Name: Wigner 111 - Colourful and Deep
Start: 2013-11-11T06:00:00+01:00
End: 2013-11-14T22:00:00+01:00
Location: Hungarian Academy of Sciences

Wigner 111 - Colourful and Deep

from Monday, 11 November 2013 (06:00) to Thursday, 14 November 2013 (22:00)

Monday, 11 November 2013

08:00

08:00 - 09:00
Room: Ceremonial Hall (Díszterem)

09:00

09:00 - 09:20
Room: Ceremonial Hall (Díszterem)
09:20 Quantum Theory viewed from Wigner Phase Space - Wolfgang P. Schleich (Institute für Quantenphysik, Universitat Ulm)
Quantum Theory viewed from Wigner Phase Space
- Wolfgang P. Schleich (Institute für Quantenphysik, Universitat Ulm)
09:20 - 10:00
Room: Ceremonial Hall (Díszterem) Eugene Paul Wigner’s formulation [1, 2] of quantum mechanics in phase space is completely equivalent to the ones by Werner Heisenberg, Erwin Schrödinger or Richard Feynman but offers many insights into the inner workings of quantum theory usually hidden behind the opaque curtain of the respective formalism. In the present talk we review some of them having led to the construction of focusing wave packets in free space [3], or the astonishing properties [4] of s-waves giving rise to measures of entanglement [5] based on the negative parts of the Wigner function, and tunneling [6] analyzed from phase space making contact with Unruh radiation. References [1] E.P. Wigner, On the quantum correction for thermodynamic equilibrium, Phys. Rev. 40, 749-759 (1932) [2] W.P. Schleich, Quantum Optics in Phase Space, (VCH-Wiley, Weinheim, 2001) [3] I. Bialynicki-Birula, M.A. Cirone, J.P. Dahl, M. Fedorov, and W.P. Schleich, In- and outbound spreading of a free-particle s-wave, Phys. Rev. Lett. 89, 060404 (2002) [4] J.P. Dahl, S. Varro, A. Wolf, and W.P. Schleich, Wigner functions of s waves, Phys. Rev. A 75, 052107 (2007) [5] J.P. Dahl, H. Mack, A. Wolf, and W.P. Schleich, Entanglement versus negative domains of Wigner functions, Phys. Rev. A 74, 042323 (2006) [6] D.M. Heim, W.P. Schleich, P.M. Alsing, J.P. Dahl, and S. Varro, Tunneling of an energy eigenstate through a parabolic barrier viewed from Wigner phase space, Phys. Lett. A 377, 1822-1825 (2013)
10:00 Quantum RMS Deviation and Heisenbergs Error‐Disturbance Relation - Paul Busch
Quantum RMS Deviation and Heisenbergs Error‐Disturbance Relation
- Paul Busch
10:00 - 10:40
Room: Ceremonial Hall (Díszterem) It has been claimed in recent research publications that Heisenberg’s idea of an accuracy-disturbance trade-off in quantum measurements has been theoretically and experimentally falsified. Here we analyze this claim and show that it is based on a combination of two factors: (a) a restricted perspective on measurement uncertainty relations that focuses on state-dependent measures of error and disturbance rather than considering them figures of merit for measuring devices; (b) the use of a generalization of Gauss’ root-mean-square deviation that is based on the problematic concept of noise operator. We present an alternative operationally significant quantum generalization of root-mean- square deviation and using this we obtain a valid formulation of a Heisenberg-type error- disturbance relation for position and momentum.
10:40 Coffee break
Coffee break
10:40 - 11:00
Room: Ceremonial Hall (Díszterem)
11:00 Effective Image Recognition using High-Order Symmetry of Correlated Orbital Angular Momentum (OAM) States - Alexander V. Sergienko
Effective Image Recognition using High-Order Symmetry of Correlated Orbital Angular Momentum (OAM) States
- Alexander V. Sergienko
11:00 - 11:30
Room: Ceremonial Hall (Díszterem) A major contribution of Wigner's work was the introduction of group theory to study both the dynamics and the classification of states in quantum mechanics. The use of rotational symmetry to study the properties of angular momentum eigenstates is particularly associated with him. Following along a similar path, it is shown here that advances in the study of entangled two-photon states allow the rapid detection of rotational symmetries in complex macroscopic objects, and that knowledge of this symmetry structure can allow identification, and in some circumstances reconstruction, of the object. This suggests some possible future applications.
11:30 Wigner crystals - New realizations of an old idea - Jenő Sólyom (Wigner RCP of the HAS)
Wigner crystals - New realizations of an old idea
- Jenő Sólyom (Wigner RCP of the HAS)
11:30 - 12:00
Room: Ceremonial Hall (Díszterem)
12:15 Lunch
Lunch
12:15 - 13:45
14:00 The role of Wigner's 1939 Representation Theory in ongoing Foundational Changes of Quantum Field Theory - Bert Schroer
The role of Wigner's 1939 Representation Theory in ongoing Foundational Changes of Quantum Field Theory
- Bert Schroer
14:00 - 14:40
