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X-WR-CALNAME:Physics & Astronomy
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X-WR-CALDESC:Events for Physics & Astronomy
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DTSTART:20130310T080000
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BEGIN:VEVENT
DTSTART;TZID=America/Chicago:20140123T160000
DTEND;TZID=America/Chicago:20140123T180000
DTSTAMP:20260610T184211
CREATED:20150125T213247Z
LAST-MODIFIED:20230207T160004Z
UID:10363277-1390492800-1390500000@uwm.edu
SUMMARY:Biophysics Seminar: Jason Tenboer
DESCRIPTION:The Physics department Biophysics Seminars are usually on Thursday afternoons from 4:00-6:00 pm in Room 481. Refreshments are served from 4:00-4:15 pm in the same room. \nSBL1 and SBL2: in-house tools for XFEL experiment preparation\nJason Tenboer\, Research Assistant\, Physics Dept.
URL:https://uwm.edu/physics/event/biophysics-seminar-jason-tenboer-2/
LOCATION:Physics 481 – UW-Milwaukee\, 1900 E Kenwood Blvd\, Milwaukee\, WI\, 53211
CATEGORIES:Biophysics Seminars
X-TRIBE-STATUS:
GEO:43.0754208;-87.886051
X-APPLE-STRUCTURED-LOCATION;VALUE=URI;X-ADDRESS=Physics 481 – UW-Milwaukee 1900 E Kenwood Blvd Milwaukee WI 53211;X-APPLE-RADIUS=500;X-TITLE=1900 E Kenwood Blvd:geo:-87.886051,43.0754208
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=America/Chicago:20140131T144500
DTEND;TZID=America/Chicago:20140131T160000
DTSTAMP:20260610T184211
CREATED:20150122T190005Z
LAST-MODIFIED:20151119T171953Z
UID:10363266-1391179500-1391184000@uwm.edu
SUMMARY:Colloquium: Dr. Ivan Agullo
DESCRIPTION:The Physics department colloquia are usually on Friday afternoons at 3 pm in Room 135. Coffee and cookies are served at 2:45 pm in the same room. Anyone is welcome. \nQuantum Gravity and the Observable Universe\nDr. Ivan Agullo\, Assistant Professor\, Dept. of Physics & Astronomy\, Louisiana State University \nAn important difficulty in the search for a satisfactory theory of quantum gravity is the absence of experimental guidance. The astonishing improvement in cosmological observations attained in the last few years offers an exciting opportunity to change this situation. It is believed that the anisotropies observed in the CMB and in the distribution of galaxies were originated in the very early universe.  Observing their details could therefore tell us about physics in such extreme conditions. \nIn this talk I will review the physics of the genesis of cosmic non-uniformities\, paying special attention to the interplay between quantum effects and gravitation. I will describe how cosmological observations can provide detailed information about processes where the relationship between gravity and quantum mechanics plays a crucial role.
URL:https://uwm.edu/physics/event/colloquium-dr-ivan-agullo/
LOCATION:Physics 135 – UW-Milwaukee\, 1900 E Kenwood Blvd\, Milwaukee\, WI\, 53211
CATEGORIES:Physics Colloquia
X-TRIBE-STATUS:
GEO:43.0754208;-87.886051
X-APPLE-STRUCTURED-LOCATION;VALUE=URI;X-ADDRESS=Physics 135 – UW-Milwaukee 1900 E Kenwood Blvd Milwaukee WI 53211;X-APPLE-RADIUS=500;X-TITLE=1900 E Kenwood Blvd:geo:-87.886051,43.0754208
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=America/Chicago:20140213T160000
DTEND;TZID=America/Chicago:20140213T180000
DTSTAMP:20260610T184211
CREATED:20150125T212935Z
LAST-MODIFIED:20230207T160029Z
UID:10363276-1392307200-1392314400@uwm.edu
SUMMARY:Biophysics Seminar: Dr. Russell Fung
DESCRIPTION:The Physics department Biophysics Seminars are usually on Thursday afternoons from 4:00-6:00 pm in Room 481. Refreshments are served from 4:00-4:15 pm in the same room. \nTowards Extracting Dynamics Below Timing Jitter by Manifold-based Machine Learning\nDr. Russell Fung\, Senior Scientist\, UWM Physics Dept.
URL:https://uwm.edu/physics/event/biophysics-seminar-dr-russell-fung/
LOCATION:Physics 481 – UW-Milwaukee\, 1900 E Kenwood Blvd\, Milwaukee\, WI\, 53211
CATEGORIES:Biophysics Seminars
X-TRIBE-STATUS:
GEO:43.0754208;-87.886051
X-APPLE-STRUCTURED-LOCATION;VALUE=URI;X-ADDRESS=Physics 481 – UW-Milwaukee 1900 E Kenwood Blvd Milwaukee WI 53211;X-APPLE-RADIUS=500;X-TITLE=1900 E Kenwood Blvd:geo:-87.886051,43.0754208
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=America/Chicago:20140227T160000
DTEND;TZID=America/Chicago:20140227T180000
DTSTAMP:20260610T184211
CREATED:20150125T212325Z
LAST-MODIFIED:20230207T160037Z
UID:10363272-1393516800-1393524000@uwm.edu
SUMMARY:Biophysics Seminar: Karl Koebke
DESCRIPTION:The Physics department Biophysics Seminars are usually on Thursday afternoons from 4:00-6:00 pm in Room 481. Refreshments are served from 4:00-4:15 pm in the same room. \nMethods for the Study of Nitric Oxide Reactive Heme Proteins\nKarl Koebke\, Research Assistant\, UWM Chemistry Dept.
