UMD_CMNS_Physics_S1_CMYK

  • Home
  • About Us
    • Physics Administration
    • Directions
    • Awards
    • Student Awards
    • Make a Donation
    • News
      • Research News
      • Department News
      • Newsletters
  • People
    • All
    • Faculty
      • Current
      • Emeritus
      • Adjunct
      • Affiliate
      • Research Professors
    • Research Scientists
    • Postdocs
    • Staff
    • Lecturers
    • Visitors
    • Graduate Students
  • Research
    • Research Areas
      • AI and Physical Sciences
      • Astro Metrology
      • Atomic, Molecular & Optical
      • Biophysics
      • Chemical Physics
      • Condensed Matter Experiment
      • Condensed Matter Theory
      • Cosmic Ray Physics
      • Elementary Particles
      • Gravitation Experiment
      • Gravitational Theory
      • High Energy Physics
      • Nonlinear Dynamics, Chaos and Complex Systems
      • Nuclear Physics
      • Particle Astrophysics
      • Physics Education Research
      • Plasma Physics
      • Plasma Theory
      • Quantum Science and Technology
      • Quarks, Hadrons and Nuclei
      • Space Physics
    • Centers & Institutes
  • Academics
    • OSES Home (Student Services)
    • OSES News
    • Undergraduate Program
      • Prospective Students
      • Apply Now
      • Degree Requirements and Policies
      • Scholarships
      • Undergraduate Research
      • Advising
      • Undergraduate Forms
      • Undergraduate Events
      • Departmental Honors
      • Society of Physics Students
      • FAQ
      • Undergraduate Student Committee
    • Graduate Program
      • Prospective Students
      • Open House
      • Degree Requirements
      • Graduate Resources
      • Deadlines and Forms
      • PhD Defenses
        • PhD Defenses 2025
        • PhD Defenses 2024
        • PhD Defenses 2023
        • PhD Defenses 2022
        • PhD Defenses 2021
        • PhD Defenses 2020
        • PhD Defenses 2019
        • PhD Defenses 2018
        • PhD Defenses 2017
        • PhD Defenses 2016
      • Events
      • Scholarships & Awards
      • Qualifier
      • Graduate Student Organizations
      • FAQ
    • Student Opportunities
      • GRAD-MAP
      • Graduate Student Organizations
      • Outreach Volunteering
      • Society of Physics Students
      • NSF S-STEM Program
      • Undergraduate Research
      • Women in Physics
      • Undergraduate Quantum Association
    • Courses
    • Academic Support
    • NSF S-STEM Program
    • Teaching Assistants
    • Where's my TA?
  • Events
    • Calendar
    • Physics Colloquia
    • Event Submission
    • W.J. Carr Lecture
    • Research Interaction Team (RIT) Math/Physics
    • Mechanick Quantum Biology Lecture
    • Irving and Renee Milchberg Endowed Lectureship
    • Charles W. Misner Endowed Lectureship in Gravitational Physics
    • John S. Toll Endowed Lecture
    • Prange Prize Lecture
    • Maryland Day
    • Outreach
      • Outreach Home
      • Physics is Phun
      • Discovery Days
    • Summer Programs
      • Physics Makers Camp
      • Physics of Quidditch
      • Science Discovery Camp
      • Advanced Physics Summer Program
      • Toolkit for Success
    • CUWiP
    • Vortex Makerspace
  • Services
    • Computing Services
    • Conference Room Reservations
    • Department Operations Directory
    • Electronic and Mechanical Development
    • Hiring Procedures
    • Lecture Demo
    • Mental Health Resources
    • Physics Ombudspersons
    • Printing Services
      • Poster Print Request
    • Proposal Submissions
    • Purchase Order
    • Suggestion Box
    • Textbook Order Form

Cold Atoms Offer a Glimpse of Flat Physics

Details
Category: Research News
Published: Monday, January 07 2019 09:45

These days, movies and video games render increasingly realistic 3-D images on 2-D screens, giving viewers the illusion of gazing into another world. For many physicists, though, keeping things flat is far more interesting.

One reason is that flat landscapes can unlock new movement patterns in the quantum world of atoms and electrons. For instance, shedding the third dimension enables an entirely new class of particles to emerge—particles that that don’t fit neatly into the two classes, bosons and fermions, provided by nature. These new particles, known as anyons, change in novel ways when they swap places, a feat that could one day power a special breed of quantum computer.

But anyons and the conditions that produce them have been exceedingly hard to spot in experiments. In a pair of papers published this week in Physical Review Letters, JQI Fellow Alexey Gorshkov and several collaborators proposed new ways of studying this unusual flat physics, suggesting that small numbers of constrained atoms could act as stand-ins for the finicky electrons first predicted to exhibit low-dimensional quirks.

"These two papers add to the growing literature demonstrating the promise of cold atoms for studying exotic physics in general and anyons in particular," Gorshkov says. "Coupled with recent advances in cold atom experiments—including by the grougorshkov anyon 1aSimulated images from two papers showing anyons spreading preferentially to the left in a 1-D grid (left) and a novel phase of matter that may arise from atoms constrained to move in 2-D (right). (Images courtesy of the authors)p of Ian Spielman at JQI—this work hints at exciting experimental demonstrations that might be just around the corner."

