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<NewsItem contentIssues="true" id="72311" important="false" status="posted" url="https://beta.my.umbc.edu/groups/physics/posts/72311">
<Title>James N. Reeves, a CSST Visiting Scientist, wins award</Title>
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<![CDATA[
    <div class="html-content">James N. Reeves, a CSST Visiting Scientist, wins an award from the Italian government for a research project he worked on while visiting UMBC.  He is 3rd from the left in the photo.<br><br>
    <u>PRESS RELEASE:</u> <br>
    <strong>A study on black holes to receive the 2017 Aspen Award</strong><br>
    <br><em>A debate on the future of research and the economics of space exploration, with Nobel Prize Winner Samuel C.C. Ting, Luciano Maiani and Dr. Colleen Hartman del NASA Goddard Space Flight Center</em><br><br>
    
    Rome, October 26,  2017 – Today Thursday, October 26, from 10:30am to 1pm, at the Aspen offices at Piazza Navona 114, the ceremony took place for the <strong>2017 edition of the Aspen Institute Italia Award for scientific research and collaboration between Italy and the United States.</strong> The recipient of this year’s prize – now in its second year – is a research project entitled <strong>“Wind from the black hole accretion disk driving a molecular outflow in an active galaxy”</strong>. <br><br>
    
    The study was featured on the cover of Nature on March 26, 2015. By comparing data drawn from two powerful telescopes, the authors demonstrated how the wind from black holes contributes to the formation of new stars in diverse galaxies. They also showed how the very evolution of galaxies depends on the black holes at their centers. The work contained in this study was first begun by Bruno Rossi and Riccardo Giacconi (Nobel for Physics, 2002).<br><br>
    
    The prize will be awarded following a panel debate entitled “Looking up: Space Research, Space Economy”.  The event will be open to the press. Participants will include Samuel C. C. Ting, Nobel Prize winner, Thomas Dudley Cabot, Professor of Physics at MIT; Roberto Battiston, President of the Italian Space Agency; Colleen Hartman, NASA Goddard Space Flight Center; Paolo Savona, Vice  Chairman of Aspen Institute Italia; Lucio Stanca, Vice Chairman of Aspen Institute Italia; Luciano Maiani, Professor Emeritus of Theoretical Physics at La Sapienza University in Rome.<br><br>
    
    The award-winning authors are: Francesco Tombesi, Researcher and Assistant Professor of Astrophysics at University of Rome Tor Vergata, Assistant Research Scientist at the Department of Astronomy of the University of Maryland, College Park - USA; Astrophysicist at the NASA – Goddard Space Flight Center - USA; Marcio B. Meléndez Hernández Research Scientist in the Astronomy Department at University of Maryland; Sylvain Veilleux, Professor of Astronomy and Joint Space Science Institute Fellow at the University of Maryland;<strong> James N. Reeves, Professor, University of Maryland, Baltimore County  - USA; Astrophysics Group, School of Physical and Geographical Sciences, Keele University - United Kingdom</strong>; Eduardo González Alfonso, Professor of Physics and Mathematics at Spain’s University of Alcalá;  Christopher S. Reynolds, Professor of Astronomy and Joint Space Science Institute Fellow at the University of Maryland.<br><br><h6>
    
    
    Aspen Institute Italia Award for scientific research and collaboration between Italy and the United States</h6>
    Established in 2016, this annual award honors a research contribution to theoretical or applied natural sciences that is the product of collaboration between scientists and/or research organizations in Italy and the United States. The aim of the award is to raise the profile of collaborative efforts between the two countries in research in the natural sciences and its associated applications, by granting a cash prize of forty thousand euros for the winning entry. The Aspen Institute Italia Award builds on the commitment of the institute to organize initiatives and events exploring issues related to scientific culture and technological innovation, with a special focus on their relevance to Italy. The Announcement of the Winning Entry, the Call for Entries, the Award Rules, the Award Entry form, and all other relevant information can be found on the Aspen Italia website at <a href="http://www.aspeninstitute.it/en/aspen-institute-italia-award-scientific-research-and-collaboration-between-italy-and-united-states" rel="nofollow external" class="bo">www.aspeninstitute.it/en/aspen-institute-italia-award-scientific-research-and-collaboration-between-italy-and-united-states.
    </a></div>
]]>
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<Summary>James N. Reeves, a CSST Visiting Scientist, wins an award from the Italian government for a research project he worked on while visiting UMBC.  He is 3rd from the left in the photo.   PRESS...</Summary>
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<NewsItem contentIssues="true" id="72306" important="false" status="posted" url="https://beta.my.umbc.edu/groups/physics/posts/72306">
<Title>Dr. T. Jane Turner Discusses Black Holes in GRIT-X talk</Title>
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<![CDATA[
    <div class="html-content"><strong>Here Be Dragons: Investigating Black Holes in Galaxy Nuclei</strong><br><br>Astronomers have discovered that every galaxy has a huge black hole at its core, millions to billions of times the mass of our Sun. In most galaxies, these black holes are only revealed by their gravitational influence. However, in a few percent of galaxies gas and dust are actively falling on to the central black hole, resulting in large amounts of radiation being produced from close to the event horizon. Turner will discuss what we can learn by studying these exotic systems.<br><br>
    
