Dimensions Department of Physics & Astronomy

Total Page:16

File Type:pdf, Size:1020Kb

Dimensions Department of Physics & Astronomy Dimensions Department of Physics & Astronomy Photo courtesy of Guohua Wei IN THIS ISSUE: ­Faculty News ­Alumni Focus ­Selected Publications ­2015 Graduate and Masters Students ­Research Staff ­Society of Physics Students ­Graduate Achievements ­Department Events ­Undergraduate Achievements Faculty News Claude­André Faucher­Giguère's research group Vicky Kalogera has accepted an inviation to serve on (GalForm @ NU) is part ofa multi-institution team that the Committee on Astronomy and Astrophysics (CAA) has been awarded a large amount oftime to use the ofthe National Research Council. The CAA's purpose Hubble Space Telescope to map the gas flows around is to support scientific progress in astronomy and the Andromeda galaxy. It will be the first time ever that astrophysics and assist the federal goverment in they will be able to produce a spatially-resolved map of integrating and planning programs in these fields. It is the gas around a galaxy other than the Milky Way. This a joint committee ofthe Space Studies Board and the work is very important because these gas flows regulate Board on Physics andAstronomy under the National how galaxies grow. The observations will be led by Academies ofSciences, Engineering, and Medicine in collaborators at the University ofNotre Dame and the Washington, D.C.. group at Northwestern will develop the theoretical tools needed for the interpretation ofthe Hubble Prof. Kalogera has received the 2015 Hans A.Bethe observations. This ambitious project, called Project Prize. This distinguished award is given to individuals AMIGA (Absorption Maps In the Gas ofAndromeda), who have made outstanding contributions to will require an enormous 150 hours ofHubble Space astrophysics, nuclear physics, nuclear astrophysics. Telescope time. Past recipients have included James Lattimer, Stan This new award ofa large amount oftime to use the Woosley, Gordon Baym, John Bahcall, and others. Hubble Space Telescope builds on a recent pilot study http://www.aps.org/programs/honors/prizes/bethe.cfm led by the Notre Dame collaborators which has recently garnered much media attention. Prof. Kalogera has been elected to the Large Synoptic http://hubblesite.org/newscenter/archive/releases/2015/ Survey Telescope Corporation’s (LSSTC) Executive 15/full/ Board ofDirectors. In this capacity, Prof. Kalogera will participate in the oversight and administration ofthe Gerald Gabrielse, a former chair ofthe Harvard Corporation. Physics Department, is coming to Northwestern to http://www.lsst.org/ found and direct a Center for Fundamental Physics at Low Energy (CFP). Amember ofthe National In August, Prof. Kalogera spoke to nearly 40 Office for Academy ofSciences, Gabrielse is world renowened Research staffmembers at NU Knowledge at Noon, a for his high-precision tests ofthe Standard Model and faculty research presentation series. The series is its fundamental symmetries, and for starting low designed to allow staffto learn directly from energy antiproton and antihydrogen physics. The Northwestern faculty about the exciting research that Department ofPhysics & Astronomy is excited that the takes place at our institution. The series also aims to Gabrielse group and the CFP will add low energy foster connections across Office for Research staffby particle physics done using novel methods from providing the opportunity for them to meet in person. atomic, molecular, and optical physics to the many In her talk, "NU Astronomy: Big Data, Telescope cutting edge research opportunities offered to its Innovation, and the Cosmos," Dr. Kalogera covered a graduate students and postdocs. Gabrielse has briefhistory ofastronomy, but she focused mainly on prestigious awards for both his research and his the very near future: the importance ofbig data and the teaching, and will be the department's first Board of value oftwo large, related initiatives, the Large Trustees Professor. Synoptic Survey Telescope (LSST) and the Laser http://www.northwestern.edu/newscenter/stories/2015/1 Interferometer Gravitational-Wave Observatory 1/physicist-gerald-gabrielse-to-join-northwestern-.html (LIGO). https://ligo.caltech.edu/ Fall 2015 1 ­ Dimensions