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Đây là tóm tắt các bài giảng đó:
http://www.vaec.gov.vn/inst/school/Index1.htm#Scientific%20Program
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Research at VATLY.
Pierre Darriulat
Institute for Nuclear Science and Technology
An introductory presentation of the ongoing cosmic ray research being done at VATLY (past, present and future) will be given. It will be followed by a tour of the lab, the students being arranged in small groups of six or so.
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Observation of Cosmic Rays
Tiina Suomijärvi
IPN-Orsay, France
Lectures will treat the following topics:
1) Origin of cosmic rays
The lecture will give an overview on the origin of cosmic rays and their propagation in the Universe as an introduction to different detection methods that are used for their observation.
2) Detection methods
The lecture will shortly describe different detection methods used for cosmic rays of different nature (charged particles, gammas and neutrinos). Both direct detection by satellite or balloon experiments and detection methods based on shower detection will be discussed. New methods such as detection of cosmic rays by radioemission are also described.
3) Experiments
The lecture will present some of the current experiments detecting high energy gamma rays, neutrinos and charged particles. The data obtained by these experiments will also be discussed.
4) The Pierre Auger Observatory (Surface Detector)
The lecture will describe the Surface Detector of the Pierre Auger Observatory and discuss the first results obtained by the observatory.
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Relativistic approaches to study nuclear structure
Jie Meng
School of Physics, Peking University, Beijing 100871,China
Center of Theoretical Nuclear Physics, National laboratory of Heavy Ion
Accelerator of Lanzhou, Lanzhou 730000,China
Institute of Theoretical Physics, the Chinese Academy of Science, Beijing
100080,China;

After the introduction on nuclear structure model, a brief review on the relativistic nuclear structure models and their applications are presented, including the solution of the Dirac equations and the Relativistic Mean Field (RMF) theory in basis expansion and coordinate space, Relativistic Continuum Hartree-Bogoliubov (RCHB) theory together with its extension for axial symmetric case, the description of exotic nuclei, the continuum in RMF theory, relativistic spin and pseudo-spin symmetry, the Halos at the neutron drip line in nuclei and hyper-nuclei, and new magic number in superheavy nuclei, etc.
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?oNuclear Astrophysics?
Shigeru KUBONO
Center for Nuclear Study (CNS), University of Tokyo
This is an introduction course to nuclear astrophysics.
Recent astronomical observations and the scope of the field will be also touched on. The outline of the lecture is as follows:
(1) Nuclear physics in the universe - Nuclear phenomena, nuclear physics
(2) Standard model of evolution
(3) Synthesis of Oxygen - In He-burning
(4) Experimental methods
(5) Creation of the primordial universe
(6) Solar model and the pp-chain
(7) CNO cycle and explosive H-burning - Novae, X-ray burst
(8) s-process and heavy element synthesis
(9) Neutrino processes
(10) r-process in supernovae and cosmo-chronology
(11) Scope
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Nuclear Structure Studies by Direct Reactions
with Radioactive Beams
Peter Egelhof
GSI Darmstadt, Germany

