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VERSION:2.0
PRODID:-//Institute for Advanced Study//NONSGML kigkonsult.se iCalcreator 2.41.92//
CALSCALE:GREGORIAN
UID:7d90ef41-a6b8-490e-a892-d7a792d7c4b2
X-WR-TIMEZONE:UTC
X-WR-CALNAME:IAS Astrophysics
BEGIN:VEVENT
UID:e424910c-5e1a-4606-9b1a-5dd3d962eb2b-0
DTSTAMP:20260420T184811Z
CREATED:20260127T095857Z
DESCRIPTION:Topic: Setting Agenda for the Term\n\nMore: https://www.ias.edu
 /sns/events/institute-advanced-studyprinceton-university-gravitational-wav
 es-meeting-2
DTSTART:20260127T183000Z
DTEND:20260127T193000Z
LAST-MODIFIED:20260127T095922Z
LOCATION:PGI (4th floor of Jadwin)
SUMMARY:Institute for Advanced Study/Princeton University Gravitational Wav
 es Meeting
URL:https://www.ias.edu/sns/events/institute-advanced-studyprinceton-univer
 sity-gravitational-waves-meeting-2
END:VEVENT
BEGIN:VEVENT
UID:05e915ce-6b65-41d8-8d17-4291a7ef6f5f-0
DTSTAMP:20260420T184811Z
CREATED:20260204T140013Z
DESCRIPTION:Topic: Dynamics of stellar binaries in nuclear star clusters\n
 \nSpeakers: Mark Dodici\, University of Toronto\n\nMore: https://www.ias.e
 du/sns/events/institute-advanced-study-astrophysics-seminar-153\n\nBinary 
 stars in the central parsecs of galaxies are involved in the\nproduction o
 f several modern astronomical phenomena\, including\nhypervelocity stars\,
  repeating partial tidal disruption events\, and\ndust-enshrouded objects 
 around Sgr A*. I present an overview of some\nkey aspects of the dynamical
  evolution of these binaries. In\nparticular\, I discuss recent theoretica
 l results suggesting that up to\nhalf of the stellar binaries in the centr
 al parsec of the Milky Way\nshould shrink to near-contact separations over
  their main sequence\nlifetimes. I then consider how the gravitational pot
 ential induced by\nan active galactic nucleus disk may sculpt this populat
 ion. Finally\, I\nattempt to connect these theories to observational puzzl
 es surrounding\nsome of the binary-related phenomena listed above.
DTSTART:20260205T160000Z
DTEND:20260205T170000Z
LAST-MODIFIED:20260204T140125Z
LOCATION:Bloomberg Lecture Hall
SUMMARY:Institute for Advanced Study Astrophysics Seminar
URL:https://www.ias.edu/sns/events/institute-advanced-study-astrophysics-se
 minar-153
END:VEVENT
BEGIN:VEVENT
UID:653cee25-80b5-4505-8b14-00abc7b7c5ad-0
DTSTAMP:20260420T184811Z
CREATED:20260127T100039Z
DESCRIPTION:Topic: TBA\n\nMore: https://www.ias.edu/sns/events/institute-ad
 vanced-studyprinceton-university-gravitational-waves-meeting-3
DTSTART:20260210T183000Z
DTEND:20260210T193000Z
LAST-MODIFIED:20260212T181440Z
LOCATION:PGI (4th floor of Jadwin)
SUMMARY:Institute for Advanced Study/Princeton University Gravitational Wav
 es Meeting
URL:https://www.ias.edu/sns/events/institute-advanced-studyprinceton-univer
 sity-gravitational-waves-meeting-3
END:VEVENT
BEGIN:VEVENT
UID:35400c98-7229-44a8-82ac-ce58f15707d5-0
DTSTAMP:20260420T184811Z
CREATED:20260127T120329Z
DESCRIPTION:Topic: Theory for innovative cosmological tests of dark matter-
 baryon interactions \n\nSpeakers: Yacine Ali-Haimoud\, New York University
 \n\nMore: https://www.ias.edu/sns/events/institute-advanced-study-astrophy
 sics-seminar-140\n\nAmong many things\, dark matter could be made of new f
 undamental or\ncomposite particles\, which may feebly interact with nuclei
  or\nelectrons (“baryons”)\, as well as with themselves. Cosmological\nobs
 ervables are a promising avenue to test such interactions\, and are\ncompl
 ementary to direct-detection experiments\, in particular for\nprobing rela
 tively light dark matter particles. In this talk I will\nmotivate two proj
 ects to build theoretical tools for innovative and\nhigher-sensitivity cos
 mological tests of dark matter interactions --\nin the hopes to recruit he
 lp in finishing them! In Project 1\, I\npropose to expand and implement a 
 new framework allowing us to study\ndark matter- baryon interactions and d
 ark matter self-interactions\nsimultaneously and self-consistently: the Bo
 ltzmann-Fokker-Planck\n(BFP) formalism\, which I introduced in arXiv:1811.