Jens Koch co-organizedandlecturedattheinternational Chemistry ofEarth's Interior, Quantum Optics and research workshop "Nonequilibrium physics ofdriven- Quantum Information. Applied Physics prepares graduates dissipative many-body systems," hosted by the Center for professional careers in science and technology, for Quantum Technology at the University ofKwazulu- ranging from academics to industry. Natal, South Africa, 21-25 September, 2015. Professor Koch is also an invited lecturer at the workshop "Many- James Sauls has been named Visiting Scholar ofthe body physics with light," hosted by the Kavli Institute Institute for Materials Science at Los Alamos National for Theoretical Physics at the University ofCalifornia, Laboratory. Professor Sauls delivered lectures on Santa Barbara. frontiers in hybrid quantum materials and devices, and on Shane Larson, Research Associate Professor and electrodynamics oftopological superconductors at Los Astronomer at Adler Planetarium, has been elected a Alamos. Fellow ofthe American Physical Society. His citation commends him for "Impacting science and society through the integration ofpublic engagement and research, and for empowering generations offuture Selected Publications scientists by his example." Prof. Larson spoke to a group of25 NU staffers from Claude­André Faucher­Giguère across Weinberg with his presentation, "Whispers Supernova feedback in an inhomogeneous interstellar from the Cosmos." He shared his enthusiasm as both medium by Davide Martizzi, Claude-André Faucher- an amature astronomer and a professional Giguère, Eliot Quataert. MNRAS, 450, 504 (2015). astrophysicist, walking the audience through the past Gusty, gaseous flows ofFIRE: galactic winds in and into the future ofthe science ofgravitational cosmological simulations with explicit stellar feedback by waves. Alexander L. Muratov, L. Alexander, Dusan Keres, Erik Luijten has been elected Vice Chair ofGSOFT, Claude-André Faucher-Giguère, Philip F. Hopkins, Eliot the APS Topical Group on Soft Matter. This is a position Quataert, Norman Murray. MNRAS, 454, 2691 (2015). for multiple years, during which he will subsequently transition to become Chair Elect and then Chair ofthis Faucher-Giguère’s group is pursuing a two-pronged group. approach to solving the problem ofgalaxy formation. On one hand, the Faucher-Giguère group studies the basic Adilson E. Motter hasbeenelectedFellowofthe physical processes involved in the complex galaxy American Association for the Advancement ofScience formation process, such as energy injection from (AAAS). He is being honored “For distinguished supernova explosions. On the other hand, the group contributions to the fields ofcomplex systems and implements the physical insights into the basic physical nonlinear dynamics, particularly for advances in the processes into fully cosmological models. The following network modeling and control ofcollective dynamics in pair ofnew papers is an excellent example ofthe power complex physical and biophysical systems.” ofthis approach, in which a new understanding ofthe http://www.northwestern.edu/newscenter/stories/2015/11/ effects ofsupernovae on the interstellar medium of aaas-fellows.html galaxies developed in the first paper was used to study the generation ofgalaxy-scale outflows in a cosmological James Sauls and Erik Lujiten were appointed co- model ofgalaxy evolution. Directors ofthe Applied Physics Graduate Program on http://adsabs.harvard.edu/abs/2015MNRAS.450..504M November 1. Applied Physics is a graduate program http://adsabs.harvard.edu/abs/2015MNRAS.454.2691M offered by faculty ofWeinberg and McCormick that offers a PhD in a spectrum ofresearch opportunities in Applied Physics involving Condensed Matter Physics, Physical Chemistry, Materials Physics, Physics and Fall 2015 2 ­ Dimensions Adilson E. Motter counterparts, suggesting that Advanced LIGO could Control ofstochastic and induced switching in identify certain binaries as originating from dense stellar biophysical networks by D.K. Wells, W. L. Kath, andA. environments. E. Motter. Phys. Rev. X 5, 031036 (2015). http://journals.aps.org/prl/abstract/10.1103/PhysRevLett. 