URL:https://uwm.edu/physics/event/biophysics-seminar-karl-koebke/
LOCATION:Physics 481 – UW-Milwaukee\, 1900 E Kenwood Blvd\, Milwaukee\, WI\, 53211
CATEGORIES:Biophysics Seminars
X-TRIBE-STATUS:
GEO:43.0754208;-87.886051
X-APPLE-STRUCTURED-LOCATION;VALUE=URI;X-ADDRESS=Physics 481 – UW-Milwaukee 1900 E Kenwood Blvd Milwaukee WI 53211;X-APPLE-RADIUS=500;X-TITLE=1900 E Kenwood Blvd:geo:-87.886051,43.0754208
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=America/Chicago:20140307T144500
DTEND;TZID=America/Chicago:20140307T160000
DTSTAMP:20260610T184211
CREATED:20150122T182244Z
LAST-MODIFIED:20230207T160046Z
UID:10363264-1394203500-1394208000@uwm.edu
SUMMARY:Colloquium: Dr. Artem Rudenko
DESCRIPTION:The Physics department colloquia are usually on Friday afternoons at 3 pm in Room 135. Coffee and cookies are served at 2:45 pm in the same room. Anyone is welcome. \nReal-time Imaging of Light-induced Reactions: From Strong-field Physics to Ultrafast Photochemistry\nDr. Artem Rudenko\, Assistant Professor\, Dept. of Physics (James Macdonald Lab)\, Kansas State University \nOver the last thirty years we have witnessed rapid development of intense short-pulsed coherent radiation sources\, such as femtosecond optical and infrared lasers\, their higher-order harmonics in the extreme ultra-violet (EUV) domain\, and EUV/X-ray free-electron lasers.  These novel tools opened up a variety of exciting possibilities to visualize structure of matter\, and to trace its dynamical evolution of a length and time scales of single atom motion.  In particular\, significant advances had been made towards tracing photo-induced chemical reactions in real time\, defining properties of molecular transition states and imaging nano-scale objects with nearly atomic resolution.  Most of these measurements exploit the availability of ultrashort intense light bursts in a broad range of wavelengths\, which allows one to initiate different types of dynamics (e.g.\, create decaying excited states of an atom\, prepare a bound or continuum molecular wave packet\, etc.)\, and then to obtain snapshots of the created transient structure faster than the latter evolves (the so-called “pump-probe” scheme).  The success of this approach critically depends on our understanding of basic mechanisms of (often non-linear) light-matter interactions\, starting from the electronic response of single atoms. \nI will present an overview of the experimental program aimed to develop novel schemes of ultrafast time-resolved measurements\, and to advance our knowledge on the interaction of atoms\, molecules and nano-size particles with intense laser-like radiation of different wavelengths\, focusing on the experiments employing coincidence ion and electron imaging techniques for taking snapshots of atomic and molecular structure.  Examples will include measurements in optical\, EUV and X-ray domains.
URL:https://uwm.edu/physics/event/colloquium-dr-artem-rudenko/
LOCATION:Physics 135 – UW-Milwaukee\, 1900 E Kenwood Blvd\, Milwaukee\, WI\, 53211
CATEGORIES:Physics Colloquia
X-TRIBE-STATUS:
GEO:43.0754208;-87.886051
X-APPLE-STRUCTURED-LOCATION;VALUE=URI;X-ADDRESS=Physics 135 – UW-Milwaukee 1900 E Kenwood Blvd Milwaukee WI 53211;X-APPLE-RADIUS=500;X-TITLE=1900 E Kenwood Blvd:geo:-87.886051,43.0754208
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=America/Chicago:20140313T160000
DTEND;TZID=America/Chicago:20140313T170000
DTSTAMP:20260610T184211
CREATED:20150125T211705Z
LAST-MODIFIED:20230207T160054Z
UID:10363271-1394726400-1394730000@uwm.edu
SUMMARY:Biophysics Seminar: Natalia Stein
DESCRIPTION:The Physics department Biophysics Seminars are usually on Thursday afternoons from 4:00-6:00 pm in Room 481. Refreshments are served from 4:00-4:15 pm in the same room. \nLigand binding and reduction potentials of Cytochrome c Nitrite Reductase (CcNiR)\nNatalia Stein\, Research Assistant\, UWM Chemistry Dept.
URL:https://uwm.edu/physics/event/biophysics-seminar-natalia-stein/
LOCATION:Physics 481 – UW-Milwaukee\, 1900 E Kenwood Blvd\, Milwaukee\, WI\, 53211
CATEGORIES:Biophysics Seminars
X-TRIBE-STATUS:
GEO:43.0754208;-87.886051
X-APPLE-STRUCTURED-LOCATION;VALUE=URI;X-ADDRESS=Physics 481 – UW-Milwaukee 1900 E Kenwood Blvd Milwaukee WI 53211;X-APPLE-RADIUS=500;X-TITLE=1900 E Kenwood Blvd:geo:-87.886051,43.0754208
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=America/Chicago:20140327T160000
DTEND;TZID=America/Chicago:20140327T180000
DTSTAMP:20260610T184211
CREATED:20150125T211230Z
LAST-MODIFIED:20230207T160139Z
UID:10363270-1395936000-1395943200@uwm.edu
SUMMARY:Biophysics Seminar: Dr. Peter Schwander
DESCRIPTION:The Physics department Biophysics Seminars are usually on Thursday afternoons from 4:00-6:00 pm in Room 481. Refreshments are served from 4:00-4:15 pm in the same room. \nThe Ribosome – 3D Movie of a Brownian Machinge\nDr. Peter Schwander\, Senior Scientist\, UWM Physics Dept.
URL:https://uwm.edu/physics/event/biophysics-seminar-dr-peter-schwander/
LOCATION:Physics 481 – UW-Milwaukee\, 1900 E Kenwood Blvd\, Milwaukee\, WI\, 53211
CATEGORIES:Biophysics Seminars
X-TRIBE-STATUS:
GEO:43.0754208;-87.886051
X-APPLE-STRUCTURED-LOCATION;VALUE=URI;X-ADDRESS=Physics 481 – UW-Milwaukee 1900 E Kenwood Blvd Milwaukee WI 53211;X-APPLE-RADIUS=500;X-TITLE=1900 E Kenwood Blvd:geo:-87.886051,43.0754208
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=America/Chicago:20140328T144500
DTEND;TZID=America/Chicago:20140328T160000
DTSTAMP:20260610T184211
CREATED:20150122T174531Z
LAST-MODIFIED:20230207T160147Z
UID:10363262-1396017900-1396022400@uwm.edu
SUMMARY:Colloquium: Dr. Claude-André Faucher-Giguère
DESCRIPTION:The Physics department colloquia are usually on Friday afternoons at 3 pm in Room 135. Coffee and cookies are served at 2:45 pm in the same room. Anyone is welcome. \nFeedback-Regulated Star Formation on Galactic and Cosmological Scales\nDr. Claude-André Faucher-Giguère\, Northwestern University \nA central problem in galaxy formation is to understand why star formation is so inefficient. Within individual galaxies\, gas is converted into stars at a rate two orders of magnitude slower than unimpeded gravitational collapse predicts\, a fact embodied in the low normalization of the observed Kennicutt-Schmidt (K-S) relationship between star formation rate surface density and gas surface density. Star formation in galaxies is also globally inefficient in the sense that the stellar mass in dark matter halos is a small fraction of the universal baryon fraction. I will show that these two facts can be explained by the self-regulation of star formation by feedback from massive stars. Within galaxies\, stellar feedback drives turbulence that supports the interstellar medium against collapse and the K-S law is set by the low strength of gravity relative to stellar feedback. The energy input from the same stellar feedback processes drive powerful galactic outflows that remove most of the gas accreted from the intergalactic medium before it has time to turn into stars. Using cosmological hydrodynamical simulations from our FIRE project (“Feedback In Realistic Environments”)\, I will show that gas removal by star formation-driven galactic winds successfully explains the observed galaxy stellar mass function\, at least for galaxies less massive than the Milky Way\, and discuss the observational signatures of circum-galactic gas flows. Feedback from massive black holes may be required to explain the quenching of galaxies much more massive than the Milky Way.