    The GRIT-X-2017 talk may be found on YouTube<br><a href="https://www.youtube.com/watch?v=d_ljtbnPMRk" rel="nofollow external" class="bo">https://www.youtube.com/watch?v=d_ljtbnPMRk</a><br></div>
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<Summary>Here Be Dragons: Investigating Black Holes in Galaxy Nuclei  Astronomers have discovered that every galaxy has a huge black hole at its core, millions to billions of times the mass of our Sun. In...</Summary>
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<PostedAt>Mon, 27 Nov 2017 09:36:14 -0500</PostedAt>
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<NewsItem contentIssues="true" id="72301" important="false" status="posted" url="https://beta.my.umbc.edu/groups/physics/posts/72301">
<Title>New Article by graduate student Peter Breiding</Title>
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<![CDATA[
    <div class="html-content">“Fermi Non-detections of Four X-Ray Jet Sources and Implications for the IC/CMB Mechanism”<br><br>
     Peter Breiding<sup>1</sup>, Eileen T. Meyer<sup>1</sup>, Markos Georganopoulos<sup>1,2</sup>, M. E. Keenan<sup>1</sup>, N. S. DeNigris<sup>1</sup>, and Jennifer Hewitt<sup>1</sup> <br><br>
    The Astrophysical Journal, Volume 849, Number 2  <br><br>
    URL: <a href="http://iopscience.iop.org/article/10.3847/1538-4357/aa907a/meta" rel="nofollow external" class="bo">http://iopscience.iop.org/article/10.3847/1538-4357/aa907a/meta</a><br><br>
    Abstract:  Since its launch in 1999, the <em>Chandra</em> X-ray observatory has discovered several dozen X-ray jets associated with powerful quasars. In many cases, the X-ray spectrum is hard and appears to come from a second spectral component. The most popular explanation for the kpc-scale X-ray emission in these cases has been inverse-Compton (IC) scattering of Cosmic Microwave Background (CMB) photons by relativistic electrons in the jet (the IC/CMB model). Requiring the IC/CMB emission to reproduce the observed X-ray flux density inevitably predicts a high level of gamma-ray emission, which should be detectable with the <em>Fermi</em> Large Area Telescope (LAT). In previous work, we found that gamma-ray upper limits from the large-scale jets of 3C 273 and PKS 0637−752 violate the predictions of the IC/CMB model. Here, we present <em>Fermi</em>/LAT flux density upper limits for the X-ray jets of four additional sources: PKS 1136–135, PKS 1229–021, PKS 1354+195, and PKS 2209+080. We show that these limits violate the IC/CMB predictions at a very high significance level. We also present new <em>Hubble Space Telescope</em> observations of the quasar PKS 2209+080 showing a newly detected optical jet, and Atacama Large Millimeter/submillimeter Array band 3 and 6 observations of all four sources, which provide key constraints on the spectral shape that enable us to rule out the IC/CMB model.</div>
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<Summary>“Fermi Non-detections of Four X-Ray Jet Sources and Implications for the IC/CMB Mechanism”    Peter Breiding1, Eileen T. Meyer1, Markos Georganopoulos1,2, M. E. Keenan1, N. S. DeNigris1, and...</Summary>
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<NewsItem contentIssues="true" id="71890" important="false" status="posted" url="https://beta.my.umbc.edu/groups/physics/posts/71890">
<Title>Dr. Pelton appointed as Managing Editor for Nanophotonics</Title>
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<![CDATA[
    <div class="html-content">Dr. Matthew Pelton has begun a position as Managing Editor for Nanophotonics, an open-access journal that focuses on the interaction of photonics with nanostructures (2016 impact factor 4.492). <br><br> URL: <a href="https://www.degruyter.com/view/j/nanoph" rel="nofollow external" class="bo">https://www.degruyter.com/view/j/nanoph</a></div>
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<Summary>Dr. Matthew Pelton has begun a position as Managing Editor for Nanophotonics, an open-access journal that focuses on the interaction of photonics with nanostructures (2016 impact factor 4.492)....</Summary>
