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Researchers Measure Casimir Torque for the First Time

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Category: Research News
Published: Thursday, December 20 2018 14:03

Casimir crop

Physics researchers and members of the Institute for Research in Electronics and Applied Physics worked with the Department of Electrical and Computer Engineering to measure for the first time an effect that was predicted more than 40 years ago, called the Casimir torque. 

When placed together in a vacuum less than the diameter of a bacterium (one micron) apart, two pieces of metal attract each other. This is called the Casimir effect. The Casimir torque—a related phenomenon that is caused by the same quantum electromagnetic effects that attract the materials—pushes the materials into a spin. Because it is such a tiny effect, the Casimir torque has been difficult to study. The research team, which includes members from UMD's departments of electrical and computer engineering and physics and Institute for Research in Electronics and Applied Physics, has built an apparatus to measure the decades-old prediction of this phenomenon and published their results in the December 20th issue of the journal Nature.

"This is an interesting situation where industry is using something because it works, but the mechanism is not well-understood," said Jeremy Munday, the leader of the research. "For LCD displays, for example, we know how to create twisted liquid crystals, but we don't really know why they twist. Our study proves that the Casimir torque is a crucial component of liquid crystal alignment. It is the first to quantify the contribution of the Casimir effect, but is not the first to prove that it contributes."

The device places a liquid crystal just tens of nanometers from a solid crystal. With a polarizing microscope, the researchers then observed how the liquid crystal twists to match the solid's crystalline axis.

The team used liquid crystals because they are very sensitive to external forces and can twist the light that passes through them. Under the microscope, each imaged pixel is either light or dark depending on how twisted the liquid crystal layer is. In the experiment, a faint change in the brightness of a liquid crystal layer allowed the research team to characterize the liquid crystal twist and the torque that caused it.

The Casimir effect could make nanoscale parts move and can be used to invent new nanoscale devices, such as actuators or motors.

"Think of any machine that requires a torque or twist to be transmitted: driveshafts, motors, etc.," said Munday. "The Casimir torque can do this on a nanoscale."

Knowing the amount of Casimir torque in a system can also help researchers understand the motions of nanoscale parts powered by the Casimir effect.

The team tested a few different types of solids to measure their Casimir torques, and found that each material has its own unique signature of Casimir torque.

The measurement devices were built in UMD's Fab Lab, a shared user facility and cleanroom housing tools to make nanoscale devices.

In the past, the researchers also made the first measurements of a repulsive Casimir force and a measurement of the Casimir force between two spheres. They have also made some predictions that could be confirmed if the current measurement technique can be refined; Munday reports they are testing other materials to control and tailor the torque.

Munday is an associate professor of electrical and computer engineering in UMD's A. James Clark School of Engineering, and his lab is housed in UMD's Institute for Research in Electronics and Applied Physics, which enables interdisciplinary research between its natural science and engineering colleges.

"Experiments like this are helping us better understand and control the quantum vacuum. It's what one might call 'the physics of empty space,' which upon closer examination seems to be not so empty after all," said John Gillaspy, the physics program officer who oversaw National Science Foundation funding of the research.

"Classically, the vacuum is really empty—it is, by definition, the absence of anything," said Gillaspy. "But quantum physics predicts that even the most empty space that one can imagine is filled with 'virtual' particles and fields, quantum fluctuations in pure emptiness that lead to subtle, but very real, effects that can be measured and even exploited to do things that would otherwise be impossible. The universe contains many complicated things, yet there are still unanswered questions about some of the simplest, most fundamental phenomena—this research may help us to find some of the answers."

 Original story: https://energy.umd.edu/news/story/researchers-make-liquid-crystals-do-the-twist

Sankar Das Sarma and Ian Spielman Named 2018 Highly Cited Researchers

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Category: Department News
Published: Wednesday, December 05 2018 11:53

Sankar Das Sarma and Ian Spielman join six other faculty members in the University of Maryland’s College of Computer, Mathematical, and Natural Sciences included on Clarivate Analytics’ 2018 list of Highly Cited Researchers, a compilation of influential names in science.

Sankar Das Sarma is a Richard E. Prange Chair and Distinguished University Professor in Physics, Joint Quantum Institute Fellow, and Condensed Matter Theory Center Director. Das Sarma was included in all previous compilations of this list in 2017, 2016, 2015, 2014 and 2001.