115.051101 Noise caused by fluctuations at the molecular level is a fundamental part ofintracellular processes. This study James Sauls presents a scalable, quantitative least-action method to Superfluid phases of3He in nano-scale channels by predict and control noise-induced switching between Joshua Wiman, and J. A. Sauls. Physical Review B 92, different states in genetic networks that, conveniently, 144515 (2015); DOI: 10.1103/PhysRevB.92.144515 can also control transitions between stable states in the We consider superfluid 3He confined within long absence ofnoise. This framework offers a systems cylindrical channels and report new theoretical approach to identifying the key factors for rationally predictions for the equilibrium phases under strong manipulating biophysical dynamics. confinement. Four stable phases are found: a polar phase This article has been the subject ofseveral independent stable in the vicinity of , a strongly anisotropic, news articles, including: Tc cylindrical analog ofthe bulk B phase stable at -Network control: Letting noise lead the way - Research sufficiently low temperatures, and two chiral A-like team leverage cells’ noisy nature to keep them healthy, phases with distinctly
Recommended publications
  • Public Events September 2018
    Public Events September 2018 Subscribe to this publication by emailing Carol Chen atSubscribe [email protected] to this publication by emailing Shayla Butler at [email protected] Table of Contents Overview Fall Event Highlights ............................................................................................. 3 Northwestern Events Arts and Performances .......................................................................................... 8 Living Neighborhood and Community Relations Leisure and Social ......................................................................................... 10 1603 Orrington Avenue, Suite 1730 Norris Mini Courses Evanston, IL 60201 Around Campus www.northwestern.edu/communityrelations ARTica (art studio) Norris Outdoors Northwestern Music Academy Dave Davis Religious Services ......................................................................................... 13 Executive Director [email protected] Sports, Health, and Wellness 847-491-8434 Northwestern Wildcat Athletics ................................................................... 14 Recreation ..................................................................................................... 18 Academic Lectures To receive this publication electronically One Book, One Northwestern: Danielle Allen, Our Declaration .............. 20 every month, please email Shayla Butler at Academic Lectures ....................................................................................... 21 [email protected]
    [Show full text]
  • Cross Country
    NORTHWESTERN Cross Country Self-Guided Tour PARKING INFORMATION ADDRESS: Walter Athletics Center 2255 Campus Drive Evanston, IL 60208 ATHLETICS FACILITIES MAP North Ryan Campus Fieldhouse Parking Walter Garage Athletics Parking Center Lot Parking Lot ON WEEKDAYS Please park in the North Campus Parking Garage as shown above. There is an $9 daily charge for parking during the week. Upon arrival, head towards the main entrance of the Walter Athletics Center, designated by the star on the map. You will see Martin Stadium (soccer field) to begin the tour. ON WEEKENDS Parking is free on weekends. We recommend parking in the staff parking lot on the far right of the map. Upon arrival, head towards Martin Stadium (soccer field) to begin the tour. CaMPUS TOUR PATH END START PART 1: LAKEFRONT Practice Fields The Walter Athletics Center overlooks Lake Michigan, Martin Stadium, and Hutcheson Field. We use these fields for drills, strides, and yoga. Kellogg Global Hub Beyond the practice field is the Kellogg Global Hub. Completed in 2017, this 415,000-square foot building is home to the top-5 business school in the country and even has a fitness center, lockers, and a café for its students and faculty. Lakefront Trail The Lakefront Trail has two beaches and a sailing center to rent paddleboards, kayaks, and boats. The green is Wi-Fi enabled so students can study. There is a great running path and a bonfire pit as well. Running on the Trail We use the trail as a tempo loop most frequently, but the trail itself continues past the University all the way to downtown Chicago.
