Isospin Symmetry Breaking in Nuclear Physics
内藤 智也 (数理創造プログラム 基礎科学特別研究員)
Properties of neutron stars, such as the mass and radius relation, are one of the hot topics in astrophysics. Nuclear interaction determines such properties and available data of neutron stars are rather limited; hence, theoretical and experimental studies on nuclear physics help to understand neutron star properties. Protons and neutrons have almost the same properties apart from their charge, which is called isospin symmetry. Accordingly, the nuclear interaction also has isospin symmetry. However, tiny contribution of isospin symmetry breaking of nuclear interaction gives large systematic uncertainty for discussion of neutron star properties.
Categorification of the Jones polynomial
佐野 岳人 (数理創造プログラム 基礎科学特別研究員)
Jones polynomial is a knot invariant discovered by V. F. R. Jones in 1984. Not only that it is a useful mathematical tool, the discovery led to opening up a new research area, quantum topology, which connects quantum mechanics and low-dimensional topology. In 2000, M. Khovanov introduced a “categorification of the Jones polynomial”, which is now called Khovanov homology, and made categorification one of the fundamental concept in knot theory.
The "species" concept in biology. What is a "species" anyway?
ホセ サイード・グティエレス オルテガ (数理創造プログラム 基礎科学特別研究員)
"Species" is one of the most important concepts in biology. It refers to a group of organisms that share characteristics. Even if we don't study biology, most of the times it is easy to tell when two organisms belong to two different species. However, in biology, there is no a consensus on what a "species" is. There are a lot of definitions, and it seems that there is not a definition that can generalize the whole idea of species. In this short talk, I will discuss why some definitions of species are not applicable to certain fields in biology. Take home message: "species" is a unit that is very useful for research, but in many senses, it seems to be just an arbitrary grid that we put on the continuous biodiversity.
Data analysis, parameter estimation and error bars
カトゥリン・ボシゥメン (数理創造プログラム 副プログラムディレクター / Professor, Department of Physics, Ryerson University, Canada)
Even though my research is focused on virophysics, most of my day-to-day work consists in estimating the values of a model's parameters based on observational data. In this talk, I want to introduce the simple mathematics and computational methods involved in parameter estimation, and some of the common pitfalls. I will use specific example from my past and current work.
How do you measure the distance between the Earth and the Sun?
長瀧 重博 (数理創造プログラム 副プログラムディレクター / 理化学研究所 開拓研究本部 (CPR) 長瀧天体ビッグバン研究室 主任研究員)
Accurate measurement of distance is crucial to understanding the universe. In 1998, about 25 years ago, human beings became convinced that the universe is filled with dark energy, which was revealed by accurately determining the distance to supernovae locations. It is the first step in measuring the distance in the universe to determine the distance between the Earth and the Sun. How do you determine the distance between the Earth and the Sun? Of course, you cannot use a ruler from the Earth to the Sun. Once the distance between the Earth and the Sun is determined, the mass of the Sun can be obtained. Once the distance to the Sun is known, the radius of the Sun can also be determined. Then, by using physics, we can understand what is going on inside the Sun even though we cannot see the inside of the Sun by photons. From this understanding, we know that the Sun has a life span of about 5 billion years and that human beings have only about 1 billion years left to live on the Earth. In this 15-minute talk, I would like to present how to determine the distance between the Sun and the Earth.
Origami Embeddings of flat tori
坪井 俊 (数理創造プログラム 副プログラムディレクター / 武蔵野大学)
Flat tori appear in many places in mathematics; in complex analysis, in geometry, in algebra, ... It cannot be smoothly isometrically embedded in the 3-dimensional Euclidean space but Nash and Kuiper showed that it is possible in C1 smoothability in 1954-55. It is natural to ask whether we can embed flat tori isometrically as a piecewise-linear object, and Burago-Zalgaller showed it possible in 1996. Their construction is theoretically simple but actually complicated to show it as an object. But Henry Segerman gave a nice simple embedding, a Hinged Flat Torus, and this lead us to find a simple isometric piecewise-linear embedding for the flat torus of any modulus, which I am happy to talk about.
A dynamical proposal to resolve the cosmological constant problem
難波 亮 (数理創造プログラム 上級研究員)
Our universe is observed to be expanding at an accelerated rate. The expansion is driven by some unknown object that has a constant energy density, thus called "cosmological constant" (a.k.a. dark energy). Since gravitational effects, which drive the expansion, do not discriminate any forms of matter/energy, this constant is expected to receive various contributions from high-energy physics. However, the observed value of the constant is smaller than the theoretical expectation by many orders of magnitute, the discrepancy called the cosmological constant problem. A mechanism has been proposed to cancel the large contributions by a classical dynamics in the early universe, but it essentially empties the universe altogether, not just the cosmological constant. We propose a concrete scenario that subsequently "reheats" the universe with energetic matter, thus completing the mechanism of the cosmological constant relaxation.
