Angry Birds to star in particle physics board game

From SciTech Gaming:  Angry Birds to star in particle physics board game

After teaching gamers that physics can be fun, the Angry Birds may soon be doing the same thing for —yowza!— quantum physics.

 

Rovio Entertainment and CERN, the European Organization for Nuclear Research, are developing “fun learning experiences” to engage children with science, TechCrunch reported.

 

“Modern physics has been around for 100 years, but it’s still a mystery to many people. Working together with Rovio, we can teach kids quantum physics by making it fun and easy to understand,” TechCrunch quoted CERN’s Head of Education, Rolf Landua, as saying.

 

Landua spoke about the collaboration at the Frankfurt Book Fair where the Rovio launch took place.

 

He added this is "a great fit for both sides, combining physics and Angry Birds in a fun way."

Fun from CERN
 

"Rovio has a great platform, with a broad reach and highly engaged fans, which makes this collaboration very promising. With Rovio and Angry Birds Playground, we get a great channel to communicate what CERN does,” he added.

 

Peter Vesterbacka, Rovio Mighty Eagle and CMO, added that with Playground products, "kids can have fun and learn more about physics than they would’ve in the ‘old-fashioned’ style of learning.”

 

TechCrunch quoted Rovio as saying the collaboration will involve co-producing learning support materials with CERN, initially including books and a board game.

 

"More products will be added later, the company said," TechCrunch said.

 

New initiative

 

TechCrunch said this is part of Rovio's new initiative to use the power of Angry Birds as a brand to be a learning aid.

 

Rovio already started a learning program called "Angry Birds Playground" for children aged 3 to 8, based on the Finnish National Curriculum for kindergarten. — TJD, GMA News

 

