KICP in the News
Researchers Provide New Insight Into Dark Matter Halos
PennNews, April 19, 2017
Many scientists now believe that more than 80 percent of the matter of the universe is locked away in mysterious, as yet undetected, particles of dark matter, which affect everything from how objects move within a galaxy to how galaxies and galaxy clusters clump together in the first place.
This dark matter extends far beyond the reach of the furthest stars in the galaxy, forming what scientists call a dark matter halo. While stars within the galaxy all rotate in a neat, organized disk, these dark matter particles are like a swarm of bees, moving chaotically in random directions, which keeps them puffed up to balance the inward pull of gravity.
Bhuvnesh Jain, a physics professor in Penn's School of Arts & Sciences, and postdoc Eric Baxter are conducting research that could give new insights into the structure of these halos.
The researchers wanted to investigate whether these dark matter halos have an edge or boundary.
"People have generally imagined a pretty smooth transition from the matter bound to the galaxy to the matter between galaxies, which is also gravitationally attracted to the galaxies and clusters," Jain said. "But theoretically, using computer simulations a few years ago, researchers at the University of Chicago showed that for galaxy clusters a sharp boundary is expected, providing a distinct transition that we should be able to see through a careful analysis of the data."
Using a galaxy survey called the Sloan Digital Sky Survey, or SDSS, Baxter and Jain looked at the distribution of galaxies around clusters. They formed a team of experts at the University of Chicago and other institutions around the world to examine thousands of galaxy clusters. Using statistical tools to do a joint analysis of several million galaxies around them, they found a drop at the edge of the cluster. Baxter and collaborator Chihway Chang at the University of Chicago led a paper reporting the findings, accepted for publication in the Astrophysical Journal.
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KICP Members: Chihway Chang; Andrey V. Kravtsov; Surhud More
KICP Students: Eric J. Baxter; Benedikt Diemer
Scientific projects: SDSS Supernova Survey (SDSS SS); Sloan Digital Sky Survey (SDSS)
NASA to launch telescope on super-pressure balloon in search for cosmic rays
UChicago News, April 6, 2017
Prof. Angela Olinto leads project to collect data at near-space altitudes
The National Aeronautics and Space Administration is preparing to use a super-pressure balloon to launch into near space a pioneering telescope designed to detect ultra-high-energy cosmic rays as they interact with the Earth's atmosphere.
"We're searching for the most energetic cosmic particles that we’ve ever observed," said Angela V. Olinto, the Homer J. Livingston Distinguished Service Professor at the University of Chicago and principal investigator of the project, known as the Extreme Universe Space Observatory-Super Pressure Balloon. "The origin of these particles is a great mystery that we'd like to solve. Do they come from massive black holes at the center of galaxies? Tiny, fast-spinning stars? Or somewhere else?"
The extremely rare particles hit the atmosphere at a rate of only one per square kilometer per century. To assure that it will capture some of the particles, the telescope's camera takes 400,000 images a second as it casts a wide view back toward the Earth.
Preparations are complete in Wanaka, New Zealand for the balloon's launch, which will happen as soon as scientists and engineers have the right weather conditions. Researchers hope the balloon will stay afloat for up to 100 days, thereby setting a record for an ultra-long duration flight.
NASA describes the super-pressure balloon as the "most persnickety" of all the flight and launch vehicles it operates. Launching the balloon depends on just the right weather conditions on the surface of the Earth all the way up to 110,000 feet, where the balloon travels.
The project will set the stage for a space mission currently being planned. "That would enlarge even more the volume of the atmosphere that we can observe at one time," said Olinto, who serves as chair of UChicago's Department of Astronomy and Astrophysics. "We need to observe a significantly large number of these cosmic messengers to discover what are their sources and how they interact at their energetic extremes."
When an ultra-high-energy cosmic ray reaches the Earth's atmosphere, it induces a series of interactions that stimulates a large cosmic ray shower. The new telescope, which detects at night, will capture the ultra-violet fluorescence produced by the interaction of these particle showers with the nitrogen molecules in the air.
"High-energy cosmic rays have never been observed this way from space," said Lawrence Wiencke, professor of physics at the Colorado School of Mines and co-leader of the project. "This mission to a sub-orbital altitude is a pioneering opportunity for us. Our international collaboration is very excited about this launch and about the new data that will be collected along the way."
The project lends itself to participation by graduate and undergraduate students, Olinto said. Leo Allen and Mikhail Rezazadeh, two UChicago undergraduates, built an infrared camera under the supervision of UChicago Prof. Stephan Meyer and Olinto to observe the cloud coverage at night under EUSO-SPB.
Sixteen countries were involved with the design of the telescope. The U.S. team, funded by NASA, is led by UChicago, Colorado School of Mines, Marshall Space Flight Center, University of Alabama at Huntsville and Lehman College at the City University of New York.
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KICP Members: Stephan S. Meyer; Angela V. Olinto
KICP Students: Leo Allen; Mikhail Rezazadeh
A recharged debate over the speed of the expansion of the universe could lead to new physics
AAAS, March 8, 2017
It was the early 1990s, and the Carnegie Observatories in Pasadena, California, had emptied out for the Christmas holiday. Wendy Freedman was toiling alone in the library on an immense and thorny problem: the expansion rate of the universe.
Carnegie was hallowed ground for this sort of work. It was here, in 1929, that Edwin Hubble first clocked faraway galaxies flying away from the Milky Way, bobbing in the outward current of expanding space. The speed of that flow came to be called the Hubble constant.
Freedman's quiet work was soon interrupted when fellow Carnegie astronomer Allan Sandage stormed in. Sandage, Hubble's designated scientific heir, had spent decades refining the Hubble constant, and had consistently defended a slow rate of expansion. Freedman was the latest challenger to publish a faster rate, and Sandage had seen the heretical study.
"He was so angry," recalls Freedman, now at the University of Chicago in Illinois, "that you sort of become aware that you're the only two people in the building. I took a step back, and that was when I realized, oh boy, this was not the friendliest of fields."
The acrimony has diminished, but not by much. Sandage died in 2010, and by then most astronomers had converged on a Hubble constant in a narrow range. But in a twist Sandage himself might savor, new techniques suggest that the Hubble constant is 8% lower than a leading number. For nearly a century, astronomers have calculated it by meticulously measuring distances in the nearby universe and moving ever farther out. But lately, astrophysicists have measured the constant from the outside in, based on maps of the cosmic microwave background (CMB), the dappled afterglow of the big bang that is a backdrop to the rest of the visible universe. By making assumptions about how the push and pull of energy and matter in the universe have changed the rate of cosmic expansion since the microwave background was formed, the astrophysicists can take their map and adjust the Hubble constant to the present-day, local universe. The numbers should match. But they don't.
