Special Topics Available
From time to time, courses are offered as a Special Topic that complement the regular range of electives. General administrative details of the course can be seen at Special Topics. Special Topics are open to all members of the OIST Community.
Special Topics on offer in the coming year are listed below. More are added as we receive the information. Multiple modules may be taken (if offered as a series, please take all in the series). Special Topics are recorded on your transcript, if you are enrolled as a PhD student. Successful completion of each Special Topic is awarded 1 credit. Written assessment of some kind is required for credit to be awarded. You may choose to audit instead, when you do not need to complete the assessment tasks, but no credit will be awarded (make this choice when you enroll, as retrospective conversion from not-for-credit to credit status is not permitted).
Newest courses are at the top of this list.
AY2021/2022 Term 2 (January - April 2021)
Cerebral Cortical Networks in Rodents and Primates
Dr Razvan Gamanut, Monash University, Australia (Sponsored by Prof Kenji Doya)
14 weeks, 1.5 hours per week, Room and Time TBD
In neuroscience, there is a concerted effort underway to clarify the structure and function of the cerebral cortex, which is arguably the most important component of the mammalian brain. To this end, rodents and non-human primates currently receive a special focus. On the one hand an expanding suite of genetic tools are available for use in rodents, especially in mice and rats, and on the other hand non-human primates such as marmosets and macaques show some of the most complex neuroanatomical and neurophysiological features, close to those in humans. What has the research revealed so far in this quest? We will explore a select set of findings at cellular and regional level, primarily in the mentioned species, from which we will extract rules of neuroanatomical arrangement and of neurophysiological processing in the cerebral cortex of the two orders. The first sessions will be dedicated to topographical organisation and inter-regional connections. Then we will focus on the modular and hierarchical processing in the visual cortex. Finally, we will look at the default mode network and its involvement in introspection, together with the claustrum and its unique relations with the cerebral cortex.
Student Learning Outcomes
At the completion of this course, students will be able to
• Compare and contrast comparative neuroanatomical features in the cortex of rats and mice, and of marmosets and macaques.
• Discuss common rules of neuroanatomical arrangement and of neurophysiological processing in the cerebral cortex of the two orders, including the canonical microcircuit, the default mode network, and the interaction with the claustrum.
• Describe the application of modern genetic, optical, and electrophysiological techniques in network mapping and tracing connections.
• Describe hierarchical and non-hierarchical processing in the visual cortex.
This will be assessed by two written exams.
01. Introduction to the course and to cerebral cortex
02. Theoretical constraints on connectivity with brain size
03. Connectivity, brain size and species
04. The role of weak projections
05. Components of the visual cortex
06. Exam 1
07. The canonical microcircuit
08. Modular processing in the visual cortex
09. Hierarchical processing in the visual cortex
10. Dorsal and ventral streams
11. Non-hierarchical processing in the visual cortex
12. Default mode network
14. Exam 2
No required prior knowledge as the course will introduce the necessary concepts and include discussions of the techniques.
Primarily neuroscience students, but students in other life sciences, in physical sciences or engineering are also welcome.
Textbook or required reading
Students will receive up to five relevant scientific articles six days before each class, and are required to read their abstracts and the methods.
Assessment will be in the form of two exams, one after the first 5 classes and worth 30% of the final grade, and the second at the end of the course, worth 70%. The exams will have questions from each class about the techniques discussed and the research findings. The questions will be based on the content of the lectures.
AY2021/2022 Term 1 (September - December 2021)
Covariant Physics and Black Hole Thermodynamics
Drs. Josh Kirklin, Isha Kotecha, and Fabio Mele, Hoehn Unit (Sponsored by Prof Philipp Hoehn)
15 weeks, 1 hour per week, Friday 1300-1400 in Lab 4 F15
General covariance is one of the fundamental principles underlying gravity. It says that the laws of physics do not depend on our choice of coordinates. Geometrically speaking, this means that we can apply any diffeomorphism to a physical system without changing its properties. In other words, diffeomorphisms are a kind of gauge symmetry. In this course, we will explore an elegant modern perspective on general covariance, using an approach known as the covariant phase space formalism. This formalism tells you how to treat covariant theories using classical Hamiltonian mechanics. Quantum gravity must be a quantisation of this classical theory. This means that we can learn a lot about some aspects of the quantum theory using the covariant phase space approach. For example, the laws of black hole thermodynamics are a reflection of the fact that black holes are quantum objects. We will show how key fundamental thermodynamical properties of the black hole, such as its entropy, can be understood using the covariant phase space. We will also discuss more general properties of black hole thermodynamics. Finally, we will explore the connection between gauge symmetry and quantum entanglement, and how this relates to the thermodynamics of spacetime itself.