Viewpoint: Heavy into Stability

From Physics.com:  Viewpoint: Heavy into Stability

In 1940, the first synthetic element heavier than uranium—neptunium-239—was produced by bombarding uranium with neutrons. Since then, nuclear scientists have ventured into the search for new heavy elements, expanding the frontiers of the physical world. The creation of elements with atomic number beyond that of uranium is challenging, as the half-life of elements decreases with increasing atomic number. However, nuclear theories have predicted that a so-called “island of stability” exists for certain superheavy elements of the nuclide chart, which should have half-lives ranging from minutes to many years.
The search for this island of stability has led to the creation of elements with up to 118 protons. The last element to be discovered was 117 [1] (see 9 April, 2010 Viewpoint), filling in the final gap on the list of observed elements up to element 118. Now, writing in Physical Review Letters, Yuri Oganessian at the Joint Institute for Nuclear Research (JINR), Russia, and colleagues report on a second production campaign for element 117 [2], which verifies their initial findings and provides a new comprehensive characterization of the decay chains of two isotopes of the 117 element. Their results confirm that we are indeed approaching the shores of the island of stability.
The stability of nuclides is a function of proton ($Z$) and neutron ($N$) number, as illustrated in Fig. 1. A connected region (“continent”) of stable elements is found for lighter elements, ending at the lead–bismuth “cape.” All elements with an atomic number exceeding 82 (lead) are unstable, with decreasing half-life for higher atomic numbers. However, a first region of relative stability appears around the isotopes of thorium and uranium ($Z$ equal to 90 and 92, respectively) whose lifetimes are comparable with the age of the universe. Elements with atomic number greater than that of uranium (transuranium elements) have only been produced in laboratory experiments (see the historical review in Ref. [3]). The progress in this field is impressive: 26 new, manmade heavy elements have been synthesized within 60 years. Some of these elements (up to californium) can be produced in macroscopic quantities in nuclear reactors, using neutron capture processes to form heavier elements from actinides.
Elements beyond uranium should become more and more unstable as they get heavier, as Coulomb repulsion starts to be stronger than the strong force that holds the nucleus together. But in the late sixties, Glenn T. Seaborg postulated the existence of a relatively stable region of superheavy elements, an island of stability. This idea is based on the nuclear shell model, which describes the atomic nucleus as made of shells, similar to the well-known electronic shell model for atoms. Nuclear theorists, including myself [4, 5], predicted that the stability of nuclei with so-called closed proton and neutron shells should counteract the repelling Coulomb forces. In isotopes with so-called “magic” proton and neutron numbers, neutrons and protons completely fill the energy levels of a given shell in the nucleus. Those particular isotopes will have a longer lifetime than nearby ones. According to theory, this second island of stability should be located around proton number $114$ or $120$ and neutron number $184$. Reaching this island of stability would open new horizons in nuclear physics and technology, enabling the production of superheavy nuclides in macroscopic quantities and with sufficiently long half-life to carry out actual experiments. This would allow us to test our understanding of nuclear matter and to possibly exploit such long-lived elements for applications in medicine or chemistry.
Substantial progress in the synthesis of superheavy nuclei was achieved at the GSI Helmholtz Centre for Heavy Ion Research in Germany, where the elements with $Z=108$ to $112$ have been synthesized for the first time in fusion reactions of heavy projectiles (from iron to zinc) with lead and bismuth targets [6]. Unfortunately, in these projectile–target combinations only the proton-rich isotopes of superheavy elements with very short half-lives can be produced, as they lie outside the island of nuclear stability. Within the last ten years, researchers at JINR have successfully synthesized six new heavy elements with $Z=113$–$118$ by following a different approach: instead of a heavy projectile, a high-intensity beam of lighter atoms (calcium-48) is aimed at heavy actinide targets made of uranium or transuranium elements. The use of neutron richer calcium-48 allows the synthesis of nuclides with neutron number closer to that needed for stability.
Up until 2010, there was a gap between elements 116 and 118. The obstacle towards the production of element 117 was that the appropriate target material, berkelium-249 (${}^{249}\text{Bk}$) with 97 protons, has a short half-life of only 330 days. In 2009, several milligrams of ${}^{249}\text{Bk}$ were produced at Oak Ridge National Laboratory in the US—enough to prepare a target and to perform the first experiment for the synthesis of element 117 at JINR [1]. In early March of 2012, a new portion of ${}^{249}\text{Bk}$, $12\text{mg}$, was shipped again from Oak Ridge to JINR, where physicists started the second production campaign for the synthesis of element 117.
The results of this campaign, reported in the paper by Oganessian et al. [2], confirm that a reliable method for the production of 117 exists. The authors can now state with confidence that two isotopes of this element, ${}^{293}117$ and ${}^{294}117$, have been synthesized and provide a comprehensive characterization of their decay properties. Two decay chains of ${}^{294}117$ and five decay chains of ${}^{293}117$ were detected. Oganessian et al. also observe a concomitant decay chain of element 118. This occurs because, at the time of the experiment, part of the ${}^{249}\text{Bk}$ target material had already decayed into californium-249, which can generate element 118 in a fusion reaction with calcium-48. The measured lifetimes of the 117 isotopes and other elements along its decay chain are long, lying in the millisecond-to-second range. This is consistent with shell-model predictions, confirming that these elements are indeed located at the southwest shores of the island of stability. The consistent results emerging from the two productions campaigns at JINR may get the authors close to laying claim on naming the new element.
What are the prospects of reaching deeper into the center of the island of stability? Although fairly long lived, the isotopes of superheavy elements produced in the experiments with calcium-48 are still neutron deficient: each isotope needs six to eight more neutrons to lie within the island. This occurs because heavier stable atoms must have a larger neutron/proton ratio that lighter atoms. Thus creating a heavy atom by fusion of two lighter ones inevitably leads to an atom that has too few neutrons and too many protons to be stable. One would then deduce that there is no way to the island of stability. However, pathways towards the center of the island of stability may exist. Recent theoretical studies carried out in my research group suggest that superheavy nuclei located at the top left side of the island of stability, formed in ordinary fusion reactions, could get rid of excess protons via ${\beta }^{+}$ decay [7]. Other alternatives to get to the right neutron number might exploit neutron capture, rather than fusion: such techniques would require the exposure of heavy elements, such as uranium, to very high neutron fluxes. Theory shows that this could be achieved in hypothetical small-scale underground nuclear explosions [8] or by using pulsed nuclear reactors of the next generation, if their neutron fluence per pulse is increased by about three orders of magnitude.
While the island of stability is now more firmly in sight, the jury is still out on what navigation plan will turn out to be successful.