 09903. The goal is\nto expand the BFP framework to incorporate dark matter
 \nself-interactions with arbitrary strengths\, and implement it into the\n
 Boltzmann code CLASS. In Project 2\, I motivate quantifying a\ncompletely 
 novel signature of dark matter-baryon scattering\, namely\nnon-Gaussianity
  in the Cosmic Microwave Background (CMB) arising from\nthe non-linearity 
 of the dark matter-baryon momentum-exchange rate.\nThis idea has similarit
 ies with a previous study my former student\nJensen and I conducted on pri
 mordial black holes\, which I will\nbriefly highlight.
DTSTART:20260212T160000Z
DTEND:20260212T170000Z
LAST-MODIFIED:20260210T134316Z
LOCATION:Bloomberg Lecture Hall
SUMMARY:Institute for Advanced Study Astrophysics Seminar
URL:https://www.ias.edu/sns/events/institute-advanced-study-astrophysics-se
 minar-140
END:VEVENT
BEGIN:VEVENT
UID:2054bf5c-9cd1-4aab-a74e-ae1a547770aa-0
DTSTAMP:20260420T184811Z
CREATED:20260127T120408Z
DESCRIPTION:Topic: Rethinking about gravitational instability as a planet f
 ormation scenario\n\nSpeakers: Cristiano Longarini\, University of Cambrid
 ge\n\nMore: https://www.ias.edu/sns/events/institute-advanced-study-astrop
 hysics-seminar-141\n\nThe ubiquity of substructures in protoplanetary disc
 s has opened\ndebate regarding the alignment of planet formation timescale
 s with\nprotostellar disc evolution. Under the hypothesis of the planetary
 \ninterpretation\, a robust conclusion is that a substantial part of the\n
 planet formation process must overlap with the time when protostellar\ndis
 cs are likely to be young and\, possibly\, gravitationally unstable.\nHist
 orically\, gravitational instability has been proposed as a pathway\nfor p
 lanetary formation. However\, it lost favour due to the higher\nlikelihood
  of forming stellar companions rather than planets.\nNevertheless\, recent
 ly\, this scenario has gained new interest\, when\nthe synergy between gra
 vitational instability and dust dynamics is\nconsidered.\n\nIn this talk\,
  I will discuss the interplay between dust dynamics and\ngravitational ins
 tability. Gravitational instability is responsible\nfor the formation of a
  large scale spiral structure\, that efficiently\ntraps dust. There\, the 
 dust concentration can be so high that it\nbecomes unstable\, possibly col
 lapsing into Earth-mass objects. We\nanalytically characterise this behavi
 our\, and we confirm it through\nnumerical simulations\, showing that plan
 etary cores at large radii can\nbe efficiently formed in young protostella
 r discs.
DTSTART:20260219T160000Z
DTEND:20260219T170000Z
LAST-MODIFIED:20260212T180956Z
LOCATION:Bloomberg Lecture Hall
SUMMARY:Institute for Advanced Study Astrophysics Seminar
URL:https://www.ias.edu/sns/events/institute-advanced-study-astrophysics-se
 minar-141
END:VEVENT
BEGIN:VEVENT
UID:b43e6abc-d826-4b91-aafd-4a7a95ba223b-0
DTSTAMP:20260420T184811Z
CREATED:20260202T164527Z
DESCRIPTION:Topic: A Theory for Collisionless Relaxation: Origin of the NFW
  Profile in Cold Dark Matter Halos\n\nSpeakers: Uddipan Banik\, Institute 
 for Advanced Study\n\nMore: https://www.ias.edu/sns/events/ias-physicsastr
 o-meeting-2
DTSTART:20260224T193000Z
DTEND:20260224T210000Z
LAST-MODIFIED:20260204T145811Z
LOCATION:Bloomberg Lecture Hall (IAS)
SUMMARY:IAS Physics+Astro Meeting
URL:https://www.ias.edu/sns/events/ias-physicsastro-meeting-2
END:VEVENT
BEGIN:VEVENT
UID:df74f190-a22b-413d-8210-0bdf91e47580-0
DTSTAMP:20260420T184811Z
CREATED:20260127T120501Z
DESCRIPTION:Topic: Hierarchical few body problem at High Eccentricity is a 
 simple pendulum\n\nSpeakers: Ygal Klein\, Institute for Advanced Study\n\n
 More: https://www.ias.edu/sns/events/institute-advanced-study-astrophysics
 -seminar-142\n\nI will present and discuss new analytical solutions to hig
 h\neccentricity perturbed Keplerian orbits undergoing Kozai-Lidov\noscilla
 tions. In particular\, I will show that the complex dynamics of\nhierarchi
 cal few body stellar systems - can be reduced to simple\npendulum models t
 hat predict the long-term evolution of the system.\nExamples of the soluti
 ons include: The octupole term effect\, both for\na massive and non massiv
 e perturber\,  and a precessing quadrupole\npotential emerging from higher
  multiplicity (4 bodies etc.)