Ian Spielman is an Adjunct Professor of Physics, JQI Fellow and National Institute of Standards and Technology (NIST) Fellow. Spielman was also included in the 2017 compilation.

Four New Gravitational Wave Events Detected from Black Hole Mergers

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Category: Research News
Published: Monday, December 03 2018 12:20

GWTC 1 masses.croppedThe Virgo Collaboration and the LIGO Scientific Collaboration, which includes UMD Physics Professors Peter Shawhan and Alessandra Buonanno, announced the detection of four new gravitational wave events from black hole mergers. (Image: LIGO-Virgo/Frank Elavsky/Northwestern) 

 University of Maryland physicists contribute to identification of events that now total 10 black hole mergers and one neutron star merger

Scientists announced four new observations of gravitational waves—ripples in the fabric of spacetime—from the final moments of black hole mergers.

The twin Laser Interferometer Gravitational-Wave Observatory (LIGO) detectors—located in Livingston, Louisiana, and Hanford, Washington—and the Virgo detector located near Pisa, Italy detected the gravitational wave events. The Virgo Collaboration and the LIGO Scientific Collaboration (LSC) announced the discoveries on December 1, 2018, at the Joint Space-Science Institute’s  Gravitational Wave Physics and Astronomy Workshop hosted by the University of Maryland in College Park, Maryland. Two scientific papers describing these new findings have been initially published on the arXiv repository of electronic preprints and include a catalog of all gravitational wave detections and candidate events observed to date.

“These results mark an evolution in the way we are thinking about binary black hole mergers detected by LIGO and Virgo,” said Peter Shawhan, a UMD professor of physics and an LSC principal investigator who serves as the LSC’s data analysis committee chair. “While we carefully determine the properties of the individual events, such as the masses and spins of the black holes, we are also looking at the big picture: the distribution of these properties and what that can tell us about how massive stars live and die.”

Gravitational waves carry information about their origins and about the nature of gravity that cannot otherwise be obtained. During a two-year span, physicists on the LIGO and Virgo teams detected gravitational waves from 10 black hole mergers and one merger of neutron stars, which are the dense, spherical remains of stellar explosions. The four new observations—named GW170729, GW170809, GW170818 and GW170823 for the dates they were detected—include some record breakers.

One of the new events, GW170729, is the most massive and distant gravitational wave source ever observed. This black hole merger, which happened roughly 5 billion years ago, transformed an equivalent energy of almost five solar masses into gravitational energy.

Another new event, GW170818, was triangulated well in the sky by the LIGO and Virgo detectors, making it the second-best localized gravitational wave source after the neutron star merger. The position of the binary black holes, located 2.5 billion light-years from Earth, was identified in the sky with a precision of 39 square degrees.

A major contributor to this accomplishment was Alessandra Buonanno—a UMD College Park Professor of Physics and LSC principal investigator who also has an appointment as director at the Max Planck Institute for Gravitational Physics in Potsdam, Germany. Buonanno has led the effort to develop highly accurate models of gravitational waves that black holes generate in the final process of orbiting and colliding with each other. The scientists use these waveform models to localize the source in the sky and identify it as a pair of orbiting black holes.

“State-of-the-art waveform models, advanced data processing and better calibration of the instruments have allowed us to infer astrophysical parameters of previously announced events more accurately and discover four new gravitational wave transients from black hole mergers,” Buonanno said. “I look forward to the next observing run in spring 2019, where we expect to detect more than two black hole mergers per month of collected data.” 

The scientific papers describing the new findings include a catalog of all gravitational wave detections and candidate events observed from September 12, 2015 to August 25, 2017.

Scientists observed GW170817—the merger of two neutron stars—in both gravitational waves and light. Shawhan and his students at UMD worked with other LIGO and Virgo team members to establish a program to quickly share information about each gravitational wave event candidate, including sky location, with astronomers. This enabled astronomers to look for the event with their telescopes and other instruments, marking an exciting new chapter in multi-messenger astronomy, a field in which cosmic objects are observed simultaneously in different forms of radiation.

“The one neutron star merger in the catalog, GW170817, may look a bit lonely, but we have learned so many things about it by looking at the gravitational wave data together with the incredibly rich range of follow-up observations,” said Shawhan, who is also a fellow of the Joint Space-Science Institute. “Still, we have a lot of unanswered questions about the population of binary neutron stars that future data should fill in for us.”

