Brian Keating

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Brian Keating
Brian Keating 2022.jpg
BornSeptember 9, 1971  OOjs UI icon edit-ltr-progressive.svg
Alma mater
Occupation
Awards
Website https://briankeating.com   OOjs UI icon edit-ltr-progressive.svg
Academic career
Institutions
Thesis A search for the large angular scale polarization of the cosmic microwave background
Doctoral advisor Peter Timbie

Brian Gregory Keating (born September 9, 1971) is an American cosmologist. He works on observations of the cosmic microwave background, leading the BICEP, POLARBEAR2 and Simons Array experiments. He received his PhD in 2000, and is a distinguished professor of physics at University of California, San Diego, since 2019. He is the author of two books, Losing The Nobel Prize and Into the Impossible.

Contents

Personal life

Keating was born on September 9, 1971, [1] the son of the mathematician James Ax, [2] and his wife Barbara. [3] When he was about seven, his parents divorced and his mother remarried, and the young Brian took his stepfather's name, Keating. He was out of contact with his father for the next 15 years, reconnecting only when he was a graduate student. Keating grew up in Dobbs Ferry, New York. [3] He has 3 brothers. Kevin, Nick and Shaya. [2]

As a youth, Keating was a member of the Catholic Church, although he's reported that his mother and stepfather were non-observant Jews. He later became an atheist, and subsequently he became Jewish, currently describing himself as a 'practicing devout agnostic'. [2]

As well as a cosmologist, he is a pilot with a multi-engine turbine license. [4] He was a trustee of Math for America, San Diego in 2006–2014, Angel Flight West in 2010–2015, and the National Museum of Mathematics in 2014–2017. He is currently a trustee of San Diego Air & Space Museum since 2013, and is on the Ruben H. Fleet Museum advisory council since 2017. [5]

Education and career

Keating received his B.S. degree in Physics from the Case Western Reserve University in 1993. [4] [5] He then obtained his M.S. degree in Physics from Brown University in 1995, and subsequently studied for his Ph.D. also at Brown. [5] His thesis, titled A search for the large angular scale polarization of the cosmic microwave background and supervised by Peter Timbie, was accepted in 2000. [6] He started as a National Science Foundation (NSF) postdoctoral fellow at the California Institute of Technology in 2001 [7] until 2004. He was an assistant professor at the University of California, San Diego from 2004, before being promoted to associate professor there in 2009. [5] He received an NSF career grant in 2005, and a Presidential Early Career Award in 2006. [8] Keating was one of three scientists, along with Jonathan Kaufman and Bradley Johnson, to receive the Buchalter Cosmology Prize in 2014. [9] He became co-director of the Ax Center for Experimental Cosmology and the Joan & Irwin Jacobs Program in Astrophysics in 2013. [5]

Keating became a professor at UC San Diego in 2014. [5] He became a Fellow of the American Physical Society in 2016. [10] [11] In 2019 he became the Chancellor’s Distinguished Professor of Physics at UC San Diego, [10] [12] in the Center for Astrophysics & Space Sciences, [13] which is part of the Department of Physics. [14] Keating received an Excellence in Stewardship Award in 2018/19, and is an honorary member of the National Society of Black Physicists. [15] He is co-director of the Arthur C. Clarke Center for the Human Imagination at UC San Diego. [16] He received the Horace Mann Medal from Brown University Graduate School in 2022. [17]

Research

Keating researches cosmology, focusing on the study of the cosmic microwave background and its relationship to the origin and evolution of the universe. [18] He conceived the BICEP (Background Imaging of Cosmic Extragalactic Polarization) instrument, which observed from the South Pole. [19] BICEP received a NASA Group Achievement Award in 2010. [20] In 2016 he convinced the Simons Foundation, controlled by his biological father's business partner and former classmate, to provide US$38.4m of funding for what later became the Simons Array, [21] and in 2019 a US$20m grant from the Simons Foundation led to the creation of the Simons Observatory, [22] followed by an additional US$4.6m in 2021. [23] Keating co-leads POLARBEAR2 and the Simons Array in Chile, [15] and has raised around US$100m of funding for CMB telescopes. [24] He has two patents, on a "wide-bandwidth polarization modulator for microwave and mm-wavelengths" in 2009, [25] and "Tunnel junction fabrication" in 2016. [26]

Podcast and outreach

Keating presenting at the Royal Institution in 2023 Brian Keating at the Royal Institution 2023 10.jpg
Keating presenting at the Royal Institution in 2023