References

1. Yu.Ts. Oganessian et al., “Synthesis of a New Element with Atomic Number Z=117,” Phys. Rev. Lett. 104, 142502 (2010).
2. Y. T. Oganessian et al., “Production and Decay of the Heaviest Nuclei 293,294 117 and 294 118,” Phys. Rev. Lett. 109, 162501 (2012).
3. G. T. Seaborg and W. D. Loveland, The Elements Beyond Uranium (John Wiley and Sons, New York, 1990)[Amazon][WorldCat].
4. S. G. Nilsson, S. G. Thompson, and C. F. Tsang, “Stability of Superheavy Nuclei and Their Possible Occurrence in Nature,” Phys. Lett. 28B, 458 (1969).
5. U. Mosel and W. Greiner, “On the Stability of Superheavy Nuclei Against Fission,” Z. Phys. A 222, 261 (1969); Also in the Proposal for the Establishment of GSI: Frankfurt-Darmstadt-Marburg (1967).
6. S. Hofmann and G. Munzenberg, “The Discovery of the Heaviest Elements,” Rev. Mod. Phys. 72, 733 (2000).
7. V. I. Zagrebaev, A. V. Karpov, and W. Greiner, “Possibilities for Synthesis of New Isotopes of Superheavy Elements in Fusion Reactions,” Phys. Rev. C 85, 014608 (2012).
8. V. I. Zagrebaev, A. V. Karpov, I. N. Mishustin, and W. Greiner, “Production of Heavy and Superheavy Neutron-Rich Nuclei in Neutron Capture Processes,” Phys. Rev. C 84, 044617 (2011).

 