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<NewsItem contentIssues="true" id="71889" important="false" status="posted" url="https://beta.my.umbc.edu/groups/physics/posts/71889">
<Title>New article by Dr. Matthew Pelton in Nano Letters</Title>
<Body>
<![CDATA[
    <div class="html-content">“Nonmonotonic dependence of Auger recombination rate on shell thickness for CdSe/CdS core/shell nanoplatelets.”<br><br>
    Matthew Pelton, Jordan J. Andrews, Igor Fedin, Dmitri V. Talapin, Haixu Leng, and Stephen K. O’Leary<br><br>
    Nano Letters, Vol. 17, Page 6900 (2017)<br><br>
    URL: <a href="http://pubs.acs.org/doi/full/10.1021/acs.nanolett.7b03294" rel="nofollow external" class="bo">http://pubs.acs.org/doi/full/10.1021/acs.nanolett.7b03294</a><br><br>
    Abstract:  Non-radiative Auger recombination limits the efficiency with which colloidal semiconductor nanocrystals can emit light when they are subjected to strong excitation, with important implications for application of the nanocrystals in light-emitting diodes and lasers.  This has motivated attempts to engineer the structure of the nanocrystals in order to minimize Auger rates.  Here, we study Auger recombination rates in CdSe/CdS core/shell nanoplatelets, or colloidal quantum wells.  Using time-resolved photoluminescence measurements, we show that the rate of biexcitonic Auger recombination has a non-monotonic dependence on the shell thickness, initially decreasing, reaching a minimum for shells with thickness of 2 – 4 monolayers, and then increasing with further increases in the shell thickness.  This non-monotonic behavior has not previously been observed for biexcitonic recombination in quantum dots, most likely due to inhomogeneous broadening that is not present for the nanoplatelets.</div>
]]>
</Body>
<Summary>“Nonmonotonic dependence of Auger recombination rate on shell thickness for CdSe/CdS core/shell nanoplatelets.”   Matthew Pelton, Jordan J. Andrews, Igor Fedin, Dmitri V. Talapin, Haixu Leng, and...</Summary>
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<NewsItem contentIssues="true" id="71087" important="false" status="posted" url="https://beta.my.umbc.edu/groups/physics/posts/71087">
<Title>New article by Dr. Sebastian Deffner in Journal of Physics</Title>
<Body>
<![CDATA[
    <div class="html-content">“Quantum speed limits: from Heisenberg's uncertainty principle to optimal quantum control”<br><br>
    Sebastian Deffner and Steve Campbell<br><br>
    Journal of Physics A: Mathematical and Theoretical, Volume 50, Number 45 <br><br>
    URL: <a href="http://iopscience.iop.org/article/10.1088/1751-8121/aa86c6" rel="nofollow external" class="bo">http://iopscience.iop.org/article/10.1088/1751-8121/aa86c6</a><br><br>
    Abstract:  One of the most widely known building blocks of modern physics is Heisenberg's indeterminacy principle. Among the different statements of this fundamental property of the full quantum mechanical nature of physical reality, the uncertainty relation for energy and time has a special place. Its interpretation and its consequences have inspired continued research efforts for almost a century. In its modern formulation, the uncertainty relation is understood as setting a fundamental bound on how fast any quantum system can evolve. In this topical review we describe important milestones, such as the Mandelstam–Tamm and the Margolus–Levitin bounds on the quantum speed limit, and summarise recent applications in a variety of current research fields—including quantum information theory, quantum computing, and quantum thermodynamics amongst several others. To bring order and to provide an access point into the many different notions and concepts, we have grouped the various approaches into the minimal time approach and the geometric approach, where the former relies on quantum control theory, and the latter arises from measuring the distinguishability of quantum states. Due to the volume of the literature, this topical review can only present a snapshot of the current state-of-the-art and can never be fully comprehensive. Therefore, we highlight but a few works hoping that our selection can serve as a representative starting point for the interested reader.<br><br>
    