It could be that one approach has it wrong. The two sides are searching for flaws in their own methods and each other's alike, and senior figures like Freedman are racing to publish their own measures. "We don't know which way this is going to land," Freedman says.
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KICP Members: Wendy L. Freedman; Daniel Scolnic
New World-Leading Limit on Dark Matter Search from PICO Experiment
SNOLAB News, February 27, 2017
The PICO Collaboration is excited to announce that the PICO-60 dark matter bubble chamber experiment has produced a new dark matter limit after analysis of data from the most recent run. This new result is a factor of 17 improvement in the limit for spin-dependent WIMP-proton cross-section over the already world-leading limits from PICO-2L run-2 and PICO-60 CF3I run-1 in 2016.
The PICO-60 experiment is currently the world's largest bubble chamber in operation; it is filled with 52 kg of C3F8 (octafluoropropane) and is taking data in the ladder lab area of SNOLAB. The detector uses the target fluid in a superheated state such that a dark matter particle interaction with a fluorine nucleus causes the fluid to boil and creates a tell tale bubble in the chamber.
The PICO experiment uses digital cameras to see the bubbles and acoustic pickups to improve the ability to distinguish between dark matter particles and other sources when analysing the data.
The superheated detector technology has been at the forefront of spin-dependent (SD) searches, using various refrigerant targets including CF3I, C4F10 and C2ClF5, and two primary types of detectors: bubble chambers and droplet detectors. PICO is the leading experiment in the direct detection of dark matter for spin-dependent couplings and is developing a much larger version of the experiment with up to 500 kg of active mass.
The PICO Collaboration would like to acknowledge the support of the National Sciences and Engineering Research Council of Canada (NSERC) and the Canada Foundation for Innovation (CFI) for funding.
This work was also supported by the U.S. Department of Energy Office of Science and the US National Science Foundation under Grants PHY-1242637, PHY-0919526, PHY-1205987 and PHY-1506377, and in part by the Kavli Institute for Cosmological Physics at the University of Chicago through grant PHY-1125897, and an endowment from the Kavli Foundation and its founder Fred Kavli.
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KICP Members: Juan I. Collar
Scientific projects: COUPP/PICO
Kumiko Kotera: doing beautiful physics without giving up on family, art and the rest of the world
e-EPS, February 24, 2017
Kumiko Kotera is a young researcher in Astrophysics, at the Institut d'Astrophysique de Paris, (IAP) of the French Centre National de la Recherche Scientifique (CNRS). She builds theoretical models to probe the most violent phenomena in the Universe, by deciphering their so-called "astroparticle" messengers (cosmic rays, neutrinos and photons). Today, she is one of the leaders of the international project GRAND (Giant Radio Array for Neutrino Detection), that aims at detecting very-high energy cosmic neutrinos. In 2016, she received a prestigious award: the CNRS bronze medal for her important achievements.
Lucia Di Ciaccio: Do you have any female 'physicist cult figure' or 'role model'?
Kumiko Kotera: Angela Olinto, professor at the University of Chicago, is undoubtedly my mentor. She struggled to build her brilliant career at a time when female physicists were far more isolated than today and opened the path for all of us. She showed me how one can be strong, respected, and do beautiful physics without ever giving up on kindness, family, art, and the rest of the world.
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KICP Members: Angela V. Olinto
Abigail Vieregg has been awarded a Sloan Research Fellowship
The University of Chicago News Office, February 21, 2017
Five UChicago faculty members have earned 2017 Sloan Research Fellowships: Bryan Dickinson, assistant professor of chemistry; Suriyanarayanan Vaikuntanathan, assistant professor of chemistry; Joseph Vavra, associate professor of economics at the University of Chicago Booth School of Business; Abigail Vieregg, assistant professor of physics; and Alessandra Voena, associate professor of economics.
Abigail Vieregg is interested in answering questions about the nature of the universe at its highest energies through experimental work in particle astrophysics and cosmology. In particle astrophysics, she focuses on searching for the highest energy neutrinos that come from the most energetic sources in the universe. In cosmology, Vieregg works with a suite of telescopes at the South Pole to help determine what happened during the first moments after the Big Bang by measuring the polarization of the cosmic microwave background.
Vieregg was a NASA Earth and Space Sciences Graduate Fellow at UCLA and a National Science Foundation Office of Polar Programs Postdoctoral Fellow at the Harvard-Smithsonian Center for Astrophysics.
Vieregg joined the UChicago faculty in 2014.
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KICP Members: Abigail G. Vieregg
Scientific projects: BICEP2/The Keck Array/BICEP3
Cosmos Controversy: The Universe Is Expanding, but How Fast?
The New York Times, February 21, 2017
by Dennis Overbye, The New York Times
A small discrepancy in the value of a long-sought number has fostered a debate about just how well we know the cosmos.
There is a crisis brewing in the cosmos, or perhaps in the community of cosmologists. The universe seems to be expanding too fast, some astronomers say. Recent measurements of the distances and velocities of faraway galaxies don't agree with a hard-won "standard model" of the cosmos that has prevailed for the past two decades. The latest result shows a 9 percent discrepancy in the value of a long-sought number called the Hubble constant, which describes how fast the universe is expanding. But in a measure of how precise cosmologists think their science has become, this small mismatch has fostered a debate about just how well we know the cosmos. "If it is real, we will learn new physics," said Wendy Freedman of the University of Chicago, who has spent most of her career charting the size and growth of the universe.
Michael S. Turner of the University of Chicago said, "If the discrepancy is real, this could be a disruption of the current highly successful standard model of cosmology and just what the younger generation wants - a chance for big discoveries, new insights and breakthroughs."
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KICP Members: Wendy L. Freedman; Daniel Scolnic; Michael S. Turner
Galactic X-rays could point to dark matter proof
BBC News, February 2, 2017
by Edwin Cartlidge, BBC News
KICP Senior Member Dan Hooper discusses a recent claim of the detection of the 3.5 keV X-ray line in our Galaxy with the BBC.
"The new paper claims a modest detection," said Dr Hooper, "but it doesn't sway me very strongly at this point."