Student Learning Outcomes
At the completion of this course, students will be able to use the covariant phase space formalism to analyse a covariant field theory, and apply it to the study of black hole thermodynamics. They will also understand some broader properties of black hole and spacetime thermodynamics. This will be assessed by a short essay on a topic TBD.
Detailed content (arranged by class session, or arranged in topics, with description)
1. Geometry of phase space, the symplectic form.
2. Hamiltonian mechanics.
3. Gauge symmetry and constraints in mechanics.
4. Covariant field theories.
5. Geometry of field space.
6. Gauge symmetry and constraints in field theory.
7. Global symmetries and large gauge symmetries.
8. Conserved charges in general relativity.
9. Black hole spacetimes and symmetries.
10. Energy, angular momentum and electric charge.
11. Black hole entropy as a Noether charge.
12. The laws of black hole thermodynamics.
13. Entanglement and gauge symmetry.
14. The first law of entanglement entropy.
15. Spacetime thermodynamics and the Einstein equations.
Target Students Theoretical physicists / mathematicians with some familiarity with quantum mechanics, thermodynamics, field theory and general relativity.
Introductory Lectures on Black Hole Thermodynamics, T. Jacobson.
Black Hole Entropy is Noether Charge, Robert M. Wald.
Advanced Lectures on General Relativity, Geoffrey Compère
AY2020/2021 Term 3 (May - August 2021)
Supersymmetric Quantum Mechanics and Morse Theory
Dr. Slava Lysov, Neiman Unit (sponsored by Yasha Neiman)
13 weeks, 2 x 1 hour per week, Tuesday and Thursday 1400-1500 in L4E01 except the four dates:
May 20, Thursday - L4E45
May 25, Tuesday - L4E48
June 17, Thursday - L4E48
July 15, Thursday - L4E48
Companion Course to Supersymmetric Field Theories and Superstrings (below)
Modern theoretical physics has a deep connection with modern mathematics. The foundations of this connection were established by Edward Witten in his works around the 1980s. We will use Witten's paper "Supersymmetry and Morse theory" as prime reference for the course. It is a scientific paper, so it assumes some background knowledge of both supersymmetry and Morse theory, which we will cover in the rest of the course. The second part of the course will be focused on two different approach to the Morse theory: the standard mathematical one, based on differential geometry and topology, and the physical one using supersymmetric quantum mechanics.
1. Introduction to topological invariants and cohomology.
2. Differential forms and de Rham cohomology.
3. Quantum mechanics of a particle on Riemann manifold.
4. Grassmann variables.
5. Introduction to supersymmetric quantum mechanics.
6. Superspace formalism.
7. Supersymmetric sigma model as a de Rham theory.
8. Superpotential as a Morse function.
9. Morse theory.
10. Morse complex for de Rham cohomology.
11. Tunneling in quantum mechanics.
12. Instantons in supersymmetric sigma model.
13. Vacuum degeneracy lift by instantons as a Morse complex for de Rham cohomology.
Students should have some knowledge of quantum mechanics and differential geometry.
There will be biweekly home assignments.
E. Witten, "Supersymmetry and Morse theory," J. Diff. Geom. 17 (1982) no.4, 661-692.
Hori, K., Thomas, R., Katz, S., Vafa, C., Pandharipande, R., Klemm, A., Vakil, R. and Zaslow, E., 2003. Mirror Symmetry (Vol. 1). American Mathematical Soc.