Keating has hosted the Clarke Center Into the Impossible podcast since 2016. [5] It takes its name from the second of Clarke's three laws: "The only way of discovering the limits of the possible is to venture a little way past them into the impossible." Each episode is a long-form conversation with nobel laureates, scientists, writers and other notable individuals such as Stephen C. Meyer (an advocate of the pseudoscience of intelligent design [28] [29] ), Noam Chomsky, Eric Weinstein, Jill Tarter, Sara Seager, and nobel prize winners interviewed for his books, [16] lasting around an hour. As of 2022 it has hosted 11 Nobel Prize winners and two recipients of the Pulitzer Prize. [24] It reached 200,000 subscribers in 2024. [30]

Keating also appeared in The Michael Shermer Show  [ d ] podcast in 2019, [31] and the Lex Fridman Podcast in 2022. [32] He has also recorded videos for PragerU, [33] and has talked about popular science connected with The Witcher television series. [34] He appeared in the "Mysteries Of The Moon" episode of The UnXplained. [35]

He also teaches astronomy to high school students since 2012 as part of his outreach work, [15] [5] and has given presentations to over 3,000 K-12 students since 1994. [5]

He has also co-narrated a 21-hour audio book of Galileo Galilei's Dialogue Concerning the Two Chief World Systems in 2022. [36]

Books about the Nobel Prize

Keating is critical of the way that Nobel Prizes are organized, saying that "No scientist arrives alone in Stockholm." He has written two books on the topic. [37] The Nobel Prize was a motivating factor in Keating's career due to his academic rivalry with his father. [38]

Losing The Nobel Prize (2018)

Keating published his first book Losing the Nobel Prize: A Story of Cosmology, Ambition, and the Perils of Science’s Highest Honor on April 24, 2018. [3] [19] The book describes the BICEP and BICEP2 experiments, which were located at the South Pole and were devised to detect and map the polarization of the cosmic microwave background radiation leftover from the Big Bang. BICEP2's data showed strong polarization signals that were announced to be cosmological in origin, but were later shown by Planck satellite data to be caused by polarized interstellar dust.

The first part of the book describes the background behind cosmological inflation, and the second covers BICEP2. The third section focuses on Keating's issues with the Nobel Prize, including lack of diversity in the recipients, that the prize can't be awarded posthumously, [18] the maximum of three laureates per prize, which excludes larger groups from receiving it, [39] and the secrecy around nominations. According to Keating, all of these "reward an outdated version of science", [40] and "better science comes from inclusivity, collaboration, and innovation". [19] He argues that the science Nobel Prizes have strayed from the original intent of Alfred Nobel's will, and may hinder scientific progress by fostering unnecessary, and sometimes destructive, competition. [41] He proposed that half a Nobel prize should go to the leaders of a collaboration, with the other half awarded to the rest of the team of scientists working on the project. [42]

Into the Impossible (2021)

His second book, Into the Impossible, was published in 2021. [1] It features interviews with Nobel Prize winners Adam Riess, Rainer Weiss, Sheldon Glashow, Carl Wieman, Roger Penrose, Duncan Haldane, Frank Wilczek, John C. Mather and Barry Barish. [43]

Related Research Articles

<span class="mw-page-title-main">Cosmic microwave background</span> Trace radiation from the early universe

The cosmic microwave background is microwave radiation that fills all space in the observable universe. It is a remnant that provides an important source of data on the primordial universe. With a standard optical telescope, the background space between stars and galaxies is almost completely dark. However, a sufficiently sensitive radio telescope detects a faint background glow that is almost uniform and is not associated with any star, galaxy, or other object. This glow is strongest in the microwave region of the radio spectrum. The accidental discovery of the CMB in 1965 by American radio astronomers Arno Penzias and Robert Wilson was the culmination of work initiated in the 1940s.

<span class="mw-page-title-main">Wilkinson Microwave Anisotropy Probe</span> NASA satellite of the Explorer program

The Wilkinson Microwave Anisotropy Probe (WMAP), originally known as the Microwave Anisotropy Probe, was a NASA spacecraft operating from 2001 to 2010 which measured temperature differences across the sky in the cosmic microwave background (CMB) – the radiant heat remaining from the Big Bang. Headed by Professor Charles L. Bennett of Johns Hopkins University, the mission was developed in a joint partnership between the NASA Goddard Space Flight Center and Princeton University. The WMAP spacecraft was launched on 30 June 2001 from Florida. The WMAP mission succeeded the COBE space mission and was the second medium-class (MIDEX) spacecraft in the NASA Explorer program. In 2003, MAP was renamed WMAP in honor of cosmologist David Todd Wilkinson (1935–2002), who had been a member of the mission's science team. After nine years of operations, WMAP was switched off in 2010, following the launch of the more advanced Planck spacecraft by European Space Agency (ESA) in 2009.

