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BEGIN:VEVENT
DTSTAMP:20260111T114049
DTSTART;TZID=America/Detroit:20260205T143000
DTEND;TZID=America/Detroit:20260205T160000
SUMMARY:Workshop / Seminar:Culture\, History and Politics (CHiP)
DESCRIPTION:- January 15: Cho Han\n- January 22: Marni Morse\n- January 29: Jiyeon Lee\n- February 5: Tess Hamilton\n- February 12: Álvaro Cabrera\n- February 19: Jarron Long\n- February 26: Xianni Zhang\n- March 12: Sarah Farr and Christian Castro-Martinez\n- March 19: Danyelle Reynolds\n- March 26: Vanessa Jiménez-Read\n- April 2: Abigail Skalka and Julieta Goldenberg\n- April 9: Eric Freeburg\n- April 16: TBD
UID:143661-21893602@events.umich.edu
URL:https://events.umich.edu/event/143661
CLASS:PUBLIC
STATUS:CONFIRMED
CATEGORIES:Graduate Student
LOCATION:LSA Building - 4147
CONTACT:
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BEGIN:VEVENT
DTSTAMP:20260127T070323
DTSTART;TZID=America/Detroit:20260205T150000
DTEND;TZID=America/Detroit:20260205T160000
SUMMARY:Workshop / Seminar:Biomedical Engineering (BME 500) Seminar Series
DESCRIPTION:Brain tumors are organized as active nematic liquid crystals\n\nAbstract:\nWhether gliomas consist of random accumulations of cells or are self-organizing remains unknown.  If large scale order exists\, it should manifest as invariant structures across different tumors. Recently\, we described the existence of oncostreams\, fascicles of elongated mesenchymal-like cells that are found in gliomas in both rodent and human tumors. In this presentation\, I will discuss that glioma brain tumors in vivo\, and in vitro\, are structured as active nematic liquid crystals. Building on our previous work that gliomas exhibit self-organized\, aligned\, multicellular structures\, termed oncostreams\, I will show that gliomas display nematic order\, topological defects\, disclinations\, and quasi-long range order in 2D and in 3D. Significantly\, the amount of nematic order scales with tumor aggression - suggesting crystalline order contributes to tumor malignancy - constituting a novel potential therapeutic target for this incurable cancer. Potential novel therapeutic approaches based on this new understanding of the structure of gliomas will be discussed. \n\nBio:\nDr. Lowenstein graduated MD\, Ph.D. from the University of Buenos Aires\, Argentina. Following postdoctoral work at The Johns Hopkins University\, NIH\, and Oxford University he opened his first lab at the University of Dundee\, Scotland. Subsequently\, he has taught and researched at the University of Wales\, Cardiff\, the University of Manchester\, UK\, and UCLA and Cedars-Sinai Medical Center\, in Los Angeles\, CA. He has been at the University of Michigan since 2011. His interests lie in understanding and curing brain tumors. Most recently\, he has been exploring the physical organization of brain tumors\, as will be discussed during his presentation.
UID:144608-21895563@events.umich.edu
URL:https://events.umich.edu/event/144608
CLASS:PUBLIC
STATUS:CONFIRMED
CATEGORIES:seminar,Biointerfaces,Biology,biomedical,biomedical engineering,Bioninterfaces,Biosciences,bme,engineer,engineering,Medicine,Michigan Engineering,Biotechnology
LOCATION:Lurie Biomedical Engineering (formerly ATL) - 1130
CONTACT:
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BEGIN:VEVENT
DTSTAMP:20250805T113918
DTSTART;TZID=America/Detroit:20260205T150000
DTEND;TZID=America/Detroit:20260205T170000
SUMMARY:Social / Informal Gathering:Hopwood Tea
DESCRIPTION:Enjoy coffee\, tea\, and refreshments in a beautiful\, book-filled space. Check out a book from the Hopwood library or engage with other readers and writers. All are welcome.
UID:136054-21877787@events.umich.edu
URL:https://events.umich.edu/event/136054
CLASS:PUBLIC
STATUS:CONFIRMED
CATEGORIES:Books,Creative Writing,English Language And Literature,Food,Free,Graduate Students,Hopwood Program,Literary Arts,Literature,The Helen Zell Writers' Program,Undergraduate Students,Well-being,Writing,Ann Arbor
LOCATION:Angell Hall - 1176 (Hopwood Room)
CONTACT:
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BEGIN:VEVENT
DTSTAMP:20260121T165852
DTSTART;TZID=America/Detroit:20260205T150000
DTEND;TZID=America/Detroit:20260205T163000
SUMMARY:Lecture / Discussion:IOE 899:  Mohammed Safayet Arefin
DESCRIPTION:Head-Mounted Display (HMD) interfaces are designed to present virtual information within users' real-world view\, enhancing their perception of the real world and supporting effective task execution. Effective human performance with an HMD depends strongly on the design of its interface. Three key components are visual depth\, clutter\, and transparency. HMD interface visual depth is the distance between the user’s eyes and the virtual information displayed in the real-world view. HMD interface clutter denotes the amount of virtual information shown. HMD interface transparency aims to balance the legibility of virtual elements and the visibility of the real-world environment seen through the HMD. This talk presents some of our recent findings on these issues\, with an emphasis on human performance and perception.
UID:144273-21895101@events.umich.edu
URL:https://events.umich.edu/event/144273
CLASS:PUBLIC
STATUS:CONFIRMED
CATEGORIES:Industrial And Operations Engineering,Michigan Engineering,Graduate Students,Graduate,899 Seminar Series
LOCATION:Industrial and Operations Engineering Building - 1680
CONTACT:
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BEGIN:VEVENT
DTSTAMP:20260129T161017
DTSTART;TZID=America/Detroit:20260205T153000
DTEND;TZID=America/Detroit:20260205T162000
SUMMARY:Lecture / Discussion:The Department of Astronomy 2025-2026 Colloquium Series Presents:
DESCRIPTION:\"Investigating the Effects of SMBH Feedback on Galaxy Morphology using FIRE-2 Simulations\"\n\nIn the local universe\, low-mass irregular galaxies (stellar mass ~ 10^9 M_sun) and Milky Way mass disk galaxies (stellar mass ~ 10^10 M_sun) are typically star-forming\, while massive\, elliptical galaxies (stellar mass ~ 10^11 M_sun) are usually “quenched” or not forming stars. Simulations have shown that supermassive black hole (SMBH) feedback shuts down star formation in these massive galaxies and is required to reproduce the observed galaxy population at low redshift. The details of how SMBH Feedback corresponds to galaxy morphology are still not fully understood. To elucidate the effects of SMBH Feedback on galaxy morphology\, we analyze a subset of 9 Milky Way-mass galaxies with live SMBH feedback from the Feedback In Realistic Environments (FIRE) simulations. Using circularity (epsilon = J_z/J_c(E)) as a proxy for morphology\, we investigate how the presence of SMBH feedback energetics\, like heating and outflows/winds\, disrupts star formation and the subsequent morphological evolution of galaxies over cosmic time. We find that SMBH feedback reduces star formation across three evolutionary phases corresponding to spheroidal\, thick disk\, and thin disk morphologies. The effect of SMBH during the disk formation phase results in more spheroidal-shaped galaxies under SMBH Feedback than without.
UID:144801-21895955@events.umich.edu
URL:https://events.umich.edu/event/144801
CLASS:PUBLIC
STATUS:CONFIRMED
CATEGORIES:astronomy,astrophysics
LOCATION:West Hall - 411
CONTACT:
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