An Introduction to Supersymmetric Field Theories and (Super)Strings
Dr. Mirian Tsulaia, Neiman Unit (sponsored by Yasha Neiman)
13 weeks, 1.5 hours per week Monday afternoons 1300-1430 in B714a
The course consists of three parts: Bosonic strings, Supersymmetric Field Theories and Superstrings. We start with a description of Open and Closed bosonic strings: we describe their classical actions, a quantization and the corresponding spectrum.
We explain how to compute the partition function of the closed bosonic string on torus. Further we consider interacting bosonic strings and derive the Veneziano amplitude. Then we discuss a compactification on a circle and finally introduce non perturbative objects, so called D-branes. As a preparation to the superstrings, we cover some topics from N=1 supersymmetric field theories and supergravities. We describe N=1 superspace, superfields in general and chiral and vector superfields in particular. Then we give a brief introduction to four-dimensional N=1 supergravity and to higher dimensional supergravities. We tentatively plan to cover some selected topics in supersymmetric field theories such as elements of Minimal Supersymmetric Standard Model and nonperturbative superpotentials. In the final part of the course, we explain how to generalize the topics that we covered for bosonic strings to the case of superstrings.
1. Introduction, dual models
2. Bosonic string action, equations of motion
3. Quantization. States and operators
4. Partition function on torus
5. Compactification on a circle, T duality
6. D branes
7. Veneziano amplitude
8. N=1 SUSY algebra and its representations
9. Superspace, superfields
10. Supersymmetric Lagrangians
11. Perturbation theory
12. Spontaneous SUSY breaking, Supergravities
13. Selected topics: MSSM, Nonperturbative Superpotentials, Superstrings
Students should have some familiarity with quantum field theory and general relativity.
M.B. Green, J.H. Schwarz, E. Witten 'Superstring Theory'
J. Wess, J. Bagger "Supersymmetry and Supergravity"
C. Angelantonj, A. Sagnotti ''Open Strings'' Physics Reports 371 (2002), 1; hep-th/0204089
R. J. Szabo, ''BUSSTEPP lectures on string theory: An Introduction to string theory and D-brane dynamics,'', hep-th/0207142
J. D. Lykken "Introduction to Supersymmetry" hep-th/9612114
Introduction to Modern Astrophysics
Dr Alessandro Trani, University of Tokyo (Visiting Scholar, sponsored by Yasha Neiman)
13 weeks, 1.5 hours per week on Thursday mornings 10:00 - 11:30 in B711
A gentle introduction to the topics of modern astrophysics. We will start from the most fundamental topics, such as stellar structure and evolution, and gradually venture towards the 'hot topics' of contemporary astrophysics, namely exoplanets and gravitational waves. The aim is to provide the students with the essential knowledge to navigate the current landscape of astrophysical research, and put them into contact with the latest breakthroughs in the field. The emphasis will be put on our theoretical understanding of the Universe, rather than on observational techniques. If time allows, some notions of computational astrophysics will be discussed.
Class 1: Why study astrophysics? Telescopes and the electromagnetic spectrum
Class 2: The celestial sphere, parallax, dopplershift
Class 3: What is a star? Stellar structure and equilibria
Class 4: The lives of stars. From protostars to giants. The Hertzsprung–Russell diagram.
Class 5: The death of stars. Black holes, white dwarfs and neutron stars
Class 6: Binary stars. The gravitational two-body problem
Class 7: Interacting binaries. Tides, Roche lobe overflow, common envelope evolution
Class 8: Keplerian orbital elements. The solar system
Class 9: Planetary dynamics and origin of the solar system
Class 10: Exoplanets and how to find them
Class 11: Stellar clusters. Evolution and dynamics
Class 12: Gravitational waves I. Discovery and astrophysical conundrums
Class 13: Gravitational waves II. Formation pathways & pitfalls
Assumed knowledge: The students should have an undergraduate-level background in mathematics, physics or statistics. Specifically, a few classes will require some degree of familiarity with differential equations, Newtonian mechanics and thermodynamics.
Karttunen H., Kroger P., et al. - Fundamental Astronomy (5th ed.)
Kippenhanh R., et al. - Stellar Structure and Evolution (2nd ed.)
Carroll B.W., Ostlie D.A. - An Introduction to Modern Astrophysics (2nd ed.)
