Qaisar Shafi | |
|---|---|
 Dr. Shafi in 2020 | |
| Nationality | Pakistani, American, British |
| Alma mater | Imperial College |
| Awards | Fellow of the American Physical Society; Alexander von Humboldt Prize (1997) |
| Scientific career | |
| Fields | Theoretical Physics, Cosmology |
| Doctoral advisor | Abdus Salam |
| Doctoral students | Cem Salih Ün |
Qaisar Shafi is a Pakistani-American theoretical physicist and the Inaugural Bartol Research Institute Professor of Physics at the University of Delaware. [1]
Shafi grew up in Karachi, Pakistan and lived there until his early teens when his family moved to London, United Kingdom. [2] After graduating as valedictorian from Holland Park School, London, UK, he studied physics at Imperial College, London, where he received both his B.Sc. Honors and PhD. His PhD advisor was the late Nobel Laureate Professor Abdus Salam, whom he subsequently joined at the International Centre for Theoretical Physics (ICTP) in Trieste, Italy. [3] Shafi was awarded an Alexander von Humboldt Prize and spent some years in Germany (Munich, Aachen, and Freiburg). [4] In 1978, he received his Habilitation with Venia Legendi from the University of Freiburg. He then spent two years at CERN (Geneva, Switzerland) after which he moved to the United States. [5] Since 1983, Shafi has been a faculty member at the Bartol Research Institute, University of Delaware, which in 2005 merged with the Department of Physics and Astronomy.
Shafi has done pioneering research in areas ranging from Grand Unification to Kaluza-Klein theories, to inflationary cosmology and supersymmetric theories, and he is widely regarded as a leader in these fields. He has published more than 300 papers in refereed journals, among them many of the most prestigious in the field, lectured at close to 250 conferences, workshops, and universities. [6]
Contemporary high energy physics could be subdivided into the energy frontier, the cosmic frontier and the intensity frontier. Shafi, whose work is highly interdisciplinary, has made pioneering contributions in all three areas. Shafi’s work has focused on Grand Unified Theories (GUTs), Yukawa coupling unification, dark matter and collider physics, inflationary cosmology, topological defects, thermal inflation, superstring phenomenology and related topics. [7] His pioneering works include:
Shafi has done also extensive outreach work for the scientific community. From the early 1980s until 1997, he organized/co-organized several weeks long summer schools at the International Centre for Theoretical Physics in Trieste. For more than fifteen years, Shafi was one of the key organizers for each summer school. [22]
In addition, he was also one of the principal organizers of the BCVSPIN (acronym denoting the countries Bangladesh-China-Vietnam-Sri Lanka-Pakistan-India-Nepal) schools, which he co-founded in 1989 with Professors Abdus Salam, Jogesh Pati and Yu-Lu. [23] [24] The concept underlying BCVSPIN was to allow young scientists living in underserved regions to engage in research. Professor Shafi organized, lectured at, and led numerous BCVSPIN schools as well as associated preparatory schools, and thus helped lay the groundwork for the successful careers of many graduate students and postdoctoral fellows while also keeping track of their progress. He directed or co-directed the BCVSPIN summer schools from 1989 to 1997 and after a hiatus of several years, caused by the shifting political climate in Nepal, single-handedly resurrected the school in 2007, organizing highly successful schools in China, Vietnam and also branching out to Mexico. [25]
Qaisar Shafi is married to Monika Shafi, the Elias Ahuja Professor Emerita of German Literature at the University of Delaware. They have a daughter and a son. [26]
In physical cosmology, cosmic inflation, cosmological inflation, or just inflation, is a theory of exponential expansion of space in the very early universe. Following the inflationary period, the universe continued to expand, but at a slower rate. The re-acceleration of this slowing expansion due to dark energy began after the universe was already over 7.7 billion years old.
Grand Unified Theory (GUT) is any model in particle physics that merges the electromagnetic, weak, and strong forces into a single force at high energies. Although this unified force has not been directly observed, many GUT models theorize its existence. If the unification of these three interactions is possible, it raises the possibility that there was a grand unification epoch in the very early universe in which these three fundamental interactions were not yet distinct.
The ekpyrotic universe is a cosmological model of the early universe that explains the origin of the large-scale structure of the cosmos. The model has also been incorporated in the cyclic universe theory, which proposes a complete cosmological history, both the past and future.
Supersymmetry is a theoretical framework in physics that suggests the existence of a symmetry between particles with integer spin (bosons) and particles with half-integer spin (fermions). It proposes that for every known particle, there exists a partner particle with different spin properties. There have been multiple experiments on supersymmetry that have failed to provide evidence that it exists in nature. If evidence is found, supersymmetry could help explain certain phenomena, such as the nature of dark matter and the hierarchy problem in particle physics.
Cosmic strings are hypothetical 1-dimensional topological defects which may have formed during a symmetry-breaking phase transition in the early universe when the topology of the vacuum manifold associated to this symmetry breaking was not simply connected. Their existence was first contemplated by the theoretical physicist Tom Kibble in the 1970s.