Viewpoint: Heavy into Stability

From Physics: Viewpoint: Heavy into Stability

In 1940, the first synthetic element heavier than uranium—neptunium-239—was produced by bombarding uranium with neutrons. Since then, nuclear scientists have ventured into the search for new heavy elements, expanding the frontiers of the physical world. The creation of elements with atomic number beyond that of uranium is challenging, as the half-life of elements decreases with increasing atomic number. However, nuclear theories have predicted that a so-called “island of stability” exists for certain superheavy elements of the nuclide chart, which should have half-lives ranging from minutes to many years.
The search for this island of stability has led to the creation of elements with up to 118 protons. The last element to be discovered was 117 [1] (see 9 April, 2010 Viewpoint), filling in the final gap on the list of observed elements up to element 118. Now, writing in Physical Review Letters, Yuri Oganessian at the Joint Institute for Nuclear Research (JINR), Russia, and colleagues report on a second production campaign for element 117 [2], which verifies their initial findings and provides a new comprehensive characterization of the decay chains of two isotopes of the 117 element. Their results confirm that we are indeed approaching the shores of the island of stability.
The stability of nuclides is a function of proton (Z) and neutron (N) number, as illustrated in Fig. 1. A connected region (“continent”) of stable elements is found for lighter elements, ending at the lead–bismuth “cape.” All elements with an atomic number exceeding 82 (lead) are unstable, with decreasing half-life for higher atomic numbers. However, a first region of relative stability appears around the isotopes of thorium and uranium (Z equal to 90 and 92, respectively) whose lifetimes are comparable with the age of the universe. Elements with atomic number greater than that of uranium (transuranium elements) have only been produced in laboratory experiments (see the historical review in Ref. [3]). The progress in this field is impressive: 26 new, manmade heavy elements have been synthesized within 60 years. Some of these elements (up to californium) can be produced in macroscopic quantities in nuclear reactors, using neutron capture processes to form heavier elements from actinides.
Elements beyond uranium should become more and more unstable as they get heavier, as Coulomb repulsion starts to be stronger than the strong force that holds the nucleus together. But in the late sixties, Glenn T. Seaborg postulated the existence of a relatively stable region of superheavy elements, an island of stability. This idea is based on the nuclear shell model, which describes the atomic nucleus as made of shells, similar to the well-known electronic shell model for atoms. Nuclear theorists, including myself [4, 5], predicted that the stability of nuclei with so-called closed proton and neutron shells should counteract the repelling Coulomb forces. In isotopes with so-called “magic” proton and neutron numbers, neutrons and protons completely fill the energy levels of a given shell in the nucleus. Those particular isotopes will have a longer lifetime than nearby ones. According to theory, this second island of stability should be located around proton number 114 or 120 and neutron number 184. Reaching this island of stability would open new horizons in nuclear physics and technology, enabling the production of superheavy nuclides in macroscopic quantities and with sufficiently long half-life to carry out actual experiments. This would allow us to test our understanding of nuclear matter and to possibly exploit such long-lived elements for applications in medicine or chemistry.
Substantial progress in the synthesis of superheavy nuclei was achieved at the GSI Helmholtz Centre for Heavy Ion Research in Germany, where the elements with Z=108 to 112 have been synthesized for the first time in fusion reactions of heavy projectiles (from iron to zinc) with lead and bismuth targets [6]. Unfortunately, in these projectile–target combinations only the proton-rich isotopes of superheavy elements with very short half-lives can be produced, as they lie outside the island of nuclear stability. Within the last ten years, researchers at JINR have successfully synthesized six new heavy elements with Z=113–118 by following a different approach: instead of a heavy projectile, a high-intensity beam of lighter atoms (calcium-48) is aimed at heavy actinide targets made of uranium or transuranium elements. The use of neutron richer calcium-48 allows the synthesis of nuclides with neutron number closer to that needed for stability.
Up until 2010, there was a gap between elements 116 and 118. The obstacle towards the production of element 117 was that the appropriate target material, berkelium-249 (249Bk) with 97 protons, has a short half-life of only 330 days. In 2009, several milligrams of 249Bk were produced at Oak Ridge National Laboratory in the US—enough to prepare a target and to perform the first experiment for the synthesis of element 117 at JINR [1]. In early March of 2012, a new portion of 249Bk, 12mg, was shipped again from Oak Ridge to JINR, where physicists started the second production campaign for the synthesis of element 117.
The results of this campaign, reported in the paper by Oganessian et al. [2], confirm that a reliable method for the production of 117 exists. The authors can now state with confidence that two isotopes of this element, 293117 and 294117, have been synthesized and provide a comprehensive characterization of their decay properties. Two decay chains of 294117 and five decay chains of 293117 were detected. Oganessian et al. also observe a concomitant decay chain of element 118. This occurs because, at the time of the experiment, part of the 249Bk target material had already decayed into californium-249, which can generate element 118 in a fusion reaction with calcium-48. The measured lifetimes of the 117 isotopes and other elements along its decay chain are long, lying in the millisecond-to-second range. This is consistent with shell-model predictions, confirming that these elements are indeed located at the southwest shores of the island of stability. The consistent results emerging from the two productions campaigns at JINR may get the authors close to laying claim on naming the new element.
What are the prospects of reaching deeper into the center of the island of stability? Although fairly long lived, the isotopes of superheavy elements produced in the experiments with calcium-48 are still neutron deficient: each isotope needs six to eight more neutrons to lie within the island. This occurs because heavier stable atoms must have a larger neutron/proton ratio that lighter atoms. Thus creating a heavy atom by fusion of two lighter ones inevitably leads to an atom that has too few neutrons and too many protons to be stable. One would then deduce that there is no way to the island of stability. However, pathways towards the center of the island of stability may exist. Recent theoretical studies carried out in my research group suggest that superheavy nuclei located at the top left side of the island of stability, formed in ordinary fusion reactions, could get rid of excess protons via β+ decay [7]. Other alternatives to get to the right neutron number might exploit neutron capture, rather than fusion: such techniques would require the exposure of heavy elements, such as uranium, to very high neutron fluxes. Theory shows that this could be achieved in hypothetical small-scale underground nuclear explosions [8] or by using pulsed nuclear reactors of the next generation, if their neutron fluence per pulse is increased by about three orders of magnitude.
While the island of stability is now more firmly in sight, the jury is still out on what navigation plan will turn out to be successful.