URL:https://uwm.edu/physics/event/colloquium-dr-claude-andre-faucher-giguere/
LOCATION:Physics 135 – UW-Milwaukee\, 1900 E Kenwood Blvd\, Milwaukee\, WI\, 53211
CATEGORIES:Physics Colloquia
X-TRIBE-STATUS:
GEO:43.0754208;-87.886051
X-APPLE-STRUCTURED-LOCATION;VALUE=URI;X-ADDRESS=Physics 135 – UW-Milwaukee 1900 E Kenwood Blvd Milwaukee WI 53211;X-APPLE-RADIUS=500;X-TITLE=1900 E Kenwood Blvd:geo:-87.886051,43.0754208
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=America/Chicago:20140410T160000
DTEND;TZID=America/Chicago:20140410T180000
DTSTAMP:20260610T184211
CREATED:20150125T210833Z
LAST-MODIFIED:20160315T175504Z
UID:10363269-1397145600-1397152800@uwm.edu
SUMMARY:Biophysics Seminar: Jennifer McGarry
DESCRIPTION:The Physics department Biophysics Seminars are usually on Thursday afternoons from 4:00-6:00 pm in Room 481. Refreshments are served from 4:00-4:15 pm in the same room. \nTo Be Announced\nJennifer McGarry\, Research Assistant\, UWM Biochemistry Dept.
URL:https://uwm.edu/physics/event/biophysics-seminar-jennifer-mcgarry/
LOCATION:Physics 481 – UW-Milwaukee\, 1900 E Kenwood Blvd\, Milwaukee\, WI\, 53211
CATEGORIES:Biophysics Seminars
X-TRIBE-STATUS:
GEO:43.0754208;-87.886051
X-APPLE-STRUCTURED-LOCATION;VALUE=URI;X-ADDRESS=Physics 481 – UW-Milwaukee 1900 E Kenwood Blvd Milwaukee WI 53211;X-APPLE-RADIUS=500;X-TITLE=1900 E Kenwood Blvd:geo:-87.886051,43.0754208
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=America/Chicago:20140418T144500
DTEND;TZID=America/Chicago:20140418T160000
DTSTAMP:20260610T184211
CREATED:20150102T170718Z
LAST-MODIFIED:20230207T160158Z
UID:10435314-1397832300-1397836800@uwm.edu
SUMMARY:Colloquium: Dr. Bruce Allen
DESCRIPTION:The Physics department colloquia are usually on Friday afternoons at 3 pm in Room 135. Coffee and cookies are served at 2:45 pm in the same room. Anyone is welcome. \nThe Einstein@Home Search for Gravitational Waves and Neutron Stars\nDr. Bruce Allen\, Albert Einstein Institute (Hannover\, Germany) \nEinstein@Home is a volunteer distributed computing project with more than 350\,000 participants. Like other volunteer computing projects\, Einstein@Home harvests idle computer cycles from the laptop and desktop computers of the general public.  This provides enormous computing power\, on the scale of some of the world’s fastest supercomputers\, but at very low cost. \nI describe the current status of the Einstein@Home search for new neutron stars\, using data from the Laser Interferometer Gravitational-wave Observatory (LIGO)\, from the Arecibo and Parkes radio telescopes\, and from the Fermi gamma-ray satellite.  The sensitivity of these searches is limited by computing power\, so the Einstein@Home approach allows the detection of weaker signals than more conventional approaches.  In the past few years\, Eienstein@Home has discovered more than 50 new pulsars\, including a number of particularly interesting and exotic systems.
URL:https://uwm.edu/physics/event/colloquium-dr-bruce-allen/
LOCATION:Physics 135 – UW-Milwaukee\, 1900 E Kenwood Blvd\, Milwaukee\, WI\, 53211
X-TRIBE-STATUS:
GEO:43.0754208;-87.886051
X-APPLE-STRUCTURED-LOCATION;VALUE=URI;X-ADDRESS=Physics 135 – UW-Milwaukee 1900 E Kenwood Blvd Milwaukee WI 53211;X-APPLE-RADIUS=500;X-TITLE=1900 E Kenwood Blvd:geo:-87.886051,43.0754208
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=America/Chicago:20140424T160000
DTEND;TZID=America/Chicago:20140424T180000
DTSTAMP:20260610T184211
CREATED:20150125T210352Z
LAST-MODIFIED:20230207T160206Z
UID:10363268-1398355200-1398362400@uwm.edu
SUMMARY:Biophysics Seminar: Dr. Gabriel Biener
DESCRIPTION:The Physics department Biophysics Seminars are usually on Thursday afternoons from 4:00-6:00 pm in Room 481. Refreshments are served from 4:00-4:15 pm in the same room. \nOptical Micro-Spectroscope with Exquisite Sensitivity and Spectral Resolution: Design\, Characterization\, and Applications\nDr. Gabriel Biener\, Research Associate\, UWM Physics Dept.
URL:https://uwm.edu/physics/event/biophysics-seminar-dr-gabriel-biener-2/
LOCATION:Physics 481 – UW-Milwaukee\, 1900 E Kenwood Blvd\, Milwaukee\, WI\, 53211
CATEGORIES:Biophysics Seminars
X-TRIBE-STATUS:
GEO:43.0754208;-87.886051
X-APPLE-STRUCTURED-LOCATION;VALUE=URI;X-ADDRESS=Physics 481 – UW-Milwaukee 1900 E Kenwood Blvd Milwaukee WI 53211;X-APPLE-RADIUS=500;X-TITLE=1900 E Kenwood Blvd:geo:-87.886051,43.0754208
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=America/Chicago:20140425T144500
DTEND;TZID=America/Chicago:20140425T160000
DTSTAMP:20260610T184211
CREATED:20150102T165245Z
LAST-MODIFIED:20151119T171732Z
UID:10435313-1398437100-1398441600@uwm.edu
SUMMARY:Colloquium: Dr. Sokrates T. Pantelides
DESCRIPTION:The Physics department colloquia are usually on Friday afternoons at 3 pm in Room 135. Coffee and cookies are served at 2:45 pm in the same room. Anyone is welcome. \nProbing Complex Materials One Atom at a Time by a Combination of Theory and Microscopy\nDr. Sokrates T. Pantelides\, University Distinguished Professor of Physics and Engineering\, Dept. of Physics and Astronomy & Dept. of Electrical Engineering & Computer Science\, Vanderbuilt University and Materials Science and Techonogy Division\, Oak Ridge National Laboratory \nCalculations based on density functional theory using high-performance computers have made enormous strides in describing the atomic-scale properties of complex materials.  In parallel\, aberration-corrected scanning transmission electron microscopy has reached extraordinary levels of spatial and energy resolution\, in both imaging and electron-energy-loss spectroscopy.  The combination of theory and microscopy provides an unparalleled probe to unravel the atomic-scale processes that control vital properties for electronic\, optoelectronic\, and energy-related applications.  Your are invited to a journey through the wide world of complex materials structures – semiconductors\, superconductors\, complex oxides\, graphene\, ultrasmall nanoparticles – for a first-hand experience of the nanoscale. \nResearch supported by DOE Basic Energy Sciences; primary collaborator; Steve Pennycook (formerly at ORNL).
