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Carlos Silvestre Frenk | |
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![]() Frenk in 2012 | |
Born | 27 October 1951 |
Citizenship | British, German and Mexican |
Alma mater | University of Mexico (BSc) University of Cambridge (PhD) |
Known for | Navarro–Frenk–White profile |
Spouse | Dr. Susan Frenk |
Children | 2 |
Scientific career | |
Fields | Astrophysics |
Institutions | Durham University University of Sussex University of California, Santa Barbara University of California, Berkeley |
Thesis | Globular clusters in the galaxy and in the Large Magellanic Cloud (1981) |
Doctoral advisor | Bernard J. T. Jones |
Doctoral students | Ben Moore Gillian Wilson |
Website | https://astro.dur.ac.uk/~csf/homepage/index.html |
Carlos Silvestre Frenk CBE FRS (born 27 October 1951) is a Mexican-British cosmologist. [1] Frenk graduated from the National Autonomous University of Mexico and the University of Cambridge, spending his early research career in the United States before settling in the United Kingdom. He joined Durham University in 1986 and has served as the Ogden Professor of Fundamental Physics at the Durham University Department of Physics since 2001. [2]
Frenk's research has focused on galaxy formation, including his use of complex computer simulations to test theories on the origins and evolution of the universe. Alongside Marc Davis, George Efstathiou, and Simon White, he published a series of papers supporting the validity of the cold dark matter hypothesis. He was elected a Fellow of the Royal Society in 2004, among other recognitions. [2]
Carlos Frenk was born in Mexico City, Mexico, the eldest of six children. [3] His younger brother, Julio Frenk, is the former Mexican Secretary of Health. [4] His father, a German-Jewish physician, emigrated from Germany before World War II, while his mother was a Mexican–Spanish pianist. [5]
Frenk initially studied engineering at the National Autonomous University of Mexico before switching to theoretical physics, earning his undergraduate degree in 1976. [1] [5] He graduated in 1976 and received the Gabino Barreda Medal. [6]
In 1976, he secured a British Council Fellowship and enrolled at the University of Cambridge to read Part III of the Mathematical Tripos, which he completed in 1977. He remained at Cambridge for doctoral studies under the supervision of Bernard J. T. Jones. [7] His doctoral research explored the properties of the Milky Way, theorizing that the galaxy was surrounded by embedded dark matter. [6]
At Cambridge, Frenk shifted his research focus to cosmology and met future collaborator Simon White. [8] [6]
Following Cambridge, Frenk worked as a postdoctoral researcher at the University of California, Berkeley, where he assisted Marc Davis in interpreting his research which was based on a galaxy survey conducted during Davis' previous appointment at Harvard. Davis, Frenk, and White collaborated on research into the early state of the universe through the use of computer modelling. [6]
During the late 1970s, the neutrino had emerged as a natural dark matter candidate. In 1983, Davis, Frenk, and White argued in a paper that dark matter could not be made of neutrinos because, even if neutrinos had the required mass, they would move too quickly to be able to clump together and form galaxies. [6] [9] [10]
In 1983, Frenk left Berkeley for nearby Santa Barbara. He was officially attached to the University of Sussex from 1984 to 1985. [3] During these two years, he divided his time between Britain and America, alternating between three months in Santa Barbara and three at the University of Sussex. [11]
Davis, Frenk, and White recruited George Efstathiou, a recent PhD from Durham University, to help them with computational implementation. [6] [12] With Efstathiou, the group worked on a series of papers, focusing on the supersymmetric theory that dark matter particles were cold. [6]
In 1985, Frenk and his collaborators published a paper in The Astrophysical Journal sharing the first simulations of cold dark matter, which supported the validity of the now widely accepted cold dark matter theory for the formation of galaxies and other cosmic structures. [13] [a] [3]
In 1986, Frenk was appointed Lecturer at Durham University, later being promoted to Reader in 1991 and then full Professor in 1993. [3] [6]
Frenk and White's theories faced significant competition from other dark matter theories in the 80s and 90s. [6] The most prominent competing theory was Modified Newtonian dynamics, proposed by Israeli physicist Mordehai Milgrom in 1981. [14] Evidence from the Cosmic Background Explorer offered support for Frenk and White in 1993. [6]
In 1994, White was based at the Max Planck Institute for Astrophysics, and he and Frenk joined their institutions with other computational astronomers to form the Virgo Consortium, which had access to the supercomputing centre of the Max Planck Society in Garching and received funding from the UK government's 1994 High Performance Computing Initiative to build additional supercomputing resources. [6]
By the mid-1990s, the cold dark matter model had become widely accepted, and the focus of cosmological simulations shifted from the distribution of cold dark matter halos to the shapes of those halos. [13]
In 1996 and 1997, Frenk, White, and lead author Julio Navarro of the University of Arizona published results based on their analysis of halos from cold dark matter simulations. [13] This collaboration produced the Navarro-Frenk-White profile, a model profile for dark matter halos. The model describes the spatial mass distribution of dark matter within a halo, and is currently a widely used parametrization in the study of dark matter and galaxy formation. [13]
Following an endowment from Computacenter founder Peter Ogden in 2001, Frenk was named the inaugural Ogden Professor of Fundamental Physics at Durham University. [6] [b] He became the Director of the Institute for Computational Cosmology (ICC) upon its establishment in 2001, and held this post until 2020, at which point he was succeeded by Durham colleague Shaun Cole. [15] [16]
In 2005, as a member of the Virgo Consortium, Frenk was part of a team that produced the Millennium Run.
In 2020, Frenk was named a Clarivate Citation Laureate, which recognizes highly-cited research as "Nobel Class". [17] Along with Julio Navarro and Simon White, he was named a potential winner of the Nobel Prize in Physics in 2020 and 2021. [18] [c]
Frenk is married to Dr. Susan Frenk, a lecturer in Spanish and Latin American literature and Principal of St Aidan's College. They have two sons. [11]
Frenk has an interest in architecture, which was inspired by his experience studying at the main campus of the National Autonomous University of Mexico, a UNESCO World Heritage site. [20] He has reportedly taken an active role in the design process of new buildings at Durham University. [20]
Frenk was elected a Fellow of the Royal Society (FRS) in 2004. [21] He was appointed Commander of the Order of the British Empire (CBE) in the 2017 Birthday Honours for services to cosmology and the public dissemination of basic science. [22]
He received the Gold Medal of the Royal Astronomical Society in 2014. [23]
Other awards include the Royal Society Wolfson Research Merit Award (2006), the Daniel Chalonge Medal of the Paris Observatory (2007), the George Darwin Lectureship (2010), the Fred Hoyle Medal and Prize of the Institute of Physics (2010), the Gruber Prize in Cosmology (2011), the Max Born Prize of the German Physical Society (2017), the Dirac Medal and Prize of the Institute of Physics (2020), and the Rumford Medal (2021). [24] [25] [3] [26] [27] [28]
In 2023, he was named an Honorary Fellow of King's College, Cambridge, his postgraduate alma mater. [2] [29]
Frenk made his television debut in 1986 on an episode of the Australian series Beyond 2000 . He has made numerous appearances since then, including The Sky at Night for the BBC. [2] He has also appeared on BBC Radio on multiple occasions and was interviewed by Kirsty Young for Desert Island Discs , first broadcast in 2018. [5]