References

1. Yu.Ts. Oganessian et al., “Synthesis of a New Element with Atomic Number Z=117,” Phys. Rev. Lett. 104, 142502 (2010).
2. Y. T. Oganessian et al., “Production and Decay of the Heaviest Nuclei 293,294 117 and 294 118,” Phys. Rev. Lett. 109, 162501 (2012).
3. G. T. Seaborg and W. D. Loveland, The Elements Beyond Uranium (John Wiley and Sons, New York, 1990)[Amazon][WorldCat].
4. S. G. Nilsson, S. G. Thompson, and C. F. Tsang, “Stability of Superheavy Nuclei and Their Possible Occurrence in Nature,” Phys. Lett. 28B, 458 (1969).
5. U. Mosel and W. Greiner, “On the Stability of Superheavy Nuclei Against Fission,” Z. Phys. A 222, 261 (1969); Also in the Proposal for the Establishment of GSI: Frankfurt-Darmstadt-Marburg (1967).
6. S. Hofmann and G. Munzenberg, “The Discovery of the Heaviest Elements,” Rev. Mod. Phys. 72, 733 (2000).
7. V. I. Zagrebaev, A. V. Karpov, and W. Greiner, “Possibilities for Synthesis of New Isotopes of Superheavy Elements in Fusion Reactions,” Phys. Rev. C 85, 014608 (2012).
8. V. I. Zagrebaev, A. V. Karpov, I. N. Mishustin, and W. Greiner, “Production of Heavy and Superheavy Neutron-Rich Nuclei in Neutron Capture Processes,” Phys. Rev. C 84, 044617 (2011).

 

Chinese, Russian nuclear physicists meet in Stellenbosch

From Stellenbosch University:  Chinese, Russian nuclear physicists meet in Stellenbosch

Stellenbosch University’s Department of Physics is having quite a busy end of the year, thanks to visits by two groups of international nuclear physicists. Last week, Russian physicists met with their South African counterparts, while a symposium along with Chinese researchers is taking  place this week.
The 2nd China-South Africa Joint Symposium on Nuclear Physics started on Monday (3 December) and will run until Thursday. It is being held on the Stellenbosch University campus in collaboration with academics of Peking University in China.
The 3rd South African-JINR Symposium, in conjunction with the Russian Joint Institute for Nuclear Research (JINR) was held from 27 to 30 November at Blaauwklippen outside Stellenbosch.
Both events were organised by the Nuclear Physics Research Group in the SU Department of Physics.Researchers and students from other South African institutions and research entities were also involved.
For more information, contact Prof Shaun Wyngaardt at shaunmw@sun.ac.za.

 

Cosmic Rays Help Diagnose Damaged Nuclear Reactors From Space

From Red Orbity:  Cosmic Rays Help Diagnose Damaged Nuclear Reactors From Space

Image Caption: Los Alamos National Laboratory Muon Radiography team members stand in front of the damaged Fukushima Daiichi reactor complex during a visit to determine evaluate whether Los Alamos' Scattering Method for cosmic-ray radiography could be used to image the location of nuclear materials within the reactor buildings. Credit: Los Alamos National Laboratory