The series of lectures will start with an introduction where a brief overview on the field and on the motivation for studying nuclei towards and at the limits of stability is given. It follows a more technical part, where the techniques for production of radioactive beams will be discussed, an overview on presently existing radioactive beam facilities will be given, and the various detection techniques including some examples of very recent developments of dedicated detector concepts will be presented.
The main part of the lectures will than be dedicated to a detailed discussion of direct reaction studies with radioactive beams, considering various types of reactions, such as elastic, inelastic, quasielastic scattering, breakup, transfer, etc. reactions, adressing various questions of nuclear structure physics. This will be followed by a brief overview on the physics of very rare isotopes, such as the investigation of superheavy elements, accelerator mass spectrometry, etc.
The final part of the lectures will be dedicated to the future perspectives at the next generation radioactive beam facilities with a special emphasis on the GSI future project FAIR.
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High Energy Cosmic Rays: Fundamentals, Status and Perspectives
Antonio Insolia
Univ. of Catania (Italy)
The topics covered in my lectures will be complementary to the arguments discussed by Tiina Suomijarvi. The lectures will point out the following topics:
1) Historic introduction to the cosmic ray physics
The lecture will give an overview on the first experiments on cosmic rays and their importance for the present understanding, discussing the main properties of an Extensive Air Shower (EAS) with the help of a simple EAS-like toy model. The main features of a real shower are then discussed.
2) The cosmic ray spectrum
The lecture will focus on the cosmic ray spectrum with a specific discussion of the still open problem of the expected GZK features of the spectrum and its importance. Comparison between different experimental results and models will be presented.
3) Mass composition problems
The lecture will present the status of the mass composition problem for the HECR, presenting the current approaches to the mass composition analysis. New ideas for the mass compostion analysis will also be discussed.
4) The Pierre Auger Observatory (Fluorescence Detector)
The lecture will describe the Fluorescence Detector of the Pierre Auger Observatory and discuss the first results obtained by the P. Auger Observatory.
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Mean Field Methods for Nuclear Structure
Nguyen Van Giai
IPN, Université Paris-Sud, Orsay, France

In these lectures I will give an introduction to the self-consistent mean field approach based on Skyrme-type effective interactions. This theory is presently widely used in nuclear physics and related astrophysical problems such as nucleosynthesis or the physics of neutron stars.
The first part of the lectures is devoted to the description of nuclear ground states in the framework of the Hartree-Fock (HF) and Hartree-Fock-Bogoliubov (HFB) approximations. The outline of HF and HFB methods with Skyrme forces will be given. Some recent applications to the description of nuclei and the inner crust of neutron stars will be discussed, in order to illustrate how the method is working in concrete situations. Finally, we show that an effective Skyrme force can be deduced from a Brueckner-HF theory.
In the second part we concentrate on nuclear excitations. After a brief reminder of linear response theory, we show how the random phase approximation (RPA) is a natural consequence of the time-dependent HF (TDHF) theory in the small amplitude limit. Thus, one has a unified framework for ground and excited states through the Skyrme-HF approach. When pairing correlations become important, one can generalize the RPA to quasiparticle RPA (QRPA). The formalism will be illustrated by various applications.
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Molecular structure in light nuclei
Hisashi Horiuchi
University of Kyoto, Japan
Four topics of recent studies of molecular structure in light nuclei are discussed.
1.
The first one is on the "alpha-alpha" cluster structure in Be isotopes from 8Be to neutron-dripline 14Be.
2.
The second one is on the structure of ground and excited states of 20Ne and 44Ti where "alpha+core" structures and superdeformed structure are involved.
3.
The third topic is on the superdeformation in sd-shell nuclei and its relation to nuclear molecular resonances.
4.
The final topic is on the "gas-like" states in 12C, 16O and 11B.
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MICROSCOPIC ANALYSIS OF EXCITATION OF GIANT RESONANCES BY ALPHA SCATTERING AND NUCLEAR COMPRESSIBILITY
Shalom Shlomo
Cyclotron Institute, Texas A&M University, College Station,
Texas 77843, USA
Studies of isoscalar giant monopole and dipole resonances are of particular current interest since their strength distributions, S(E), are sensitive to the value of nuclear matter (NM) incompressibility coefficient, K, which is directly related to the curvature of the NM equation of state (EOS). The EOS is very important physical quantity in the study of properties of nuclei, supernova collapse, neutron
stars and heavy-ion collisions. The main experimental tool for studying isoscalar giant resonances (GR) is inelastic alpha-particle scattering since alpha-particles are selective as to exciting isoscalar modes and the angular distributions of the excitation cross sections at small angles are characteristic for some of the multipolar modes. We emphasize that it is common in theoretical work on GR to calculate S(E) for a simple scattering operator F, within the mean-field based random phase approximation (RPA), whereas in the analysis of the cross sections one carries out distorted wave Born approximation (DWBA) calculations with a certain transition potential.
We will review the DWBA theory for calculating the excitation cross sections, employing the folding model (FM) approach for the evaluation of the optical potential and the transition potential using the ground state density and transition density, respectively. We will also review the elements of the Hartree-Fock (HF) based RPA theory for the calculation of S(E), centroid energies and transition densities of GR, with an emphasize on fully self-consistent calculations. We will examine the relation between S(E) and excitation cross sections and present results of microscopic calculations of S(E), obtained within the HF-RPA approach, and of excitation cross sections, obtained using the FM-DWBA pproach with ground state density and transition densities deduced from HF-RPA calculations. The implications of these results will be discussed.