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KICP Members: Daniel Hooper
Research reinforces role of supernovae in clocking the universe
UChicago News, January 4, 2017
How much light does a supernova shed on the history of universe?
New research by cosmologists at the University of Chicago and Wayne State University confirms the accuracy of Type Ia supernovae in measuring the pace at which the universe expands. The findings support a widely held theory that the expansion of the universe is accelerating and such acceleration is attributable to a mysterious force known as dark energy. The findings counter recent headlines that Type Ia supernova cannot be relied upon to measure the expansion of the universe.
Using light from an exploding star as bright as entire galaxies to determine cosmic distances led to the 2011 Nobel Prize in physics. The method relies on the assumption that, like lightbulbs of a known wattage, all Type Ia supernovae are thought to have nearly the same maximum brightness when they explode. Such consistency allows them to be used as beacons to measure the heavens. The weaker the light, the farther away the star. But the method has been challenged in recent years because of findings the light given off by Type Ia supernovae appears more inconsistent than expected.
"The data that we examined are indeed holding up against these claims of the demise of Type Ia supernovae as a tool for measuring the universe," said Daniel Scolnic, a postdoctoral scholar at UChicago's Kavli Institute for Cosmological Physics and co-author of the new research published in Monthly Notices of the Royal Astronomical Society. "We should not be persuaded by these other claims just because they got a lot of attention, though it is important to continue to question and strengthen our fundamental assumptions."
One of the latest criticisms of Type Ia supernovae for measurement concluded the brightness of these supernovae seems to be in two different subclasses, which could lead to problems when trying to measure distances. In the new research led by David Cinabro, a professor at Wayne State, Scolnic, Rick Kessler, a senior researcher at the Kavli Institute, and others, they did not find evidence of two subclasses of Type Ia supernovae in data examined from the Sloan Digital Sky Survey Supernovae Search and Supernova Legacy Survey. The recent papers challenging the effectiveness of Type Ia supernovae for measurement used different data sets.
A secondary criticism has focused on the way Type Ia supernovae are analyzed. When scientists found that distant Type Ia supernovae were fainter than expected, they concluded the universe is expanding at an accelerating rate. That acceleration is explained through dark energy, which scientists estimate makes up 70 percent of the universe. The enigmatic force pulls matter apart, keeping gravity from slowing down the expansion of the universe.
Yet a substance that makes up 70 percent of the universe but remains unknown is frustrating to a number of cosmologists. The result was a reevaluation of the mathematical tools used to analyze supernovae that gained attention in 2015 by arguing that Type Ia supernovae don't even show dark energy exists in the first place.
Scolnic and colleague Adam Riess, who won the 2011 Nobel Prices for the discovery of the accelerating universe, wrote an article for Scientific American Oct. 26, 2016, refuting the claims. They showed that even if the mathematical tools to analyze Type Ia supernovae are used "incorrectly," there is still a 99.7 percent chance the universe is accelerating.
The new findings are reassuring for researchers who use Type Ia supernovae to gain an increasingly precise understanding of dark energy, said Joshua A. Frieman, senior staff member at the Fermi National Accelerator Laboratory who was not involved in the research.
"The impact of this work will be to strengthen our confidence in using Type Ia supernovae as cosmological probes," he said.
Citation: "Search for Type Ia Supernova NUV-Optical Subclasses," by David Cinabro and Jake Miller (Wayne State University); and Daniel Scolnic and Ashley Li (Kavli Institute for Cosmological Physics at the University of Chicago); and Richard Kessler (Kavli Institute for Cosmological Physics at University of Chicago and the Department of Astronomy and Astrophysics at the University of Chicago). Monthly Notices of the Royal Astronomical Society, November 2016. DOI: 10.1093/mnras/stw3109"
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KICP Members: Joshua A. Frieman; Richard Kessler; Daniel Scolnic
Scientific projects: SDSS Supernova Survey (SDSS SS); Sloan Digital Sky Survey (SDSS)
Have Astronomers Decided Dark Energy Doesn't Exist?
Scientific American, October 26, 2016
No, they haven't, although plenty of recent headlines have suggested otherwise.
This week, a number of media outlets have put out headlines like "The universe is expanding at an accelerating rate, or is it?" and "The Universe Is Expanding But Not At An Accelerating Rate New Research Debunks Nobel Prize Theory." This excitement is due to a paper just published in Nature's Scientific Reports called "Marginal evidence for cosmic acceleration from Type Ia supernovae," by Nielsen, Guffanti and Sarkar.
Once you read the article, however, it's safe to say there is no need to revise our present understanding of the universe. All the paper does is slightly reduce our certainty in what we know - and then only by discarding most of the cosmological data on which our understanding is based. It also ignores important details in the data it does consider. And even if you leave aside these issues, the headlines are wrong anyway. The study concluded that we're now only 99.7 percent sure that the universe is accelerating, which is hardly the same as "it's not accelerating."
The initial discovery that the universe is expanding at an accelerating rate was made by two teams of astronomers in 1998 using Type Ia Supernovae as cosmic measuring tools. Supernovae -- exploding stars -- are some of the most powerful blasts in the entire cosmos, roughly equivalent to a billion-billion-billion atomic bombs exploding at once. Type Ia's are a special kind of supernova in that, unlike other supernovae, they all explode with just about the same luminosity every time likely due to a critical mass limit. This similarity means that the differences in their observed brightness are almost entirely based on how far away they are. This makes them ideal for measuring cosmic distances. Furthermore, these objects are relatively common, and they are so bright that we can see them billions of light years away. This shows us how the universe appeared billions of years ago, which we can compare to how it looks today.
These supernovae are often called "standard candles" for their consistency, but they're more accurately "standardizable candles," because in practice, their precision and accuracy can be improved still further by accounting for small differences in their explosions by observing how long the explosion takes to unfold and how the color of the supernovae are reddened by dust between them and us. Finding a way to do these corrections robustly was what led to the discovery of the accelerating universe.
The recent paper that has generated headlines used a catalog of Type Ia supernovae collected by the community (including us) which has been analyzed numerous times before. But the authors used a different method of implementing the corrections - and we believe this undercuts the accuracy of their results. They assume that the mean properties of supernovae from each of the samples used to measure the expansion history are the same, even though they have been shown to be different and past analyses have accounted for these differences. However, even ignoring these differences, the authors still find that there is roughly a 99.7 percent chance that the universe is accelerating - very different from what the headlines suggest.