URL:https://uwm.edu/physics/event/colloquium-dr-sokrates-t-pantelides/
LOCATION:Physics 135 – UW-Milwaukee\, 1900 E Kenwood Blvd\, Milwaukee\, WI\, 53211
CATEGORIES:Physics Colloquia
X-TRIBE-STATUS:
GEO:43.0754208;-87.886051
X-APPLE-STRUCTURED-LOCATION;VALUE=URI;X-ADDRESS=Physics 135 – UW-Milwaukee 1900 E Kenwood Blvd Milwaukee WI 53211;X-APPLE-RADIUS=500;X-TITLE=1900 E Kenwood Blvd:geo:-87.886051,43.0754208
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=America/Chicago:20140502T144500
DTEND;TZID=America/Chicago:20140502T160000
DTSTAMP:20260610T184211
CREATED:20141229T173125Z
LAST-MODIFIED:20230207T160219Z
UID:10435312-1399041900-1399046400@uwm.edu
SUMMARY:Colloquium: Dr. Nick Gnedin
DESCRIPTION:The Physics department colloquia are usually on Friday afternoons at 3 pm in Room 135. Coffee and cookies are served at 2:45 pm in the same room. Anyone is welcome. \nSimulating Cosmic Reionization\nDr. Nick Gnedin\, Professor at the University of Chicago and Scientist at Fermilab \nI will review the field of numerical simulations of cosmic reionization: the process of ionizing of intergalactic medium by high redshift galaxies and quasars.  I will describe the main physical processes that are important for modeling reionization\, explain how these processes are incorporated in computer simulations\, and will use simulations to gain insight into the actual reionization process. \nI will finish with an illustration of how the exponential progress in the computer industry allows us to solve problems that we could not even dream about a mere 10 years ago.
URL:https://uwm.edu/physics/event/colloquium-dr-nick-gnedin/
LOCATION:Physics 135 – UW-Milwaukee\, 1900 E Kenwood Blvd\, Milwaukee\, WI\, 53211
CATEGORIES:Physics Colloquia
X-TRIBE-STATUS:
GEO:43.0754208;-87.886051
X-APPLE-STRUCTURED-LOCATION;VALUE=URI;X-ADDRESS=Physics 135 – UW-Milwaukee 1900 E Kenwood Blvd Milwaukee WI 53211;X-APPLE-RADIUS=500;X-TITLE=1900 E Kenwood Blvd:geo:-87.886051,43.0754208
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=America/Chicago:20140508T144500
DTEND;TZID=America/Chicago:20140508T160000
DTSTAMP:20260610T184211
CREATED:20141229T165134Z
LAST-MODIFIED:20230207T160227Z
UID:10435311-1399560300-1399564800@uwm.edu
SUMMARY:Colloquium: Dr. Zhong Ren
DESCRIPTION:The Physics department colloquia are usually on Friday afternoons at 3 pm in Room 135. Coffee and cookies are served at 2:45 pm in the same room. Anyone is welcome. \nMechanics and Dynamics of Protein Structures\nDr. Zhong Ren\, CEO-Renz Research \nMy research integrates experimental and computational approaches in dynamic crystallography to study mechanics and dynamics during protein function.  I will present an example to illustrate how a K+ channels gating ring achieves its function for clean opening and closing.  I will also present a recent study on the cooperative mechanism of human hemoglobin (doi:10.1371/journal.pone.0077141 and ~363) and demonstrate how a structural meta-analysis is employed to extract structural dynamics from increasingly abundant entries in the Protein Data Bank.  I will show several experimental and computational advances that would suit different types of protein crystals in dynamic studies\, which include light sensitive systems such as photoreceptors and light inert enzymes.  Finally\, I will propose a viable technical route to push time resolution of single crystal diffraction down to sub-ps using XFEL sources and speculate on what kind of structural signal that could be captured.  The structural changes we have recently observed in a simpler hemoglobin from an invertebrate at 100 ps and a fraction of such synchrotron bunch provide confidence for future XFEL experiments.
URL:https://uwm.edu/physics/event/colloquium-dr-zhong-ren/
LOCATION:Physics 135 – UW-Milwaukee\, 1900 E Kenwood Blvd\, Milwaukee\, WI\, 53211
CATEGORIES:Physics Colloquia
X-TRIBE-STATUS:
GEO:43.0754208;-87.886051
X-APPLE-STRUCTURED-LOCATION;VALUE=URI;X-ADDRESS=Physics 135 – UW-Milwaukee 1900 E Kenwood Blvd Milwaukee WI 53211;X-APPLE-RADIUS=500;X-TITLE=1900 E Kenwood Blvd:geo:-87.886051,43.0754208
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=America/Chicago:20140509T144500
DTEND;TZID=America/Chicago:20140509T160000
DTSTAMP:20260610T184211
CREATED:20141222T163917Z
LAST-MODIFIED:20230207T160233Z
UID:10435310-1399646700-1399651200@uwm.edu
SUMMARY:Colloquium: Robert H. Austin
DESCRIPTION:The Physics department colloquia are usually on Friday afternoons at 3 pm in Room 135.  Coffee and cookies are served at 2:45 pm in the same room.  Anyone is welcome. \nThe Physics of the Games Cancer Plays\nDr. Robert H. Austin\, Department of Physics\, Princeton University \nCancer is a complex condition with strong ecological elements\, often consisting of stromal cells as well as cancer cells.  Stromal cell provide protection from drug-induced apoptosis in cancer via secreting growth signals and further mediate cancer cell growth and survival under treatment.  I’ll talk about a microfluidic ecology which mimics the bone marrow ecology under chemotherapy\, including extracellular matrix and stromal cells\, drug gradients\, and weakly connected micro-habitats\, to visualize the dynamics of multiple myeloma and stromal cell interactions and the emergence of resistance.  We model the observed spatial dynamics of emergent resistance using spatial evolutionary game theory\, with (i) fitness as a function of population composition and drug concentration\, and  (ii) spatial coupling via diffusive migration and fitness-driven migration of the cells. \nI’ll show that the spatial structure of a complex microecology and the stress of chemotherapy transforms a prisoner’s dilemma into a coordination game\, and enables the coexistence of multiple myeloma and stromal cells within the drug gradient\, and show that evolutionary game theory applied to two interacting cell populations can yield quantitative prediction of future densities of the two cell populations based on their fitness as a function of population composition.  I believe that evolutionary game theory successfully predicts the future densities of strains of bone marrow stromal and cancer cells\, and opens the possible clinical use of such analysis for predicting and controlling cancer progression.