Room: Ceremonial Hall (Díszterem) Presently quantum field theory is undergoing significant changes which started with the solution of an old problem: the quantum field theory behind the third positive energy Wigner representation class ("infinite spin")in terms of of string-localized generating fields. This in turn led to foundational changes for the other two classes: the m>0 and the m=0 finite helicity class The stringlocal description of these two classes leads among other things to the extension of renormalizability for any spin and the "adiabatic equivalence principle" makes sure that the physical content is the same as in the nonrenormalizable pointlike description i.e. stringlocal fields play the role of a different "field coordinatization" of the same QFT. The special case m>0, s=1 amounts to a Hilbert space analog of the BRST operator gauge description in Krein space in which the subalgebra of pointlike fields coincides with the gauge invariant observables. The stringlike approach leads to new insights into the Higgs mechanism and confinement. Last but not least it reveals that the noncompact localization properties of the third Wigner class matter as those which astrophysicists ascribe to dark matter.
14:40 Relativistic Wigner functions - Iwo Białynicki-Birula (Polish Academy of Sciences, Warsaw)
Relativistic Wigner functions
- Iwo Białynicki-Birula (Polish Academy of Sciences, Warsaw)
14:40 - 15:20
Room: Ceremonial Hall (Díszterem) Owing to the processes of particle creation and annihilation relativistic quantum mechanics does not exist as a consistent theory and it must be replaced by quantum field theory. Nevertheless the original construction of Wigner (and Szilard) can be extended in a natural manner to quantum field theory just by replacing wave functions by the field operators [1]. The expectation value in a one-particle state of such an object reduces in the nonrelativistc approximation to the standard Wigner function. Of course, in full quantum field theory the evolution equation for the Wigner function involves higher order functions that are built from products of more than two field operators and the hierarchy of such equations does not close. However, when the coupling to the external field plays the dominant role and the mutual interaction can be neglected, one obtains the evolution equation similar to the transport equation for the standard Wigner function that in some cases can be solved analytically. One important application of this construction is the description of electron-positron pair creation by an applied electromagnetic field. Every quantum field theory allows for the construction of the Wigner function from field operators but for the electromagnetic field (and also for other bosonic fields) there is also an entirely different construction that leads to a Wigner functional. The arguments of this functional are not points in the phase space but the electric and magnetic fields. Still, this functional shares many properties with the good old Wigner function and it enables one to learn something new about the properties of the quantized electromagnetic field. In particular, this construction gives a new insight into the statistical properties of the electromagnetic field at finite temperature. References: [1] I. Bialynicki-Birula, P. Gornicki and J. Rafelski, Phys. Rev. D 44, 1825 (1991).
15:20 Coffee break
Coffee break
15:20 - 15:40
Room: Ceremonial Hall (Díszterem)
15:40 Bell's inequalities: "From Einstein, Bell, Wigner, to entangled quantum bits: a new quantum era" - Alain Aspect (Institut d'Optique, Palaiseau)
Bell's inequalities: "From Einstein, Bell, Wigner, to entangled quantum bits: a new quantum era"
- Alain Aspect (Institut d'Optique, Palaiseau)
15:40 - 16:20
Room: Ceremonial Hall (Díszterem)
16:20 Nuclear Physics at GSI and FAIR - Horst Stöcker
Nuclear Physics at GSI and FAIR
- Horst Stöcker
16:20 - 17:00
Room: Ceremonial Hall (Díszterem) The international Facility for Antiproton and Ion Research in Europe (FAIR) is the largest fundamental science facility under construction worldwide. FAIR has been founded by Finland, France, Germany, India, Poland, Romania, Russia, Slovenia and Sweden. From 2018 onwards, FAIR will provide unique opportunities for cutting-edge research in nuclear, hadron and particle physics, atomic and anti-matter science, high density plasmas and applications in condensed matter, biology and the bio-medical- and material sciences. A global community of 3000 scientists from 51 countries prepare for outstanding research in the APPA, CBM, NUSTAR and PANDA detector collaborations. A cutting edge accelerator complex with eight storage and superconducting synchrotron rings and several linacs is constructed with the GSI Helmholtz Centre for Heavy Ion Research in Darmstadt, Germany.
17:00 Neutron Stars, Black Holes, and Gamma Ray Bursts: three events with Eugen Wigner in Princeton - Remo Ruffini
Neutron Stars, Black Holes, and Gamma Ray Bursts: three events with Eugen Wigner in Princeton
- Remo Ruffini
17:00 - 17:40
Room: Ceremonial Hall (Díszterem)
18:30