In one of the two new papers, the scientists carefully investigate the characteristics of the merging black hole population. Most notably, the researchers found that almost all black holes formed from stars are lighter than 45 times the mass of the sun.

“The LIGO and Virgo collaborations have worked hard to release the event properties and also the data in which these signals were found so that other scientists can analyze them with their own tools and compare them with theories of stellar evolution and gravitational wave emission,” Shawhan added.

The first detection of gravitational waves, observed on September 14, 2015, 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.

###

This press release was adapted from text provided by the LIGO and Virgo Collaborations.

The research paper, “GWTC-1: A Gravitational-Wave Transient Catalog of Compact Binary Mergers Observed by LIGO and Virgo during the First and Second Observing Runs,” by the LIGO Scientific Collaboration and the Virgo Collaboration, was presented December 1, 2018 at the Joint Space-Science Institute–Gravitational Wave Physics and Astronomy Workshop and is available on the arXiv.

The research paper, “Binary Black Hole Population Properties Inferred from the First and Second Observing Runs of Advanced LIGO and Advanced Virgo,” by the LIGO Scientific Collaboration and the Virgo Collaboration, was presented December 1, 2018 at the Joint Space-Science Institute–Gravitational Wave Physics and Astronomy Workshop and is available on the arXiv.

Media Relations Contact: Abby Robinson, 301-405-5845, This email address is being protected from spambots. You need JavaScript enabled to view it.

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About LIGO and Virgo
LIGO is funded by the National Science Foundation (NSF) and operated by Caltech and MIT, which conceived of LIGO and led the Initial and Advanced LIGO projects. Financial support for the Advanced LIGO project was led by the NSF with Germany (Max Planck Society), the U.K. (Science and Technology Facilities Council) and Australia (Australian Research Council-OzGrav) making significant commitments and contributions to the project. More than 1,200 scientists from around the world participate in the effort through the LIGO Scientific Collaboration, which includes the GEO Collaboration. A list of additional partners is available at https://my.ligo.org/census.php.

The Virgo collaboration consists of more than 300 physicists and engineers belonging to 28 different European research groups: six from Centre National de la Recherche Scientifique (CNRS) in France; 11 from the Istituto Nazionale di Fisica Nucleare (INFN) in Italy; two in the Netherlands with Nikhef; the MTA Wigner RCP in Hungary; the POLGRAW group in Poland; Spain with IFAE and the Universities of Valencia and Barcelona; two in Belgium with the Universities of Liege and Louvain; Jena University in Germany; and the European Gravitational Observatory (EGO), the laboratory hosting the Virgo detector near Pisa in Italy, funded by CNRS, INFN, and Nikhef. A list of the Virgo Collaboration can be found at http://public.virgo-gw.eu/the-virgo-collaboration/. More information is available on the Virgo website at www.virgo-gw.eu.

About the College of Computer, Mathematical, and Natural Sciences
The College of Computer, Mathematical, and Natural Sciences at the University of Maryland educates more than 9,000 future scientific leaders in its undergraduate and graduate programs each year. The college's 10 departments and more than a dozen interdisciplinary research centers foster scientific discovery with annual sponsored research funding exceeding $175 million.

 
 
 

Sundrum Win APS Sakurai Prize

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Category: Department News
Published: Tuesday, November 06 2018 09:56

Sundrum 2018 levineRaman Sundrum. Photo: Faye Levine

The American Physical Society awarded its 2019 J.J. Sakurai Prize for Theoretical Particle Physics to Raman Sundrum, a Distinguished University Professor of Physics at the University of Maryland. Sundrum’s collaborator on two key papers, Harvard University Physics Professor Lisa Randall, also received the award. 

Sundrum and Randall were honored for making a number of theoretical predictions that set off a wave of experiments searching for theoretical subatomic particles—experiments that are still active today, almost two decades later.

“As a theoretical physicist, I always hope my ideas are ultimately connected to experiments that examine the nature of reality,” said Sundrum, who also holds the John S. Toll Chair in Physics and directs the Maryland Center for Fundamental Physics. “It’s very meaningful to me that this prize was awarded for motivating experimental searches for new particles.”