Furthermore, the overwhelming confidence astronomers have that the universe is expanding faster now than it was billions of years ago is based on much more than just supernova measurements. These include tiny fluctuations in the pattern of relic heat after the Big Bang (i.e., the cosmic microwave background) and the modern day imprint of those fluctuations in the distribution of galaxies around us (called baryon acoustic oscillations). The present study also ignores the presence of a substantial amount of matter in the Universe, confirmed numerous times and ways since the 1970's, further reducing the study confidence. These other data show the universe to be accelerating independently from supernovae. If we combine the other observations with the supernova data, we go from 99.99 percent sure to 99.99999 percent sure. That's pretty sure!
We now know that dark energy, which is what we believe causes the expansion of the universe to accelerate, makes up 70 percent of the universe, with matter constituting the rest. The nature of dark energy is still one of the largest mysteries of all of astrophysics. But there has been no active debate about whether dark energy exists and none about whether the universe is accelerating since this picture was cemented a decade ago.
There are now many new large surveys, both on the ground and in space, whose top priority over the next two decades is to figure out exactly what this dark energy could be. For now, we have to continue to improve our measurements and question our assumptions. While this recent paper does not disprove any theories, it is still good for everyone to pause for a second and remember how big the questions are that we are asking, how we reached the conclusions we have to date and how seriously we need to test each building block of our understanding.
Dan Scolnic and Adam G. Riess
Dan Scolnic is a Hubble and KICP Fellow at The Kavli Institute For Cosmological Physics at The University of Chicago. He works on multiple surveys, including The Dark Energy Survey, Pan-STARRS, Foundation and WFIRST, to use Type Ia Supernovae to measure dark energy. Adam G. Riess is an astrophysicist at Johns Hopkins University and the Space Telescope Science Institute. His research on distant supernovae revealed that the expansion of the universe is accelerating, a discovery for which he shared the 2011 Nobel Prize in Physics.
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KICP Members: Daniel Scolnic
KICP member Daniel Holz discusses Gravitational Waves on PBS' The Good Stuff
The Good Stuff, October 13, 2016
In 2015 scientists working at the Laser Interferometer Gravitational-Wave observatory, or LIGO, detected gravitational waves for the first time. But how did they do it? What is a gravitational wave? And why is confirming something that Albert Einstein predicted a hundred years ago one of the greatest scientific achievements of the past century?
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KICP Members: Ben Farr; Daniel E. Holz
KICP Students: Hsin-Yu Chen; Zoheyr Doctor
Physics Confronts Its Heart of Darkness
Scientific American, September 1, 2016
Cracks are showing in the dominant explanation for dark matter. Is there anything more plausible to replace it?
Physics has missed a long-scheduled appointment with its future - again. The latest, most sensitive searches for the particles thought to make up dark matter - the invisible stuff that may comprise 85 percent of the mass in the cosmos - have found nothing. Called WIMPs (weakly interacting massive particles), these subatomic shrinking violets may simply be better at hiding than physicists thought when they first predicted them more than 30 years ago. Alternatively, they may not exist, which would mean that something is woefully amiss in the underpinnings of how we try to make sense of the universe. Many scientists still hold out hope that upgraded versions of the experiments looking for WIMPs will find them but others are taking a second look at conceptions of dark matter long deemed unlikely.
Whatever dark matter is, it is not accounted for in the Standard Model of particle physics, a thoroughly-tested "theory of almost everything" forged in the 1970s that explains all known particles and all known forces other than gravity. Find the identity of dark matter and you illuminate a new path forward to a deeper understanding of the universe - at least, that is what physicists hope.
WIMPs would get their gravitational heft from being somewhere between one and a thousand times the mass of a proton. Their sole remaining connection to our familiar world would be through the weak nuclear force, which is stronger than gravity but only active across tiny distances on the scale of atomic nuclei. If they exist, WIMPs should surround us like an invisible fog, their chances of interacting with ordinary matter so remote that one could pass through light-years of elemental lead unscathed.
Undaunted, experimentalists have spent decades devising and operating enough cleverly named WIMP detectors to overflow your average can of alphabet soup. (CDEX, CDMS, CoGeNT, COUPP and CRESST are just the most notable examples that start with the letter C.) The delicate work of detecting any weak, rare and fleeting interactions of WIMPs with atoms requires isolation and solitude, confining most detectors to caverns, abandoned mines and other outlier subterranean spaces.
One of the latest null results in the search for WIMPs came from the Large Underground Xenon (LUX) experiment, a third of a ton of liquid xenon held at a frosty -100 degrees Celsius inside a giant water-filled tank buried one and a half kilometers beneath the Black Hills of South Dakota. There, shielded from most sources of contaminating noise, researchers have spent more than a year's worth of time looking for flashes of light emanating from WIMPs striking xenon nuclei. On July 21 they announced they had seen none.
The next disappointment came on August 5 from the most powerful particle accelerator ever built: CERN's Large Hadron Collider (LHC) near Geneva, Switzerland. In 2012 after it found the Higgs boson - the Standard Modelâ€™s long-predicted final particle that imbues others with mass - many theorists believed the next blockbuster result from the LHC would be a discovery of how the Higgs (or other hypothesized particles very much like it) helps produce the WIMPs thought to suffuse the cosmos. Since spring 2015 the LHC has been pursuing these ideas by smashing protons together at unprecedentedly high energies at rates of up to a billion per second, pushing into new frontiers of particle physics. Early on, two independent teams had spied a telltale anomaly in the subatomic wreckage, an excess of energy from proton collisions that hinted at new physics perhaps produced by WIMPs (or, to be fair, many additional exotic possibilities). Instead, as the LHC smashed more protons and collected more data, the anomaly fizzled out, indicating it had been a statistical fluke.
Taken together, these two null results are a double-edged sword for dark matter. On one hand, their new constraints on the plausible masses and interactions of WIMPs are priming plans for next-generation detectors that could offer better chances of success. On the other, they have ruled out some of the simplest and most cherished WIMP models, raising fresh fears that the long-postulated particles might be a multidecadal detour in the search for dark matter.
Edward "Rocky" Kolb, a cosmologist now at the University of Chicago who in the 1970s helped lay the foundations for the generations of WIMP hunts to come, declared the 2010s "the decade of the WIMP" but now admits the search has not gone as planned. "We are now more in the dark about dark matter than we were five years ago," he says. So far, Kolb says, most theorists have responded by "letting a thousand WIMPs bloom," creating ever-more baroque and exotic theories to explain how WIMPs have managed to dodge all our detectors.