    Please see the <a href="https://news.umbc.edu/umbcs-sebastian-deffner-explains-how-the-quantum-speed-limit-may-put-brakes-on-quantum-computers/" rel="nofollow external" class="bo">UMBC news</a> release for more details.<br><br>
    
    <em>Image: Sebastian Deffner, photo by Marlayna Demond ’11 for UMBC.</em></div>
]]>
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<Summary>“Quantum speed limits: from Heisenberg's uncertainty principle to optimal quantum control”   Sebastian Deffner and Steve Campbell   Journal of Physics A: Mathematical and Theoretical, Volume 50,...</Summary>
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<NewsItem contentIssues="true" id="69919" important="false" status="posted" url="https://beta.my.umbc.edu/groups/physics/posts/69919">
<Title>Zhibo Zhang wins NSF funding for multi-disciplinary training</Title>
<Body>
<![CDATA[
    <div class="html-content">Dr. Zhang from the Physics Department and his multi-disciplinary team, including Drs. Jianwu Wang and Aryya Gangopadhyay from the Department of Information Systems and Dr. Matthias Gobbert from the Department of Mathematics and Statistics win a grant from the National Science Foundation (NSF) to launch  first-of-its-kind multi-disciplinary training on “Atmospheric Physics + Big Data + High Performance Computing”.<br><br> Dr. Zhang is the leader of the Aerosol, Cloud, Radiation-Observation and Simulation (ACROS) group.<br><br>Please see <a href="http://news.umbc.edu/umbc-receives-nsf-grant-to-launch-first-of-its-kind-big-data-and-high-performance-computing-training-for-researchers-across-disciplines/" rel="nofollow external" class="bo">UMBC news</a> release for more details.</div>
]]>
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<Summary>Dr. Zhang from the Physics Department and his multi-disciplinary team, including Drs. Jianwu Wang and Aryya Gangopadhyay from the Department of Information Systems and Dr. Matthias Gobbert from...</Summary>
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<PostedAt>Tue, 05 Sep 2017 11:14:38 -0400</PostedAt>
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<NewsItem contentIssues="true" id="69363" important="false" status="posted" url="https://beta.my.umbc.edu/groups/physics/posts/69363">
<Title>Dr. Zhai appointed as Associate Editor for Opt. Express</Title>
<Body>
<![CDATA[
    <div class="html-content">In recognizing his expertise in light scattering, radiative transfer, and remote sensing of environment, Dr. Pengwang Zhai has been appointed as an Associate Editor for Optics Express. His nomination was unanimously approved by The Optical Society (OSA)’s Board of Editors.  Dr. Zhai will serve for three years starting on Aug. 7, 2017.</div>
]]>
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<Summary>In recognizing his expertise in light scattering, radiative transfer, and remote sensing of environment, Dr. Pengwang Zhai has been appointed as an Associate Editor for Optics Express. His...</Summary>
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<NewsItem contentIssues="false" id="69305" important="false" status="posted" url="https://beta.my.umbc.edu/groups/physics/posts/69305">
<Title>Pengwang Zhai wins NASA award on ocean color remote sensing</Title>
<Body>
<![CDATA[
    <div class="html-content"><div>Ocean color radiometry provides a vital Earth observation data record, which is important for monitoring water quality and water resources, ecological forecasting, detecting and assessing harmful algal blooms, and many other applications.  For these reasons, NASA has invested in ocean color missions for several decades, which have accumulated a plethora of ocean color data and benefited many societal and economic applications.<br><br>
    
    Despite the great progress, it remains a challenging task to perform ocean color remote sensing in complex scenes involving absorbing aerosols, and coastal and in-land waters due to complicate transportation process of light between the atmosphere and ocean. This has restrained the community’s ability to understand the global water cycle, primarily in terms of water quality. In recent years, new technologies and remote sensing methods are proposed to improve ocean color retrieval in coastal regions. The use of polarimetric data is one of the most promising methods that can improve ocean color imagery interpretation and lead to better ocean property remote sensing.<br><br>
    