Một trường học mới:
Rencontres du Vietnam ?" Institute of Physics and Electronics, Hanoi
XII-th VIETNAM SCHOOL OF PHYSICS
Nha trang, 26 December 2005 ?" 07 January 2006
http://www.iop.vast.ac.vn/activities/vsop/vsop12/index.htm

Vào ngày 7 tháng 9 này vì GS Pierre Darriulat giảng bài học ở cái trường học trên sẽ bắt đầu đưa chuỗi bài giàng về Modern Astrophysics tại Trường Đại học khoa học tự nhiên Hànội, Nguyên Trãi. Các bạn quan tâm thì có thể download bài giảng ở đây: http://www.vaec.gov.vn/inst/English/About/VATLY/4_Academic%20links/Lectures/astrophysics.pdf
Giờ giảng là 9h đến 12h thì phải còn địa điểm phòng nào và nhà nào thì mình không rõ nưa, bạn nào có đến thì hỏi và post lại lên đây đê cho các bạn khác đỡ phải đi tìm.

Osaka University-Asia Pacific-Vietnam National University,
Hanoi Forum 2005​

Sept. 27 - Sept. 29, 2005
International Convention centre
Hanoi, Vietnam
http://www.osaka-hanoi-forum.org/

Các lecture của bài giảng của trường học ở trên đã được đưa lên mạng, các bạn quan tâm có thể download về đọc:
http://www.vaec.gov.vn/inst/school/#Scientific%20Program

Nature''s Greatest Puzzles,
Trường học này đã kết thúc từ năm ngoái, nhưng mà tớ thấy nó có nhiều bài hay và bai giảng của nó được ghi lại bằng hình ảnh nên có thể nghe giảng trực tuyến được, nếu các bạn quan tâm thì download về nghe.
http://www.slac.stanford.edu/econf/C040802/program.htm
Monday, August 2 Where and What is Dark Matter?

9:00 - 10:00 AM Nature''s Greatest Puzzles C. Quigg
10:00 - 10:30 Coffee Break
10:30 - 11:30 Dark Matter Candidates T. Baltz
11:30 - 11:45 Coffee Break
11:45 - 12:45 Evidence for Dark Matter R. Gaitskell
12:45 - 2:00 Lunch
2:00 - 2:30 Results from CDMS B. Cabrera
2:30 - 3:00 Searching for the Axion L. Rosenberg
3:00 - 3:30 Weak Lensing: A Probe of Dark Matter and Dark Energy A. Refregier
4:00 - 6:00 Discussion Session
6:00 PM Welcome Reception
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Tuesday, August 3 How Massive are Neutrinos?

9:00 - 10:00 AM Theory Basics B. Kayser
10:00 - 10:30 Coffee Break
10:30 - 11:30 Experimental Neutrino Oscillations G. Gratta
11:30 - 11:45 Coffee Break
11:45 - 12:45 Neutrinos in Cosmology T. Weiler
12:45 - 2:00 PM Lunch
2:00 - 2:45 Recent Results from Super K D. Casper
2:45 - 3:15 Recent Results from K2K M. Yokoyama
3:15 - 3:45 Neutrinoless Double Beta Decay S. Elliott
4:00 - 6:00 Tours of SLAC
6:00 PM Dinner
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Wednesday, August 4 What are the implications of Neutrino Mass?