DTSTART:20260226T160000Z
DTEND:20260226T170000Z
LAST-MODIFIED:20260225T155442Z
LOCATION:Bloomberg Lecture Hall
SUMMARY:Institute for Advanced Study Astrophysics Seminar
URL:https://www.ias.edu/sns/events/institute-advanced-study-astrophysics-se
 minar-142
END:VEVENT
BEGIN:VEVENT
UID:2ebca16c-98ac-48f8-bafd-9ec1dfd1e696-0
DTSTAMP:20260420T184811Z
CREATED:20260127T120547Z
DESCRIPTION:Topic: Improving Neutron Star Mergers with Advanced Computation
 al Methods\n\nSpeakers: Jacob Fields\, Institute for Advanced Study\n\nMor
 e: https://www.ias.edu/sns/events/institute-advanced-study-astrophysics-se
 minar-143\n\nContinual improvements to our observational capabilities prom
 ise a\nwealth of data from binary neutron star systems in the coming years
 \nand decades\, which will find broad applications across several fields\n
 of physics. However\, the current generation of models for interpreting\nt
 hese events contain uncertainties and systematic errors that make\nthem un
 suitable for future events. In this talk\, I will discuss how\nsome of the
 se problems arise from limitations in numerical relativity.\nI will then f
 ocus on recent efforts to help address some of these\nlimitations through 
 more efficient computational techniques and more\naccurate numerical metho
 ds. In each case\, I will also highlight\nscience applications that are be
 ing enabled by these improvements.
DTSTART:20260305T160000Z
DTEND:20260305T170000Z
LAST-MODIFIED:20260227T192532Z
LOCATION:Bloomberg Lecture Hall
SUMMARY:Institute for Advanced Study Astrophysics Seminar
URL:https://www.ias.edu/sns/events/institute-advanced-study-astrophysics-se
 minar-143
END:VEVENT
BEGIN:VEVENT
UID:8e15ef8c-8a0a-41e3-9672-b9add952912f-0
DTSTAMP:20260420T184811Z
CREATED:20260127T120705Z
DESCRIPTION:Topic: Which Microphysics Matters? The Case for Dust Dynamics\n
 \nSpeakers: Nadine Soliman\, Institute for Advanced Study\n\nMore: https:/
 /www.ias.edu/sns/events/institute-advanced-study-astrophysics-seminar-144
 \n\nAbstract: Numerical simulations of galaxies and the interstellar\nmedi
 um are now reaching resolutions where small-scale physical\nprocesses can 
 be resolved directly. This raises a natural question:\nwhich pieces of mic
 rophysics must be modeled explicitly in order to\ncapture the behavior of 
 astrophysical systems? In this talk I will\nargue that dust provides a par
 ticularly natural place to begin. Dust\ngrains interact simultaneously wit
 h radiation\, thermal balance\,\nchemical networks\, and gas dynamics\, pr
 ocesses that are critical to\nthe evolution of astrophysical environments.
  Yet in most simulations\ndust is assumed to remain perfectly coupled to t
 he gas\, reducing it to\na passive source of opacity and erasing its dynam
 ical role.\n\nUsing a combination of simulations and analytical arguments\
 , I will\npresent work that relaxes this assumption and follows dust as a
 \ndynamically distinct component. I consider several environments\,\ninclu
 ding AGN-driven winds\, star-forming molecular clouds\, and\nmagnetized du
 sty plasmas. In each case\, allowing dust to move relative\nto the gas pro
 duces qualitative changes that are absent when dust and\ngas are assumed t
 o move together. These include modifications to the\nstructure of radiatio
 n-driven outflows\, systematic effects on the\ncomposition and efficiency 
 of star formation\, and new pathways for\nseeding magnetic fields in the e
 arly Universe.\n\nTaken together\, these results illustrate how grain-scal
 e dust physics\npropagates upward to shape the large-scale structure and e
 volution of\nastrophysical systems.