There is, of course, another possibility - that WIMPs are not the solution to dark matter we should be looking for. "WIMPs emerged as a simple, elegant, compelling explanation for a complex phenomenon," Kolb says. "And for every complex phenomenon there is a simple, elegant, compelling explanation that is wrong."
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KICP Members: Edward W. Kolb
James W. Cronin, Nobel laureate and pioneering physicist, 1931-2016
UChicago News, August 27, 2016
Scholar remembered for groundbreaking research on particle physics and cosmic rays
James W. Cronin, a pioneering scientist who shared the Nobel Prize in physics in 1980 for his groundbreaking work on the laws governing matter and antimatter and their role in the universe, died Aug. 25 in Saint Paul, Minn. He was 84.
Cronin, SM'53, PhD'55, spent much of his career at the University of Chicago, first as a student and then a professor. A University Professor Emeritus of Physics and Astronomy & Astrophysics, he was remembered this week as a mentor, collaborator and visionary.
"He inspired us all to reach further into the unknown with deep intuition, solid scientific backing and poetic vision," said Angela Olinto, the Homer J. Livingston Distinguished Service Professor in Astronomy and Astrophysics. "He accepted his many recognitions and accolades with so much humility that he encouraged many generations to follow his vision."
Edward "Rocky" Kolb, dean of the Physical Sciences Division and the Arthur Holly Compton Distinguished Service Professor in Astronomy and Astrophysics, described Cronin as â€śa person of real honesty and integrity who was a mentor and friend to so many people."
"Just like in basketball, there are good players in science, but the greatest players are the ones who make the people around them better. Jim was that great player," Kolb said.
Cronin's research that resulted in the Nobel Prize came in 1964 while he was working with Val Fitch at the Brookhaven National Laboratory. The two scientists, who were Princeton University professors at the time, observed the first example of nature's preference for matter over antimatter. Without the phenomenon, which physicists refer to as charge-parity violation, no matter would exist in the universe.
Cronin and Fitch studied the short-lived subatomic particles that appeared after the collision of accelerated protons and the nucleus of an atom. They observed indirect charge-parity violation, which is the unbalanced mixing of neutral subatomic kaon particles with their charged antiparticles. Called the Fitch-Cronin effect, the finding showed that some physical laws are violated when the direction of time is reversed. It also lent support for the big bang theory of the universe's origin.
Cronin later in his career shifted his focus, becoming co-leader of the Pierre Auger Project. The $50 million international collaboration of 250 scientists across 16 nations focused on the mysterious sources of rare but extremely powerful cosmic rays that periodically bombard Earth. The project led to the creation of the Auger Observatory, which consists of a vast array of cosmic-ray detectors in Argentina.
"It was 25 years ago since Jim and I first conceived the idea of what became the Auger Collaboration. It was definitely a great partnership as we drummed up financial and scientific support for the collaboration," said Alan Watson, emeritus professor of physics at the University of Leeds and a fellow of the Royal Society.
The collaboration has made definitive measurements on the energy spectrum of cosmic rays, on the patterns of their arrival directions, and on their mass compositions. It also has conducted particle physics research, measuring phenomena that far exceed the energies of the Large Hadron Collider.
"It's been an outstanding success, and it's still going strong," Watson said.
Drawing inspiration from Fermi
Cronin was born on Sept. 29, 1931, in Chicago, while his father was a graduate student in classical languages and literatures at the University of Chicago. The younger Cronin received a bachelor's from Southern Methodist University in 1951 before returning to the University of Chicago as a National Science Foundation Fellow to earn his master's and doctoral degrees.
Cronin met his first wife, Annette Martin, while both were students at the University. She died in 2005, and Cronin married Carol McDonald (nee Champlin) in late 2006.
Cronin began his scientific career at Brookhaven before becoming a member of the physics faculty at Princeton in 1958. In 1971, he joined the University of Chicago, where he was appointed the University Professor of Physics. He became University Professor Emeritus of Physics and Astronomy & Astrophysics in 1997.
Cronin shared a birthdate with Prof. Enrico Fermi, who earned the Nobel Prize in Physics in 1938. Cronin, who knew Fermi from his graduate school days at UChicago, organized a symposium in 2001 to mark the 100th anniversary of Fermi's birth, and was editor of the resulting book, Fermi Remembered. It included contributions from seven Nobel Prize recipients and many other scientists who studied under or worked with Fermi at UChicago.
"What's significant about Fermi is if you look through his career, he never just did the same thing. He kept moving on to new scientific challenges," Cronin once said of Fermi. The same statement also could be applied to Cronin and his research shift from high-energy physics to ultra-high-energy cosmic rays.
Cronin's honors include the University of Chicago Alumni Medal (2013), election as a foreign member of the Royal Society of London (2007), Distinguished Graduate Award of SMU's Dedman College (2004), Legion dâ€™honneur of France (2001), National Medal of Science (1999), University of Chicago's Quantrell Award for Excellence in Undergraduate Teaching (1994), Laureate of Lincoln Academy of Illinois (1981), Ernest Lawrence Memorial Award for outstanding contributions in the field of atomic energy (1977), John Price Wetherill Medal of the Franklin Institute (1975) and the Research Corporation Award (1968).
In 1990 Cronin delivered the Ryerson Lecture, which provides an opportunity each year for a distinguished faculty member to address the UChicago community on significant aspects of his or her research.
He was a member of the National Academy of Sciences, American Academy of Arts and Sciences, American Physical Society, American Philosophical Society, Accademia Nazionale dei Lincei of Italy, Mexican Academy of Sciences and the Russian Academy of Sciences. Cronin also had received honorary doctorates from l'Universite Pierre et Marie Curie, University of Leeds, Universite de Franche Conte, Novo Gorica Polytechnique of Slovenia, University of Nebraska, the University of Santiago de Compostela, the Colorado School of Mines, and the Karlsruhe Institute of Technology.. Cronin served as international chair of the College de France in 1999-2000.
Cronin is survived by his wife, Carol; daughter, Emily Grothe; son, Daniel Cronin; and six grandchildren: James, Cathryn, Caroline, Meredith, Alex and Marlo. A daughter, Cathryn Cranston, died in 2011.