9:00 - 10:00 AM Theory Basics B. Kayser
10:00 - 10:30 Coffee Break
10:30 - 11:30 Experimental Neutrino Oscillations G. Gratta
11:30 - 11:45 Coffee Break
11:45 - 12:45 Neutrinos in Astrophysics G. Fuller
12:45 - 2:00 PM Lunch
2:00 - 3:00 Results from SNO D. Waller
3:00 - 3:30 Results from Amanda II S. Barwick
3:30 - 4:00 Neutrino Physics at MiniBoone S. Zeller
4:00 - 6:00 Discussion Session
6:00 PM Poster Session
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Thursday, August 5 What are the Origins of Mass?

9:00 - 10:00 AM Higgs Basics M. Peskin
10:00 - 10:30 Coffee Break
10:30 - 11:30 Precision EW Measurements and the Higgs Mass B. Marciano
11:30 - 11:45 Coffee Break
11:45 - 12:45 The Origin of Mass in QCD S. Chivukula
12:45 - 2:00 PM Lunch
2:00 - 2:30 Top and W Masses at the Tevatron S. Miller
2:30 - 3:00 Higgs Searches at the Tevatron S. Snyder
3:30 - 12:00 AM Lick Observatory Tour
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Friday, August 6 Why is there a spectrum of Fermion Masses?

9:00 - 10:00 AM Higgs Basics M. Peskin
10:00 - 10:30 Coffee Break
10:30 - 11:30 Precision EW Measurements and the Higgs Mass B. Marciano
11:30 - 11:45 Coffee Break
11:45 - 12:45 Neutrino Mass R. Mohapatra
12:45 - 2:00 Lunch
2:00 - 2:30 Properties of the Top Quark C. Clement
2:30 - 3:15 Higgs at LC and LHC A. De Roeck
3:15 - 3:45 Final Results from E158 Y. Kolomensky
3:45 - 4:15 Higgsless Models in Extra Dimensions C. Csaki
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Monday, August 9 Why is Gravity So Weak?

9:00 - 10:00 AM Solving the Hierarchy Problem J. Lykken
10:00 - 10:30 Coffee Break
10:30 - 11:30 Introduction to Extra Dimensions T. Rizzo
11:30 - 11:45 Coffee Break
11:45 - 12:45 Gravity and Strings S. Giddings
12:45 - 2:00 Lunch
2:00 - 2:30 Tests of Short Distance Gravity S. Smullin
2:30 - 3:15 General Relativity with Double Pulsars M. Kramer
3:15 - 3:45 Searches for Extra Dimensions at the Tevatron G. Landsberg
4:00 - 6:00 PM Discussion Session
6:00 PM Dinner
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Tuesday, August 10 Is Nature Supersymmetric?

9:00 - 10:00AM SUSY Basics X. Tata
10:00 - 10:30 Coffee Break
10:30 - 11:30 SUSY Basics X. Tata
11:30 - 11:45 Coffee Break
11:45 - 12:45 SUSY and Cosmology K. Matchev
12:45 - 2:00 PM Lunch
2:00 - 2:30 Direct Accelerator Searches for SUSY S. Wang
2:30 - 3:00 LHC/LC and SUSY K. Desch
3:00 - 3:30 Searching for SUSY in B Decays Y. Okada
3:30 - 4:00 Final (or Recent) Muon g-2 Results P. Shagin
4:00 - 6:00 SLAC Tour
6:00 Poster Session
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Wednesday, August 11 Why is the Universe made of Matter and not Anti-Matter?

9:00 - 10:00 AM How do we know Antimatter is Absent P. Coppi
10:00 - 10:30 Coffee Break
10:30 - 11:30 Lepto and Baryogenesis M. Trodden
11:30 - 11:45 Coffee Break
11:45 - 12:45 Can BSM CP Violation Generate the Baryon Asymmetry? C. Wagner
12:45 - 2:00 PM Lunch
2:00 - 3:00 CP Violation in B Meson Decays L. Lanceri
3:00 - 3:45 Search for Cosmological Antimatter R. Streitmatter
4:00 - 6:00 Discussion Session
6:00 Social Hour and Soccer Game
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Thursday, August 12 Where do Ultra High Energy Cosmic Rays Come?