DTSTART:20260312T150000Z
DTEND:20260312T160000Z
LAST-MODIFIED:20260309T125953Z
LOCATION:Bloomberg Lecture Hall
SUMMARY:Institute for Advanced Study Astrophysics Seminar
URL:https://www.ias.edu/sns/events/institute-advanced-study-astrophysics-se
 minar-144
END:VEVENT
BEGIN:VEVENT
UID:1e6227bf-48a6-4413-a611-8ff462207888-0
DTSTAMP:20260420T184811Z
CREATED:20260127T121854Z
DESCRIPTION:Topic: Multiscale Problems in Astrophysics\n\nSpeakers: Greg Br
 yan\, Columbia University\; Rachel Somerville\, CCA\, Faltiron\n\nMore: ht
 tps://www.ias.edu/sns/events/institute-advanced-study-multi-scale-initiati
 ve-1
DTSTART:20260313T160000Z
DTEND:20260313T180000Z
LAST-MODIFIED:20260309T130732Z
LOCATION:Rubenstein Commons | Meeting Room 5
SUMMARY:Institute for Advanced Study Multi-Scale Initiative
URL:https://www.ias.edu/sns/events/institute-advanced-study-multi-scale-ini
 tiative-1
END:VEVENT
BEGIN:VEVENT
UID:4a9cfef8-1d8c-4fbe-a3de-7a0713928625-0
DTSTAMP:20260420T184811Z
CREATED:20260202T191125Z
DESCRIPTION:More: https://www.ias.edu/sns/events/ias-max-planck-ias-ntu-cen
 ter-kick-conference\n\nORGANIZERS:\nNima Arkani-Hamed\nGiovanni Maria Toma
 selli\nFrancisco Vazão\nMatias Zaldarriaga\n\nThis event is the kick-off c
 onference for the Max Planck-IAS-NTU\nCenter for Particle Physics\, Cosmol
 ogy\, and Geometry. It is a\ncollaboration between the Max Planck Institut
 e for Physics in Garching\n(Germany)\, the Institute for Advanced Study in
  Princeton (USA)\, and\nthe National Taiwan University in Taipei (Taiwan).
  It aims to bring\ntogether researchers from particle physics\, cosmology\
 , and mathematics\nto foster collaboration\, bridge gaps between these fie
 lds\, and gain\nnew insights into the universe that would otherwise be ina
 ccessible\nfrom each field alone. \n\nSome of the topics discussed in this
  conference will include: quantum\nfield theory\, scattering amplitudes\, 
 inflationary physics\,\ncosmological correlators\, CMB physics\, gravitati
 onal waves\,\nlarge-scale structure of the universe\, dark matter\, positi
 ve geometry\,\nalgebraic geometry\, and combinatorics.\n\nTo register to a
 ttend the conference\, please click here\n[https://urldefense.com/v3/__htt
 ps://www.eventbrite.com/e/max-planck-ias-ntu-center-kick-off-conference-ti
 ckets-1981955746992?aff=oddtdtcreator__\;!!NubF!JVm4njuMM0iXMo21hGB--UlWcy
 sZxVngv446bHsjf6Rh0ATfeB4cn3PbaSgNsNDXdyPcLM5DZkA$]. \nRegistration is lim
 ited to 100 participants.  THE DEADLINE TO\nREGISTER IS MONDAY\, FEBRUARY 
 23\, 2026.\n\nTHERE IS A NON-REFUNDABLE REGISTRATION FEE OF $49.87.  You m
 ust be a\ncurrent faculty member\, researcher\, or graduate student at an
 \naccredited institution to register and attend. Registration includes\nal
 l coffee breaks\, lunches\, a welcome reception\, and two dinners\nduring 
 the conference program. Accommodations and travel expenses are\nnot includ
 ed in the conference fee.
DTSTART:20260316T130000Z
DTEND:20260316T220000Z
LAST-MODIFIED:20260202T191810Z
LOCATION:Wolfensohn Hall
SUMMARY:IAS Max Planck-IAS-NTU Center Kick-off Conference
URL:https://www.ias.edu/sns/events/ias-max-planck-ias-ntu-center-kick-confe
 rence
END:VEVENT
BEGIN:VEVENT
UID:4a9cfef8-1d8c-4fbe-a3de-7a0713928625-1
DTSTAMP:20260420T184811Z
CREATED:20260202T191125Z
DESCRIPTION:More: https://www.ias.edu/sns/events/ias-max-planck-ias-ntu-cen
 ter-kick-conference\n\nORGANIZERS:\nNima Arkani-Hamed\nGiovanni Maria Toma
 selli\nFrancisco Vazão\nMatias Zaldarriaga\n\nThis event is the kick-off c
 onference for the Max Planck-IAS-NTU\nCenter for Particle Physics\, Cosmol
 ogy\, and Geometry. It is a\ncollaboration between the Max Planck Institut
 e for Physics in Garching\n(Germany)\, the Institute for Advanced Study in
  Princeton (USA)\, and\nthe National Taiwan University in Taipei (Taiwan).