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KICP Members: James W. Cronin; Edward W. Kolb; Angela V. Olinto
Scientific projects: Pierre Auger Observatory (AUGER)
Allusionist 41: Getting Toasty
theallusionist.org, August 22, 2016
When you choose to spend the winter in Antarctica, you'll be prepared for it to be cold. You know that nobody will be leaving or arriving until springtime. And you're braced for months of darkness. But a few weeks after the last sunset, you might find you can't even string a sentence together. And even if you can, that sentence may only make sense in Antarctica.
To explain why are Antarctica veteran Allison 'Sandwich' Barden, endocrinologist Tom Baranski, and astrophysicists Amy Lowitz and Christine Moran, reporting from the South Pole in the depths of winter.
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Scientific projects: South Pole Telescope (SPT)
The Particle That Wasn't
The New York Times, August 8, 2016
A great "might have been" for the universe, or at least for the people who study it, disappeared Friday.
Last December, two teams of physicists working at CERN's Large Hadron Collider reported that they might have seen traces of what could be a new fundamental constituent of nature, an elementary particle that is not part of the Standard Model that has ruled particle physics for the last half-century.
A bump on a graph signaling excess pairs of gamma rays was most likely a statistical fluke, they said. But physicists have been holding their breath ever since.
If real, the new particle would have opened a crack between the known and the unknown, affording a glimpse of quantum secrets undreamed of even by Einstein. Answers to questions like why there is matter but not antimatter in the universe, or the identity of the mysterious dark matter that provides the gravitational glue in the cosmos. In the few months after the announcement, 500 papers were written trying to interpret the meaning of the putative particle.
On Friday, physicists from the same two CERN teams reported that under the onslaught of more data, the possibility of a particle had melted away.
"We don't see anything," said Tiziano Camporesi of CERN, the European Organization for Nuclear Research and a spokesman for one of the detector teams known as C.M.S., on the eve of the announcement. "In fact, there is even a small deficit exactly at that point."
His statement was echoed by a member of the competing team, known as Atlas. James Beacham, of Ohio State University, said, "As it stands now, the bumplet has gone into a flatline."
The new results were presented in Chicago at the International Conference of High Energy Physics, ICHEP for short, by Bruno Lenzi of CERN for the Atlas team, and Chiara Rovelli for their competitors named for their own detector called C.M.S., short for Compact Muon Solenoid.
The presentations were part of an outpouring of dozens of papers from the two teams on the results so far this year from the collider, all of them in general agreement with the Standard Model.
The main news is that the collider, which had a rocky start, exploding back in 2008, is now running "swimmingly" in CERN's words, producing up to a billion proton-proton collisions a second.
"We're just at the beginning of the journey," said Fabiola Gianotti, CERNâ€™s director-general, in a statement.
Michael Turner, a cosmologist at the University of Chicago, said, "Energy is the great tool of discovery, so going from 8 TeV to 13 TeV is a really big deal. Keep your fingers crossed."
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KICP Members: Michael S. Turner
Angela Olinto received distinguished service professorship
UChicago News, July 21, 2016
Faculty members recognized with named, distinguished service professorships
Ten faculty members have received named professorships or have been named distinguished service professors. Luc Anselin, John R. Birge, John List and Angela Olinto received distinguished service professorships; and Ethan Bueno de Mesquita, Michael Franklin, Christopher Kennedy, Jason Merchant, Haresh Sapra and Nir Uriel received named professorships.
Angela Olinto has been named the Homer J. Livingston Distinguished Service Professor in Astronomy & Astrophysics and the College.
Olinto has made important contributions to the physics of quark stars, inflationary theory, cosmic magnetic fields and particle astrophysics. Her research interests span theoretical astrophysics, particle and nuclear astrophysics, and cosmology. She has focused much of her recent work on understanding the origins of the highest-energy cosmic rays and neutrinos.
Olinto is an elected fellow of the American Association for the Advancement of Science for her distinguished contributions to the field of astrophysics, particularly exotic states of matter and extremely high-energy cosmic ray studies at the Pierre Auger Observatory in Argentina. She now leads the International collaboration of the Extreme Universe Space Observatory mission that will fly in a NASA super pressure balloon in 2017 and will be first to observe tracks of ultra-energy particles from above.
She also is a fellow of the American Physical Society and has received the Chaire dâ€™Excellence Award of the French Agence Nationale de Recherche. Olinto has received the Llewellyn John and Harriet Manchester Quantrell Award for Excellence in Undergraduate Teaching, as well as the Faculty Award for Excellence in Graduate Teaching and Mentoring.
Olinto joined the UChicago faculty in 1996.
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KICP Members: Angela V. Olinto
Angela Olinto: the 114th Congress Hearing - Astronomy, Astrophysics, and Astrobiology
Committee on Science, Space and Technology, 114th Congress, July 12, 2016
Joint Space Subcommittee and Research and Technology Subcommittee Hearing - Astronomy, Astrophysics, and Astrobiology
Tuesday, July 12, 2016 - 10:00am
- Space Subcommittee Chairman Brian Babin (R-Texas)
- Research and Technology Subcommittee Chairwoman Barbara Comstock (R-Va.)
- Chairman Lamar Smith (R-Texas)
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KICP Members: Angela V. Olinto
Simulations foresee hordes of colliding black holes in observatory's future
UChicago News, June 28, 2016
New calculations predict that the Laser Interferometer Gravitational wave Observatory (LIGO) will detect approximately 1,000 mergers of massive black holes annually once it achieves full sensitivity early next decade.
The prediction, published online June 22 in the journal Nature, is based on computer simulations of more than a billion evolving binary stars. The simulations are based on state-of-the-art modeling of the physics involved, informed by the most recent astronomical and astrophysical observations.
"The main thing we find is that what LIGO detected makes sense," said Daniel Holz, associate professor in physics and astronomy at the University of Chicago and a co-author of the Nature paper. The simulations predict the formation of black-hole binary stars in a range of masses that includes the two already observed. As more LIGO data become available, Holz and his colleagues will be able to test their results more rigorously.
The paper's lead author, Krzysztof Belczynski of Warsaw University in Poland, said he hopes the results will surprise him, that they will expose flaws in the work. Their calculations show, for example, that once LIGO reaches full sensitivity, it will detect only one pair of colliding neutron stars for every 1,000 detections of the far more massive black-hole collisions.
"Actually, I would love to be proven wrong on this issue. Then we will learn a lot," Belczynski said.