<span class="mw-page-title-main">Arno Allan Penzias</span> American physicist (1933–2024)

Arno Allan Penzias was an American physicist and radio astronomer. Along with Robert Woodrow Wilson, he discovered the cosmic microwave background radiation, for which he shared the Nobel Prize in Physics in 1978.

<span class="mw-page-title-main">Rashid Sunyaev</span> Russian astronomer (born 1943)

Rashid Alievich Sunyaev is a German, Soviet, and Russian astrophysicist of Tatar descent. He got his MS degree from the Moscow Institute of Physics and Technology (MIPT) in 1966. He became a professor at MIPT in 1974. Sunyaev was the head of the High Energy Astrophysics Department of the Russian Academy of Sciences, and has been chief scientist of the Academy's Space Research Institute since 1992. He has also been a director of the Max Planck Institute for Astrophysics in Garching, Germany since 1996, and Maureen and John Hendricks Distinguished Visiting Professor in the School of Natural Sciences at the Institute for Advanced Study in Princeton since 2010.

The discovery of cosmic microwave background radiation constitutes a major development in modern physical cosmology. In 1964, US physicist Arno Allan Penzias and radio-astronomer Robert Woodrow Wilson discovered the cosmic microwave background (CMB), estimating its temperature as 3.5 K, as they experimented with the Holmdel Horn Antenna. The new measurements were accepted as important evidence for a hot early Universe and as evidence against the rival steady state theory as theoretical work around 1950 showed the need for a CMB for consistency with the simplest relativistic universe models. In 1978, Penzias and Wilson were awarded the Nobel Prize for Physics for their joint measurement. There had been a prior measurement of the cosmic background radiation (CMB) by Andrew McKellar in 1941 at an effective temperature of 2.3 K using CN stellar absorption lines observed by W. S. Adams. Although no reference to the CMB is made by McKellar, it was not until much later after the Penzias and Wilson measurements that the significance of this measurement was understood.

In physical cosmology, the inflationary epoch was the period in the evolution of the early universe when, according to inflation theory, the universe underwent an extremely rapid exponential expansion. This rapid expansion increased the linear dimensions of the early universe by a factor of at least 1026 (and possibly a much larger factor), and so increased its volume by a factor of at least 1078. Expansion by a factor of 1026 is equivalent to expanding an object 1 nanometer (10−9 m, about half the width of a molecule of DNA) in length to one approximately 10.6 light years (about 62 trillion miles) long.

<i>Planck</i> (spacecraft) European cosmic microwave background observatory; medium-class mission in the ESA Science Programme

Planck was a space observatory operated by the European Space Agency (ESA) from 2009 to 2013. It was an ambitious project that aimed to map the anisotropies of the cosmic microwave background (CMB) at microwave and infrared frequencies, with high sensitivity and small angular resolution. The mission was highly successful and substantially improved upon observations made by the NASA Wilkinson Microwave Anisotropy Probe (WMAP).

<span class="mw-page-title-main">South Pole Telescope</span> Telescope at the South Pole

The South Pole Telescope (SPT) is a 10-metre (390 in) diameter telescope located at the Amundsen–Scott South Pole Station, Antarctica. The telescope is designed for observations in the microwave, millimeter-wave, and submillimeter-wave regions of the electromagnetic spectrum, with the particular design goal of measuring the faint, diffuse emission from the cosmic microwave background (CMB). The first major survey with the SPT—designed to find distant, massive, clusters of galaxies through their interaction with the CMB, with the goal of constraining the dark energy equation of state—was completed in October 2011. In early 2012, a new camera (SPTpol) was installed on the SPT with even greater sensitivity and the capability to measure the polarization of incoming light. This camera operated from 2012–2016 and was used to make unprecedentedly deep high-resolution maps of hundreds of square degrees of the Southern sky. In 2017, the third-generation camera SPT-3G was installed on the telescope, providing nearly an order-of-magnitude increase in mapping speed over SPTpol.

<span class="mw-page-title-main">Atacama Cosmology Telescope</span> Telescope in the Atacama Desert, northern Chile

The Atacama Cosmology Telescope (ACT) was a cosmological millimeter-wave telescope located on Cerro Toco in the Atacama Desert in the north of Chile. ACT made high-sensitivity, arcminute resolution, microwave-wavelength surveys of the sky in order to study the cosmic microwave background radiation (CMB), the relic radiation left by the Big Bang process. Located 40 km from San Pedro de Atacama, at an altitude of 5,190 metres (17,030 ft), it was one of the highest ground-based telescopes in the world.