URL:https://uwm.edu/physics/event/colloquium-robert-h-austin/
LOCATION:Physics 135 – UW-Milwaukee\, 1900 E Kenwood Blvd\, Milwaukee\, WI\, 53211
CATEGORIES:Physics Colloquia
X-TRIBE-STATUS:
GEO:43.0754208;-87.886051
X-APPLE-STRUCTURED-LOCATION;VALUE=URI;X-ADDRESS=Physics 135 – UW-Milwaukee 1900 E Kenwood Blvd Milwaukee WI 53211;X-APPLE-RADIUS=500;X-TITLE=1900 E Kenwood Blvd:geo:-87.886051,43.0754208
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=America/Chicago:20140512T144500
DTEND;TZID=America/Chicago:20140512T160000
DTSTAMP:20260610T184211
CREATED:20141128T185445Z
LAST-MODIFIED:20230207T160242Z
UID:10423501-1399905900-1399910400@uwm.edu
SUMMARY:Colloquium: Dr. Steffen Lindert
DESCRIPTION:The Physics department colloquia are usually on Friday afternoons at 3 pm in Room 135.  Coffee and cookies are served at 2:45 pm in the same room.  Anyone is welcome. \nComputational Methods for Protein Structure Prediction\, Protein Dynamics and Drug Discovery\nDr. Steffen Lindert\, Post Doctoral Researcher\, Department of Pharmacology\, University of California-San Diego \nComputational methods are very useful for investigating biological systems. In addition to simulating molecular scale events that may not be probed easily by experiment\, simulations can also inform experiments and vice versa.  Here\, three main computational methods are applied to probe biological processes and systems: molecular dynamics\, de novo protein structure prediction using sparse experimental restraints\, and computer-aided drug discovery.  More specifically\, molecular dynamics methods are used to investigate the opening and closing properties of the hydrophobic patch in Troponin C\, an important process in the contraction of heart muscle cells.  Furthermore\, the development of EM-Fold\, a software tool to fold proteins into medium resolution cryoEM density maps is presented. EM-Fold is able to predict the structure of large helical proteins with atomic detail.  Finally\, the relaxed complex scheme\, a computer-aided drug discovery method accounting for receptor flexibility\, was used to find potent inhibitions of two enzymes involved in bacterial cell wall synthesis.  The lead compound was shown to be effective in animal models and to have synergistic activity with methicillin.
URL:https://uwm.edu/physics/event/colloquium-dr-steffen-lindert/
LOCATION:Physics 135 – UW-Milwaukee\, 1900 E Kenwood Blvd\, Milwaukee\, WI\, 53211
CATEGORIES:Physics Colloquia
X-TRIBE-STATUS:
GEO:43.0754208;-87.886051
X-APPLE-STRUCTURED-LOCATION;VALUE=URI;X-ADDRESS=Physics 135 – UW-Milwaukee 1900 E Kenwood Blvd Milwaukee WI 53211;X-APPLE-RADIUS=500;X-TITLE=1900 E Kenwood Blvd:geo:-87.886051,43.0754208
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=America/Chicago:20140515T144500
DTEND;TZID=America/Chicago:20140515T160000
DTSTAMP:20260610T184211
CREATED:20141128T182857Z
LAST-MODIFIED:20230207T160249Z
UID:10423500-1400165100-1400169600@uwm.edu
SUMMARY:Colloquium: Dr. Peter Schwander
DESCRIPTION:The Physics department colloquia are usually on Friday afternoons at 3 pm in Room 135.  Coffee and cookies are served at 2:45 pm in the same room.  Anyone is welcome. \nMapping Dynamic Nature of Molecular Machines that constitute Life\nDr. Peter Schwander\, Senior Scientist\, UW-Milwaukee (Tampa\, FL) \nFighting disease and maintaining life requires a good understanding of the machinery inside living cells.  These biological molecular machines go permanently through many conformational states\, and each state is structurally only slightly different from the previous one.  Single-particle methods take individual snapshots of molecules\, one at a time.  Single-particle methods thus avoid averaging over states and are therefore ideally suited to study conformations.  When  successful\, this allows compiling 3D movies of molecular machines at work. \nA novel analytic approach\, based on manifold embedding\, allows model-free\, quantitative analysis of the degrees of freedom and the energy landscape underlying continuous conformational changes from single-particle methods.  This approach has been successfully applied to snapshots of the eukaryotic ribosome taken with a cryogenetic electron microscope (cryoEM).  The results constitute the first direct evidence of the intersubunit rotation in three dimensions\, and suggest the ribosome to act like a Brownian ratchet. \nSimilar to cryoEM\, the emerging X-ray Free Energy Laser (XFEL) allows taking snapshots from single molecules before the intense beam destroys them\, XFEL thus provides a new source of single-particle snapshots to study conformations and will complement the more established cryoEM in the near future.
URL:https://uwm.edu/physics/event/colloquium-dr-peter-schwander/
LOCATION:Physics 135 – UW-Milwaukee\, 1900 E Kenwood Blvd\, Milwaukee\, WI\, 53211
CATEGORIES:Physics Colloquia
X-TRIBE-STATUS:
GEO:43.0754208;-87.886051
X-APPLE-STRUCTURED-LOCATION;VALUE=URI;X-ADDRESS=Physics 135 – UW-Milwaukee 1900 E Kenwood Blvd Milwaukee WI 53211;X-APPLE-RADIUS=500;X-TITLE=1900 E Kenwood Blvd:geo:-87.886051,43.0754208
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=America/Chicago:20140718T144500
DTEND;TZID=America/Chicago:20140718T160000
DTSTAMP:20260610T184211
CREATED:20141126T211303Z
LAST-MODIFIED:20230207T160300Z
UID:10423499-1405694700-1405699200@uwm.edu
SUMMARY:Colloquium: Justin Ellis
DESCRIPTION:The Physics department colloquia are usually on Friday afternoons at 3 pm in Room 135.  Coffee and cookies are served at 2:45 pm in the same room.  Anyone is welcome. \nSearching for Gravitational Waves With Pulsar Timing Arrays\nJustin Ellis\, PhD Candidate\, UWM Dept. of Physics \nGravitational Waves (GWs) are tiny ripples in the fabric of space-time predicted by Einstein’s theory of General Relativity.  Pulsar timing arrays (PTAs) offer a unique opportunity to detect low frequency GWs in the near future.  Such a detections would be complementary to both LISA and LIGO GW efforts.  In this frequency band\, the expected source of GWs are Supermassive Black Hole Binaries (SMBHBs) and they will most likely form in an ensemble creating a stochastic GW background with the possibility of a few nearby/massive sources that will be individually resolvable.  A direct detection of GWs will open a new window into the fields of astronomy and astrophysics by allowing us to constrain the coalescence rate of SMBHBs\, providing further tests on the theory of General Relativity\, and giving us access to properties of black holes not accessible by current astronomical techniques. \nThis dissertation work focuses primarily on the development of several robust data analysis pipelines for the detection and characterization of continuous GWs and a stochastic GW background.  The data analysis problem for PTAs is quite diffficult as one must fully take into account the timing model that must be fit in order to obtain the residuals\, uneven sampling (including large gaps)\, and potential red noise processes.  The data analysis techniques presented here can handle all of these effects completely while allowing additional freedom in parameterizing the noise present in the data.  The accumulation of work from this dissertation has resulted in a fully functional\, robust\, and efficient data analysis pipeline that has been successfully applied to the 5- and 9-year NANOGrav data releases.