  It aims to bring\ntogether researchers from particle physics\, cosmology\
 , and mathematics\nto foster collaboration\, bridge gaps between these fie
 lds\, and gain\nnew insights into the universe that would otherwise be ina
 ccessible\nfrom each field alone. \n\nSome of the topics discussed in this
  conference will include: quantum\nfield theory\, scattering amplitudes\, 
 inflationary physics\,\ncosmological correlators\, CMB physics\, gravitati
 onal waves\,\nlarge-scale structure of the universe\, dark matter\, positi
 ve geometry\,\nalgebraic geometry\, and combinatorics.\n\nTo register to a
 ttend the conference\, please click here\n[https://urldefense.com/v3/__htt
 ps://www.eventbrite.com/e/max-planck-ias-ntu-center-kick-off-conference-ti
 ckets-1981955746992?aff=oddtdtcreator__\;!!NubF!JVm4njuMM0iXMo21hGB--UlWcy
 sZxVngv446bHsjf6Rh0ATfeB4cn3PbaSgNsNDXdyPcLM5DZkA$]. \nRegistration is lim
 ited to 100 participants.  THE DEADLINE TO\nREGISTER IS MONDAY\, FEBRUARY 
 23\, 2026.\n\nTHERE IS A NON-REFUNDABLE REGISTRATION FEE OF $49.87.  You m
 ust be a\ncurrent faculty member\, researcher\, or graduate student at an
 \naccredited institution to register and attend. Registration includes\nal
 l coffee breaks\, lunches\, a welcome reception\, and two dinners\nduring 
 the conference program. Accommodations and travel expenses are\nnot includ
 ed in the conference fee.
DTSTART:20260317T130000Z
DTEND:20260317T220000Z
LAST-MODIFIED:20260202T191810Z
LOCATION:Wolfensohn Hall
SUMMARY:IAS Max Planck-IAS-NTU Center Kick-off Conference
URL:https://www.ias.edu/sns/events/ias-max-planck-ias-ntu-center-kick-confe
 rence
END:VEVENT
BEGIN:VEVENT
UID:4a9cfef8-1d8c-4fbe-a3de-7a0713928625-2
DTSTAMP:20260420T184811Z
CREATED:20260202T191125Z
DESCRIPTION:More: https://www.ias.edu/sns/events/ias-max-planck-ias-ntu-cen
 ter-kick-conference\n\nORGANIZERS:\nNima Arkani-Hamed\nGiovanni Maria Toma
 selli\nFrancisco Vazão\nMatias Zaldarriaga\n\nThis event is the kick-off c
 onference for the Max Planck-IAS-NTU\nCenter for Particle Physics\, Cosmol
 ogy\, and Geometry. It is a\ncollaboration between the Max Planck Institut
 e for Physics in Garching\n(Germany)\, the Institute for Advanced Study in
  Princeton (USA)\, and\nthe National Taiwan University in Taipei (Taiwan).
  It aims to bring\ntogether researchers from particle physics\, cosmology\
 , and mathematics\nto foster collaboration\, bridge gaps between these fie
 lds\, and gain\nnew insights into the universe that would otherwise be ina
 ccessible\nfrom each field alone. \n\nSome of the topics discussed in this
  conference will include: quantum\nfield theory\, scattering amplitudes\, 
 inflationary physics\,\ncosmological correlators\, CMB physics\, gravitati
 onal waves\,\nlarge-scale structure of the universe\, dark matter\, positi
 ve geometry\,\nalgebraic geometry\, and combinatorics.\n\nTo register to a
 ttend the conference\, please click here\n[https://urldefense.com/v3/__htt
 ps://www.eventbrite.com/e/max-planck-ias-ntu-center-kick-off-conference-ti
 ckets-1981955746992?aff=oddtdtcreator__\;!!NubF!JVm4njuMM0iXMo21hGB--UlWcy
 sZxVngv446bHsjf6Rh0ATfeB4cn3PbaSgNsNDXdyPcLM5DZkA$]. \nRegistration is lim
 ited to 100 participants.  THE DEADLINE TO\nREGISTER IS MONDAY\, FEBRUARY 
 23\, 2026.\n\nTHERE IS A NON-REFUNDABLE REGISTRATION FEE OF $49.87.  You m
 ust be a\ncurrent faculty member\, researcher\, or graduate student at an
 \naccredited institution to register and attend. Registration includes\nal
 l coffee breaks\, lunches\, a welcome reception\, and two dinners\nduring 
 the conference program. Accommodations and travel expenses are\nnot includ
 ed in the conference fee.
DTSTART:20260318T130000Z
DTEND:20260318T220000Z
LAST-MODIFIED:20260202T191810Z
LOCATION:Wolfensohn Hall
SUMMARY:IAS Max Planck-IAS-NTU Center Kick-off Conference
URL:https://www.ias.edu/sns/events/ias-max-planck-ias-ntu-center-kick-confe
 rence
END:VEVENT
BEGIN:VEVENT
UID:4a9cfef8-1d8c-4fbe-a3de-7a0713928625-3
DTSTAMP:20260420T184811Z
CREATED:20260202T191125Z
DESCRIPTION:More: https://www.ias.edu/sns/events/ias-max-planck-ias-ntu-cen
 ter-kick-conference\n\nORGANIZERS:\nNima Arkani-Hamed\nGiovanni Maria Toma
 selli\nFrancisco Vazão\nMatias Zaldarriaga\n\nThis event is the kick-off c
 onference for the Max Planck-IAS-NTU\nCenter for Particle Physics\, Cosmol
 ogy\, and Geometry. It is a\ncollaboration between the Max Planck Institut
 e for Physics in Garching\n(Germany)\, the Institute for Advanced Study in
  Princeton (USA)\, and\nthe National Taiwan University in Taipei (Taiwan).