Binney J., Tremaine S. - Galactic Dynamics (2nd ed.)
Assessment: 100% final presentation
Introduction to Machine Learning
Dr. Mirian Tsulaia, Neiman Unit (sponsored by Yasha Neiman)
13 weeks, 1.5 hours per week Wednesday afternoons 1300-1430 in L4F01 (first class only is B250)
A good follow-on for students who take Prof Fukai's course B32 Statistical Modelling.
In order to familiarize students with the basic skills used in Machine Learning and Data Science, we shall cover some relevant topics from Statistical Learning and provide examples of practical applications of the theory. We shall briefly cover some basic concepts from Python programming language. Further, we give an introduction to libraries such as Numpy and Pandas which are commonly used in data science. Then we shall cover various regression and classification methods. For each of these methods we shall first give a theoretical description. After that, we shall demonstrate how this approach can be implemented for a specific problem in science or in business by building a corresponding model using Python.
Finally, we shall give an introduction to more advanced topics such as Deep Learning. In particular, we shall explain the theoretical foundations of Artificial Neural Networks, Convolutional Neural Networks, Recurrent Neural Networks, and Boltzmann Machines. Finally, we shall explain to which kind of problems these algorithms can be applied.
Topic 1: Python crash course
Topic 2: NumPy
Topic 3: Pandas
Topic 4: Linear regression
Topic 5: Multiple Linear regression
Topic 6: Logistic Regression
Topic 7: K Nearest Neighbors
Topic 8: Decision Trees
Topic 9: Support Vector Machines
Topic 10: K-Means Clustering
Topic 11: Principal Component analysis
Topic 12: Artificial Neural Networks, Convolutional Neural Networks
Topic 13: Recurrent Neural Networks, Boltzmann Machine
"An Introduction to Statistical Learning"
by James, Witten, Hastie and Tibshirani
"A High-Bias, Low-Variance Introduction to Machine Learning for Physicists" . arXiv 1803.08823
by Mehta, Wang, Day, Richardson, Bukov, Fisher, and Schwab
Bring your laptops with Python installed! (Preferably the Jupyter Notebook or Spyder.)
AY2019/2020 Term 1 (September - December 2019)
Biological Networks. Bioinformatics and modelling.
Professor Igor Goryanin (OIST adjunct professor)
Professor Anatoly Sorokin (Moscow Physical Technical Institute)
2019 October 21 onwards
Day 1: Oct 21 (Mon), 3 – 5pm
Theory: introduction, Enzymes kinetics (Goryanin)
Day 2: Oct 23 (Wed), 3 – 5 pm
Theory: Metabolic Pathways, Graph analysis of Biological networks. Standards in Systems Biology (Goryanin)
Day 3: Oct 24 (Thurs), 3 – 5 pm
Theory: Stoichiometric matrix and its properties. Flux Balance Analysis. Extreme pathways (Goryanin)
Day 4: Oct 25 (Fri), 3 – 5 pm
Theory: Metabolic Engineering and synthetic biology (Goryanin)
Day 5: Oct 28 (Mon), 3 – 5pm
Theory: Applications in Systems Biology (Goryanin)
Day 5: Oct 29 (Tue), 3 – 5pm
Theory: Introduction, installing software (Goryanin/Sorokin)
Day 6: Oct 30 (Wed), 3 – 5pm
Theory: Cytoscape, SBGN. Analysis and reconstruction of metabolic networks (Goryanin/Sorokin)
Day 7: Oct 31 (Thurs), 3 – 5pm
Theory: Flux Balance Analysis. Stoichiometric matrix and its properties. Extreme pathways. Practical. FBA with pyCOBRA/Sybi. Modeling of mutations and environment changes (Goryanin/Sorokin)
Day 8: Nov 1 (Fri), 3 – 5pm
Theory and Practical: Metagenomes analysis (Goryanin/Boerner)
AY2018/2019 Term 3 (May - August 2019)
Efficient Scientific Computing with Julia
Taught by Valentin Churavy, PhD student at MIT
Under the approval of Prof Ulf Skoglund, Dean of the Graduate School
Scientific computing is a cornerstone of research, many scientific projects now involve coding in some form — may it be modeling, simulations or data analysis — and doing so in a performant and reproducible manner is a requirement to contribute effectively. This course uses Julia to teach the fundamentals of best practices for reproducible code, performance analysis, and contributing to open-source. It furthermore focuses on aspects of HPC computing necessary to analysis and study large problems — in particular GPU computing.