    Pengwang Zhai, assistant professor of physics, is an expert in light transport in atmosphere and ocean environment. He and co-investigators propose to tackle this complicate problem by combining polarimetric and ocean color radiometric observation. Polarimetric observation will be used to characterize aerosol size and composition, which will in turn be used to identify and separate light contributions from the atmosphere and ocean, a procedure called atmospheric correction. Atmospheric correction is a necessary step towards appropriate interpretation of ocean color imagery.<br><br>
    
    NASA has selected Dr. Zhai’s research team to receive an award to perform the proposed research. Dr. Zhai, as the PI, will lead this research, which involves collaboration among researchers from UMBC, NASA's Goddard Space Flight Center, NASA’s Langley Research Center, and Universities Space Research Association. Upon successful development, this research will contribute the community with a reliable and accurate ocean color retrieval algorithm that is applicable to large geographical areas and more accurate environmental data record.<br><br>
    
    <div><a href="https://physics.umbc.edu/wp-content/uploads/sites/97/2025/12/zhai-nasagrant.jpg" rel="nofollow external" class="bo"><img src="https://physics.umbc.edu/wp-content/uploads/sites/97/2025/12/zhai-nasagrant.jpg" alt="A large phytoplankton blooms captured by NASA MODIS-AQUA sensor on 8 October 2014. Browner, sediment-laden waters are also visible along the coast of Alaska." width="7504" height="4421" style="max-width: 100%; height: auto;"></a><br></div><div>
    <em>A large phytoplankton blooms captured by NASA MODIS-AQUA sensor on 8 October 2014. Browner, sediment-laden waters are also visible along the coast of Alaska. Image Credit: NASA Ocean Biology Processing Group (OBPG)</em></div></div></div>
]]>
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<Summary>Ocean color radiometry provides a vital Earth observation data record, which is important for monitoring water quality and water resources, ecological forecasting, detecting and assessing harmful...</Summary>
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<ThumbnailAltText>dr. pengwang zhai</ThumbnailAltText>
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<PostedAt>Mon, 07 Aug 2017 12:08:42 -0400</PostedAt>
<EditAt>Fri, 12 Dec 2025 11:58:39 -0500</EditAt>
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<NewsItem contentIssues="true" id="69209" important="false" status="posted" url="https://beta.my.umbc.edu/groups/physics/posts/69209">
<Title>New article by Dr. Matthew Pelton in Nature Communications</Title>
<Body>
<![CDATA[
    <div class="html-content">“A room temperature continuous-wave nano-laser using colloidal quantum wells.”<br><br>
    Zhili Yang, Matthew Pelton, Igor Fedin, Dmitri V. Talapin, and Edo Waks<br><br>
    Nature Communications, Vol. 8, Page 143 (2017)<br><br>
    URL: <a href="https://www.nature.com/articles/s41467-017-00198-z" rel="nofollow external" class="bo">https://www.nature.com/articles/s41467-017-00198-z</a><br><br>
    Abstract:  Colloidal semiconductor nanocrystals have emerged as promising active materials for solution-processable opto-electronic and light-emitting devices. In particular, the development of nanocrystal lasers is currently experiencing rapid progress. However, these lasers require large pump powers, and realizing an efficient low-power nanocrystal laser has remained a difficult challenge.  Here we demonstrate a nanolaser using colloidal nanocrystals that exhibits a threshold input power of less than 1 mW, the lowest reported threshold for any laser using colloidal emitters. We use CdSe/CdS core-shell nanoplatelets, which are efficient nanocrystal emitters with the electronic structure of quantum wells, coupled to a photonic-crystal nanobeam cavity that attains high coupling efficiencies.  The device achieves stable continuous-wave lasing at room temperature, which is essential for many photonic and opto-electronic applications.  Our results show that colloidal nanocrystals are suitable for compact and efficient opto-electronic devices based on versatile and inexpensive solution-processable materials.</div>
]]>
</Body>
<Summary>“A room temperature continuous-wave nano-laser using colloidal quantum wells.”   Zhili Yang, Matthew Pelton, Igor Fedin, Dmitri V. Talapin, and Edo Waks   Nature Communications, Vol. 8, Page 143...</Summary>
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