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VERSION:2.0
CALSCALE:GREGORIAN
PRODID:UW-Madison-Physics-Events
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SEQUENCE:3
UID:UW-Physics-Event-8635
DTSTART:20240226T180000Z
DTEND:20240226T191500Z
DTSTAMP:20260413T223336Z
LAST-MODIFIED:20240222T185002Z
LOCATION:1227 Engineering Hall
SUMMARY:"From the laboratory to astrophysics: the Rayleigh-Taylor inst
 ability"\, Plasma Physics (Physics/ECE/NE 922) Seminar\, Dr. Bhuvana S
 rinivasan\, Director\, PLASMAWISE Laboratory - Univ of Washington
DESCRIPTION:Recent breakthroughs in inertial conﬁnement fusion have 
 demonstrated fusion ignition\, but signiﬁcant physics and engineerin
 g challenges remain to truly achieve energy breakeven. Hydrodynamic mi
 x at material interfaces is known to be detrimental for laser-driven a
 nd pulsed-power-driven inertial conﬁnement fusion implosions. Hence\
 , mitigation of mix remains an open challenge. The Rayleigh-Taylor ins
 tability (RTI)\, which occurs when the interface between two ﬂuids w
 ith different densities is accelerated\, has been known to play a crit
 ical role in producing hydrodynamic mix at material interfaces. The RT
 I is an ubiquitous instability and RTI-like features and growth have b
 een noted in astrophysical observations. The presence of magnetic ﬁe
 lds\, plasma transport\, and kinetic effects can signiﬁcantly alter 
 the evolution of the RTI\, which may explain discrepancies between num
 erical simulations and observations. These will be discussed in this t
 alk. Other high-energy-density research relevant to pulsed-power implo
 sions such as the growth of the electrothermal instability that can se
 ed the late-time RTI will be discussed brieﬂy. There is a need for h
 igh-ﬁdelity computational models to study high-energy-density plasma
 s. A hierarchy of models\, ranging from magnetohydrodynamic (MHD) to f
 ully kinetic\, are developed and applied across a wide range of parame
 ter regimes in the PLASMAWISE laboratory at the University of Washingt
 on.<br>\n<br>\n<br>\nBio:\nBhuvana Srinivasan is an Associate Prof
 essor in the William E. Boeing Department of Aeronautics and Astronaut
 ics at the University of Washington. Prior to this appointment\, she w
 as an Associate Professor in the Kevin T. Crofton Department of Aerosp
 ace and Ocean Engineering at Virginia Tech where she developed a progr
 am in computational plasma physics. Prior to joining Virginia Tech\, s
 he was a postdoc and a scientist at the Los Alamos National Laboratory
 . She is the director of the PLASMAWISE Laboratory (previously the Pla
 sma Dynamics Computational Laboratory at Virginia Tech). The primary r
 esearch areas in her group include plasma-material interactions in thr
 usters and fusion devices\, instabilities in high-energy-density fusio
 n and astrophysical plasmas\, ionospheric plasma instabilities\, and n
 umerical algorithm development for fluid and kinetic models. She is a 
 recipient of the NSF CAREER award\, the 2017 Outstanding Assistant Pro
 fessor award and the 2019 Faculty Fellow awarded by the Dean of the Co
 llege of Engineering at Virginia Tech. She was appointed to the Endowe
 d Crofton Faculty Fellowship in Engineering from 2021-2023. She is a m
 ember of the Fusion Energy Sciences Advisory Committee to the U.S. Dep
 artment of Energy and serves on the Executive Committee for the Americ
 an Physical Society Division of Plasma Physics. She is also active in 
 Diversity\, Equity\, and Inclusion (DEI) efforts as the past Chair of 
 the DEI committee in the aerospace and ocean engineering department at
  Virginia Tech\, as a member of the Committee on Women+ in Plasma Phys
 ics\, and through her involvement with the Center for the Enhancement 
 of Engineering Diversity at Virginia Tech.
URL:https://www.physics.wisc.edu/events/?id=8635
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