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Tribute given at the Memorial Service for Prof Edmund Zingu held on 25 April 2013 at the University of the Western Cape May 18, 2013

Posted by International.Chair in : Astronomy and Astrophysics (ASTRO), Condensed Matter and Materials Physics (CMMP), History, Policy and Education (HPE) , 1 comment so far

by Prof Patricia Whitelock

I have been asked by Simon Connell, the current President of SAIP to pay tribute to Edmund on behalf of SAIP, but I have also been asked by Ted Williams, the director of the South African Astronomical Observatory to speak on behalf of SAAO. That is important for me as I first met Edmund Zingu in 1995 at the 175th anniversary of the observatory and I came to know him as a personal friend as well as a valued colleague. He was then head of physics at UWC and I had the pleasure of showing him around and was impressed and intrigued by his interest and perceptive questions.  It was the start of a relationship between SAAO and UWC that has gradually strengthened over the years and which will ultimately allow the two organizations to do great things in astrophysics.

You will have your personal memories of Edmund but he was best known to the broader community through his service with SAIP and that is what I want to talk about. As you have already heard Edmund served on the Council of the SAIP for 8 years from 1999 to 2006, as VP from two years while I was President then as President from 2003 to 2004. It would not be an exaggeration to say that when Edmund joined the Council, physics in SA was in crisis. The numbers of undergraduate students enrolling had been dropping for several years, the image of physics among the public and decision makers was poor, finance for physics projects was very limited and the SAIP itself, particularly its leadership, was not representative of the community of physicists in SA,  and people rightly wanted to know what SAIP was going to do.

By the time Edmund left the SAIP council, physics in SA was in a very different place. That was of course due to the combined efforts of a number people, but Edmund was without question was one of the most important. In 2001 Council set up a transformation committee with a very broad mandate to look at all aspects of the SAIP. Edmund and I both served on that committee. The initial driving force for transformation came from Nithaya Chetty, but Edmund, who chaired the committee while he was VP, was absolutely crucial in keeping the debate focused and most importantly keeping us all talking to each other.

These years were particularly exciting as we grappled with the problems in physics at the same time as attempting to restructure the SAIP to play a more relevant role in SA society. My entire experience of working with Edmund was a positive one.  He was someone you could test ideas on and who would tell you very gently and very sympathetically when and why you had got it wrong.  I don’t know if we could have done what we did without him, but I very much doubt it. What I am certain of is that it would have been more difficult and there would have been many more casualties and more blood on the walls. I would like to quote from Jaynie Padayachee, who was secretary of the SAIP during my and Edmund’s presidency and who was also secretary of the transformation committee: “The one thing about Edmund that will always stay with me, is that he personified diplomacy. It was really inspirational (in this world of too many words and opinions) knowing someone who took the time to think about what he was going to say before he said it. “

During my term as President I quickly came to rely on Edmund’s judgment and his support above anything and anyone else.  I suspect that there are many others who must have had similar experiences. He was never heavy handed or unpleasantly forceful, when things were said that he did not agree with he would gently point out that not everyone had the same experience and that there were other ways of looking at issues. It was quiet, it was gentle, it was undemonstrative and it dramatically effective. I quote from Jappie Engelbrecht, who is the treasurer of SAIP, as he was when Edmund and I were President: Japie after reading Simon Connell’s words about Edmund responded “I have nothing to add except my sadness at the passing of a truly great South African, whose impact on my own life enabled me to transform to our new democracy.”His words apply to many of us who worked with Edmund.

Those transformation activities resulted in a revised constitution and by-laws for the SAIP, more involvement of the specialist groups in council, a president who was directly elected by the membership, and a new mindset and symbolism of a new logo to prove it. That of course took several more years.

At roughly the same time that we started the transformation process, in fact really as part of the same initiative we established the process that culminated in an international panel review and the production of a document: “Shaping the future of physics in South Africa”.  This process was lead by Edmund during his presidency and must have taken up a huge amount of his personal time. This led to a new strategy for physics, and among other things establishment of the National Institute of Theoretical Physics (NITheP) and to the increased financial support from government that enabled SAIP to appoint an Executive Officer – which has been so important in allowing SAIP to do things more professionally.

One of the international participants in the shaping the future process, was Jim Gates, who as many of you know is now on USA President’s scientific advisory panel. The following words were written by Jim Gates and express Edmund’s role better than I can:

I am certain now that the Shaping Report has served exceedingly well as a national strategy and planning document for the South African physics community in a manner that none of its authors had foreseen in terms of its scope, duration or effectiveness. Dr. Zingu’s management of the entire Shaping process was a marvelous testament of his dedicated to the health of the physics field in South Africa.   His skills as a manager of personnel were on direct display, from my perspective, in the assembly of the International panel. He chose persons from S.A., from Europe, and the U.S.A. as a reflection of his understanding of the international and global nature of the interaction required for physics to thrive in S.A. in the new millennium. He also saw the International Panel was assembled in such a way as to be a final executive part of the process that lived up to his high expectation and vision.

The Shaping Report is among the greatest of tributes to Dr. Zingu as it continues almost a decade latter to have a substantial impact on thinking about South African physics. The report challenged all of the stake-holding communities to plan on multiple levels. “

He goes on to describe his personal gratitude to Edmund as a mentor for giving him the skills that he has particularly needed and which prepared him for his role as advisor to President Barack Obama

Since leaving the SAIP Council Edmund has continued to serve the community. In particular he has again played the leadership role in the Review of Physics Teaching, which is currently underway – the next big hurdle in the success of physics in SA, or indeed globally. I have no direct experience of his work with this, but Simon Connell tells me that he handled the project magnificently. In fact has been so well constructed by Edmund that neither SAIP nor CHE have any concern about its completion.

There can be no doubt that Physics and South Africa are better off because Edmund Zingu was who he was, when he was. We,as physicists and as friends of Edmund, have every reason to thank his family and to join them in celebration of a life extraordinarily well lived in the service of our community.

In Memoriam: Edmund C. Zingu April 26, 2013

Posted by International.Chair in : Condensed Matter and Materials Physics (CMMP), History, Policy and Education (HPE), Physics Education Research (PER), Technology Transfer, Business Development and Entrepreneurism (TBE) , 2comments

Zingu
Professor Edmund Zingu served on the South African Institute of Physics (SAIP) Council from 1999 to 2006, and was President of the SAIP from 2003 to 2004.  He was in fact the first black President in the history of the SAIP[1].