Sundrum studies theoretical particle physics, which seeks to understand the subatomic particles that make up the world around us. The laws of physics—the laws of quantum mechanics, in particular—strongly suggest that such particles should be far heavier than physicists have observed them to be. This disparity is nicknamed the “hierarchy puzzle.”

In 1999, Sundrum and Randall published two papers in the journal Physical Review Letters that have been cited nearly 20,000 times in all. Their work proposed an extra dimension of space that is capable of distorting, or warping, space and time as a solution to the puzzle. People do not experience this dimension because unlike the three dimensions of space, which go on forever, this dimension is highly limited: it is more like an extradimensional, subatomic “bubble.” 

However, this dimension can affect particles. In particular, it can dramatically change the mass of particles, making the “true” mass of the particle match the mass predicted by quantum mechanics.

Sundrum and Randall’s work, which became known as the Randall-Sundrum models, makes a number of other predictions. In particular, it predicts the existence of new types of gravitons, which are theoretical particles that carry the force of gravity. This prediction inspired experiments to look for gravitons using the Large Hadron Collider (LHC), the world’s largest particle accelerator located at CERN near Geneva, Switzerland.

“These gravitons would be microscopic gravitational waves bouncing around the extra dimension, so you need a big magnifying glass, which is what the LHC is,” Sundrum said. “Our work has also inspired experiments to search for all kinds of other particles that might exist in the extra dimension. It continues to be an active area of study.”

Sundrum learned about theoretical particle physics as an undergraduate student at the University of Sydney in Australia.

“One day, I came upon a Scientific American article about particle physics,” Sundrum said. “I didn’t even know there was such a thing until I saw that article, but I found the subject so interesting that I decided to study it.”

After receiving his B.S. in mathematics and physics from the University of Sydney in 1984, Sundrum studied elementary particle theory at Yale University, where he received his Ph.D. in 1990. He then took several postdoctoral positions, including one at Boston University from 1996 to 1999. 

At Boston University, he studied “dark energy,” a theoretical form of energy that permeates the universe. Sundrum published a number of papers that tackled the topic using extra dimensions. These papers caught the attention of Randall, who invited Sundrum to collaborate. While they did not solve the mysteries of dark energy, their results turned out to be applicable to the hierarchy problem. 

“Our finding was completely unexpected,” Sundrum said. “I threw myself at the problem of dark energy and failed, but my failure spun off into a solution for the hierarchy problem.”

After taking a faculty position at the Johns Hopkins University, Sundrum came to UMD in 2010, where he continues to study particle physics in extra dimensions and other topics. Today, he is especially interested in warped extra dimensions as a source of macroscopic gravitational waves—such as those detected by the Laser Interferometer Gravitational-Wave Observatory (LIGO).

In 2018, Sundrum and three colleagues from the Maryland Center for Fundamental Physics—Michael Geller, Anson Hook and Yuhsin Tsai—wrote a paper that is accepted for publication in the journal Physical Review Letters proposing to study the gravitational wave background. Unlike gravitational wave signals from black hole or neutron star mergers, signals from the gravitational wave background can originate from collisions between extradimensional bubbles in the very early universe. These extradimensional bubbles are related to the “bubbles” that make it possible to theoretically solve the hierarchy problem and can potentially teach scientists about the early universe. 

“Our study showed that gravitational wave background signals should not be evenly spread across the entire universe, but would rather have hot spots and cold spots,” Sundrum said. “Importantly, the pattern of the hot spots could tell us about how the universe was operating at the very beginning, possibly even before the Big Bang.” 

###

The paper, “Primordial Anisotropies in the Gravitational Wave Background from Cosmological Phase Transitions,” Michael Geller, Anson Hook, Raman Sundrum and Yuhsin Tsai, is forthcoming in the journal Physical Review Letters.

The paper, “An Alternative to Compactification,” Lisa Randall and Raman Sundrum, was published in the journal Physical Review Letters on December 6, 1999.

The paper, “Large Mass Hierarchy from a Small Extra Dimension,” Lisa Randall and Raman Sundrum, was published in the journal Physical Review Letters on October 25, 1999.

Media Relations Contact: Irene Ying, 301-405-5204, This email address is being protected from spambots. You need JavaScript enabled to view it.

For a full listing of 2019 APS Award Recipients visit: http://www.aps.org/programs/honors/new-recipients.cfm

 

 

 

 

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