  It aims to bring\ntogether researchers from particle physics\, cosmology\
 , and mathematics\nto foster collaboration\, bridge gaps between these fie
 lds\, and gain\nnew insights into the universe that would otherwise be ina
 ccessible\nfrom each field alone. \n\nSome of the topics discussed in this
  conference will include: quantum\nfield theory\, scattering amplitudes\, 
 inflationary physics\,\ncosmological correlators\, CMB physics\, gravitati
 onal waves\,\nlarge-scale structure of the universe\, dark matter\, positi
 ve geometry\,\nalgebraic geometry\, and combinatorics.\n\nTo register to a
 ttend the conference\, please click here\n[https://urldefense.com/v3/__htt
 ps://www.eventbrite.com/e/max-planck-ias-ntu-center-kick-off-conference-ti
 ckets-1981955746992?aff=oddtdtcreator__\;!!NubF!JVm4njuMM0iXMo21hGB--UlWcy
 sZxVngv446bHsjf6Rh0ATfeB4cn3PbaSgNsNDXdyPcLM5DZkA$]. \nRegistration is lim
 ited to 100 participants.  THE DEADLINE TO\nREGISTER IS MONDAY\, FEBRUARY 
 23\, 2026.\n\nTHERE IS A NON-REFUNDABLE REGISTRATION FEE OF $49.87.  You m
 ust be a\ncurrent faculty member\, researcher\, or graduate student at an
 \naccredited institution to register and attend. Registration includes\nal
 l coffee breaks\, lunches\, a welcome reception\, and two dinners\nduring 
 the conference program. Accommodations and travel expenses are\nnot includ
 ed in the conference fee.
DTSTART:20260319T130000Z
DTEND:20260319T210000Z
LAST-MODIFIED:20260202T191810Z
LOCATION:Wolfensohn Hall
SUMMARY:IAS Max Planck-IAS-NTU Center Kick-off Conference
URL:https://www.ias.edu/sns/events/ias-max-planck-ias-ntu-center-kick-confe
 rence
END:VEVENT
BEGIN:VEVENT
UID:affc63ed-e3b5-48bd-ad4f-4b09b317bb2e-0
DTSTAMP:20260420T184811Z
CREATED:20260127T120746Z
DESCRIPTION:Topic: TBA\n\nMore: https://www.ias.edu/sns/events/institute-ad
 vanced-study-astrophysics-seminar-145
DTSTART:20260319T150000Z
DTEND:20260319T160000Z
LAST-MODIFIED:20260313T142355Z
LOCATION:Bloomberg Lecture Hall
SUMMARY:Institute for Advanced Study Astrophysics Seminar
URL:https://www.ias.edu/sns/events/institute-advanced-study-astrophysics-se
 minar-145
END:VEVENT
BEGIN:VEVENT
UID:dd07ad97-11ad-4d7a-8b5a-35991a5e4f8d-0
DTSTAMP:20260420T184811Z
CREATED:20260127T120822Z
DESCRIPTION:Topic: Numerical Modeling of Plasmas Across Fluid and Kinetic R
 egimes\n\nSpeakers: Chuanfei Dong\, Institute for Advanced Study\n\nMore: 
 https://www.ias.edu/sns/events/institute-advanced-study-astrophysics-semin
 ar-146\n\nPlasmas exhibit a wide range of behaviors across fluid and kinet
 ic\nregimes\, governing key processes in diverse laboratory\, space\, and
 \nastrophysical environments. Understanding these systems requires\nnumeri
 cal models with varying levels of physical fidelity\, including\nmagnetohy
 drodynamic (MHD)\, multi-moment multifluid\, and\nparticle-in-cell (PIC) a
 pproaches\, as well as combined methods such as\nhybrid-PIC and adaptively
  embedded particle-in-cell (MHD-AEPIC)\nmodels. These approaches enable us
  to capture multiscale dynamics and\na broad range of plasma processes.\n
 \nIn this talk\, I will present several examples that connect plasma\ndyna
 mics across scales using different modeling approaches\, including\nlocal 
 simulations of magnetic reconnection and turbulence\, as well as\nglobal s
 tudies of star–planet interactions in our solar system and\nbeyond. I will
  also demonstrate how modern machine learning techniques\ncan be leveraged
  to incorporate kinetic physics into fluid models\,\nenabling them to repr
 oduce kinetic simulation results without\nexplicitly resolving phase-space
  dynamics.