He played crucial leadership roles in many projects, particularly in physics related development issues.  He was Vice President of the IUPAP, and Chair of the C13 Commission on Physics for Development.  He was primarily responsible for bringing to South Africa the iconic ‘Physics for Sustainable Development’ conference in 2005[2] as a part of the International Year of Physics.  This conference cast a distinct spotlight on physics as an instrument for development in Africa.

We would like to specifically mention his tremendous contribution to two extremely important projects of the Institute.  The first was the highly successful Shaping the Future of Physics, where he contributed to the design of the project and also served as chair of the Management and Policy Committee that oversaw the international review in 2003.

The Shaping the Future of Physics in South Africa report was written by a body designated as the ‘International Panel’ or IP.  The IP was composed of M. A. Hellberg (convenor), M. Ducloy, K. Bharuth-Ram, K. Evans-Lutterodt, I. Gledhill, G. X. Tessema, A.W. Wolfendale, and S. J Gates.  The report has served exceedingly well as a national strategy and planning document for the South African physics community in a manner that none of its authors had foreseen in terms of its scope, duration or effectiveness.

Dr. Zingu’s management of the entire Shaping process was a marvelous testament of his dedication to the health of the physics field in South Africa.  His skills as a manager of personnel were on direct display in the assembly of the IP.  He advocated for selection of representatives from South Africa (Bharuth-Ram, Gledhill, and Hellberg), from Europe (Ducloy, and Wolfendale), and the USA (Evans-Lutterodt, Gates, and Tessema) as a reflection of his understanding of the global nature of the interactions required for physics to thrive in South Africa in the new millennium.  He also saw to it that the IP was assembled in such a way as to be a final executive part of the process that lived up to his high expectation and vision.

The Shaping Report is among the greatest of tributes to Dr. Zingu as it continues almost a decade later to have a substantial impact on thinking about South African physics.  The report challenged all of the stake-holding communities to plan on multiple levels.  Projects like the projects like the SAIP Executive Office, National Institute for Theoretical Physics (NiTheP), South African National Research Network (SANReN), SA-CERN, and SKA-Africa have become a reality.  The report called also for the possibility of other ‘flagship’ projects such as a South African synchrotron, to drive the large scale development of the field, and there has been significant encouraging progress here.  At the more granular level there was a call for transformation so that the field would be open to all citizens of the country.  Physics in South Africa has grown significantly since then, largely because of the implementation of many of the recommendations from the Review.  Also during this time Dr. Zingu authored the very influential article, Promoting Physics and Development in Africa, which appeared in Physics Today[3].

For one of us (Gates), the Shaping Report was preparation for service as a policy advisor for both the Governor of Maryland (via my role on the Maryland State Board of Education) and for President Barack Obama (via my role on the U.S. President’s Council of Advisors on Science & Technology – PCAST).  These accomplishments are due in part to Edmund’s confidence in me and his abilities as a mentor.  I owe this great South African an enormous debt of gratitude for how he challenged me to grow professionally.

The second project was the Review of Undergraduate Physics Education.  Once again he contributed to the design of the Review and chaired the Management and Policy Committee.  He led the development of the South Africa Draft Benchmark Statement for Physics Training, and guided the Review process, including the partnership with the Council for Higher Education.  The Review of Physics Training is well advanced but still in progress.

Professor Zingu began his physics career at the University of the Western Cape (UWC).  He was a materials physicist, and with his collaborators at Cornell University invented a new method to study atomic diffusion by transmission electron microscopy[4].  Later he studied diffusion phase transitions in thin films due to induced thermal stress[5].  He had a period of employment at Turfloop, QwaQwa Campus, then as Head of the Physics Department and later Dean of Basic Sciences (1990-1993) at MEDUNSA.  He later returned to UWC and served as Head of the Physics Department (1994-1998), and finally Vice Rector of Mangosuthu University of Technology in Umlazi, Durban until the time of his retirement.

Edmund was a pioneer for physics in post-apartheid South Africa, a visionary, a tireless campaigner for strengthening the discipline of physics* and, above all, a true gentleman.  His leadership and contributions were characterized by sensitivity, perceptiveness, vision, ethics, wisdom, global standards and great industry.  He will be sorely missed.

Simon Connell
President, South African Institute of Physics (2012-2014)

Nithaya Chetty
President, South African Institute of Physics (2007-2009)

S. James Gates, Jr.
President, National Society of Black Physicists (1996-1998)

More comments from Dr. Zingu’s friends and colleagues

Professor Zingu was a dear friend and professional colleague over the past ten years.  He was extremely helpful during the deliberations of the 2004 Review of iThemba LABS that I chaired for the National Research Foundation.  During that time, Professor Zingu was President of the South African Institute of Physics.  In another effort, he was one of the main drivers in working with Professor Alfred Msezane of Clark Atlanta University and a number of us at the African Laser Centre to organize the 1st US-Africa Advanced Studies Institute on Photon Interactions with Atoms and Molecules.  That institute convened in Durban during November 2005, just after the World Conference on Physics and Sustainable Development, which was part of the United Nation’s International Year of Physics.  Professor Zingu leaves a tremendous legacy for all African and other peoples to emulate.  We will miss his kind demeanor and tremendous insights into the future.
Sekazi K. Mtingwa

I met Prof. Edmund Zingu nearly 20-years ago in November 1995 at the University of the Western Cape, in Cape Town, where he was Chair of the Physics Department. Edmund invited me on my first travel to South Africa for nearly two-weeks to  lecture on Ultrafast Optical Phenomena at several institutions — U. of Port Elizabeth, the National Accelerator Centre, U. of Cape Town, U. of Witwatersrand, U. of the Western Cape and the Foundation for Research Development (analog of the US National Science Foundation). This was the first and only time that I spent time away from my family during Thanksgiving, and Edmund provided a warm and inviting environment for my visit. I spent several days with Edmund’s wonderful family and learned a great deal about South Africa and its people. Arriving not long after the release of Nelson Mandela and the official end of Apartheid, Edmund with his gentle, soft-spoken and brilliant nature alleviated my natural apprehension of visiting South Africa at that time. I had a truly wonderful visit and scientific exchange orchestrated by Prof. Edmund Zingu and I am truly saddened by the loss of this extraordinary individual — my deepest condolences go out to his family.
Anthony M. Johnson

Two weeks ago, at a diaspora gathering for STEM in Africa, the challenge that African scientists face on the continent was discussed. The critical question was “How can academics in Africa get the attention of the leaders?”  The idea of international advisory panels modeled after the 2004 Shaping panel was received with much enthusiasm. The composition of the panel, the charge to the panel, and the implementation was such a testimony of the high quality of the leadership of SAIP under Edmond Zingu. May he rest in peace.
Tessema G.X.