In the first paper, which was selected as an Editors’ Suggestion, Gorshkov and colleagues proposed looking for a new experimental signature of anyons—one that might be visible in a small collection of atoms hopping around in a 1-D grid. Previous work suggested that such systems might simulate the swapping behavior of anyons, but researchers only knew of ways to spot the effects at extremely cold temperatures. Instead, Fangli Liu, a graduate student at JQI, along with Gorshkov and other collaborators, found a way to detect the presence of anyons without needing such frigid climes.

Ordinarily, atoms spread out symmetrically over time in a 1-D grid, but anyons will generally favor the left over the right or vice versa. The researchers argued that straightforward changes to the laser used to create the grid would make the atoms hop less like themselves and more like anyons. By measuring the way that the number of atoms at different locations changes over time, it would then be possible to spot the asymmetry expected from anyons. Furthermore, adjusting the laser would make it easy to switch the favored direction in the experiment.

"The motivation was to use something that didn’t require extremely cold temperatures to probe the anyons," says Liu, the lead author of the paper. "The hope is that maybe some similar ideas can be used in more general settings, like looking for related asymmetries in two dimensions."

In the second paper, Gorshkov and a separate group of collaborators found theoretical evidence for a new state of matter closely related to a Laughlin liquid, the prototypical example of a substance with topological order. In a Laughlin liquid, particles—originally electrons—find elaborate ways of avoiding one another, leading to the emergence of anyons that carry only a fraction of the electric charge held by an electron.

"Anyons are pretty much still theoretical constructs," says Tobias Grass, a postdoctoral researcher at JQI and the lead author of the second paper, "and experiments have yet to conclusively demonstrate them."

Although fractional charges have been observed in experiments with electrons, many of their other predicted properties have remained unmeasurable. This makes it hard to search for other interesting behavior or to study Laughlin liquids more closely. Grass, Gorshkov and their colleagues suggested a way to manipulate the interactions between a handful of atoms and discovered a new state of matter that mixes characteristics of the Laughlin liquid and a less exotic crystal phase.

The atoms in this new state avoid one another in a similar way as electrons in a Laughlin liquid, and they also fall into a regular pattern like in a crystal—albeit in a strange way, with only half of an atom occupying each crystal site. It’s a unique mix of crystal symmetry and more complex topological order—a combination that has received little prior study.

"The idea that you have a bosonic or fermionic system, and then from interactions there emerges completely different physics—that’s only possible in lower dimensions," Grass says. "Having an experimental demonstration of any of these phases is just interesting from a fundamental perspective."

Story by Chris Cesare

 
Reference Publication
"Asymmetric Particle Transport and Light-Cone Dynamics Induced by Anyonic Statistics," Fangli Liu, James R. Garrison, Dong-Ling Deng, Zhe-Xuan Gong, Alexey V. Gorshkov, Phys. Rev. Lett., 121, 250404 (2018)
"Fractional Quantum Hall Phases of Bosons with Tunable Interactions: From the Laughlin Liquid to a Fractional Wigner Crystal," Tobias Graß, Przemyslaw Bienias, Michael J. Gullans, Rex Lundgren, Joseph Maciejko, Alexey V. Gorshkov, Phys. Rev. Lett., 121, 253403 (2018)
Research Contact: Alexey Gorshkov, This email address is being protected from spambots. You need JavaScript enabled to view it.; Tobias Grass, This email address is being protected from spambots. You need JavaScript enabled to view it.; Fangli Liu, This email address is being protected from spambots. You need JavaScript enabled to view it.
Media Contact: Chris Cesare, This email address is being protected from spambots. You need JavaScript enabled to view it.
Original story: https://jqi.umd.edu/news/cold-atoms-offer-glimpse-flat-physics

Researchers Measure Casimir Torque for the First Time

Details
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

Details
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

Details
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.

University of Maryland
College of Computer, Mathematical, and Natural Sciences
2300 Symons Hall
College Park, MD 20742
www.cmns.umd.edu
@UMDscience

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.

 
 
 

More Articles ...

  1. Sundrum Win APS Sakurai Prize
  2. Jarzynski Wins APS Onsager Prize
  3. UMD Alumnus Wins Breakthrough New Horizons Prize
  4. Fast-flowing electrons may mimic astrophysical dynamos

Page 106 of 239

  • Start
  • Prev
  • 101
  • 102
  • 103
  • 104
  • 105
  • 106
  • 107
  • 108
  • 109
  • 110
  • Next
  • End
  • Physics Administration
  • Directions
  • Awards
  • Student Awards
  • Make a Donation
  • News
    • Research News
    • Department News
    • Newsletters

College and University Links

UMD_CMNS_Physics_P1_CMYK_W

 

UMD-Primary-Logo-White

Department of Physics

University of Maryland
College Park, MD 20742-4111
Phone: 301.405.3401

 

Questions or Comments? Send us an e-mail.

Information

  • Campus Directory
  • Scholarship Opportunities
  • Undergraduate Research Opportunities
  • Prospective Undergraduates
  • Interactive Campus Map
  • Metrorail Map
  • UMShuttle Routes
  • Make a Donation 
  • Web Accessibility
  • Twitter
Department of Physics - University of Maryland - College Park, MD 20742