Spring 2018: Difference between revisions

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!style="width:20%" align="left" | host(s)
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|January 29
|January 29
| Dan Knopf (UT Austin)
| Dan Knopf (UT Austin)
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|February 12
|February 12
| Louis Fan (UW)
| Sam Krupa (UT-Austin)
|[[#Louis Fan |  TBD ]]
|[[#Sam Krupa |  TBD ]]
| Kim & Tran
| Lee
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|-  
|February 19
|February 19
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| Hongwei Gao (UCLA)
| Hongwei Gao (UCLA)
|[[#Hongwei Gao |  TBD ]]
|[[#Hongwei Gao |  TBD ]]
| Tran
|-
|March 19
| Huy Nguyen (Princeton)
|[[#Huy Nguyen |  TBD ]]
| Lee
|-
|April 9
| reserved
|[[# |  TBD ]]
| Tran
| Tran
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|-  

Latest revision as of 19:13, 22 January 2018

PDE GA Seminar Schedule Spring 2018

date speaker title host(s)
January 29 Dan Knopf (UT Austin) Non-Kähler Ricci flow singularities that converge to Kähler-Ricci solitons Angenent
February 5 Andreas Seeger (UW) TBD Kim & Tran
February 12 Sam Krupa (UT-Austin) TBD Lee
February 19 Maja Taskovic (UPenn) TBD Kim
March 5 Khai Nguyen (NCSU) TBD Tran
March 12 Hongwei Gao (UCLA) TBD Tran
March 19 Huy Nguyen (Princeton) TBD Lee
April 9 reserved TBD Tran
April 21-22 (Saturday-Sunday) Midwest PDE seminar Angenent, Feldman, Kim, Tran.
April 25 (Wednesday) Hitoshi Ishii (Wasow lecture) TBD Tran.

Abstracts

Dan Knopf

Title: Non-Kähler Ricci flow singularities that converge to Kähler-Ricci solitons

Abstract: We describe Riemannian (non-Kähler) Ricci flow solutions that develop finite-time Type-I singularities whose parabolic dilations converge to a shrinking Kähler–Ricci soliton singularity model. More specifically, the singularity model for these solutions is the “blowdown soliton” discovered by Feldman, Ilmanen, and Knopf in 2003. Our results support the conjecture that the blowdown soliton is stable under Ricci flow. This work also provides the first set of rigorous examples of non-Kähler solutions of Ricci flow that become asymptotically Kähler, in suitable space-time neighborhoods of developing singularities, at rates that break scaling invariance. These results support the conjectured stability of the subspace of Kähler metrics under Ricci flow.