Brett Smith for redOrbit.com – Your Universe Online
They may not be using alien technology, but physicists from Los Alamos National Laboratory are looking to outer space for help in diagnosing a damaged nuclear reactors like the one that caused massive evacuations around the Fukushima Daiichi plant in March 2011.
According to their report in the journal Physical Letters, the research team from Los Alamos National Laboratory has found a way to use cosmic ray radiation to accurately create a detailed image of the inside of a damaged reactor core. This technology could be used to implement more effective cleanup operations, since knowing where radioactive materials are located is key to implementing effective strategies.
In their experiment, the team of scientists compared two methods for detecting hazardous material: a traditional transmission method and the Los Alamos’ scattering method for cosmic-ray radiography. According to the researchers’ report, the latter method proved to be superior.
“Within weeks of the disastrous 2011 tsunami, Los Alamos’ Muon Radiography Team began investigating use of Los Alamos’ muon scattering method to determine whether it could be used to image the location of nuclear materials within the damaged reactors,” explained the study’s lead author Konstantin Borozdin of Los Alamos’ Subatomic Physics Group.
“As people may recall from previous nuclear reactor accidents, being able to effectively locate damaged portions of a reactor core is a key to effective, efficient cleanup,” he said. “Our paper shows that Los Alamos’ scattering method is a superior method for gaining high-quality images of core materials.”
Cosmic-ray, or muon, radiography uses the particles that are generated when radiation from outer space collides with the Earth’s atmosphere. These cosmic rays, known as muons, can be used to create images in the same way as X-rays, expect that muons are produced naturally and constantly come in contact with the human body without any known harmful effects.
Muons are particularly useful in working with radioactive material because “high-Z” materials, like uranium, scatter them differently than the surrounding containment materials – allowing scientists to pinpoint the locations of radioactive material if they know how the muons are being diffused.
Using a computer model, the team was able to simulate a damaged reactor with radioactive material scattered throughout the virtual power plant. They were then able to compare the accuracy of both the traditional scanning methods and the Los Alamos scattering method in finding what material was indeed missing from the model reactor and where it was located over a six-week period.
The Los Alamos method demonstrated that it was able to accurately provide the detailed information that the scientists were looking for.
“We now have a concept by which the Japanese can gather crucial data about what is going on inside their damaged reactor cores with minimal human exposure to the high radiation fields that exist in proximity to the reactor buildings,” Borozdin explained.
“Muon images could be valuable in more effectively planning and executing faster remediation of the reactor complex.”
The researchers noted that this detection technology could also be applied to security measures in the post-9/11 era. They said muon radiation detectors would be non-invasive, yet able to spot heavily shielded contraband in minutes without the need to open a potentially dangerous vehicle or container.

 

High Honor for Two Physicists

From UCR Today:  High Honor for Two Physicists

RIVERSIDE, Calif. — Two physicists at the University of California, Riverside — Richard Seto and Jing Shi — have been elected as fellows of the American Physical Society (APS).  Only 250 researchers received the high honor this year.
The APS represents more than 50,000 members, including physicists in academia, national laboratories and industry in the United States and throughout the world.  Fellowship in the society is limited to no more than one half of one percent of the membership.  The evaluation process for fellowship election is done entirely by one’s professional peers.
Seto, a professor of physics and astronomy, was elected an APS Fellow “for creative experimentation and leadership in the study of hadronic matter under extreme conditions including measurements and analysis leading to the discovery of the strongly-interacting Quark Gluon Plasma (sQGP).”
Seto works in the field of relativistic heavy ion physics — a blend between nuclear physics and particle physics — that focuses on the properties of bulk systems governed by the theory of strong interactions or Quantum Chromodynamics.  His research is carried out on the PHENIX experiment at the Relativistic Heavy Ion Collider at the Brookhaven National Laboratory, where very high energy collisions of heavy nuclei are available. This has led to the discovery of the strongly-interacting Quark Gluon Plasma, a state of matter in which the protons and neutrons in a nucleus are melted into their constituent quarks and gluons.
The author or coauthor of more than 170 papers in scholarly journals, Seto has served on the Nuclear Science Advisory Committee, which advises the Department of Energy and the National Science Foundation on research priorities in nuclear science; the program committee for the Division of Nuclear Physics of American Physical Society; the editorial board for Physics Review C; and as PHENIX deputy spokesperson.  Currently, he serves on the PHENIX Executive Committee, which advises the management of the experiment.  Seto received his doctoral degree from Columbia University in 1983.
Shi, also a professor of physics and astronomy, was elected an APS Fellow “for his pioneering work in spin transport in organic semiconductors and organic molecules.”
At UCR, his research endeavors include experimental condensed matter physics. Currently, he is working on the charge and spin transport in carbon-based and other novel electronic materials.
He has published nearly 90 papers in scholarly journals including two in Nature, one in Science, and six in Physical Review Letters.  He holds 11 US patents and provisional patents.   His many awards and honors include the highly competitive Research Innovation Award in 2000 from the Research Corporation as well as the IBM Faculty Award in 2009.  He received his doctoral degree from the University of Illinois at Urbana-Champaign in 1994.
The APS works to advance and diffuse the knowledge of physics through its outstanding research journals, scientific meetings and education, outreach, advocacy and international activities.