9:00 - 10:00 AM Ultra High Energy Cosmic Rays T. Stanev
10:00 - 10:30 Coffee Break
10:30 - 11:30 Cosmic Acceleration Mechanisms R. Blandford
11:30 - 11:45 Coffee Break
11:45 - 12:45 Understanding the Atmosphere as a Calorimeter for UHE Cosmic Rays G. Schatz
12:45 - 2:00 PM Lunch
2:00 - 2:45 Results from Auger R. Cintra Shellard
2:45 - 3:15 Results from HESS W. Hofmann
3:15 - 3:45 Radio Detection of UHE Cosmic Rays and Neutrinos P. Gorham
4:00 - 6:00 Discussion Session
6:00 PM Dinner
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Friday, August 13 Did the Universe Inflate at Birth?

9:00 - 10:00 AM Inflation Basics M. Kamionkowski
10:00 - 10:30 Coffee Break
10:30 - 11:30 Inflation Basics M. Kamionkowski
11:30 - 11:45 Coffee Break
11:45 - 12:45 Inflation and String Theory A. Linde
12:45 - 2:00 PM Lunch
2:00 - 2:45 Road Map to the Future F. Gilman
2:45 - 3:45 The Last Word on Nature''s Greatest Puzzles N. Arkani-Hamed