    [Show full text]
  • The INT @ 20 the Future of Nuclear Physics and Its Intersections July 1 – 2, 2010
    The INT @ 20 The Future of Nuclear Physics and its Intersections July 1 – 2, 2010 Program Thursday, July 1: 8:00 – 8:45: Registration (Kane Hall, Rom 210) 8:45 – 9:00: Opening remarks Mary Lidstrom, Vice Provost for Research, University of Washington David Kaplan, INT Director Session chair: David Kaplan 9:00 – 9:45: Science & Society 9:00 – 9:45 Steven Koonin, Undersecretary for Science, DOE The future of DOE and its intersections 9:45 – 10:30: Strong Interactions and Fundamental Symmetries 9:45 – 10:30 Howard Georgi, Harvard University QCD – From flavor SU(3) to effective field theory 10:30 – 11:00: Coffee Break Session chair: Martin Savage 11:00 – 11:30 Silas Beane, University of New Hampsire Lattice QCD for nuclear physics 11:30 – 12:00 Paulo Bedaque, University of Maryland Effective field theories in nuclear physics 12:00 – 12:30 Michael Ramsey-Musolf, University of Wisconsin Fundamental symmetries of nuclear physics: A window on the early Universe 12:30 – 2:00: Lunch (Mary Gates Hall) 1 Thursday, July 1 2:00 – 5:00: From Partons to Extreme Matter Session chair: Gerald Miller 2:00 – 2:30 Matthias Burkardt, New Mexico State University Transverse (spin) structure of hadrons 2:30 – 3:00 Barbara Jacak, SUNY Stony Brook Quark-gluon plasma: from particles to fields? 3:00 – 3:45 Raju Venugopalan, Brookhaven National Lab Wee gluons and their role in creating the hottest matter on Earth 3:45 – 4:15: Coffee Break Session chair: Krishna Rajagopal 4:15 – 4:45 Jean-Paul Blaizot, Saclay Is the quark-gluon plasma strongly or weakly coupled? 4:45
    [Show full text]
  • Biographical Notice of Professor S. W. Burnham of Chicago
    * 4' 509 7 142 Biographical Notice of Professor S. W. Burnham of Chicago. By the death in Chicago, March I I, 192 I, of Professor Sherburne Wesley Burnham, the celebrated dis- coverer of double stars, America has lost one of her most illustrious astronomers, and double-star astronomy its most eminent cultivator since the days of W. Herschel and K Struve, who laid the foundations of this branch of the science about a century ago. Professor Burnham was born at Thetford, Vermont, Dec. 12, 1838, and thus he attained the age of 82 years and 3 months. Though retired from active observing for about ten years, Bumham had enjoyed moderately good health for his years and somewhat frail build, and finally succumbed to weakness accentuated by a fall, in which a hip was broken. After this misfortune he lingered some three weeks, without extreme suffering, yet the shock proved too great for the feeble recuperative power incident to his advanced age. Burnham was married in the years of his early manhood, and is survived by his aged widow, several sons and daughters, including a number of grandchildren. A more detailed account of his family will be given by Professor 3.E. Barnard, in a biographical notice soon to appear in Popular Astronomy. Here it must suffice to give an outline of his scientific career, which has left so deep an impress on the science of his country and of his age. In his youth this future celebrated astronomer had received only a common school education; but already in the days of the civil war he happened to become possessed of a copy of Burritt's Geography of the Heavens, which so interested him that it turned his attention to astronomy, and he lived to devote to this science over half a century of active observation and research, with the largest telescopes in the world.
    [Show full text]
  • Annual Commencement / Northwestern University
    ) O^e J-[undred and ^orty -^ifth ^nnual Qommencement ( une 20, 2003 ^'Jsforthwestern University One Hundred and Forty-Fifth ANNUAL Commencement 6 P.M., Friday, June 20, 2003 Ryan Field Evanston, Illinois University Seal and Motto Soon after Northwestern University was redesigned the seal, retaining the book University and the date of its founding. founded, its Board of Trustees adopted and light rays and adding two quota- This seal, which remains Northwestern's an official corporate seal. This seal, ap- tions. On the pages of the open book official signature, was approved by the proved on June 26, 1856, consisted of an he placed a Greek quotation from the Board of Trustees on December 5, 1890. open book surrounded by rays of light Gospel of Saint John, chapter 1, verse and circled by the words Northwestern 14, translating to The Word . full of The full text of the University motto, University, Evanston, Illinois. grace and truth. Circling the book are adopted on June 17, 1890, is from the first three words, in Latin, of the the Epistle of Paul the Apostle to the Thirty years later Daniel Bonbright, University motto: Quaecumque sunt vera Philippians, chapter 4, verse 8 (King professor of Latin and a member of (Whatsoever things are true).. The outer James Version). Northwestern's original faculty. border of the seal carries the name of the NORTHWESTERN UNIVERSITY ^^/hatsoever things are true, whatsoever things are honest, whatsoever things are just, whatsoever things are pure, whatsoever things are lovely, whatsoever things are ofgood report; ifthere be any virtue, and ifthere be any praise, think on these things.