18:30 - 22:00
Tuesday, 12 November 2013
08:30
08:30 - 10:10
Room: Small Chamber Hall (Kisterem)
Contributions

08:30 The quest for gravitational waves: Status of the current ground-based projects I. - Jean-Yves Vinet

08:55 The quest for gravitational waves: Status of the current ground-based projects II. - Federico Ferrini

09:20 ET: the Einstein Telescope; designing the third Generation of Gravitational Wave - Harald Lück

09:45 Gravitational Wave Detection from Space: The eLISA Mission - Karsten Danzmann
08:30 - 10:10
Room: Ceremonial Hall (Díszterem)
Contributions

08:30 Eugene P. Wigners Visionary Contributions to Generations I through IV Fission Reactors - Frank Carre

08:55 The reactor ALLEGRO and the sustainable nuclear energy in Central Europe - János Gadó

09:20 Overview of EU Demo Design and R&D Studies - Jon Harman

09:45 Progress in Magnetic Fusion and ITER - Jean Jacquinot
08:30 - 10:10
Room: Great Lecture Hall (Nagyterem)
Contributions

08:30 Branched Hamiltonians and Supersymmetry - Thomas L. Curtright (University of Miami, USA)

08:55 Deformation quantization: Quantum mechanics lives and works in phase‐space - Cosmas K. Zachos (Argonne National Laboratory, USA)

09:20 A cellular automaton perspective on the linearity of quantum mechanics - Hans Thomas Elze (Universitá di Pisa. Italy)

09:45 Newton Force from Wave Function Collapse: a Testable Emergence Time - Lajos Diósi
08:30 - 10:10
Room: Reading Room (Felolvasó terem)
Contributions

08:30 Wigner function in action: Classical description of measurement back-action - Juha Javanainen (University of Connecticut, USA)

08:55 Sequential quantum measurements - János A. Bergou

09:20 Nonlocal interferometry using Schrödinger cats - James D. Franson (University of Maryland, USA)

09:45 Wigner function and probability representation of quantum states - Vladimir Man'ko
10:10 Coffee break
Coffee break
10:10 - 10:30
Room: Ceremonial Hall (Díszterem)
10:30
10:30 - 12:12
Room: Small Chamber Room (Kisterem)
Contributions

10:30 The LUNA experiment at Gran Sasso Laboratory - Alessandra Guglielmetti

10:55 The unreasonable effectiveness of experiments in constraining nova nucleosynthesis - Anjou Parikh

11:20 The Trojan Horse Method: Recent Applications to Nuclear Astrophysics - Claudio Spitaleri

11:45 Colored condensates deep inside compact stars - David Blaschke
10:30 - 12:01
Room: Ceremonial Hall (Díszterem)
Contributions

10:30 Possible Outcome of Fusion-fission Power Plant by 2050 and beyond - Boris V. Kuteev

10:55 Hungarian contribution to the success of ITER - Sándor Zoletnik (Wigner RCP of the HAS)

11:20 Energy Flow Control - Örs Legeza (Wigner RCP of the HAS)
10:30 - 12:00
Room: Great Lecture Hall (Nagyterem)
Contributions

10:30 Classical and Quantum Parts in Madelung Variables - Péter Ván (Wigner RCP of the HAS)

10:55 Operational Geometry on de Sitter Spacetime - Chryssomalis Chryssomalakos

11:20 The Unreasonable Effectiveness of Supersymmetry - Volker Schomerus (DESY, Theory Group)
10:30 - 12:10
Room: Reading Room (Felolvasó terem)
Contributions