To this excellent tribute, I would like to add my personal sadness at the passing of a truly great South African, whose impact on my own life enabled me to transform to our new democracy.
Japie Engelbrecht

 


[1] Physics Today, Vol 54 (9) Sept 2001, p 27, http://dx.doi.org/10.1063/1.1420507

[2] Physics World, October 2005, pp 12-13, http://physicsworld.com/cws/archive/print/18/10

[3] Physics Today, Vol 57 (1) Jan 2004, p 37, http://dx.doi.org/10.1063/1.1650068

[4] Chen, S. H., L. R. Zheng, J. C. Barbour, E. C. Zingu, L. S. Hung, C. B. Carter, and J. W. Mayer. “Lateral-diffusion couples studied by transmission electron microscopy.” Materials Letters 2, no. 6 (1984): 469-476. http://dx.doi.org/10.1016/0167-577X(84)90075-2

Zingu, E. C., J. W. Mayer, C. Comrie, and R. Pretorius. “Mobility of Pd and Si in Pd2Si.” Physical Review B 30, no. 10 (1984): 5916. http://dx.doi.org/10.1103/PhysRevB.30.5916

[5] Zingu, E. C., and B. T. Mofokeng. “Diffusional Phase Transformation under Induced Thermal Stress.” In MRS Proceedings, vol. 230, no. 1. Cambridge University Press, 1991. http://dx.doi.org/10.1557/PROC-230-145

Zingu, E. C., and B. T. Mofokeng. “Stress Relaxation During Diffusional Phase Transformation Under Induced Thermal Stress.” In Materials Research Society Symposium Proceedings, vol. 308, pp. 85-85. Materials Research Society, 1994. http://dx.doi.org/10.1557/PROC-308-85

Diale, M., C. Challens, and E. C. Zingu. “Cobalt self‐diffusion during cobalt silicide growth.” Applied Physics Letters, vol. 62, no. 9 (1993): pp 943-945. http://dx.doi.org/10.1063/1.108527

[6] P. Whitelock,  Tribute given at the Memorial Service for Prof Edmund Zingu held on 25 April 2013 at the University of the Western Cape

Dr. Kartik Sheth, ALMA, and SKA March 19, 2013

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by JC Holbrook

National Society of Black Physicists members Eric Wilcots and Kartik Sheth were part of a new initiative to foster radio astronomy collaborations with South African astronomers and students. Last week marked the official inauguration of ALMA, the Atacama Large Millimeter/Submillimeter Array, in the high altitude Atacama desert of Chile, South America. I was able to sit down with Dr. Sheth to discuss the broader issue of radio astronomy and South Africa.

“I think this celebration was the culmination of thirty years worth of work from a lot of different people. The inauguration of the array was a chance for us to celebrate how much hard work has gone into it.” Dr. Sheth said of the inauguration ceremony in Chile. “We started science operations September 30th of 2011. We have been collecting data for over two and a half years, because even with a small ALMA it is still the most powerful [millimeter/submillimeter] telescope in the world.”

Since ALMA is an array of dishes similar to the radio dishes of the Very Large Array in New Mexico, even during construction as each dish was put into place and connected, the astronomers were already using what was available to collect data. Thus, the months of science data collection with ALMA before the official inauguration.

I pointed out, “You were not even there!”

Dr. Sheth laughed, “Only the dignitaries were invited, so a lot of people from the political arena in the twenty-five plus countries that are part of ALMA. President Piñera inaugurated ALMA…For me it doesn’t mean much… but I’m kinda sad that I’m not there because I really wanted to be there. But I knew that I wasn’t going to be invited, so coming here [to South Africa] really was driven by the NASSP deadline for Master’s proposals.” NASSP is the National Astrophysics and Space Sciences Programme in South Africa. In 2010, I began writing a book about NASSP. The program is a dramatic success story about educating underrepresented groups in astrophysics and space sciences. NASSP include one honor year and a two year masters of science degree. Nearly all NASSP students are funded by the program.

Dr. Sheth explained, “The idea is to foster bridges between the faculty here that are taking on students who eventually want to work with MeerKat and SKA. But MeerKAT and SKA are not built, yet. So, what we would really like the faculty to do is to think about including radio data from existing telescopes and NRAO operates four of them.”

The SKA is currently under construction, yet the South African astronomy students need to learn everything about radio astronomy and the analysis of radio data. Dr. Sheth along with other American radio astronomers is here to encourage South African astronomers and their students the opportunity to learn by working with the existing facilities and their archival data. The four facilities are ALMA, the Robert C. Byrd Greenbank telescope a single dish in West Virginia, the Jansky Very Large Array (JVLA or EVLA) which is the enhanced VLA in New Mexico, and the Very Large Baseline Array (VLBA) which is spread across the Northern Hemisphere. Thus, the visit before the NASSP deadline for submitting Masters of Science thesis proposals. Dr. Sheth hopes that a few NASSP students will propose radio astronomy projects including using NRAO facilities for their Masters work.

According to Dr. Sheth the JVLA is the Northern Hemisphere equivalent of what MeerKat will be. MeerKat is the precursor to the SKA, the Square Kilometer Array.  It is a new state of the art radio observatory currently being built in South Africa. The SKA array itself will consist of 3000 dishes spread across nine African countries: South Africa, Namibia, Botswana, Mozambique, Madagascar, Mauritius, Zambia, Ghana, and Kenya. The SKA Africa headquarters are in Cape Town, South Africa, and they will be coordinating all of the African construction. A question I thought would be uppermost in the minds of South Africans was: Will ALMA be competition for SKA?

