＜＜＜「@」を「__AT__」に置き換えています＞＞＞ Date: Mon, 05 Sep 2022 18:44:05 +0900 From: Shigeki Matsumoto To: "sg-l__AT__yukawa.kyoto-u.ac.jp"Subject: [Sg-l:6926] Workshop ""What the heck happens when the Universe boils?" (Dec. 5-9, 2022)の案内 素粒子論グループの皆様 今年度12月5-9日のスケジュールで行われるWorkshop "What the heck happens when the Universe boils?" の案内をさせて頂きます。 相転移に関わる物理の最近の発展に焦点をあてた特徴ある研究会と なっていますので、興味のある方は是非参加いただければ幸いです。 形式はハイブリッド型で、講演も受け付けていますので、 こちらもどうぞよろしくお願いします。 カブリ数物連携宇宙研究機構 松本 重貴 以下、研究会の案内です。 Dear all, We are happy to announce that the hybrid workshop "What the heck happens when the Universe boils?" is held on the following schedule: Date: December 5-9, 2022. Venue: Kavli IPMU (https://www.ipmu.jp/en) and Zoom (Hybrid style) Website: https://indico.ipmu.jp/event/414/overview The purpose of the workshop is as follows: A cosmological first-order phase transition is one of the murkiest areas of fundamental physics. However, if such a phase transition occurred, it could explain why we are here and leave startling gravitational wave signals. Further, multi-billion-dollar machines are expected to shed light on the nature of cosmological electroweak symmetry breaking in the next few decades: from next-generation particle colliders to gravitational wave detectors to searches for permanent electric dipole moments. Unless conditions turn out to be very unfavorable either for a first-order transition or electroweak baryogenesis, it will be virtually impossible to make robust statements about the viability of different models without substantial progress in understanding the underlying theory. The challenges facing our community are fourfold, 1 How to make robust predictions of charge asymmetries produced by CP-violating interactions with a bubble wall? Current methods disagree by many orders of magnitude. 2 How useful is perturbation theory in predicting the nature of a phase transition? If it is useful, how do we organize perturbation theory? 3 Can we make sense of bubble wall velocities in the ultra-relativistic and sub-relativistic regimes? 4 How well can we predict the gravitational wave spectra from macroscopic physics? In this workshop, we will bring together young researchers who are leaders in each of these areas to present their latest findings and discuss how to overcome these challenges. This workshop will have a light schedule with lots of time for discussion. Currently confirmed invited speakers: Yikun Wang (Caltech) Jorinde Van De Vis (Utrecht/Desy) Bjorn Garbrecht (Technical University of Munich) Tuomas Tenkanen (Nordita and TD Lee, Shanghai) Jyotirmoy Roy (University of Toronto Please visit the webpage mentioned above for the detail and to make a registration: We are looking forward to seeing many of you. Please also feel free to share the information with your colleagues. With best regards, Graham White Shigeki Matsumoto Satoshi Shirai %%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% Date: Fri, 11 Nov 2022 12:47:05 +0900 From: Shigeki Matsumoto To: "sg-l__AT__yukawa.kyoto-u.ac.jp" 素粒子論グループの皆様 今年度12月5-9日のスケジュールで行われるWorkshop "What the heck happens when the Universe boils?" の案内を再送させて頂きます。Hybrid形式での研究会 となっております。 相転移に関わる物理の最近の発展に焦点をあてた特徴ある研究会 となっており、初頭的なことから専門的なことまでを聞くことが出来る 講演や、議論の時間を多く用意していますので、興味のある方は 是非ご参加いただければ幸いです。 どうぞよろしくお願いします。 カブリ数物連携宇宙研究機構 松本 重貴 以下、研究会の案内です。 Dear all, We are happy to announce that the hybrid workshop "What the heck happens when the Universe boils?" is held on the following schedule: Date: December 5-9, 2022. Venue: Kavli IPMU (https://www.ipmu.jp/en) and Zoom (Hybrid style) Website: https://indico.ipmu.jp/event/414/overview The purpose of the workshop is as follows: A cosmological first-order phase transition is one of the murkiest areas of fundamental physics. However, if such a phase transition occurred, it could explain why we are here and leave startling gravitational wave signals. Further, multi-billion-dollar machines are expected to shed light on the nature of cosmological electroweak symmetry breaking in the next few decades: from next-generation particle colliders to gravitational wave detectors to searches for permanent electric dipole moments. Unless conditions turn out to be very unfavorable either for a first-order transition or electroweak baryogenesis, it will be virtually impossible to make robust statements about the viability of different models without substantial progress in understanding the underlying theory. The challenges facing our community are fourfold, 1 How to make robust predictions of charge asymmetries produced by CP-violating interactions with a bubble wall? Current methods disagree by many orders of magnitude. 2 How useful is perturbation theory in predicting the nature of a phase transition? If it is useful, how do we organize perturbation theory? 3 Can we make sense of bubble wall velocities in the ultra-relativistic and sub-relativistic regimes? 4 How well can we predict the gravitational wave spectra from macroscopic physics? In this workshop, we will bring together young researchers who are leaders in each of these areas to present their latest findings and discuss how to overcome these challenges. This workshop will have a light schedule with lots of time for discussion. Currently confirmed invited speakers: Yikun Wang (Caltech) Jorinde Van De Vis (Utrecht/Desy) Bjorn Garbrecht (Technical University of Munich) Tuomas Tenkanen (Nordita and TD Lee, Shanghai) Jyotirmoy Roy (University of Toronto Please visit the webpage mentioned above for the detail and to make a registration: We are looking forward to seeing many of you. Please also feel free to share the information with your colleagues. With best regards, Graham White Shigeki Matsumoto Satoshi Shirai