Cumrun Vafa is an Iranian-American theoretical physicist and the Hollis Professor of Mathematics and Natural Philosophy at Harvard University.
In theoretical physics, the hierarchy problem is the problem concerning the large discrepancy between aspects of the weak force and gravity. There is no scientific consensus on why, for example, the weak force is 1024 times stronger than gravity.
Sir Thomas Walter Bannerman Kibble was a British theoretical physicist, senior research investigator at the Blackett Laboratory and Emeritus Professor of Theoretical Physics at Imperial College London. His research interests were in quantum field theory, especially the interface between high-energy particle physics and cosmology. He is best known as one of the first to describe the Higgs mechanism, and for his research on topological defects. From the 1950s he was concerned about the nuclear arms race and from 1970 took leading roles in promoting the social responsibility of the scientist.
Montonen–Olive duality or electric–magnetic duality is the oldest known example of strong–weak duality or S-duality according to current terminology. It generalizes the electro-magnetic symmetry of Maxwell's equations by stating that magnetic monopoles, which are usually viewed as emergent quasiparticles that are "composite", can in fact be viewed as "elementary" quantized particles with electrons playing the reverse role of "composite" topological solitons; the viewpoints are equivalent and the situation dependent on the duality. It was later proven to hold true when dealing with a N = 4 supersymmetric Yang–Mills theory. It is named after Finnish physicist Claus Montonen and British physicist David Olive after they proposed the idea in their academic paper Magnetic monopoles as gauge particles? where they state:
There should be two "dual equivalent" field formulations of the same theory in which electric (Noether) and magnetic (topological) quantum numbers exchange roles.
Alexander Vilenkin is the Leonard Jane Holmes Bernstein Professor of Evolutionary Science and Director of the Institute of Cosmology at Tufts University. A theoretical physicist who has been working in the field of cosmology for 25 years, Vilenkin has written over 260 publications.
Savas Dimopoulos is a particle physicist at Stanford University. He worked at CERN from 1994 to 1997. Dimopoulos is well known for his work on constructing theories beyond the Standard Model.
Eternal inflation is a hypothetical inflationary universe model, which is itself an outgrowth or extension of the Big Bang theory.
Sze-Hoi Henry Tye is a Chinese-American cosmologist and theoretical physicist most notable for proposing that relative brane motion could cause cosmic inflation as well as his work on superstring theory, brane cosmology and elementary particle physics. He had his primary and secondary school education in Hong Kong. Graduated from La Salle College. He received his B.S. from the California Institute of Technology and his Ph.D. in physics from the Massachusetts Institute of Technology under Francis Low. He is the Horace White Professor of Physics, Emeritus, at Cornell University and a fellow of the American Physical Society. He joined the Hong Kong University of Science and Technology in 2011 and was the Director of HKUST Jockey Club Institute for Advanced Study during 2011-2016.
Christopher T. Hill is an American theoretical physicist at the Fermi National Accelerator Laboratory who did undergraduate work in physics at M.I.T., and graduate work at Caltech. Hill's Ph.D. thesis, "Higgs Scalars and the Nonleptonic Weak Interactions" (1977) contains one of the first detailed discussions of the two-Higgs-doublet model and its impact upon weak interactions. His work mainly focuses on new physics that can be probed in laboratory experiments or cosmology.
Renata Elizaveta Kallosh is a Russian-American theoretical physicist. She is a professor of physics at Stanford University, working there on supergravity, string theory and inflationary cosmology.
In quantum field theory in curved spacetime, there is a whole class of quantum states over a background de Sitter space which are invariant under all the isometries: the alpha-vacua. Among them there is a particular one whose associated Green functions verify a condition consisting to behave on the light-cone as in flat space. This state is usually called the Bunch–Davies vacuum or Euclidean vacuum, actually was first obtained by N.A. Chernikov and E. A. Tagirov, in 1968 and later by C. Schomblond and P. Spindel, in 1976, in the framework of a general discussion about invariant Green functions on de Sitter space. The Bunch–Davies vacuum can also be described as being generated by an infinite time trace from the condition that the scale of quantum fluctuations is much smaller than the Hubble scale. The state possesses no quanta at the asymptotic past infinity.
Augusto Sagnotti is an Italian theoretical physicist at Scuola Normale.
Peter Christopher West, born on 4 December 1951, is a British theoretical physicist at King's College, London and a fellow of the Royal Society.
Atish Dabholkar is an Indian theoretical physicist. He is currently the Director of the Abdus Salam International Centre for Theoretical Physics (ICTP) with the rank of Assistant Director-General, UNESCO. Prior to that, he was head of ICTP's High Energy, Cosmology and Astroparticle Physics section, and also Directeur de Recherche at the Centre National de la Recherche Scientifique (CNRS) at Sorbonne University in the "Laboratoire de Physique Théorique et Hautes Énergies" (LPTHE).
The Bartol Research Institute is a scientific research institution at the Department of Physics and Astronomy of the University of Delaware. Its members belong to the faculty of the University of Delaware and perform research in areas such as astroparticle physics, astrophysics, cosmology, particle physics, and space science.
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