His response, “No, not at all. ALMA operates at higher frequencies than what the SKA will operate at. They are not looking at the same part of the electromagnetic spectrum but they will be looking at the same type of objects. EVLA is a mini version of SKA. With the SKA, it will be observing thermal emission and synchrotron emission from sources…” In an email he added, “We are looking at electrons energy as they cool around star forming regions or zip around magnetic fields. So you can get a real idea of the magnetic field that pervades the Milky Way and with the SKA across cosmic time. ALMA cannot really look at atomic gas unless its at very high red shift (i.e. the lines are red shifted into the regime that ALMA can observe) and only using atomic gas tracers like ionized carbon, nitrogen, or oxygen. ALMA cannot look at the atomic hydrogen gas which is emitting in the wavelengths that MeerKat and SKA will work at. So SKA & Meerkat are looking at the atomic gas from which molecular gas forms. And the molecular gas is what ALMA looks at which from stars form. And the stars are what HST and JWST look at. So it is a nice transition.  Together these are giving you the full picture of what the universe looks like. Additionally there is a lot about magnetic fields and transient phenomena — these are also MeerKat and SKA’s core strengths. For instance, these will be excellent instruments for looking at the timing of pulsars.”

Trying to put it altogether I asked, “So, anything that is hot and has electrons moving around will be able to be studied by SKA?”

Kartik Sheth clarified, “No, I wouldn’t call it ‘hot’. The atomic gas is quite cold as well. It is hotter than the molecular gas but not hot compared to stars.”

As a student of astronomy, I had always had a fascination with the connection between wavelengths of light or color, physical properties, chemistry, and celestial bodies. Planetary nebulae, which are mentioned in my last Vector blog, in visible light appear greenish in color. The color is the result of a specific atomic transition in the oxygen atom that occurs under very low density conditions. First the oxygen has to be ionized twice, i.e. it has to have lost two electrons, then it is through collisions that the transitions producing the characteristic green lines emit. A rule-of-thumb temperature for planetary nebulae is 10,000 degrees Kelvin. Thus, if there is a celestial body that appears ‘green’ in visible light you can conclude that it might include oxygen especially if it is a nebula which tends to have low density and it should be around 10,000 degrees Kelvin. Hydrogen is also found in planetary nebulae and the strongest transition line, known as H-alpha, occurs when its electron goes from an excited state to a less excited state releasing energy in the form of red light.

In the case of ALMA and SKA, they are probing two different sections of the electromagnetic spectrum similar to studying green light or red light. In the fullness of time, SKA will cover the same wavelengths and types of celestial bodies as the EVLA but focused on the Southern sky rather than the Northern, but also be more sensitive revealing more physical details. ALMA will add to our understanding of the same region of the sky but is studying different physical properties of celestial bodies. Both will add to our understanding of the Milky Way and the Universe.

NSBP members visit South Africa to strengthen ties March 15, 2013

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NSBP members Kartik Sheth and Eric Wilcots along with National Radio Astronomy Observatory (NRAO) astronomer Scott Ransom have been in South Africa to cement linkages for a NRAO’s faculty bridge program. NSBP, the South African Institute of Physics (SAIP), NRAO and others are working together on the science dimension of the US-South Africa Bilateral Strategic Dialogue.

The visit is intended to foster partnerships in multi-wavelength astronomy research.  Last week they had meetings with astronomers and cosmologists at University of Cape Town, University of Western Cape, SAAO, the SKA Africa Project Office and the African Institute of Mathematical Sciences (AIMS).  This week they will also meet with high energy astrophysicists at the Potchefstroom campus of North-West University, University of Johannesburg, and University of Witswatersrand, as well as astronomers at the North-West University campus in Mafikeng, and the Hartebeesthoek Radio Astronomy Observatory (HartRAO).

As South Africa builds a second NASSP site, teaching and research partnerships with NRAO will be beneficial on both sides of the Atlantic. NRAO currently operates four premier radio astronomy observatories: ALMA, JVLA, GBT and the VLBA.  NRAO is likely to also be a partner in helping to train scientists across the continent to be operators and users of the African VLBI Network (AVN). The AVN project consists of converting large, redundant telecommunications dishes across Africa for radio astronomy. The AVN will become part of the global VLBI network.

In addition to major radio astronomy successes, South Africa’s strategic plan for astronomy calls for its institutions to be active in multiple wavelengths including radio, optical, gamma/x-ray, and near IR. South Africa is the host of the Southern Africa Large Telescope (SALT), the largest optical telescope in the southern hemisphere. Wilcots is a member of the SALT board. South Africa is also supporting the Namibian bid to host the Cherenkov Telescope Array (CTA), the next generation success to the H.E.S.S telescope that has been in Namibia since 2002. Following an exchange at the 2011 NSBP conference, South Africa and the LIGO Collaboration have begun exploring opportunities in gravitational wave astronomy. Already LIGO and SAIP have convened a faculty workshop and a student summer school, both in Pretoria.

In a separate but simultaneous visit, Jim Gates participated in South Africa’s National Science Festival (SciFest), giving talks at several venues around the country on science policy and supersymmetry.  ScieFest was established in 1996 to promote the public awareness, understanding and appreciation of science, technology, engineering, mathematics and innovation. The main event in Grahamstown, held in March every year, attracts 72,000 visitors from South Africa, Botswana, Lesotho, Mozambique, Namibia, Swaziland and Zimbabwe. Several government departments, listed companies, museums, NGOs, research facilities, science centers, science councils, universities, as well as small, medium and micro enterprises, both from South Africa and abroad contribute to the success of the event.

Gates was on the same program as South Africa’s Minister of Science and Technology, Derek Hanekom.  Each discussed science and innovation policy and gave their perspectives on aligning science with national priorities. Additionally Gates participated in three formal policy meetings, including one with Simphiwe Duma, CEO of the Technology Innovation Agency, and two more informal policy meetings.  In a lecture at the University of South Africa (UNISA) he and Dr. Rob Adam, former head to South Africa’s National Research Foundation, spoke on the efficacy of policy-formation surrounding STEM fields and the innovation cycle.

In other events around the country Gates met 45 students spanning the 8th through 11th grade levels at the Mae Jemison Science Reading Room in the Mamelodi township.  At Nelson Mandela Metropolitan University and the University of Johannesburg he gave talks on the strange mathematical objects found in the equations of supersymmetry.