    [Show full text]
  • Office Directory
    Office Directory 1801 MAPLE AVENUE ACCESSIBLENU ACCOUNTING SERVICES Human Resources Compensation Suite 130, 2122 Sheridan Road, 2nd Floor, 619 Clark Street, Evanston, 847-491-7516 Evanston, IL 60201 IL 60208 Human Resources Staffing Services 847-467-5530 847-491-5337 847-491-7507 fax 847-467-5531 fax 847-467-7261 Human Resources Temp Staffing Center Lauren Blanchard Pourian, Associate Nicole Van Laan, Controller 847-467-1048 Director AccessibleNU 847-491-4722 Public Safety, Center for 847-467-5530 Nicole McDonald, Assistant Controller 847-491-5476 AccessibleNU, Chicago Trademark Licensing 312-503-4042 Amy Mykytiuk, Director Accounting 847-491-3274 AccessibleNU, Chicago Fax 847-467-2764 312-503-4173 Reginold C George, Manager ABBOTT HALL Accounting Abbott Hall, 710 N. Lake Shore Drive, ACCESS SERVICES DEPARTMENT, 847-467-1359 Chicago, IL 60611 UNIVERSITY LIBRARIES Veronica Hudgins, Executive Assistant Book Store, Northwestern University University Library, 1970 Campus Drive, 847-491-4727 +1 312-503-8486 Evanston, IL 60208 Accounting Services General Support Bursar's Office, Chicago Campus 847-491-7633 847-491-5337 +1 312-503-8525 fax 847-491-5685 (ILL) Facilities Management Circulation Desk +1 312-503-8000 847-491-7633 Financial Aid Interlibrary Loan Desk +1 312-503-8722 847-491-7630 Front Desk Mathematics Library +1 312-503-8507 847-491-7627 Housekeeping Mitchell Multimedia Center +1 312-503-8526 847-491-7678 Student Accounts/Finance Services Mudd Library Circulation Desk +1 312-503-8503 847-491-3362 Transportation & Parking Chicago Periodicals
    [Show full text]
  • LIGO SCIENTIFIC COLLABORATION VIRGO COLLABORATION the LSC
    LIGO SCIENTIFIC COLLABORATION VIRGO COLLABORATION Document Type LIGO–T1100322 VIR-0353A-11 The LSC-Virgo white paper on gravitational wave data analysis Science goals, status and plans, priorities (2011–2012 edition) The LSC-Virgo Data Analysis Working Groups, the Data Analysis Software Working Group, the Detector Characterization Working Group and the Computing Committee WWW: http://www.ligo.org/ and http://www.virgo.infn.it Processed with LATEX on 2011/10/13 LSC-Virgo data analysis white paper Contents 1 Introduction 6 2 The characterization of the data 8 2.1 LSC-Virgo-wide detector characterization priorities . .8 2.2 LIGO Detector Characterization . .9 2.2.1 Introduction . .9 2.2.2 Preparing for the Advanced Detector Era . 10 2.2.3 Priorities for LIGO Detector Characterization . 11 2.2.4 Data Run Support . 11 2.2.5 Software Infrastructure . 12 2.2.6 Noise Transients . 14 2.2.7 Spectral Features . 15 2.2.8 Calibration . 16 2.2.9 Timing . 17 2.3 GEO Detector Characterization . 18 2.3.1 Introduction . 18 2.3.2 Transient Studies . 19 2.3.3 Stationary Studies . 20 2.3.4 Stability Studies . 21 2.3.5 Calibration . 21 2.3.6 Resources . 22 2.4 Virgo Detector Characterization . 22 2.4.1 Introduction . 22 2.4.2 Calibration and h-reconstruction . 23 2.4.3 Environmental noise . 24 2.4.4 Virgo Data Quality and vetoes . 26 2.4.5 Monitoring Tools . 28 2.4.6 Noise monitoring tools . 29 2.4.7 The Virgo Data Base . 31 2.4.8 Virgo detector characterization next steps .