<span class="mw-page-title-main">George Smoot</span> American astrophysicist and cosmologist

George Fitzgerald Smoot III is an American astrophysicist, cosmologist, Nobel laureate, and the second contestant to win the $1 million prize on Are You Smarter than a 5th Grader?. He won the Nobel Prize in Physics in 2006 for his work on the Cosmic Background Explorer with John C. Mather that led to the "discovery of the black body form and anisotropy of the cosmic microwave background radiation".

<span class="mw-page-title-main">Charles L. Bennett</span> American astronomer

Charles L. Bennett is an American observational astrophysicist. He is a Bloomberg Distinguished Professor, the Alumni Centennial Professor of Physics and Astronomy and a Gilman Scholar at Johns Hopkins University. He is the Principal Investigator of NASA's highly successful Wilkinson Microwave Anisotropy Probe (WMAP).

<span class="mw-page-title-main">BICEP and Keck Array</span> Series of cosmic microwave background experiments at the South Pole

BICEP and the Keck Array are a series of cosmic microwave background (CMB) experiments. They aim to measure the polarization of the CMB; in particular, measuring the B-mode of the CMB. The experiments have had five generations of instrumentation, consisting of BICEP1, BICEP2, the Keck Array, BICEP3, and the BICEP Array. The Keck Array started observations in 2012 and BICEP3 has been fully operational since May 2016, with the BICEP Array beginning installation in 2017/18.

<span class="mw-page-title-main">Uroš Seljak</span> Slovenian cosmologist

Uroš Seljak is a Slovenian cosmologist and a professor of astronomy and physics at University of California, Berkeley. He is particularly well-known for his research in cosmology and approximate Bayesian statistical methods.

<span class="mw-page-title-main">POLARBEAR</span>

POLARBEAR is a cosmic microwave background polarization experiment located in the Atacama Desert of northern Chile in the Antofagasta Region. The POLARBEAR experiment is mounted on the Huan Tran Telescope (HTT) at the James Ax Observatory in the Chajnantor Science Reserve. The HTT is located near the Atacama Cosmology Telescope on the slopes of Cerro Toco at an altitude of nearly 5,200 m (17,100 ft).

John Michael Kovac is an American physicist and astronomer. His cosmology research, conducted at the Center for Astrophysics | Harvard & Smithsonian in Cambridge, Massachusetts, focuses on observations of the Cosmic Microwave Background (CMB) to reveal signatures of the physics that drove the birth of the universe, the creation of its structure, and its present-day expansion. Currently, Kovac is Professor of Astronomy and Physics at Harvard University.

<span class="mw-page-title-main">Simons Observatory</span> Observatory in Chile

The Simons Observatory is located in the high Atacama Desert in Northern Chile inside the Chajnator Science Preserve, at an altitude of 5,200 meters (17,000 ft). The Atacama Cosmology Telescope (ACT) and the Simons Array are located nearby and these experiments are currently making observations of the Cosmic Microwave Background (CMB). Their goals are to study how the universe began, what it is made of, and how it evolved to its current state. The Simons Observatory shares many of the same goals but aims to take advantage of advances in technology to make far more precise and diverse measurements. In addition, it is envisaged that many aspects of the Simons Observatory will be pathfinders for the future CMB-S4 array.

Michele Limon is an Italian research scientist at the University of Pennsylvania. Limon studied physics at the Università degli Studi di Milano in Milan, Italy and completed his post-doctoral work at the University of California, Berkeley. He has been conducting research for more than 30 years and has experience in the design of ground, balloon and space-based instrumentation. His academic specialties include Astrophysics, Cosmology, Instrumentation Development, and Cryogenics.

Clement Laurence Pryke is an English-American physicist, focusing in astrophysics and cosmology, particularly on the cosmic microwave background.

<span class="mw-page-title-main">Hiranya Peiris</span> British astrophysicist (born 1974)

Hiranya Vajramani Peiris is a British astrophysicist at the University of Cambridge, where she holds the Professorship of Astrophysics (1909). She is best known for her work on the cosmic microwave background radiation, and interdisciplinary links between cosmology and high-energy physics. She was one of 27 scientists who received the Breakthrough Prize in Fundamental Physics in 2018 for their "detailed maps of the early universe."

Abigail Goodhue Vieregg is a professor of physics at the Enrico Fermi Institute and Kavli Institute of Cosmology, University of Chicago, specializing in neutrino astrophysics and cosmology. Her work focuses on cosmic high-energy neutrinos and mapping the cosmic microwave background.

References

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