URL:https://uwm.edu/physics/event/colloquium-justin-ellis/
LOCATION:Physics 135 – UW-Milwaukee\, 1900 E Kenwood Blvd\, Milwaukee\, WI\, 53211
CATEGORIES:Physics Colloquia
X-TRIBE-STATUS:
GEO:43.0754208;-87.886051
X-APPLE-STRUCTURED-LOCATION;VALUE=URI;X-ADDRESS=Physics 135 – UW-Milwaukee 1900 E Kenwood Blvd Milwaukee WI 53211;X-APPLE-RADIUS=500;X-TITLE=1900 E Kenwood Blvd:geo:-87.886051,43.0754208
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=America/Chicago:20140902T080000
DTEND;TZID=America/Chicago:20140902T170000
DTSTAMP:20260610T184211
CREATED:20140801T210324Z
LAST-MODIFIED:20230207T160309Z
UID:10363254-1409644800-1409677200@uwm.edu
SUMMARY:First Day of Classes
DESCRIPTION:Welcome new students and welcome back continuing students!
URL:https://uwm.edu/physics/event/first-day-of-classes/
LOCATION:WI
X-TRIBE-STATUS:
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=America/Chicago:20140905T130000
DTEND;TZID=America/Chicago:20140905T140000
DTSTAMP:20260610T184211
CREATED:20140813T211740Z
LAST-MODIFIED:20230207T160336Z
UID:10363255-1409922000-1409925600@uwm.edu
SUMMARY:CGCA Seminar: Morgan Lynch
DESCRIPTION:Morgan Lynch\, Physics\, UW-Milwaukee\nPhysics – Room 481 \nAbstract: Since the discoveries of Parker\, Hawking\, and Unruh\, namely cosmological particle creation\, black hole evaporation\, and accelerated radiation\, respectively\, a general notion has emerged that the particle content of spacetime is an observer-dependent quantity. For example\, with the Unruh effect an observer undergoing uniform acceleration\, a\, will find the Minkowski vacuum state to be a thermalized bath of particles at temperature t ~ a. Directly measuring this\, or related phenomena\, has remained outside the reach of our current experimental capabilities. Indirect measurements\, such as the acceleration-dependent lifetime of particles\, could provide a better avenue for verifying these effects. In this talk\, I will discuss how acceleration affects the decay rates of unstable particles and show a generalized formalism which includes arbitrary final state multiplicities. I will then analyze the electron and muon system and compute the transition rates and lifetimes for accelerated electrons and muons as well as the branching fractions for muon decay.
URL:https://uwm.edu/physics/event/cgca-seminar-morgan-lynch/
LOCATION:Physics 481 – UW-Milwaukee\, 1900 E Kenwood Blvd\, Milwaukee\, WI\, 53211
CATEGORIES:CGCA Seminars
X-TRIBE-STATUS:
GEO:43.0754208;-87.886051
X-APPLE-STRUCTURED-LOCATION;VALUE=URI;X-ADDRESS=Physics 481 – UW-Milwaukee 1900 E Kenwood Blvd Milwaukee WI 53211;X-APPLE-RADIUS=500;X-TITLE=1900 E Kenwood Blvd:geo:-87.886051,43.0754208
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=America/Chicago:20140905T144500
DTEND;TZID=America/Chicago:20140905T160000
DTSTAMP:20260610T184211
CREATED:20141125T182137Z
LAST-MODIFIED:20230207T160346Z
UID:10423498-1409928300-1409932800@uwm.edu
SUMMARY:Colloquium: Jean Creighton
DESCRIPTION:The Physics department colloquia are usually on Friday afternoons at 3 pm in Room 135. Coffee and cookies are served at 2:45 pm in the same room. Anyone is welcome. \nMy Adventure in the Stratosphere \nJean Creighton\, Director – UWM Manfred Olson Planetarium \nPhysics – Room 135 \nRecently\, NASA selected me to be one of the 24 Airborne Astronomy Ambassadors\, aboard the Stratospheric Observatory for Infrared Astronomy (SOFIA). We were described as “Junior Varsity” astronauts during our safety training. We met enthusiastic and committed scientists\, engineers\, and administrators who make ambitious projects such as SOFIA successful. \nI am delighted to share with you my experiences of flying at 45\,000 feet in a modified 747 equipped with a 100-inch infrared telescope.
URL:https://uwm.edu/physics/event/colloquium-jean-creighton/
LOCATION:Physics 135 – UW-Milwaukee\, 1900 E Kenwood Blvd\, Milwaukee\, WI\, 53211
CATEGORIES:Physics Colloquia
X-TRIBE-STATUS:
GEO:43.0754208;-87.886051
X-APPLE-STRUCTURED-LOCATION;VALUE=URI;X-ADDRESS=Physics 135 – UW-Milwaukee 1900 E Kenwood Blvd Milwaukee WI 53211;X-APPLE-RADIUS=500;X-TITLE=1900 E Kenwood Blvd:geo:-87.886051,43.0754208
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=America/Chicago:20140908T140000
DTEND;TZID=America/Chicago:20140908T150000
DTSTAMP:20260610T184211
CREATED:20140905T201959Z
LAST-MODIFIED:20230207T160352Z
UID:10363257-1410184800-1410188400@uwm.edu
SUMMARY:The European X-ray Free-Electron Laser:  towards an ultra-bright  high repetition rate X-ray Source
DESCRIPTION:Dr. Massimo Altarelli\, European XFEL GmbH\, Chairman of the Management Board\nPhysics – Room 481 \nThis talk will summarize the status of the European X-ray Free-Electron Laser (European XFEL) near Hamburg\, Germany. The start of operation of the LCLS at SLAC and of SACLA in Japan already produced impressive scientific results from these hard x-ray highly brilliant sources. The European facility is powered by a 17.5 GeV superconducting linear accelerator\, that will generate a much larger number of pulses per second\, up to 27\,000. It shall also provide a mode of operation based on beam distribution to two or three experiments simultaneously\, providing each of them with thousands of pulses per second. The scientific possibilities opened up by these capabilities are shortly described\, together with the current instrumental developments (in optics\, detectors\, lasers\, etc.) that are necessary to implement this program.