    [Show full text]
  • EVENT GUIDE SPECIAL ADVERTISING SECTION: This Section Was Edited and Produced by the Chicago Architecture Foundation
    ARCHITECTUREFREE FESTIVAL This weekend, get FREE, behind-the-scenes access to 200 buildings across Chicago. openhousechicago.org EVENT GUIDE SPECIAL ADVERTISING SECTION: This section was edited and produced by the Chicago Architecture Foundation. 1 PRESENTED BY About the Chicago Architecture Foundation Five years ago, the Chicago to embark on a tour, workshops for Architecture Foundation (CAF) students, lectures for adults and decided to bring a city-wide festival of field trip groups gathered around architecture and design to Chicago— our 1,000-building scale model of the quintessential city of American Chicago. architecture. London originated the In addition to Open House Chicago, “Open House” concept more than 20 CAF is best known for our 85 different years ago, New York City had several Chicago-area tours, including the top- years under its belt and even Toronto ranked tour in the city: the Chicago produced a similar festival. By 2011, it Architecture Foundation River Cruise was Chicago’s time and Open House aboard Chicago’s First Lady Cruises. Chicago was born. Our 450 highly-trained volunteer CAF was founded in 1966. As a docents lead more than 6,000 walking, STS. VOLODYMYR & OLHA UKRAINIAN CATHOLIC CHURCH (P. 10) photo by Anne Evans nonprofit organization dedicated boat, bus and L train tours each year. to inspiring people to discover why CAF also offers exhibitions, public designed matters, CAF has grown programs and education activities Ten things to know about over the years to become a hub for for all ages. Open House Chicago learning about and participating in Learn more about CAF and our architecture and design.
    [Show full text]
  • Neutron Stars
    Neutron Stars James Lattimer [email protected] Department of Physics & Astronomy Stony Brook University J.M. Lattimer, Open Nights, 9/7/2007 – p.1/25 Pulsars: The Early History 1932 Chadwick discovers the neutron. 1934 W. Baade and F. Zwicky predict existence of neutron stars as end products of supernovae. 1939 Oppenheimer and Volkoff predict upper mass limit of neutron star. 1964 Hoyle, Narlikar and Wheeler predict neutron stars rapidly rotate. 1964 Prediction that neutron stars have intense magnetic fields. 1966 Colgate and White suggest supernovae make neutron stars. 1966 Wheeler predicts Crab nebula powered by rotating neutron star. 1967 Pacini makes first pulsar model. 1967 C. Schisler discovers a dozen pulsing radio sources, including the Crab pulsar, using secret military radar in Alaska. 1967 Hewish, Bell, Pilkington, Scott and Collins discover the pulsar PSR 1919+21, Aug 6. 1968 Pulsar discovered in Crab Nebula, and it was found to be slowing down, ruling out binary models. This also clinched their connection with Type II supernovae. 1968 T. Gold identifies pulsars with magnetized, rotating neutron stars. 1968 The term “pulsar” first appears in print, in the Daily Telegraph. 1969 “Glitches” provide evidence for superfluidity in neutron star. 1971 Accretion powered X-ray pulsar discovered by Uhuru (not the Lt.). J.M. Lattimer, Open Nights, 9/7/2007 – p.2/25 Pulsars: Later Discoveries 1974 Hewish awarded Nobel Prize (but Jocelyn Bell Burnell was not). 1974 Binary pulsar PSR 1913+16 discovered by Hulse and Taylor. It shows the orbital decay due to gravitational radiation predicted by Einstein’s General Theory of Relativity.
    [Show full text]
  • January 2021 Newsletter
    APS Division of In this issue Astrophysics • April Meeting Online • Upcoming DAP election alert Electronic Newsletter January 2021 • APS Fellows • Bethe Prize Winner • Student/Postdoc Travel Grants • April Meeting: DAP and Plenary Programs & Abstract Categories • Snowmass Update APS DAP Officers 2020–2021: Finalize your plans now to attend the April 2021 meeting held virtually this year. A • Chair: Glennys Farrar number of plenary and invited sessions will • Past Chair: Joshua Frieman feature presentations by DAP members. Here are the key details: • Chair Elect: Chris Fryer • Vice Chair: Daniel Holz What: April 2021 APS Meeting ​ ​ ​ • Secretary/Treasurer: Judith Racusin When: April 17 - 20, 2021 ​ • Deputy Sec./Treasurer: Amy Furniss Where: Online ​ Abstract Deadline: Jan 8, 2021, 5 pm EST • Division Councilor: Cole Miller ​ Travel Grant Deadline: Jan 31, 2021 • Member-at-Large: Stefano Profumo ​ Early Registration Deadline: Feb 26, 2021 • Member-at-Large: Ignacio Taboada ​ Late Registration Deadline: Mar 26, 2021 ​ • Member-at-Large: Erin Kara • Member-at-Large: Laura Blecha The 2021 April Meeting will be virtual. ​ Questions? Comments? Detailed information for the meeting, including details on registration and the scientific Newsletter editors: program can be found online at https://april.aps.org/ Amy Furniss [email protected] HEADS-UP: The ELECTION for next year’s ​ ​ DAP Executive Committee and chairline will Judith Racusin be held soon. Be on the lookout for the [email protected] announcement from APS, and please vote! ​ 1 Dear DAP, Please see the January 2021 DAP newsletter below. It will be archived on the DAP website (https://www.aps.org/units/dap/newsletters/index.cfm).