邱 靖凱 (数理創造プログラム 上級研究員)
The transistor invention ushered in the era of conventional computers. However, Moore’s law will fail one day due to the unavoidable quantum limit. Scientists are building quantum computers to continue the computing era. In this talk, I will compare conventional computers and quantum computers. Furthermore, I will briefly introduce that a topological superconductor can be one of the platforms for quantum computing.
Generalized generating function for proportion values and its application
入谷 亮介 (数理創造プログラム 研究員)
I will talk about a potentially interesting and useful methodology I partly devised, based on (probability) generating function methods.
Weighted and directed XRP network
Abhijit Chakraborty (Kyoto University)
XRP is a well-known crypto currency. In this talk, I will introduce the structure of weighted directed networks from XRP transactions.
Borromean nucleus: an extreme state of the atomic nucleus
本郷 優 (数理創造プログラム 客員研究員 / Postdoctoral Research Associate, Physics Department, The University of Illinois at Chicago (UIC), USA)
I will introduce the Borromean nucleus, an exotic extreme state of the atomic nucleus.
Study on quantum interactions and number theory
若山 正人 (数理創造プログラム 特別顧問 / NTT基礎数学研究センタ 数学研究プリンシパル)
In this Coffee-meeting, I will discuss the energy spectra of certain models of quantum interactions (between photon and two-level system) and introduce the study in number theory that arise from them including future perspective and conjectures.
Derived Categories in Algebraic Geometry
小関 直記 (Postdoctoral Research Associate, School of Mathematics, University of Edinburgh, UK)
I will explain how derived categories play roles to connect various areas of mathematics, especially birational and enumerative geometry. The key ideas are "Categorifications" and "Semi-orthogonal decompositions"
Stochastic chemical reaction systems
広野 雄士 (数理創造プログラム 客員研究員 / Junior Research Group Leader/Assistant Professor, Research Division, Asia Pacific Center for Theoretical Physics, Republic of Korea)
"Chemical reactions play important roles in various fields including engineering and biology. In this talk, I plan to give a short introduction to the description of stochastic chemical reaction systems."
Universal form of stochastic equations of motion
伊丹 將人 (Kyoto University)
I will review the universal form of stochastic time evolution for slow variables in equilibrium systems and talk about one attempt to derive a universal form in nonequilibrium systems.
Determination of hadronic interactions from lattice QCD
杉浦 拓也 (数理創造プログラム 特別研究員)
The interactions between hadrons (such as proton and neutron) govern the structure of atomic nucleus. I will briefly discuss how we can define and quantify the hadronic interactions through numerical calculations of lattice QCD.
From the thermonuclear supernova to the supernova remnant
ジル・フェラン (数理創造プログラム 研究員 / 理化学研究所 開拓研究本部 (CPR) 長瀧天体ビッグバン研究室 研究員)
Type Ia supernovae (SNe) are believed to be the thermonuclear explosion of a white dwarf star, but their explosion mechanism(s) remain unclear. In this talk we make the connection with the subsequent phase, the supernova remnant (SNR), when the stellar ejecta interact with the interstellar medium. I will outline how simulations and observations can help test theoretical models, with an emphasis on our recent work based on the 3D morphology.
Cosmic origin of r-process elements?
西村 信哉 (理化学研究所 開拓研究本部 (CPR) 長瀧天体ビッグバン研究室)
The astronomical site of r-process nucleosynthesis has been a long-standing mystery in nuclear astrophysics studies. However, in recent years, there has been significant progress. We confirmed the r-process-driven transient "kilonova" associated with binary-neutron-star mergers. In this talk, I will discuss the possibility of the r-process in magneto-rotational supernovae, which are in the extreme class of core-collapse supernovae. Although this scenario is physically challenging and hypothetical, observational evidence appears to grow. Since this scenario is related to supernovae with many observational examples, we expect future direct/indirect observation. I will also discuss the theoretical perspective of observational properties.
Quantum chaos, Entanglement and Black holes
野坂 朋生 (数理創造プログラム 研究パートタイマー Ⅰ)
Quantum chaos is a notion to characterize the mechanism of how the time evolution of a quantum many body system, which should be in principle reversible, end up with the thermal equilibrium where the information of the initial condition is lost. This resembles the black hole information problem, which suggests that one can address various fundamental questions related to black holes through the study of quantum chaos. In this talk I will overview the notions of quantum chaos and black hole geometry, and then introduce an interesting phenomenon called revival where these notions are tightly entangled with each other.
マティアス・ベアヴァイン (数理創造プログラム 特別研究員)
Dimensional regularization is one of the most important tools for analytic calculations in quantum field theory. I will explain, how the concept of integration over (integer) n variables can be extended to a continuous number D, the dimension, and how this can be used to make sense of the divergent parts of quantum corrections.