October 2017: Ulrich Sperhake gave a talk to the IOP Engineering Society in Chelmsford. Subject: The direct detection of gravitational waves by LIGO and the insights already obtained from this new window on the Universe as well as the enormous potential for our search for answers to the most profound questions in astrophysics and fundamental physics. |
Year(s) Of Engagement Activity | 2017 |
Description | Science Festival 2015 |
Form Of Engagement Activity | Participation in an open day or visit at my research institution |
Part Of Official Scheme? | No |
Geographic Reach | Regional |
Primary Audience | Public/other audiences |
Results and Impact | Science Week 2015 within the University of Cambridge includes a popular open day at the Centre for Mathematical Sciences in which we participated actively. Apart from visualisation and other poster displays, a particularly popular activity was the tour of the COSMOS supercomputer. |
Year(s) Of Engagement Activity | 2015 |
Description | Web sites |
Form Of Engagement Activity | Engagement focused website, blog or social media channel |
Part Of Official Scheme? | No |
Geographic Reach | International |
Primary Audience | Public/other audiences |
Results and Impact | Our Centre for Theoretical Cosmology and COSMOS supercomputer websites include news stories of wide interest to the general public as well as more specialist audiences. These can be found at: www.ctc.cam.ac.uk www.cosmos.damtp.cam.ac.uk |
Year(s) Of Engagement Activity | 2012,2013,2014,2015,2016 |
URL | http://www.ctc.cam.ac.uk |