    [Show full text]
  • EVENT GUIDE SPECIAL ADVERTISING SECTION: This Section Was Edited and Produced by the Chicago Architecture Foundation
    ARCHITECTUREFREE FESTIVAL This weekend, get FREE, behind-the-scenes access to 200+ buildings across Chicago. openhousechicago.org EVENT GUIDE SPECIAL ADVERTISING SECTION: This section was edited and produced by the Chicago Architecture Foundation. 2 PRESENTED BY ABOUT THE CHICAGO ARCHITECTURE FOUNDATION Six years ago, the Chicago Architecture Foundation (CAF) launched the first Open House Chicago. This free, citywide festival drew 23,000 people in its first year. By 2016, it grew to 100,000 attendees, making it one of the largest architecture events in the world. This year is our biggest yet, with more than 200 sites. OHC is just one of many CAF programs that inspire people to discover why design matters. Today, when you visit CAF at 224 S. Michigan Ave., you’ll find visitors embarking on tours, FIRST CHURCH OF DELIVERANCE, BRONZEVILLE (p. 15) camps for children, lectures for adults and field trip groups gathered around our 3D model of Chicago. TEN THINGS TO KNOW ABOUT In summer 2018, CAF will open the Chicago Architecture Center at CHICAGO ARCHITECTURE CENTER — OPEN HOUSE CHICAGO (OHC) COMING IN SUMMER 2018 111 E. Wacker Dr. This new location is situated above the dock for the 1. OHC is a FREE public festival with behind-the-scenes access Chicago Architecture Foundation River CAF’s 450 expert volunteer docents to 200+ buildings across Chicago—no tickets required. Cruise aboard Chicago’s First Lady will lead 85+ tours from the Center, Cruises—the city’s top-ranked tour. by boat, bus, L train and on foot for SPECIAL CHICAGO ARCHITECTURE FOUNDATION ADVERTISING SECTION | THURSDAY, OCTOBER 12, 2017 ADVERTISING SECTION | THURSDAY, SPECIAL CHICAGO ARCHITECTURE FOUNDATION 2.
    [Show full text]
  • David Norman Schramm October 25, 1945–December 19, 1997
    NATIONAL ACADEMY OF SCIENCES D AVID NORMAN SCHRAMM 1 9 4 5 — 1 9 9 7 A Biographical Memoir by M I C H A E L S . T URNER Any opinions expressed in this memoir are those of the author and do not necessarily reflect the views of the National Academy of Sciences. Biographical Memoir COPYRIGHT 2009 NATIONAL ACADEMY OF SCIENCES WASHINGTON, D.C. DAVID NORMAN SCHRAMM October 25, 1945–December 19, 1997 B Y MICHAEL S . TURNER “ E LIVED LARGE IN ALL DIMENSIONS.” That is how Leon HLederman began his eulogy of David N. Schramm at a memorial service held in Aspen, Colorado, in December 1997. His large presence in space went beyond his 6-foot, 4-inch, 240-pound frame and bright red hair. In spite of his tragic death in a plane crash at age 52, Schramm lived large in the time dimension, too. At 18, he was married, a father, and a freshman physics major at MIT. After receiving his Ph.D. in physics from Caltech at 25, Schramm joined the faculty at the University of Texas at Austin. He left for Chicago two years later, and became the chair of the Astronomy and Astrophysics Department at the University of Chicago at age 2. He was elected to the National Academy of Sciences in 1986 at 40, became chair of the National Research Council’s Board on Physics and Astronomy at 47, and two years later became vice president for research at Chicago. He also had time for mountain climbing, summiting the highest peaks in five of the seven continents (missing Asia and Antarctica), driving a red Porsche with license plates that read “Big Bang,” and flying—owning four airplanes over his 12-year flying career and logging hundreds of hours annually.
    [Show full text]