và đây là một trường học khác nữa, các vấn đề mà các bạn khác đã mở ra nhiều topic nho nhỏ để hỏi có thể tham khảo các bài giàng ỏ đây:
http://www-conf.slac.stanford.edu/ssi/2005/program.htm
Chairman C. Prescott
9:00 - 10:00 AM General Relativity Primer S. Carroll
10:00 - 10:30 AM Refreshment Break
10:30 - 11:30 AM General Relativity Primer S. Carroll
11:30 - 11:45 AM Break
11:45 - 12:45 PM General Relativity Primer S. Carroll
12:45 - 2:15 PM Lunch
2:15 - 3:00 PM Gravity Probe - B Instrument and Data Reduction G. Keiser
3:00 - 3:45 PM Gravity Probe - B and General Relativity J. Mester
4:00 - 6:00 PM Discussion Session
6:00 PM Welcome Reception
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Tuesday, July 26
Chairman J. Jaros
9:00 - 10:00 AM Gravitational Radiation A. Buonanno
10:00 - 10:30 AM Refreshment Break
10:30 - 11:30 AM Gravity Wave Interferometers G. Gonzalez
11:30 - 11:45 AM Break
11:45 - 12:45 PM Gravity Wave Interferometers G. Gonzalez
12:45 - 2:15 PM Lunch
2:15 - 3:00 PM GR Test Using Laser and Radio Ranging Experiments K. Nordtvedt
3:00 - 3:45 PM LISA S. Larson
4:00 - 6:00 PM Discussion Session
6:00 PM Dinner
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Wednesday, July 27
Chairman T. Kamae
9:00 - 10:00 AM Gravitational Radiation A. Buonanno
10:00 - 10:30 AM Refreshment Break
10:30 - 11:30 AM General Relativity Tests with Pulsars I. Stairs
11:30 - 11:45 AM Break
11:45 - 12:45 PM Polarization in CMBR S. Church
12:45 PM - 2:15 PM Lunch
2:15 - 3:00 PM Gravitational Wave Detection with Pulsars D. Backer
3:00 - 3:45 PM Tests of Alternative Theories of Gravity G. Esposito-Farese
4:00 - 6:00 PM SLAC Tour
6:00 PM Social Hour
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Thursday, July 28
Chairman C. Prescott
9:00 - 10:00 AM Black Holes S. Hughes
10:00 - 10:30 AM Refreshment Break
10:30 - 11:30 AM Black Holes S. Hughes
11:30 - 11:45 AM Break
11:45 - 12:45 PM Neutron Stars J. Lattimer
12:45 - 2:15 PM Lunch
2:15 - 3:00 PM Role of Supermassive Black Holes in Structure Formation T. Di Matteo
3:00 - 3:45 PM Gamma Ray Bursts seen by SWIFT D. Burrows
4:00 - 6:00 PM Discussion Session
6:00 PM Poster Session
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Friday, July 29
Chairman J. Hewett
9:00 - 10:00 AM Extreme Neutron Stars C. Thompson
10:00 - 10:30 AM Refreshment Break
10:30 - 11:30 AM Neutron Stars J. Lattimer
11:30 - 11:45 AM Break
11:45 - 12:45 PM Observations of Black Holes A. Fabian
12:45 - 2:15 PM Lunch
2:15 - 3:00 PM Black Holes in the Galactic Center E. Quataert
3:00 - 3:45 PM GLAST-Large Area Telescope E. do Couto e Silva
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Monday, August 1
Chairman J. Jaros
9:00 - 10:00 AM Unifying the Forces K. Dienes
10:00 - 10:30 AM Refreshment Break
10:30 - 11:30 AM Extra Dimensions R. Sundrum
11:30 - 11:45 AM Break
11:45 - 12:45 PM Proton Decay CK Jung
12:45 - 2:15 PM Lunch
2:15 - 3:00 PM Black Holes at Accelerators B. Webber
3:00 - 3:45 PM Precision SUSY and the GUT Scale G. Blair
4:00 - 6:00 PM Discussion Session
6:00 PM Social Hour
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Tuesday, August 2
Chairman T. Kamae
9:00 - 10:00 AM Unifying the Forces K. Dienes
10:00 - 10:30 AM Refreshment Break
10:30 - 11:30 AM Extra Dimensions R. Sundrum
11:30 - 11:45 AM Break
11:45 - 12:45 PM Extra Dimension Searches at Accelerators T. Berry
12:45 - 2:15 PM Lunch
2:15 - 3:00 PM Tests of Gravity at the Millimeter Scale and Below J. Long
3:00 - 3:45 PM SUSY Searches at the Tevatron M. Schmitt
4:00 - 6:00 PM Discussion Session
6:00 PM Poster Session
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Wednesday, August 3
Chairman J. Hewett
9:00 - 10:00 AM String Cosmology E. Silverstein
10:00 - 10:30 AM Refreshment Break
10:30 - 11:30 AM Extra Dimensions R. Sundrum
11:30 - 11:45 AM Break
11:45 - 12:45 PM Probing Dark Matter Using Gravitational Lensing P. Natarajan
12:45 - 2:15 AM Lunch
2:15 - 3:00 PM News from SDSS R. Scranton
3:00 - 3:45 PM Results from Auger J. Beatty
4:00 - 6:00 PM SLAC Tour
6:00 - 8:30 PM Soccer Game
-- return to top --
Thursday, August 4
Chairman J. Jaros
9:00 - 10:00 AM String Theory for Physicists J. Lykken
10:00 - 10:30 AM Refreshment Break
10:30 - 11:30 AM String Theory for Physicists J. Lykken
11:30 - 11:45 AM Break
11:45 - 12:45 PM Cosmological Constant S. Kachru
12:45 - 2:15 PM Lunch
2:15 PM - 3:00 PM Probing Dark Matter at Colliders A. Birkedal
3:00 - 3:45 PM LSST S. Kahn
4:00 - 6:00 PM Discussion Session
6:00 PM Dinner
-- return to top --
Friday, August 5
Chairman T. Kamae
9:00 - 10:00 AM The Gravity of Dark Energy R. Kolb
10:00 - 10:30 AM Refreshment Break
10:30 - 11:30 AM String Theory for Physicists J. Lykken
11:30 - 11:45 AM Break
11:45 - 12:45 PM Beyond Einstein: Embarking on the Second Century of Relativity R. Kolb

Một trang web về các thông tin mới cũng như các trường học trong nước cũng như nước ngoài về vật lý hiện đại mà các bạn có thể đăng ký tham dự.
http://interactions.org/cms/

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