URL:https://uwm.edu/physics/event/special-seminar/
LOCATION:Physics 481 – UW-Milwaukee\, 1900 E Kenwood Blvd\, Milwaukee\, WI\, 53211
CATEGORIES:Biophysics Seminars
X-TRIBE-STATUS:
GEO:43.0754208;-87.886051
X-APPLE-STRUCTURED-LOCATION;VALUE=URI;X-ADDRESS=Physics 481 – UW-Milwaukee 1900 E Kenwood Blvd Milwaukee WI 53211;X-APPLE-RADIUS=500;X-TITLE=1900 E Kenwood Blvd:geo:-87.886051,43.0754208
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=America/Chicago:20140912T130000
DTEND;TZID=America/Chicago:20140912T140000
DTSTAMP:20260610T184211
CREATED:20140814T144812Z
LAST-MODIFIED:20230207T160401Z
UID:10363256-1410526800-1410530400@uwm.edu
SUMMARY:CGCA Seminar: Thomas Kupfer
DESCRIPTION:Thomas Kupfer\, Radboud University Nijmegen\nThe evolution of compact binaries – Binary white dwarf systems as strong gravitational wave sources \nAbstract: Hot subdwarf B stars (sdBs) are hot core helium-burning stars with a large fraction found in short-period binaries with white dwarf (WD) companions. During their further evolution\, these systems will become compact double white dwarf binaries and due to gravitational wave radiation the orbit will shrink further where they will go into contact at an orbital period of about 5 min. Having the correct mass ratio a merger of the system is prevented and an ultracompact AM CVn type binary is formed. AM CVn systems are a small group of mass transferring ultracompact binaries evolving towards longer periods with decreasing mass accretion rates. They are important as strong low-frequency Galactic gravitational wave sources and the most compact ones will act as verification sources for upcoming space based gravitational wave detectors like eLISA/NGO.  \nIn this talk I will report on the results of a population study of compact sdB binaries and show that the average mass of WDs in those binaries is significantly lower than found for single WDs with some being good candidates to evolve into an AM CVn type binary. Furthermore\, I will discuss the latest results on some particularly interesting AM CVn type binaries and show a possible way to detect the most compact systems with orbital periods well below 10 minutes which will belong to the strongest Galactic gravitational sources in the low-frequency regime.
URL:https://uwm.edu/physics/event/gravitation-cosmology-astrophysics-seminar/
LOCATION:Physics 481 – UW-Milwaukee\, 1900 E Kenwood Blvd\, Milwaukee\, WI\, 53211
CATEGORIES:CGCA Seminars
X-TRIBE-STATUS:
GEO:43.0754208;-87.886051
X-APPLE-STRUCTURED-LOCATION;VALUE=URI;X-ADDRESS=Physics 481 – UW-Milwaukee 1900 E Kenwood Blvd Milwaukee WI 53211;X-APPLE-RADIUS=500;X-TITLE=1900 E Kenwood Blvd:geo:-87.886051,43.0754208
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=America/Chicago:20140912T144500
DTEND;TZID=America/Chicago:20140912T160000
DTSTAMP:20260610T184211
CREATED:20141114T192956Z
LAST-MODIFIED:20230207T160409Z
UID:10420514-1410533100-1410537600@uwm.edu
SUMMARY:Colloquium: Dr. Roger Tobin
DESCRIPTION:The Physics department colloquia are usually on Friday afternoons at 3 pm in Room 135.  Coffee and cookies are served at 2:45 pm in the same room.  Anyone is welcome. \nSome Thoughts on Teaching and Learning About Energy from Third Grade to College\nDr. Roger Tobin\, Professor and Chair\, Dept. of Physics & Astronomy\, Tufts University\nPhysics – Room 135 \nEnergy is arguably the single most important concept in physics\, but the educational system does a stunningly ineffective job of enabling students to understand it or use it meaningfully.  I will discuss some of the reasons why energy is particularly challenging subject and some of the ways current practice exacerbates the problem\, and put forward some ideas for a consistent perspective that could help across a wide range of ages\, from elementary school to introductory college physics.
URL:https://uwm.edu/physics/event/colloquium-dr-roger-tobin/
LOCATION:Physics 135 – UW-Milwaukee\, 1900 E Kenwood Blvd\, Milwaukee\, WI\, 53211
CATEGORIES:Physics Colloquia
X-TRIBE-STATUS:
GEO:43.0754208;-87.886051
X-APPLE-STRUCTURED-LOCATION;VALUE=URI;X-ADDRESS=Physics 135 – UW-Milwaukee 1900 E Kenwood Blvd Milwaukee WI 53211;X-APPLE-RADIUS=500;X-TITLE=1900 E Kenwood Blvd:geo:-87.886051,43.0754208
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=America/Chicago:20140912T150000
DTEND;TZID=America/Chicago:20140912T160000
DTSTAMP:20260610T184211
CREATED:20140901T193455Z
LAST-MODIFIED:20230207T160419Z
UID:10363261-1410534000-1410537600@uwm.edu
SUMMARY:The Energy Lens: Some Thoughts on Teaching and Learning  About Energy from Third Grade to College
DESCRIPTION:Roger Tobin\, Professor and Chair\, Department of Physics & Astronomy\, Tufts University\nPhysics – Room 135 \nEnergy is arguably the single most important concept in physics\, but the educational system does a stunningly\nineffective job of enabling students to understand it or use it meaningfully. I will discuss some of the reasons why\nenergy is a particularly challenging subject and some of the ways current practice exacerbates the problem\, and put\nforward some ideas for a consistent perspective that could help across a wide range of ages\, from elementary school to introductory college physics.