Forming big black holes
The new Nature paper, which includes co-authors Tomasz Bulik of Warsaw University and Richard O'Shaughnessy of the Rochester Institute of Technology, describes the most likely black-hole formation scenario that generated the first LIGO gravitational-wave detection in September 2015. That detection confirmed a major prediction of Albert Einstein's 1915 general theory of relativity.
The paper is the most recent in a series of publications, topping a decade of analyses where Holz, Belczynski and their associates theorize that the universe has produced many black-hole binaries in the mass range that are close enough to Earth for LIGO to detect.
"Here we simulate binary stars, how they evolve, turn into black holes and eventually get close enough to crash into each other and make gravitational waves that we would observe," Holz said.
The simulations show that the formation and evolution of a typical system of binary stars results in a merger of similar masses, and after similarly elapsed times, to the event that LIGO detected last September. These black hole mergers have masses ranging from 20 to 80 times more than the sun.
LIGO will begin recording more gravitational-wave-generating events as the system becomes more sensitive and operates for longer periods of time. LIGO will go through successive upgrades over the coming years, and is expected to reach its design sensitivity by 2020. By then, the Nature study predicts that LIGO might be detecting more than 100 black hole collisions annually.
LIGO has detected big black holes and big collisions, with a combined mass greater than 30 times that of the sun. These can only be formed out of big stars.
"To make those you need to have low metallicity stars, which just means that these stars have to be relatively pristine," Holz said. The Big Bang produced mainly hydrogen and helium, which eventually collapsed into stars.
As these stars burned they forged heavier elements, which astronomers call "metals." Those stars with fewer metals lose less mass as they burn, resulting in the formation of more massive black holes when they die. That most likely happened approximately two billion years after the Big Bang, before the young universe had time to form significant quantities of heavy metals. Most of those black holes would have merged relatively quickly after their formation.
LIGO would be unable to detect the ones that merged early and quickly. But if the binaries were formed in large enough numbers, a small fraction would survive for longer periods and would end up merging 11 billion years after the Big Bang (2.8 billion years ago), recently enough for LIGO to detect.
"That's in fact what we think happened," Holz said. Statistically speaking, "it's the most likely scenario." He added, however, that the universe continues to produce binary stars in local, still pristine pockets of low metallicity that resemble conditions of the early universe.
"In those pockets you can make these big stars, make the binaries, and then they'll merge right away and we would detect those as well."
Belczynski, Holz and collaborators have based their simulations on what they regard as the best models available. They assume "isolated formation," which involves two stars forming in a binary, evolving in tandem into black holes, and eventually merging with a burst of gravitational wave emission. A competing model is "dynamical formation," which focuses on regions of the galaxy that contain a high density of independently evolving stars. Eventually, many of them will find each other and form binaries.
"There are dynamical processes by which those black holes get closer and closer and eventually merge," Holz said. Identifying which black holes merged under which scenario is difficult. One potential method would entail examining the black holes' relative spins. Binary stars that evolved dynamically are expected to have randomly aligned spins; detecting a preference for aligned spins would be clear evidence in favor of the isolated evolutionary model.
LIGO is not yet able to precisely measure black hole spin alignment, "but we're starting to get there," Holz said. "This study represents the first steps in the birth of the entirely new field of gravitational wave astronomy. We have been waiting for a century, and the future has finally arrived."
Citation: "The first gravitational-wave source from the isolated evolution of two stars in the 40-100 solar mass range," by Krzysztof Belczynski, Daniel E. Holz, Tomasz Bulik, and Richard Oâ€™Shaughnessy," Nature, Vol. 534, pp. 512-515, June 23, 2016, doi:10.1038/nature18322.
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KICP Members: Daniel E. Holz
Gravitational waves detected from second pair of colliding black holes
UChicago News, June 16, 2016
At 9:38:53 CST on Dec. 25, 2015, scientists observed gravitational waves - ripples in the fabric of spacetime - for the second time.
The gravitational waves were detected by both of the twin Laser Interferometer Gravitational-Wave Observatory detectors, located in Livingston, La., and Hanford, Wash. University of Chicago scientists led by Daniel Holz, assistant professor in physics and astronomy, are members of the LIGO collaboration.
The LIGO observatories are funded by the National Science Foundation, and were conceived, built and are operated by the California Institute of Technology and the Massachusetts Institute of Technology. The discovery, accepted for publication in the journal Physical Review Letters, was made by the LIGO Scientific Collaboration and the Virgo Collaboration using data from the two LIGO detectors.
The LIGO detectors operated for approximately four months late last year, yielding about 50 days of data. An analysis of the first 16 days of data yielded the event that the LIGO Collaboration announced in February 2016.
Black holes events
"Now weâ€™ve analyzed the rest of the data, and we have another event thatâ€™s particularly interesting," Holz said. "It's not quite as loud as the first one, but it's quite beautiful in its own way. The event is composed of smaller black holes, and at least one is spinning. This marks the official turning point from 'detector' to 'observatory.'"
Gravitational waves carry information about their origins and about the nature of gravity that cannot otherwise be obtained, and physicists have concluded that these gravitational waves were produced during the final moments of the merger of two black holes - 14 and 8 times the mass of the sun - to produce a single, more massive spinning black hole that is 21 times the mass of the sun.
"It is very significant that these black holes were much less massive than those observed in the first detection," said Gabriela Gonzalez, LIGO Scientific Collaboration spokesperson and professor of physics and astronomy at Louisiana State University. "Because of their lighter masses compared to the first detection, they spent more time - about one second - in the sensitive band of the detectors. It is a promising start to mapping the populations of black holes in our universe."
During the merger, which occurred approximately 1.4 billion years ago, a quantity of energy roughly equivalent to the mass of the sun was converted into gravitational waves. The detected signal comes from the last 27 orbits of the black holes before their merger. Based on the arrival time of the signals - with the Livingston detector measuring the waves 1.1 milliseconds before the Hanford detector - the position of the source in the sky can be roughly determined.
The first detection of gravitational waves, announced on Feb. 11, 2016, was a milestone in physics and astronomy: It confirmed a major prediction of Albert Einstein's 1915 general theory of relativity, and marked the beginning of the new field of gravitational wave astronomy.
Both discoveries were made possible by the enhanced capabilities of Advanced LIGO, a major upgrade that increases the sensitivity of the instruments compared to the first-generation LIGO detectors, enabling a large increase in the volume of the universe probed.
'With the advent of Advanced LIGO, we anticipated researchers would eventually succeed at detecting unexpected phenomena, but these two detections thus far have surpassed our expectations,' said NSF Director France A. Cordova. "NSF's 40-year investment in this foundational research is already yielding new information about the nature of the dark universe."