DTSTART:20260326T150000Z
DTEND:20260326T160000Z
LAST-MODIFIED:20260323T130932Z
LOCATION:Bloomberg Lecture Hall
SUMMARY:Institute for Advanced Study Astrophysics Seminar
URL:https://www.ias.edu/sns/events/institute-advanced-study-astrophysics-se
 minar-146
END:VEVENT
BEGIN:VEVENT
UID:95124d1d-5fdc-4612-9947-82b8484726cc-0
DTSTAMP:20260420T184811Z
CREATED:20260127T120904Z
DESCRIPTION:Topic: Inside Astronomically Realistic Black Holes\n\nSpeakers:
  Andrew Hamilton\, University of Colorado Boulder\n\nMore: https://www.ias
 .edu/sns/events/institute-advanced-study-astrophysics-seminar-147\n\nI wil
 l use a real-time general relativistic Black Hole Flight\nSimulator to sho
 w what really happens inside astronomically realistic\nblack holes. The in
 ner horizon of a rotating black hole is the most\nviolent place in the Uni
 verse\, easily reaching and surpassing energy\ndensities attained in the B
 ig Bang. What does Nature do at this\nextraordinary place?
DTSTART:20260402T150000Z
DTEND:20260402T160000Z
LAST-MODIFIED:20260330T133020Z
LOCATION:Bloomberg Lecture Hall
SUMMARY:Institute for Advanced Study Astrophysics Seminar
URL:https://www.ias.edu/sns/events/institute-advanced-study-astrophysics-se
 minar-147
END:VEVENT
BEGIN:VEVENT
UID:ec5eec67-6765-46f1-9740-fa7b8138237d-0
DTSTAMP:20260420T184811Z
CREATED:20260127T121003Z
DESCRIPTION:Topic: TBA\n\nSpeakers: Scott Gaudi\, Ohio State University\n\n
 More: https://www.ias.edu/sns/events/institute-advanced-study-astrophysics
 -seminar-148
DTSTART:20260409T150000Z
DTEND:20260409T160000Z
LAST-MODIFIED:20260127T121033Z
LOCATION:Bloomberg Lecture Hall
SUMMARY:Institute for Advanced Study Astrophysics Seminar
URL:https://www.ias.edu/sns/events/institute-advanced-study-astrophysics-se
 minar-148
END:VEVENT
BEGIN:VEVENT
UID:265eb67a-5af7-48d6-b557-7b5a9356a08b-0
DTSTAMP:20260420T184811Z
CREATED:20260127T121038Z
DESCRIPTION:Topic: Kink Instability and Its Associated Turbulence in Astrop
 hysical Jets\n\nSpeakers: Hui Li\, Los Alamos National Laboratory\n\nMore:
  https://www.ias.edu/sns/events/institute-advanced-study-astrophysics-semi
 nar-149\n\nAstrophysical jets driven by black holes are thought to undergo
  kink\ninstabilities due to the large current carried by such jets.\nDissi
 pation of magnetic energy through kink instabilities has been\nsuggested t
 o account for the high-energy radiation (often in flaring\nfashion) up to 
 many TeVs. In recent years\, galactic microquasars (such\nas SS 433) have 
 generated a lot of interests\, given its high-energy\ngamma-ray radiation 
 (up to 100s TeV\, potentially to PeV) from their\njets/lobes. Furthermore\
 , in the case of SS433\, polarized X-ray\nemissions with spatially (quasi-
 )resolved polarization angle and\ndegree were reported by IXPE. The high d
 egree of polarization implies\nlarge-scale (~ several parsecs) coherent ma
 gnetic fields. In this\ntalk\, we will present 3D magnetohydrodynamic (MHD
 ) studies of kink\ninstabilities in jets and how they produce the polariza
 tion properties\nof jets.  The properties of kink-driven turbulence will b
 e described\nand compare with the properties of Alfvenic turbulence. Parti
 cle\nacceleration in kink-driven turbulence will be presented as well. We
 \nwill end with discussing possible implications for astrophysical jets\na
 nd lobes. 