These meetings and exchanges involving NSBP and South African colleagues are all part of the evolution from ideas put into motion by the Nobel Laureate, Abdus Salaam, and the founders of the Edward Bouchet-Abdus Salaam Institute (EBASI). Over a decade ago former NSBP president, Charles McGruder, traveled to South Africa to explore possible linkages between astronomers.  That visit led to Khotso Mokhele’s participation in the 2004 NSBP conference.  At the time he was the head of South Africa’s National Research Foundation. Later NSBP won a grant from the WK Kellogg Foundation to support NSBP’s participation the NASSP program. In the year’s since, NSBP has partnered with SAIP on a number of projects, and the relationship was codified in at MOU signed at the 2011 NSBP conference and witnessed by Minister Naledi Pandor.  The relationships between NSBP, SAIP as well as colleagues across the entire continent continue to evolve and vistas are opening up in the realms of geophysics, biophysics and medical physics, nuclear and particle physics, mathematical and computational physics, as well as physics education at all levels.

Unfinished Business in Astronomy March 11, 2013

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JC Holbrook

My master’s thesis in astronomy at San Diego State University focused on the electron temperature structure of the ionized gas of planetary nebulae. I focused on two planetary nebulae: NGC 6572 and NGC 6543. I observed using the one meter telescope at Mt. Laguna Observatory with a CCD detector. Planetary nebula are created as low mass stars throw off their atmosphere during their transition to white dwarfs. My observations and analysis of NGC 6572 revealed a knot of high temperature gas well away from but connected to the nebula. I could not explain what the knot was but submitted the paper in 1992 to ApJ with my advisor Theodore Daub. The referee reports insisted that we take spectra of the knot. JPL’s Trina Ray took spectra but we still could not identify the hot knot. The project was left behind as I left SDSU for NASA and a doctorate. However, a week ago I looked up images of NGC 6572 and got a big surprise! The Hubble Space Telescope image showed a far bigger nebula than what we could detect twenty years ago! Though it has been several years, looking at the contours I estimate that the hot spot I found, which at that point was at the edge of the nebula, I have marked with a circle in the second image. The structure of NGC 6572 is much more complicated than what I was working with and it is clear that some of the assumptions that went into the temperature would need to be updated to fully determine if the knot was indeed as hot as calculated. Certainly, some eager young astronomy student has already unraveled this bit of unfinished business!

The First Telescope Has Arrived for the Total Solar Eclipse in Cairns and “Black Sun” November 11, 2012

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by JC Holbrook

Dr. Alphonse Sterling arrived safely in Cairns with telescope, mount, filters, cameras, and a suitcase. His excess baggage fees were unmentionable. The blue case is the body of the telescope. Alphonse is staying about 30 minutes to the west of Cairns in the Trinity Beach area in a very swank three bedroom apartment with ocean views. He will be sharing the apartment with scientific teammembers students Amy Steele and Roderick Gray.

In preparation for the eclipse, Alphonse has to create a ‘flat’ image as part of the calibration of the flaws in the telescope. When doing traditional night observing at an observatory, flats are taken of the dome. That is, before you start observing you put diffuse light onto the dome of the telescope and take a series of images. What is revealed is any specs of dust in the optics and other flaws. Next, the astronomer would go on to observe the celestial bodies and at dawn take another series of flats. When processing the images of the celestial bodies these flats would be used to remove the optical flaws thus flattening the images. This way what you have is just what is found in space not some artifact left by the optics of the telescope.

When doing observations of the Sun, daytime observing, creating a flat is not so simple. Alphonse has experimented with multiple different light sources to determine which is the best for creating a good flat.
What he found is he has to rig something up himself. That meant that we had to go to the hardware store to find the parts he needed!

After a long search we found: exacto knife, white cardboard, LCD flashlight, masking tape, electrical switch, compass. He had his own wire to create an external switch for his new light source. Over the next couple of days he will be putting everything together. I can’t wait to see what the final device will look like!

Be part of “Black Sun” donate today at
https://www.austinfilm.org/film-black-sun.

NSBP members descend upon Australia for more than just a total solar eclipse November 2, 2012

Posted by admin in : Astronomy and Astrophysics (ASTRO), Cosmology, Gravitation, and Relativity (CGR), Earth and Planetary Systems Sciences (EPSS), History, Policy and Education (HPE) , add a comment

The Total Solar Eclipse is just days away and will cut a path through the South Pacific. This week sees the start of NSBP members traveling to exotic locations to do more than bask in the unique environment of totality. NSBP members will meet in Cairns, Australia, which is predicted to have the best eclipse viewing. Dr. Hakeem Oluseyi of the Florida Institute of Technology will be using the eclipse to study the lower atmosphere of the Sun. He will be working with a group of students and telescopes and cameras to capture scientific images that will inform his research. Dr. Alphonse Sterling, who has yet to attend an NSBP meeting, of NASA Marshall Space Flight Center will be flying in from his assignment in Tokyo, Japan. He too will be taking images of the lower atmosphere of the Sun for his scientific research.

The opportunity to see two African American astrophysicists leading research teams and doing their science was too much for NSBP member Dr. Jarita Holbrook.  She is making a film, Black Sun, to chronicle this event. After a successful Kickstarter campaign, Dr. Holbrook and her documentary film team from KZP Productions began by filming Dr. Sterling during the May annular eclipse in Tokyo. After an amazing experience, an 8-minute short film was made chronicling the event. Now it is time to bring Hakeem into the picture!

Black Sun is still seeking funding to complete this ground-breaking film project. Donations are tax deductable via . Help Jarita to inspire the next generation of African American astrophysicists by donating today – no donation is too small!  Jarita is on her way today to lay the groundwork for the documentary. Follow her tweets @astroholbrook.

Dr. Alphonse Sterling making observations

Dr. Alphonse Sterling analyzing data

Members discuss the Higgs discovery July 6, 2012

Posted by admin in : Cosmology, Gravitation, and Relativity (CGR), Nuclear and Particle Physics (NPP) , 2comments

This is certainly an exciting development at CERN! My group and I are in the four lepton working group.  We apply a multivariate analysis to data and simulations to arrive at our results, which is in agreement and supports what was shown by Fabiola.

