Monday, November 29, 2021

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2021-12-06 / 10:00 ~ 11:30
학과 세미나/콜로퀴엄 - 박사논문심사: 확률론의 기본적인 극한 정리들에 대한 재탐구 인쇄
by 진우영(KAIST)
심사위원장 : 폴정, 심사위원 : 이지운, 남경식, 양홍석(전산학부), Greg Markowsky(Senior Lecturer, School of Mathematics, Monash University)
2021-11-30 / 16:30 ~ 17:30
IBS-KAIST 세미나 - 이산수학: Large clique subdivisions in graphs without small dense subgraphs 인쇄
by 임성혁(KAIST)
What is the largest number $f(d)$ where every graph with average degree at least $d$ contains a subdivision of $K_{f(d)}$? Mader asked this question in 1967 and $f(d) = \Theta(\sqrt{d})$ was proved by Bollob\'as and Thomason and independently by Koml\'os and Szemer\'edi. This is best possible by considering a disjoint union of $K_{d,d}$. However, this example contains a much smaller subgraph with the almost same average degree, for example, one copy of $K_{d,d}$. In 2017, Liu and Montgomery proposed the study on the parameter $c_{\varepsilon}(G)$ which is the order of the smallest subgraph of $G$ with average degree at least $\varepsilon d(G)$. In fact, they conjectured that for small enough $\varepsilon>0$, every graph $G$ of average degree $d$ contains a clique subdivision of size $\Omega(\min\{d, \sqrt{\frac{c_{\varepsilon}(G)}{\log c_{\varepsilon}(G)}}\})$. We prove that this conjecture holds up to a multiplicative $\min\{(\log\log d)^6,(\log \log c_{\varepsilon}(G))^6\}$-term. As a corollary, for every graph $F$, we determine the minimum size of the largest clique subdivision in $F$-free graphs with average degree $d$ up to multiplicative polylog$(d)$-term. This is joint work with Jaehoon Kim, Youngjin Kim, and Hong Liu.
2021-12-03 / 10:00 ~ 11:00
SAARC 세미나 - SAARC 세미나: 인쇄
by 장주희()
In astrophysical fluid dynamics, stars are considered as isolated fluid masses subject to self-gravity. A classical model to describe the dynamics of Newtonian stars is given by the gravitational Euler-Poisson system, which admits a wide range of star solutions that are in equilibrium or expand for all time or collapse in a finite time or rotate. In particular, using numerics, the Euler-Poisson system in the super-critical regime has been widely used inastrophysics literature todescribe the gravitational collapse, but its rigorous proof has been established only recently. The main challenge comes from thepressure, which actsagainstgravitational force. In this talk, I will discuss some recent progress on Newtonian dust-like collapse and self-similar collapse.
2021-12-03 / 13:00 ~ 14:00
학과 세미나/콜로퀴엄 - PDE 세미나: 인쇄
by ()
This series of lectures will focus on recent developments of the so-called a-contraction theory and its application to the study of discontinuous flow at high Reynolds numbers. We will first introduce the classical framework to study the stability of 1D shocks for compressible flows. Recent multi-D applications will be presented next, both in the context of compressible and incompressible flows.
2021-12-01 / 13:00 ~ 14:00
학과 세미나/콜로퀴엄 - PDE 세미나: 인쇄
by ()
This series of lectures will focus on recent developments of the so-called a-contraction theory and its application to the study of discontinuous flow at high Reynolds numbers. We will first introduce the classical framework to study the stability of 1D shocks for compressible flows. Recent multi-D applications will be presented next, both in the context of compressible and incompressible flows.
Events for the 취소된 행사 포함 모두인쇄
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