10:30 Spontaneous photon emission in finite-sized cavities - Gernot Alber (University of Darmstadt, Germany)

10:55 Single dopants in diamond: quantum registers and nanoscale sensors - Fedor Jelezko (University of Ulm, Germany)

11:20 ELI-ALPS: A Challenge and Opportunity for European, Regional and National Science - Dimitris Charalambidis

11:45 The role of the Wigner function in charged particle beam dynamics - Renato Fedele
12:15 Lunch
Lunch
12:15 - 13:45
14:00
14:00 - 15:40
Room: 3rd Floor Lecture Room (Kupolaterem)
Contributions

14:00 Poisson Geometry of Difference Lax Operators and Difference Galois Theory - Michel Semenov-Tian-Shansky

14:25 Group Theory Origin of Higher Spin Duality - Antal Jevicki

14:50 Hidden symmetries of scattering amplitudes in gauge theories - Gregory Korchemsky

15:15 Geometry of the nuclear shell model - Pieter Van Isacker
14:00 - 15:40
Room: Small Chamber Room (Kisterem)
Contributions

14:00 Nuclear Structure Aspects from Gamma‐decay from Giant Resonances - Angela Bracco

14:25 Interplay between Spin and Isospin in Exotic Nuclei - Tomohiro Uesaka

14:50 Towards experiments at the new ELI-NP facility - Dimiter Balabanski

15:15 Symmetries and in-medium effects - Volker Metag
14:00 - 15:40
Room: Great Lecture Hall (Nagyterem)
Contributions

14:00 A first-principles description of the anomalous and spin Hall effects in disordered alloys - Hubert Ebert

14:25 The Fermi surface of PdCrO2 - Stephen Dugdale (University of Bristol, UK)

14:50 Chiral asymmetry in nanomagnetism - Laszlo Szunyogh

15:15 Recent Advances in the Korringa‐Kohn‐Rostoker Green Function Method - Rudolf ZELLER
14:15 Megnyitó/Opening: Wigner öröksége
Megnyitó/Opening: Wigner öröksége
14:15 - 14:30
Room: Ceremonial Hall (Díszterem)
14:30 Wigner Jenő: Sokoldalú tudós a viharos 20. században - István Hargittai (Budapesti Műszaki és Gazdaságtudományi Egyetem)
Wigner Jenő: Sokoldalú tudós a viharos 20. században
- István Hargittai (Budapesti Műszaki és Gazdaságtudományi Egyetem)
14:30 - 15:40
Room: Ceremonial Hall (Díszterem) Wigner Jenő Budapestről indult, Németországban vegyészmérnöki diplomat szerzett, majd kiváló elméleti fizikus lett. A náci hatalomátvétel után az Egyesült Államokban kötött ki, ahol elméleti fizikusként és a világ első nukleáris mérnökeként is működött. Segítette új hazáját és a szabad világot az első atomreaktorok megépítésében, a 2. világháború, majd a hidegháború megnyerésében. Alkalmazta a csoportelméletet és általában szimmetriameggondolásokat a kémiai reakciók leírásában és az atomfizikában. 1963-ban fizikai Nobel-díjjal tüntették ki. Az előadás bemutatja Wigner kontinenseken és diszciplínákon keresztülívelő munkásságát és emberközelségbe hozza ezt a különleges tudóst. Eugene P. Wigner Jenő moved from Budapest to Germany, graduated as chemical engineer, and became an internationally renowned theoretical physicist. After the Nazi takeover, he moved to the US where he worked as a professor of theoretical physics and the world’s first nuclear engineer. He assisted his new home country in developing the atomic bombs, winning World War II and the Cold War. He applied group theory and symmetry considerations in the description of chemical reactions and in atomic physics. In 1963, he received the Nobel Prize in Physics. This public lecture presents Wigner’s activities that spanned continents and scientific disciplines and bring this great scientist into human proximity. The presentation will be copiously illustrated with captions in English and will include a segment from a video conversation of Wigner with Clarence Larson in 1986 in English. Irodalom/Bibliography: Hargittai István, Az öt világformáló marslakó (Budapest: Vince Kiadó, 2006). Istvan Hargittai, The Martians of Science: Five Physicists Who Changed the Twentieth Century (New York: Oxford University Press, 2006 hardcover; 2008 softcover).
15:40 Coffee break
Coffee break
15:40 - 16:00
Room: Ceremonial Hall (Díszterem)
16:00
16:00 - 17:00
Room: 3rd Floor Lecture Room (Kupolaterem)
Contributions