URL:https://uwm.edu/physics/event/the-energy-lens-some-thoughts-on-teaching-and-learning-about-energy-from-third-grade-to-college/
LOCATION:Physics 135 – UW-Milwaukee\, 1900 E Kenwood Blvd\, Milwaukee\, WI\, 53211
CATEGORIES:Physics Colloquia
X-TRIBE-STATUS:
GEO:43.0754208;-87.886051
X-APPLE-STRUCTURED-LOCATION;VALUE=URI;X-ADDRESS=Physics 135 – UW-Milwaukee 1900 E Kenwood Blvd Milwaukee WI 53211;X-APPLE-RADIUS=500;X-TITLE=1900 E Kenwood Blvd:geo:-87.886051,43.0754208
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=America/Chicago:20140918T160000
DTEND;TZID=America/Chicago:20140918T180000
DTSTAMP:20260610T184211
CREATED:20141001T200044Z
LAST-MODIFIED:20230207T160427Z
UID:10363265-1411056000-1411063200@uwm.edu
SUMMARY:Biophysics Seminar: Dr. Ali Dashti
DESCRIPTION:Dr. Ali Dashti\, Research Associate\, UWM Physics Department\nPhysics – Room 481 \nTrajectories of a Brownian Machine: The Ribosome
URL:https://uwm.edu/physics/event/biophysics-seminar-dr-ali-dashti/
LOCATION:Physics 481 – UW-Milwaukee\, 1900 E Kenwood Blvd\, Milwaukee\, WI\, 53211
CATEGORIES:Biophysics Seminars
X-TRIBE-STATUS:
GEO:43.0754208;-87.886051
X-APPLE-STRUCTURED-LOCATION;VALUE=URI;X-ADDRESS=Physics 481 – UW-Milwaukee 1900 E Kenwood Blvd Milwaukee WI 53211;X-APPLE-RADIUS=500;X-TITLE=1900 E Kenwood Blvd:geo:-87.886051,43.0754208
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=America/Chicago:20140922T160000
DTEND;TZID=America/Chicago:20140922T170000
DTSTAMP:20260610T184211
CREATED:20141003T142122Z
LAST-MODIFIED:20230207T160515Z
UID:10405474-1411401600-1411405200@uwm.edu
SUMMARY:Astronomy Club: First Meeting - Intro\, Jeopardy\, News Item (Xavi)
DESCRIPTION:
URL:https://uwm.edu/physics/event/astronomy-club-first-meeting-intro-jeopardy-news-item-xavi/
LOCATION:Physics 144 – UW-Milwaukee\, 1900 E Kenwood Blvd\, Milwaukee\, WI\, 53211
X-TRIBE-STATUS:
GEO:43.0754208;-87.886051
X-APPLE-STRUCTURED-LOCATION;VALUE=URI;X-ADDRESS=Physics 144 – UW-Milwaukee 1900 E Kenwood Blvd Milwaukee WI 53211;X-APPLE-RADIUS=500;X-TITLE=1900 E Kenwood Blvd:geo:-87.886051,43.0754208
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=America/Chicago:20140926T144500
DTEND;TZID=America/Chicago:20140926T160000
DTSTAMP:20260610T184211
CREATED:20141114T192623Z
LAST-MODIFIED:20230207T160530Z
UID:10420513-1411742700-1411747200@uwm.edu
SUMMARY:Colloquium: Dr. Eric M. Wilcots
DESCRIPTION:The Physics department colloquia are usually on Friday afternoons at 3 pm in Room 135.  Coffee and cookies are served at 2:45 pm in the same room.  Anyone is welcome. \nGalaxy Transformation and the Evolution of the Gas Content of Galaxy Groups\nDr. Eric M. Wilcots\, Dept. of Astronomy\, University of Wisconsin (Madison)\nPhysics – Room 135 \nThe current state of our understanding of the nature of the baryon content of galaxy groups\, derived largely from a large body of X-ray observations\, leaves us with two key questions.  First\, what are the relative fractions of the hot\, warm/hot\, and neutral gas in galaxy groups\, and how is each phase distributed within groups? Second\, how has the baryon content of galaxy groups evolved over time and what is its relationship to the dynamical evolution of the group? \nThe results from a number of investigations of the HI content and deep searches for diffuse synchrotron emission in groups are now shedding light on the evolution of the baryon content of galaxy groups and what impact those baryons have on the evolution of the resident galaxies.  I will review our new results tracing the impact of the intergalactic on the evolution of galaxies in groups and measurement of the baryon content of groups using bent double radio sources.
URL:https://uwm.edu/physics/event/colloquium-dr-eric-m-wilcots/
LOCATION:Physics 135 – UW-Milwaukee\, 1900 E Kenwood Blvd\, Milwaukee\, WI\, 53211
CATEGORIES:Physics Colloquia
X-TRIBE-STATUS:
GEO:43.0754208;-87.886051
X-APPLE-STRUCTURED-LOCATION;VALUE=URI;X-ADDRESS=Physics 135 – UW-Milwaukee 1900 E Kenwood Blvd Milwaukee WI 53211;X-APPLE-RADIUS=500;X-TITLE=1900 E Kenwood Blvd:geo:-87.886051,43.0754208
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=America/Chicago:20140926T144500
DTEND;TZID=America/Chicago:20140926T160000
DTSTAMP:20260610T184211
CREATED:20140901T200032Z
LAST-MODIFIED:20230207T160523Z
UID:10363259-1411742700-1411747200@uwm.edu
SUMMARY:Colloquium: Dr. Eric M. Wilcots
DESCRIPTION:The Physics department colloquia are usually on Friday afternoons at 3 pm in Room 135.  Coffee and cookies are served at 2:45 pm in the same room.  Anyone is welcome. \nGalaxy Transformation and the Evolution of the Gas Content of Galaxy Groups\nDr. Eric M. Wilcots\, Dept. of Physics\, University of Wisconsin (Madison)\nPhysics – Room 135 \nAbstract: The current state of our understanding of the nature of the baryon content of galaxy groups\, derived largely from a large body of X-ray observations\, leaves us with two key questions. First\, what are the relative fractions of the hot\, warm/hot\, and neutral gas in galaxy groups\, and how is each phase distributed within groups? Second\, how has the baryon content of galaxy groups evolved over time and what is its relationship to the dynamical evolution of the group?  \nThe results from a number of investigations of the HI content and deep searches for diffuse synchrotron emission in groups are now shedding light on the evolution of the baryon content of galaxy groups and what impact those baryons have on the evolution of the resident galaxies. I will review our new results tracing the impact of the intergalactic on the evolution of galaxies in groups and measurement of the baryon content of groups using bent double radio sources.
URL:https://uwm.edu/physics/event/colloquium-dr-eric-m-wilcots-2/
LOCATION:Physics 135 – UW-Milwaukee\, 1900 E Kenwood Blvd\, Milwaukee\, WI\, 53211
CATEGORIES:Physics Colloquia
X-TRIBE-STATUS:
GEO:43.0754208;-87.886051
X-APPLE-STRUCTURED-LOCATION;VALUE=URI;X-ADDRESS=Physics 135 – UW-Milwaukee 1900 E Kenwood Blvd Milwaukee WI 53211;X-APPLE-RADIUS=500;X-TITLE=1900 E Kenwood Blvd:geo:-87.886051,43.0754208
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=America/Chicago:20140929T040000
DTEND;TZID=America/Chicago:20140929T170000
DTSTAMP:20260610T184211
CREATED:20141003T142317Z
LAST-MODIFIED:20230207T160537Z
UID:10405475-1411963200-1412010000@uwm.edu
SUMMARY:Astronomy Club: Postdoc Activity\, News Item (Dan Gugg)
DESCRIPTION:Today in Astronomy Club: dark matter and organic molecules in the heart of the Milky Way.
URL:https://uwm.edu/physics/event/astronomy-club-postdoc-activity-news-item-dan-gugg/
LOCATION:Physics 144 – UW-Milwaukee\, 1900 E Kenwood Blvd\, Milwaukee\, WI\, 53211
X-TRIBE-STATUS:
GEO:43.0754208;-87.886051
X-APPLE-STRUCTURED-LOCATION;VALUE=URI;X-ADDRESS=Physics 144 – UW-Milwaukee 1900 E Kenwood Blvd Milwaukee WI 53211;X-APPLE-RADIUS=500;X-TITLE=1900 E Kenwood Blvd:geo:-87.886051,43.0754208
END:VEVENT
END:VCALENDAR