Advanced LIGO's next data-taking run will begin this fall. By then, further improvements in detector sensitivity are expected to allow LIGO to reach as much as 1.5 to 2 times more of the volume of the universe. The Virgo detector is expected to join in the latter half of the coming observing run.
LIGO research is carried out by the LIGO Scientific Collaboration, a group of more than 1,000 scientists from universities around the United States and in 14 other countries. More than 90 universities and research institutes in the LSC develop detector technology and analyze data; approximately 250 students are strong contributing members of the collaboration. Virgo research is carried out by the Virgo Collaboration, consisting of more than 250 physicists and engineers belonging to 19 different European research groups.
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KICP Members: Daniel E. Holz
Wendy Freedman Named 2016 Woman in Space Science
UChicago News, May 23, 2016
On Thursday, May 12, Chicago's Adler Planetarium presented the 2016 Women in Space Science Award to Wendy L. Freedman, the John & Marion Sullivan Professor of Astronomy & Astrophysics.
The annual Women in Space Science Award recognizes women who have made significant contributions to the fields of science, technology, engineering, and math (STEM) with the goal of inspiring young women to pursue careers in these disciplines. Following a luncheon and her keynote address, Professor Freedman joined approximately 250 young women from Chicago-area public schools for a series of engaging STEM workshops.
One of Professor Freedman's many achievements was initiating the Giant Magellan Telescope (GMT) Project and serving as chair of the board of directors from its inception in 2003 until 2015. The Division of the Physical Sciences joins the Adler in celebrating Wendy's accomplishments and looking forward to the amazing discoveries that await her and the GMT.
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KICP Members: Wendy L. Freedman
Scientific projects: Giant Magellan Telescope (GMT)
Prof. Michael Turner's May 5 lecture at Adler Planetarium to be simulcast nationally
UChicago News, May 5, 2016
Prof. Michael Turner will explore some of the biggest mysteries of modern cosmology in a 7:30 p.m. May 5 lecture at the Adler Planetarium. The cosmologistâ€™s Kavli Fulldome Lecture, titled "From the Big Bang to the Multiverse and Beyond," will be streamed live at 15 other institutions across North America.
Kavli Fulldome Lecture
Is the universe part of a larger multiverse? What is speeding up the expansion of the universe? Turner will address these and other mysteries that inspire modern cosmologists. His talk will stream live simultaneously at 15 other institutions across North America. This dome-cast will allow audiences across North America to immerse themselves in the live presentation and ask questions, and will include institutions like the American Museum of Natural History in New York City, the Pacific Science Center in Seattle and the H.R. MacMillan Space Centre in Vancouver, British Columbia.
A theoretical astrophysicist, Turner is the Bruce V. and Diana M. Rauner Distinguished Service Professor and director of its Kavli Institute for Cosmological Physics. Turner helped to pioneer the interdisciplinary field of particle astrophysics and cosmology. He has made seminal contributions to the current cosmological paradigm known as LambdaCDM, including the prediction of cosmic acceleration. Turner has received numerous prizes and is a member of the National Academy of Sciences.
Current list of institutions participating in the dome-cast:
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KICP Members: Michael S. Turner
Physics in your future: Brittany Kamai
APS, Women in Physics, May 2, 2016
When Brittany Kamai took her first astronomy class as a freshman at the University of Hawaii, her professor told her that we can only see about 4% of the stuff in the universe. The rest is made of mysterious substances called dark matter and dark energy. "I found it fascinating that in the entire textbook for our class, there was barely a paragraph about this crazy thing," she recalls. Inspired, Brittany decided to study physics. During the summer before her last year of college, she accepted an opportunity to do research at the Institute for Astronomy at the University of Hawaii. She was hooked. Brittany went on to join the Fisk-Vanderbilt Master's-to-PhD Bridge Program, a two-year program designed to help students with limited undergraduate research experience. She is now in the PhD program at Vanderbilt University in Tennessee. But she actually spends most of her time in Chicago, because her research is based at Fermilab, a large U.S. Department of Energy research facility in northern Illinois. Brittany is building what she calls "the world's most precise ruler" - also called a "holometer." She and her colleagues hope to use intersecting laser beams to measure space itself very precisely, so they can look for tiny differences between what they measure and what Einstein's theory of general relativity predicts about it. Brittany and her colleagues are now testing the machine and making it as accurate as possible. They have just begun to run their experiment and hope to have results very soon. She will soon finish graduate school, but plans to continue pursuing experimental research in astrophysics. She likes the variety of work she gets to do. "Sometimes it's nice to say OK, I don't have to go into the lab, I can be behind my computer," she says. "And sometimes it's like, I'm sick of this - let me go back in lab! I enjoy that." When Brittany's not doing science, she's often talking about it, and encouraging young people - especially girls - to pursue it. She sees this as an important part of her job. In the past five years, she has shared her enthusiasm for science at museums, at middle schools and high schools, and even at senior centers. "You talk to people who are 50-plus, they get super-jazzed about it, they tell their kids, their grandkids," she says. "And it's like yes! This is how you get people excited about science."
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KICP Members: Stephan S. Meyer
KICP Students: Brittany Kamai
Joshua Frieman elected to American Academy of Arts and Sciences
UChicago News, April 26, 2016
Joshua Frieman is a professor of astronomy & astrophysics and the College. He is also a member of the Kavli Institute for Cosmological Physics at UChicago and a member of the theoretical astrophysics group at Fermi National Accelerator Laboratory. He focuses his research on theoretical and observational cosmology, including studies of the nature of dark energy, the early universe, gravitational lensing, the large-scale structure of the universe and supernovae as cosmological distance indicators.
Frieman is a co-founder and director of the Dark Energy Survey, an international collaboration of more than 300 scientists from 25 institutions on three continents that investigates why the expansion of the universe is accelerating. The collaboration built a 570-megapixel camera for the four-meter Blanco Telescope at the Cerro Tololo Inter-American Observatory in Chile to conduct its observations. Previously Frieman led the Sloan Digital Sky Survey Supernova Survey, which discovered more than 500 type Ia supernovae for cosmological studies.
Frieman is an honorary fellow of the Royal Astronomical Society, and a fellow of the American Physical Society and of the American Association for the Advancement of Science.
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KICP Members: Joshua A. Frieman
Scientific projects: Dark Energy Survey (DES)