We see excesses in the gamma-gamma and four lepton channel, but not the bbar or WW channels at least in the 2011 dataset.  It may be just statistics, or the way the data is analyzed in the other channels, but the branching ratios for a Higgs boson are predicted with great confidence (only the mass is a free parameter in the SM).  The WW and bbar and tau channels have large bf, larger than gamma-gamma and 4 lepton.  The former channels have larger backgrounds and it is harder to tease out any excess.  So that may explain this question (in my mind at least it is a bit puzzling).  Also, the gamma-gamma channel can have heavy states contributing to the process that signals new physics beyond even the Higgs, if this result holds up.  And note that we don’t yet have enough data to determine the intrinsic spin or parity of whatever particle may be attributed to this excess.

What this all means is that, in my opinion, we will need to wait until more data is collected before a definitive statement can be made about a Higgs or not. Now the real work begins.  What is this new particle?  Is it the Standard Model Higgs boson?  Is it one of several new states? Is it a scalar or pseudoscalar?  Etc. Etc.  Very exciting times!

Professor O. Keith Baker, Yale University

SUSY among all the other ideas out there (extra-dimensions, branes, etc.) is the unique one that is brought to the fore by the light mass Higgs boson that seems just around the corner from having a final discovery announcement. None of the other candidates for what comes after the Higgs discovery have any such implications to my knowledge.

SUSY is also he only one that is brought to the fore if multiple Higgs bosons are ultimately found. SUSY actually requires multiple Higgs bosons and their superpartners.

The SUSY extension of the Standard Model that has been most extensively studied is called the `Minimal SUSY Standard Model’ or MSSM. As there are literally scores and scores of undetermined parameters, it is not definitive about the likely mass hierarchy of the Higgs family. There is also the NMSSM (the `next to mimimal supersymmetrical Standard Model) which has even more parameters and thus is even less definitive about the properties of any Higgs families. In fact, Superstring/M-Theory suggests that even the NMSSM is not the complete story.

There is a Minimal Supersymmetric Standard Model wiki page that has a pretty good discussion of its properties. There can be found here a discussion of the need for why at least a second Higgs boson must exist in the context of the MSSM. Also there is this lecture available on You Tube.

While the MSSM is not so predictive about the masses, it does make very definite predictions about the charges and coupling to the electroweak forces by members of the Higgs family.

Professor S. James Gates, University of Maryland-College Park

As a theorist I’d say that SUSY has “nice” properties of stabilizing the vacuum, but it also restricts the theoretical hand from just adding anything to the theory arbitrarily. For example one might ask where does the SM Lagrangian (without SUSY) for the Higgs come from (it’s just a polynomial interaction) as it does not seem to be based on a principle like the gauge principle that is used in other interactions or SUSY. The answer is that “well it works” to give spontaneously broken symmetry but there may be many ways to get into this spontaneously broken phase theoretically. Gauge theories and SUSY can control, through symmetry, what the interactions look like which also forces certain particles for consistency. That is why SUSY needs more than one Higgs for example. This makes SUSY, in some sense (limited to our imaginative ways to use SUSY) easier to rule out if Nature has no need for SUSY. But even as SUSY starts to experimentally manifest itself (and I believe it will soon), the next big question is “what breaks SUSY?”.

Professor Vincent Rodgers, University of Iowa

Even if this thing is the Higgs, this discovery itself cannot be the only new physics.  The hierarchy problem in physics (the divergence of the Higgs mass at much higher energies) requires something that stabilizes it.  The most likely candidate, as far as I can tell, is SUSY, just as Professor Gates wrote.

In SUSY, there are an additional four Higgs bosons, at least in the SUSY models I am familiar with.  So Rolf’s statement about which Higgs refers to this dilemma.  Is this thing reported on yesterday the SM Higgs, or one of the SUSY Higgs? If the latter, then there should be more waiting to be found.

SUSY is not the only solution to the hierarchy problem.  But it is probably the most developed theoretically.  In my opinion, the simplest SUSY models seem to be ruled out over much of its parameter space by some precision experiments like edm expts.  Jim may want to clarify this for me.  So if SUSY exists, it is likely some of the MSSM models, or beyond.  Also, as I understand the theory, a heavy Higgs comes into tension with SUSY.  If this 125-126 GeV thing is a Higgs, it is in a difficult but doable region for MSSM of some sort.

Professor O. Keith Baker, Yale University

The whole event was really thrilling, and I was especially glad to see the payoff from our efforts to enhance and better model the ATLAS detector’s performance in intense luminosity conditions. This demonstrates that we are ready not only for discoveries, but also for the following studies to more conclusively identify this new boson.

I concur with our theorists that even if this is a Higgs discovery, our job of explaining how the SM works so well in this energy regime will be far from finished — a lot of my recent work at ATLAS has been related to this area of SUSY and other “exotic model” searches.

But, like Keith, I am especially interested in the couplings of this new particle to third-generation fermions, where the little data ATLAS and CMS have — and it’s far too little for me to place bets yet — do leave room for a lot of surprises to come in.

The implication for hadron collider physicists of my generation — the ones too late to discover the top quark, who relentlessly probed it at the Tevatron and LHC to check for any deviations from SM predictions — is that a new space has opened up for similar tests. Once again, we can easily envision likely ways to make significant contributions to our understanding of the particle universe (hurray!).

Professor Ayana Arce, Duke University

The discovery of the Higgs-like particle is the culmination of a lot of efforts for many years by so many people. I started on the ATLAS Experiment in 1998, I contributed to various aspects of the ATLAS experiments and held many positions in the ATLAS Collaboration. I was ATLAS Higgs working group convener in 2008-2010. In this capacity, I led and directed the analysis efforts of the ATLAS Higgs working group. So, I can confidently say that my work contributed directly in the search and discovery of this new particle. It is a significant achievement that will lead to the capacity building and training for younger students, an improvement understanding of fundamental physics, and ultimately technological spin-offs to the benefits of humanity. It is truly a great pleasure for me to work with so many people across the world and to participate directly in such a monumental discovery that may revolutionize our lives in the years to come.”

Dr. Ketevi A. Assamagan, Permanent Staff Physicist, Brookhaven National Laboratory

At last – there is exciting and long awaited news of a new Higgs-like boson. South Africans scientists, students and computer experts have participated in these exciting developments. “It’s a global experiment, and we have six of our Universities participating at CERN” says Prof Jean Cleymans, leader of the SA-CERN programme, which launched almost four years ago.