16:00 Wigner and the groups in classifying elementary particles and nuclear states - József Cseh

16:25 Describing pair production in inhomogeneous external fields with the Dirac-Heisenberg-Wigner formalism - Dániel Berényi (MTA Wigner FK RMI, ELTE)
16:00 - 17:00
Room: Small Chamber Room
Contributions

16:00 Polyakov loop and charge fluctuations as probes of QCD phase transition - Krzystof Redlich

16:25 QGP Hadronization: Universal Conditions at SPS, RHIC and LHC - Johann Rafelski
16:00 - 17:00
Room: Great Lecture Hall (Nagyterem)
Contributions

16:00 Magnetic materials modelling ab-initio: fluctuating Wigner-Seitz cell magnetic moments, electron scattering resonances and strong electron correlations - Julie Staunton

16:25 Identification and characterization of solid-state single photon emitters - Ádám Gali (Wigner RCP of the HAS, BME)
Wigner Jenő a fasori diák - Eugene P. Wigner, Pupil of a Legendary School - László Kovács
Wigner Jenő a fasori diák - Eugene P. Wigner, Pupil of a Legendary School
- László Kovács
16:00 - 16:40
Room: Ceremonial Hall (Díszterem) “Naturally, we learned Physics from Sándor Mikola.” Wigner recalled. “I am proud to say that after two years of study (under his guidance at the Budapest Lutheran Gymnasium), the physics courses at the Budapest University of Technical Sciences (Műegyetem) and the Berlin Technische Hochschule seemed to be almost mere repetition.” “Never will I forget my former teachers, among them teacher of mathematics László Rátz , a genuine peadagogue and warmhearted man, who first awoke in me a love for his subject.” --Wigner wrote. We introduce during the lecture Wigner’s school years, his dearest teachers and his secondary school itself –the Budapest Lutheran (“Fasori”) Gymnasium—which compares well with the achievements of the Bronx High School of Science in the United States, New York.
17:00

17:00 - 19:00
Room: Ceremonial Hall (Díszterem)
Wednesday, 13 November 2013
09:00 Multi-entanglement of a Single Particle - Helmuth Rauch
Multi-entanglement of a Single Particle
- Helmuth Rauch
09:00 - 09:40
Room: Ceremonial Hall (Díszterem)
09:40 Poincaré Sphere and a Unified Picture of Wigners Little Groups - Young Suh Kim
Poincaré Sphere and a Unified Picture of Wigners Little Groups
- Young Suh Kim
09:40 - 10:20
Room: Ceremonial Hall (Díszterem)
10:20

10:20 - 10:30
Room: Ceremonial Hall (Díszterem)