Participants should posses some programming experience in either Julia, Python, MATLAB or C/C++. As part of the course students will design a small project, that can lead to an open-source contribution, an implementation of scientific program, or the performance improvement thereof. While the course uses Julia the knowledge should be transferable to other languages.
Computational Biology: Artificial Intelligence for Bioinformatics
Professor Hiroaki Kitano (OIST adjunct professor)
with other presenters
7/22 (Mon) 09:00-13:00: Kitano & Asai (Intro /Hands-on I Physiological Modeling)
7/23 (Tue) 09:00-13:00: Kitano (Signal Transaction/Cell Cycle)
7/24 (Wed) 09:00-13:00: Funahashi (Hands-on Ⅱ CellDesigner Modeling)
7/25 (Thu) 09:00-13:00: Kitano (AI for Life Science/Wrap-up)
Class times, room, and syllabus TBD
Dr Juan David Vasquez Jaramillo (Pauly Unit)
Statistical mechanics, a beautiful approach to equilibrium, is well known in physics for its broad range of applicability to describe the state of systems with a macroscopic number of particles. When the context changes, and the length scale is reduced as far as the Nanoscale, defining thermodynamics becomes cumbersome and new approaches must be introduced.
In the present course, we will develop the theory of quantum mechanical non-equilibrium processes from the Brownian harmonic oscilator, deriving Keldysh field theory, and putting it into context in models describing tunneling probes such as scanning tunneling microscopy (STM) or inelastic electron tunneling spectroscopy (IETS). Computer exercises will be developed to illustrate these examples and the students will be expected to be able to reproduce a scientific paper in their field of interest in relation to advanced statistical mechanics, non-equilibrium nanophysics or molecular electronics, as well they will be able to write a review on their topic of interest of maximum 25 pages and a minimum of 75 references.
20 hours (4 hours per week for 5 weeks) in Term 3
Class times and location TBD
AY2018/2019 Term 2 (January - April 2019)
States and Properties of Matter
Professor Mahesh Bandi
Offered as a series of four special topics courses presented over two terms (two courses per term). It treats the standard (gases, liquids and solids) and few exotic (polymers and colloids) classical states of matter, and explains how these states and their bulk properties emerge from the few interatomic and intermolecular forces at play. The emphasis is on developing strong physical intuition for microscopic mechanics using the simplest models that illuminate the concept. In doing so, we explain both the strengths and shortcomings of these simple models, and in particular, analyse the limiting conditions where they fail. Therefore, rather than theoretical rigour, the focus of the treatment is on performing quick order-of-magnitude calculations. As a result, although the mathematics is unsophisticated, Calculus is a pre-requisite. Wherever possible, scientific facts will be connected with the seminal experiments that established them.
Term 2, Classes Wednesday 2-4 and Thursday 3-5, Room B714a (modules 3 & 4 in term 3 at time and location TBD)
Quantum Models for Black Holes: Sachdev-Ye-Kitaev and generalizations
Professor Frank Ferrari (Université Libre de Bruxelles), Visitor in Toriumi Unit
Holography predicts that black holes can be described quantum mechanically by large N matrix models at strong coupling. We shall describe very recent ideas that have allowed to build exactly solvable models of this kind, providing an explicit quantum mechanical description of string-size black holes. These ideas are at the confluence of several different fields: condensed matter theory (disordered systems); quantum chaos; string theory and holography; matrix and tensor models (graph theory), etc. Many properties associated with black holes are found in the quantum mechanical description and will be discussed in the course, in particular the loss of unitarity at large N (and unitarity restoration at finite N), the quasi-normal behaviour, an emergent reparameterization invariance and maximal chaos.
Lectures 12 hours between 22 March to 10 April, and attendance at parts of workshop
“Workshop on recent developments in AdS/CFT” on 2 & 3 April 2019