The Department of Science and Technology selected CERN as one of its global large-scale infrastructure projects; it supports scientists in the South Africa-CERN consortium to participate in experiments to investigate the existence of the Higgs boson particle and other expected discoveries. The Department is proud of these scientists who are part of this major scientific breakthrough and celebrates this achievement with the rest of the world.

Tantalizing hints of a new particle with a mass around 126 GeV were reported in December 2011. ATLAS and CMS, two of the CERN experiments, have today not only confirmed these hints with data taken in 2012, but also done so with sufficient confidence (5 sigma each) to claim a new particle has been observed. A 5 sigma confidence means that the error due to statistical fluctuations has a probability of less than 1 in 1.7 million (or rolling a dice eight times to get a six each time). Furthermore, the new particle interacts similarly to the Higgs boson. The Higgs boson is reputed to endow mass to other particles. This new Higgs-like boson will now be subjected to intense and detailed study, over some decades, and while exploring this, we may make further surprising discoveries.

Although we don’t have a crystal ball to predict the full benefits to science and society, we note that most of today’s understanding of nature and the development of technology began with the discovery of the now familiar particles like the electron. We are at a new beginning. The LHC may also shed light on the primordial state of matter, shortly after the Big Bang, and on dark matter and dark energy.

The LHC at CERN is a global experiment, and South African participation at CERN enables the highest quality scientific research, manpower development, technology transfer and innovation. The South African computing Grid was established as a result of the CERN involvement. This is a combination of fast networks and high performance computing clusters. It forms the basis of data processing and analysis for CERN. It will also provide valuable lessons for the SKA and data intensive computing in general. Other spinoffs are expected in diagnostic and therapeutic medicine, remote sensing and nuclear technology, to name a few other fields.

Statement by SA-CERN Programme

Lessons learned (so far) from the superluminal neutrino episode April 7, 2012

Posted by admin in : Astronomy and Astrophysics (ASTRO), Cosmology, Gravitation, and Relativity (CGR), Nuclear and Particle Physics (NPP) , add a comment

Reprinted from Waves and Packets, April 7,2012 edition

With the March 15 paper of the ICARUS group claiming no advance effect for their (seven) neutrino events, it seems the urgency and interest in this matter is dwindling. OPERA spokesperson Antonio Ereditato and experimental coordinator Dario Autiero have announced their resignations, following a controversial vote of “no confidence” from the collaboration’s other leaders. Waves and Packets has asked three distinguished physicists what they think the lessons learned are from the entire episode.

“It is misconception that Einstein’s special theory of relativity says that nothing can travel faster than the speed of light. For example, electrons can travel faster than the speed of light in water. This leads to a phenomena known as Cherenkov radiation which is seen as a blue glow in nuclear reactors. In addition, for a long time it’s been speculated that subatomic particles known as a tachyons might exist. Tachyons are theoretically predicted particles that travel faster than the speed of light in a vacuum and are consistent with Einstein’s theory of relativity. For ordinary subliminal particles light acts as a barrier from above. That is ordinary matter cannot be accelerated to the speed of light. For superluminal tachyons light acts as a barrier from below. That is to say that tachyons cannot be decelerated to the speed of light. It has been conjectured that tachyons could be used to send signals back in time. To date tachyons have not been observed experimentally.” Ronald Mallett, University of Connecticut-Storrs

“I think the first thing the whole episode indicates is that there is still enormous public interest in our field. The need to explore is still felt keenly so we need to be clear that announcing results, even controversial ones, should be respected by scientists if proper peer review of those results has been performed. It also points out the absolute necessity of following through on external checks. Public review of the scientific process is not a bad thing nor is showing some humility and skepticism even about ‘sacred’ principles like special relativity. Episodes like this one give us the opportunity to address misconceptions like those surrounding the connection between special relativity and the speed of light. Showing fallibility doesn’t weaken us as long as we remain appropriate demanding of ‘extraordinary proof’ for “extraordinary results.” Larry Gladney, University of Pennsylvania

“I can think of two positive remarks to be made. The first is that, given an information leak from someone familiar with the OPERA experiment to Science magazine, the OPERA Collaboration did the right thing in going public with the information they had at hand. In the spirit of good science, they nearly begged other experiments to validate or invalidate their working hypothesis of superluminal neutrinos. It now appears that invalidation was in order, as reported by the ICARUS experiment. Over the next several months, we may anticipate half a dozen experiments on three continents providing further measurements of neutrino speed; new data will also be forthcoming from the OPERA and ICARUS experiments. My second positive remark is that many of us have been pushed by the OPERA claim to examine the deeper meaning of Special and General Relativity. While paradoxes, such as superluminal travel with inherent negation of cause and effect, are mathematically consistent with Einstein’s equations, they generally are hidden behind horizons, or require invocation of new physics such as negative energy, extra dimensions, sterile neutrinos, etc. It has been fun and educational to think about the possibilities. Any opportunity to explore a guarded secret of Nature must be seized upon. It unfortunately appears now that superluminal neutrino travel may not be one of Her guarded secrets.” Thomas Weiler, Vanderbilt University

What’s your view? Contact Waves and Packets at editors@wavesandpackets.org.

NSBP Member, Hakeem Oluseyi, selected to be a TEDGlobal 2012 Fellow March 31, 2012

Posted by admin in : Astronomy and Astrophysics (ASTRO), Cosmology, Gravitation, and Relativity (CGR), Earth and Planetary Systems Sciences (EPSS), History, Policy and Education (HPE), Photonics and Optics (POP), Technology Transfer, Business Development and Entrepreneurism (TBE) , add a comment
Florida Institute of Technology professor, Hakeem Oluseyi, has been selected to be 2012 TED Global Fellow.  He will participate in the TED conference in Edinburgh, Scotland, June 25-29.  Dr. Oluseyi is an astrophysicist, inventor and science educator whose research focuses on measuring the structure and evolution of the Milky Way galaxy and characterizing new planetary systems.  Oluseyi has lectured widely in the US and Africa.  He was one of the founding members of the African Astronomical Society and is currently an officer of the National Society of Black Physicists.  TED is a nonprofit devoted to Ideas Worth Spreading. It started out (in 1984) as a conference bringing together people from three worlds: Technology, Entertainment, Design.  Past TED Fellows include CERN’s Bilge Demirkoz, Harvard’s Michelle Borkin, and NASA’s Lucianne Walkowicz.
 