10:30 Coffee break
Coffee break
10:30 - 11:00
Room: Ceremonial Hall (Díszterem)
11:00 E. P. Wigner and the Shaping of a National Laboratory: From the Manhattan Project to the Present - Malcolm STOCKS
E. P. Wigner and the Shaping of a National Laboratory: From the Manhattan Project to the Present
- Malcolm STOCKS
11:00 - 11:40
Room: Ceremonial Hall (Díszterem) The modern Oak Ridge National Laboratory (ORNL), which is the largest of the US Department of Energy (DOE) research laboratories, had its origins in the Manhattan Project as a pilot-scale facility for the production and separation of plutonium. Although E. P. Wigner spent only a little more than a year as research director of what was then known as Clinton Laboratories, his influence on the development of ORNL extended far beyond that period. Indeed, it was Wigner who laid the foundations for many of the signature strengths that ORNL boasts today, including nuclear energy, materials and chemical sciences, neutron scattering, life sciences and arguably computational science. When discussing Wigner’s lasting impact on ORNL, it is useful to consider a series of somewhat distinct periods: Wigner pre-Clinton – the Manhattan Project and the Metallurgical Laboratory at the University of Chicago; Wigner at Clinton – his role in developing and implementing a vision for a post-war civilian nuclear research laboratory underpinned by fundamental science; Wigner after Clinton – his continuing engagement with ORNL as consultant to and friend of ORNL’s longest serving director, Alvin Weinberg; and Wigner as ORNL’s “patron saint” and the inspiration for the establishment of the prestigious Wigner Fellowships for outstanding early-career researchers and most recently for the establishment of the “Eugene P. Wigner Distinguished Lecture Series,” which brings Nobel Laureates and internationally known industrial and technical leaders to the laboratory. In dealing with these periods we will refer to much original material that will convey Wigner’s most enduring legacy: that not only is basic science a matter of joy to the individual scientist, but it can and should contribute to the well-being of humanity.
11:40 The First and Best Reactor Engineer - László Koblinger József Rónaky
The First and Best Reactor Engineer
- László Koblinger
- József Rónaky
11:40 - 12:20
Room: Ceremonial Hall (Díszterem)
12:30 Lunch
Lunch
12:30 - 13:45
14:00 Fractional and Majorana Fermions (The physics of Dirac zero-energy modes) - Roman Jackiw
Fractional and Majorana Fermions (The physics of Dirac zero-energy modes)
- Roman Jackiw
14:00 - 14:40
Room: Ceremonial Hall (Díszterem)
14:40 Carbon from Red Giants to White Dwarfs The Breit-Wigner Formula, the Wigner Limit, and the Wigner-Seitz Radius - Michael Wiescher
Carbon from Red Giants to White Dwarfs The Breit-Wigner Formula, the Wigner Limit, and the Wigner-Seitz Radius
- Michael Wiescher
14:40 - 15:20
Room: Ceremonial Hall (Díszterem) This talk will discuss on to key reactions during post-main sequence stellar evolution. Both the radiative capture reactions 12C(α,)16O and the fusion reaction 12C+12C affect the nucleosynthesis of carbon in our universe. The role of these reactions will be discussed and recent results for the reaction cross sections will be analyzed in the context of nuclear structure and reaction models formulated by Eugene Wigner. The impact of the present prediction on quiescent late stellar evolution and cataclysmic explosions will be discussed.
15:20 Coffee break
Coffee break
15:20 - 15:40
Room: Ceremonial Hall (Díszterem)
15:40 Broken Symmetries and the Higgs Boson - Dezső Horváth (Wigner RCP of the HAS)
Broken Symmetries and the Higgs Boson
- Dezső Horváth (Wigner RCP of the HAS)
15:40 - 16:20
Room: Ceremonial Hall (Díszterem) The Standard Model, the theory of particle physics, based on global and local gauge symmetries, was established 40 years ago and it seems to describe all experimental data very well. All of its elementary particles were identified and studied long ago apart from the Higgs boson. The two main experiments of the Large Hadron Collider at CERN, CMS and ATLAS in 2012 observed a new boson with properties close to those predicted for the Standard Model Higgs boson. The latest LHC results imply that the new boson is indeed the Standard Model Higgs boson and thereby prove the validity of the Brout-Englert-Higgs mechanism of spontaneous symmetry breaking. François Englert and Peter Higgs received the 2013 Nobel Prize in physics. There are several questions yet concerning the possible theoretical significance of the mass of the new particle.
16:20 Eugene Wigner: A Gedanken Pioneer of the Second Quantum Revolution - Anton Zeilinger (Universität Wien, Wien, Austria)
Eugene Wigner: A Gedanken Pioneer of the Second Quantum Revolution
- Anton Zeilinger (Universität Wien, Wien, Austria)
16:20 - 17:00
Room: Ceremonial Hall (Díszterem) Eugene Wigner pointed out very interesting consequences of Quantum Physics in elegant gedanken experiments. Due to technical progress these gedanken experiments have become real experiments and contribute to the development of novel concepts in quantum information science, often called the second quantum revolution.
17:00

17:00 - 17:20
Room: Ceremonial Hall (Díszterem)
18:00
18:00 - 21:00
Contributions

18:30 Eugene P. Wigner's Wisdom - István Hargittai
Thursday, 14 November 2013

09:00

09:00 - 10:00
Room: Aula

10:00

10:00 - 11:30
Room: In front of the

11:30

11:30 - 12:00
Room: In fromt of the

12:00

12:00 - 12:30
Room: Panoramic Conference Hall, 2nd floor, 208

12:30

12:30 - 12:50
Room: Panoramic Conference Room, 2nd floor, 208

12:50

12:50 - 14:00
Room: Panoramic Conference Room, 2nd floor, 208

14:00

14:00 - 14:15
Room: In front of the