DTSTART:20260416T150000Z
DTEND:20260416T160000Z
LAST-MODIFIED:20260413T145950Z
LOCATION:Bloomberg Lecture Hall
SUMMARY:Institute for Advanced Study Astrophysics Seminar
URL:https://www.ias.edu/sns/events/institute-advanced-study-astrophysics-se
 minar-149
END:VEVENT
BEGIN:VEVENT
UID:c2e99a2b-b472-4515-b187-11506e8a169a-0
DTSTAMP:20260420T184811Z
CREATED:20260413T182430Z
DESCRIPTION:Topic: Multi scale problems in turbulent combustion\n\nSpeakers
 : Alexei Poludnenko\, University of Connecticut\n\nMore: https://www.ias.e
 du/sns/events/institute-advanced-study-multi-scale-initiative-2
DTSTART:20260417T160000Z
DTEND:20260417T180000Z
LAST-MODIFIED:20260420T141544Z
LOCATION:Rubenstein Commons | Meeting Room 5
SUMMARY:Institute for Advanced Study Multi-Scale Initiative
URL:https://www.ias.edu/sns/events/institute-advanced-study-multi-scale-ini
 tiative-2
END:VEVENT
BEGIN:VEVENT
UID:1842cfd1-9200-41f1-8f8c-cc18043e60e2-0
DTSTAMP:20260420T184811Z
CREATED:20260127T121139Z
DESCRIPTION:Topic: Magnetospheric Accretion and Ejection\n\nSpeakers: Zhaoh
 uan Zhu\, Institute for Advanced Study\n\nMore: https://www.ias.edu/sns/ev
 ents/institute-advanced-study-astrophysics-seminar-150\n\nMagnetospheric a
 ccretion is a universal process occurring in\nmagnetized astronomical obje
 cts\, ranging from neutron stars and white\ndwarfs to young stars (YSOs) a
 nd planets. In the context of neutron\nstars\, this process is linked with
  phenomena such as X-ray pulsars and\nultra-luminous X-ray sources (ULXs).
  For YSOs\, it results in\nultraviolet (UV) excess and atomic emission lin
 es. Despite the wide\nvariance in the observation energy range\, the under
 lying physical\naccretion process exhibits many similarities\, primarily d
 ue to the\ngoverning role of magnetic fields. Understanding these dynamica
 l\nprocesses is essential for interpreting observational data and sheds\nl
 ight on the impact of accretion on star/planet evolution. We have\ncarried
  out first-principle three-dimensional magnetohydrodynamic\n(MHD) simulati
 ons to study magnetospheric accretion. I will discuss\nphysical insights g
 ained from these simulations\, which include\nfilamentary accretion due to
  the interchange instability\, magnetic\nbubbles similar to MAD disks\, st
 ar-disk torque\, field inflation\, field\nreconnection\, and episodic outf
 lows. Finally\, implications on\nexoplanets demographics will be discussed
 . 
DTSTART:20260423T150000Z
DTEND:20260423T160000Z
LAST-MODIFIED:20260420T125524Z
LOCATION:Bloomberg Lecture Hall
SUMMARY:Institute for Advanced Study Astrophysics Seminar
URL:https://www.ias.edu/sns/events/institute-advanced-study-astrophysics-se
 minar-150
END:VEVENT
BEGIN:VEVENT
UID:9435b3dd-6526-4089-9a0e-86fe78e38b07-0
DTSTAMP:20260420T184811Z
CREATED:20260127T121208Z
DESCRIPTION:Topic: TBA\n\nSpeakers: Tom Wagg\, CCA\, Flatiron Institute\n\n
 More: https://www.ias.edu/sns/events/institute-advanced-study-astrophysics
 -seminar-151
DTSTART:20260430T150000Z
DTEND:20260430T160000Z
LAST-MODIFIED:20260127T121315Z
LOCATION:Bloomberg Lecture Hall
SUMMARY:Institute for Advanced Study Astrophysics Seminar
URL:https://www.ias.edu/sns/events/institute-advanced-study-astrophysics-se
 minar-151
END:VEVENT
BEGIN:VEVENT
UID:8686e537-bf71-464a-95ac-3d5311485b14-0
DTSTAMP:20260420T184811Z
CREATED:20260127T121341Z
DESCRIPTION:Topic: TBA\n\nSpeakers: Nan Liu\, IAR Boston\n\nMore: https://w
 ww.ias.edu/sns/events/institute-advanced-study-astrophysics-seminar-152
DTSTART:20260507T150000Z
DTEND:20260507T160000Z
LAST-MODIFIED:20260127T121539Z
LOCATION:Bloomberg Lecture Hall
SUMMARY:Institute for Advanced Study Astrophysics Seminar
URL:https://www.ias.edu/sns/events/institute-advanced-study-astrophysics-se
 minar-152
END:VEVENT
BEGIN:VEVENT
UID:9896973a-5be8-4097-b6e9-32c802b4c5b2-0
DTSTAMP:20260420T184811Z
CREATED:20260420T141709Z
DESCRIPTION:Topic: TBA\n\nSpeakers: Tapio Schneider\, California Institute 
 of Technology\n\nMore: https://www.ias.edu/sns/events/institute-advanced-s
 tudy-multi-scale-initiative-3
DTSTART:20260515T160000Z
DTEND:20260515T180000Z
LAST-MODIFIED:20260420T154739Z
LOCATION:Rubenstein Commons | Meeting Room 5
SUMMARY:Institute for Advanced Study Multi-Scale Initiative
URL:https://www.ias.edu/sns/events/institute-advanced-study-multi-scale-ini
 tiative-3
END:VEVENT
END:VCALENDAR