Dr. Hakeem M. Oluseyi is an astrophysicist with research interests in the fields of solar and stellar variability, Galactic structure, and technology development.   After receiving his B.S. degrees in Physics & Mathematics from Tougaloo College in 1991, he went on earn his Ph.D. at Stanford University with an award winning dissertation, "Development of a Global Model of the Solar Atmosphere with an Emphasis on the Solar Transition Region."  His Ph.D. adviser was legendary astrophysicist, Arthur B. C.  Walker.
 
During his tenure at Stanford, Oluseyi participated in the pioneering application of normal-incidence, EUV multilayer optics to astronomical observing as a member of the Stanford team that flew the Multi-Spectral Solar Telescope Array (MSSTA) in a series of rocket flights from 1987 to 1994.  This technology has now become the standard for solar EUV imaging.  He was a major contributor to the analyses that illustrated flows in solar polar plumes for the first time and also showed for the first time that plumes were not the sources of the high-speed solar wind as was believed.  He also led the effort that discovered the structures responsible for the bulk of solar upper transition region (plasmas in the temperature range from 0.1 – 1.0 MK) emission and ultimately presented a new model for the structure of the Sun's hot atmosphere. 
 
After leaving Stanford in 1999 Dr. Oluseyi joined the technical staff at Applied Materials, Inc. where he invented several new patented processes for manufacturing next-generation, sub 0.1-micron, refractory metal transistor gate electrodes on very thin traditional and high-k dielectrics.  He also developed patented processes for in-situ spectroscopic process control and diagnostics, facilitating elimination of test wafers in semiconductor manufacturing.  This work has resulted in 7 U.S.  patents and 4 E.U.  patent.
 
In 2001 Dr. Oluseyi joined the staff of Lawrence Berkeley National Laboratory (LBNL) as an Ernest O. Lawrence Postdoctoral Fellow.  There he established a new laboratory, the CCD Production Facility, and developed new techniques for characterizing and packaging large-format, thick (300 micron), p-channel charge coupled devices (CCDs).  As a member of the SuperNova Acceleration Probe (SNAP) satellite collaboration and the Supernova Cosmology Project at LBNL, Dr. Oluseyi participated in the development of high-resistivity p-channel CCDs and performed spectroscopic observation of supernovae utilizing the Shane Spectrometer on the Lick Observatory's Nickel 3-m telescope. 
 
In January 2004 Dr. Oluseyi joined the physics faculty of The University of Alabama in Huntsville where he continued his research in solar physics, cosmology, and technology development but also focused on increasing the number of Black astrophysicists.   His efforts have thus far resulted in producing one of only two Black female solar physicists working in the U.S., mentoring a total of three African American graduate students, and six African graduate students. 
 
Oluseyi also began working extensively in Africa beginning in 2002.  He visited hundreds of schools and worked directly with thousands of students in Swaziland, South Africa, Zambia, Tanzania, and Kenya as a member of Cosmos Education in the years 2002, 2003, 2004.  In 2005 he began working with the South African Astronomical Observatory.  In 2006 he was the co-organizer of the 2006 Total Solar Eclipse Conference on Science and Culture.  Also in 2006, he co-founded a thriving Hands-On Universe branch in Nairobi, Kenya.  In subsequent years he worked with other teams dedicated to improving science research in Africa including the 2007 International Heliophysical Year conference in Addis Ababa, Ethiopia and the First Middle-East Africa, Regional IAU Meeting in Cairo, Egypt in 2008. 
 

 
Also in 2008 he began working with at-risk graduate students in the Extended Honors Program at the University of Cape Town (UCT) in collaboration with the South African Astronomical Observatory (SAAO) and the National Society of Black Physicists.  Oluseyi lectured physics and cosmology to UCT students in 2008 and 2009.  In 2010, he lectured and mentored students in the SAAO/UCT Astronomy Winter School. 
 
During 2010 and 2011, Oluseyi played a central role in establishing the African Astronomical Society (AfAS), the first continent-wide organization of African astronomy professionals.  He was a participant in the IAU-sponsored meeting of the Interim Leadership Group for forming the AfAS, and subsequently served as the Interim President of the AfAS until its official launch in April 2011. 
 
In May 2011, Oluseyi conducted a 6-city tour of South Africa as a Speaker & Specialist for the U.S. State Department.  During his visit he visited dozens of schools, museums and science centers, working with thousands of students, and a multitude of teachers, education administrators, and researchers.  In fall 2011 Oluseyi and professors at the University of Johannesburg won a grant from the U.S. State Department to found a Hands-On Universe branch in Soweto, South Africa. 
 
Oluseyi plans to return to South Africa to work with UCT students including leading observational research projects at the SAAO observatories in Sutherland.  Oluseyi also has ongoing research programs in collaboration with SAAO and University of Johannesburg scientists.
 
In January 2007 Dr. Oluseyi was invited to join the Department of Physics & Space Sciences at the Florida Institute of Technology.  He has since established a large research group that studies solar variability using space-based instruments, studies Galactic structure and stellar properties using periodic variable stars as probes, and is measuring the characteristics of extrasolar planetary systems using data from the LINEAR and KELT surveys and meter-class telescopes in North America and Chile.  He is a member of the Variables & Transients science collaboration for the Large Synoptic Survey Telescope.  Oluseyi recently founded the first observational astronomy consortium consisting primarily of minority-serving colleges and universities.
 

 
Dr. Oluseyi has won several honors including selection as a TED Global Fellow (2012), as a Speaker & Specialist for the U.S.  State Department, Outstanding Technical Innovation and Best Paper at the NSBE Aerospace Conference (2010), NASA Earth/Sun Science New Investigator fellow (2006), the 2006 Technical Achiever of the Year in Physics by the National Technical Association, selection as the Gordon & Betty Moore Foundation Astrophysics Research Fellow (2003-2005), and as an E. O. Lawrence Astrophysics Research Fellow (2001-2004), and winner of the NSBP Distinguished Dissertation award (2002).