 

CFI Visits TRIUMF

From triUMF:  CFI Visits TRIUMF

The Canada Foundation for Innovation (CFI) has become a mainstay of support for Canadian research excellence since its launch more than a decade ago.  With a new mandate that includes the stewardship of four large-science facilities across the country as well as a new strategic plan, the arms-length funding agency visited TRIUMF this Wednesday to (a) get a personal look at a number of CFI-supported projects that are based at TRIUMF and (b) to get familiar with how a national laboratory like TRIUMF manages it affairs with a good track record of relevance and performance.
Guy Levesque, director of programs at CFI, spent more than two hours at TRIUMF after lunch on November 28. Literally between planes on business in British Columbia, he made time for a visit.  The intinerary began with a meeting with TRIUMF's executive team and some of the principal investigators for active CFI projects in which TRIUMF is involved.  Reiner Kruecken presented a short overview of TRIUMF and summarized thge CFI-supported activities at the lab over the last five years.  These included, among others, the ARIEL and e-linac accelerator project led by Dean Karlen at UVic, the M-20 beamlines led by Paul Percival at SFU, the ATLAS Tier-1 Data Centre led by Mike Vetterli at SFU, the IRIS nuclear-physics experiment led by Ritu Kanungo at Saint Mary's, and the Ultra-Cold Neutrons project led by Jeff Martin at Winnipeg.  TRIUMF is not eligible to apply directly for CFI funds, but it is involved in many projects because of its unique technical and engineering skills and capabilities.  The lab also hosts some facilities and detectors led by university collaborators that exploit TRIUMF's accelerators and beams.  A rough estimate indicates that CFI funding of nealry $30M over the past five years has influenced more than $100M of activity that engages and enhances TRIUMF's role in leveraging Canadian university research. Reiner's conclusion was that Canadian leadership in subatomic physics is enabled by CFI's support and that TRIUMF provides substantial leveraging of that investment for national and international impact.  Through its core operations, TRIUMF can also serve as an ideal long-term steward for some of these on-site facilities and infrastructure.
Mr. Levesque then toured TRIUMF and met several of the key project personnel.  Around ARIEL, he saw the newly renovated Electron Hall and met project managers Gary Ridout and Franco Mammarella in addition to project leaders Lia Merminga and Remy Dawson.  In a rare moment of access, the group also visited the ARIEL civil-construction site and toured the beam tunnel and stepped inside the concrete target hall and RIB building. After shedding the extra safety gear, the group visited the Meson Hall and met Syd Kreitzman and Gerald Morris to learn more about the M-20 muon beamline and its first week of science.  Paul Schaffer led Mr. Levesque on a lightning tour of the nuclear-medicine facilities and discussed TRIUMF's relationship with commercial isotope-producer Nordion and discussed TRIUMF's long-standing research collaboration with the Pacific Parkinson's Research Centre at UBC and its expansion into more generalized neurology and brain imaging.  With a stop in ISAC-II to see IRIS, DESCANT, and a several other nuclear-physics detectors, the group then visited the ATLAS Tier-1 Data Centre and met with Operations Manager Reda Tafirout and ATLAS scientist Isabel Trigger.  The tour finished with a visit to the VECC test area where the first stage of the e-linac is being prototyped and developed.  Bob Laxdal, several students, and Ken Fong showed the RF systems and electron beamline and discussed the relationships with local industry and India's VECC laboratory.
Wrapping up the tour amidst pelting rain, Mr. Levesque thanked TRIUMF and the university hosts for the discussions.  On behalf of TRIUMF, Reiner expressed his appreciation for CFI's attention to Canadian excellence in research and innovation as well as the role that facilities like TRIUMF play in the larger enteprise.