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Overview speakers and their literature recommendations THEPschools 1987 onward 2013: Wim Beenakker (RU): SUSY phenomenology in the era of the LHC This course provides an introduction to the basic aspects of supersymmetric (SUSY) phenomenology. It covers the general structure of the minimal SUSY extension of the Standard Model, the issue of soft SUSY breaking and the translation of the SUSY parameter spectrum from the high-energy scale where the theory is formulated down to the energy scales of present-day LHC experiments. In the last part of the course the experimental implications of this "low-energy" parameter spectrum and the impact of a 125 GeV Higgs boson will be discussed. On top of that it will be sketched how renormalization-group invariants could be used to derive information on the highenergy theory from low-energy (LHC) data. Before the course starts the participants are recommended to refresh their Standard Model knowledge. Reading suggestions for the lecture course: "A Supersymmetry Primer", Stephen P. Martin, arXiv:hep-ph/9709356v6 http://arxiv.org/abs/hep-ph/9709356v6 "Supersymmetry and the MSSM: An Elementary introduction" Ian J.R. Aitchison, arXiv:hep-ph/0505105v1 http://arxiv.org/abs/hep-ph/0505105v1 Renate Loll (RU): Introduction to quantum gravity In these lectures, you will learn some basics about quantizing gravity, which is one of the outstanding challenges of theoretical high-energy physics. Building on your knowledge of quantum field theory (at the level of a first-year master course in the subject), we will first study the perturbative path integral for gravity, highlighting the differences with other field theories, and then learn about how one may think of constructing and solving a nonperturbative gravitational path integral." Literature: "There is not yet a good textbook on the subject, which would be suitable for teaching a course. What comes closest, certainly in terms of giving a comprehensive overview, is the book "Quantum Gravity" by C. Kiefer (Oxford University Press). If you are seriously interested in the subject, this is a good investment. You may also consult the review article "Quantum gravity: a progress report", by S. Carlip [arxiv: gr-qc/0108040], or the more recent "How far are we from the quantum theory of gravity?" by R. Woodard [arxiv: 0967.4238] for general background." Kyriakos Papadodimas (RUG): Introduction to AdS/CFT and its applications The outline of this course will be (literature to follow): -Part 1, Background: Confinement in gauge theories, large N expansion, black holes and the holographic bound; -Part 2, Derivation and main statement of AdS/CFT: why quantum gravity/string theory in AdS is equivalent to a lower dimensional gauge theory, matching of parameters and symmetries; -Part 3, How to compute correlation functions, relation between black holes in AdS and quark-gluon plasma; -Part 4, Applications to QCD, condensed matter, black holes and cosmology PDF slides John van Opstal (Donders Institute, RU Nijmegen): Optimal control of eye movements by the brain A major challenge in computational neuroscience and neurobiology is to understand how populations of noisy, broadly-tuned neurons in the brain can produce accurate goal- 1 directed actions, such as the fast eye movements called saccades. In my talk I will present a line of work from my group that links neurophysiological data from singlecell recordings in the rhesus monkey midbrain, to a neurocomputational model that explains how this structure programs saccadic eye movements. I will first explain why humans (and other primates) have to make saccades (we change our gaze about three times per second, throughout the day), and which problems the brain has to overcome in order to program and execute them efficiently. I will then briefly describe the properties of saccades, such as their stereotyped, nonlinear kinematics, their asymmetric velocity profiles, and the signal-dependent noise in the system, and present a simple cybernetic control scheme of the saccadic system. This scheme also specifies how populations of neurons in the midbrain are thought to encode saccades within a complex-logarithmic mapping of the sensory-motor world. Earlier models of the saccadic system have explained the nonlinear saccade properties by assuming passive nonlinear elements at a late stage of the neural circuitry. More recent neuroscience theories, however, have suggested that these characteristics may rather reflect a deliberate active strategy by the neural circuitry that is designed to optimize the speed-accuracy trade off of saccades.Yet, how the brain could implement such a strategy has so far remained elusive. I here demonstrate how the midbrain is in an ideal position to implement such an optimal strategy through the spatial-temporal dynamics of its neural population activity. Interestingly, our model is entirely linear and surprisingly simple (only two free parameters). Simulations (Goossens & Van Opstal, PLoS Computational Biology, 2012) show that the recorded activity patterns can fully account for all observed kinematic nonlinearities and spatial trajectories of saccades. John van Opstal Radboud University Nijmegen Donders Institute for Brain, Cognition and Behaviour Dept. Biophysics - Neurophysics Unit Heyendaalseweg 135, HG00.831 6525 AJ Nijmegen, NL tel.: (+31) 243 614 251 fax: (+31) 243 653 450 E-mail: [email protected] web: www.mbfys.ru.nl/~johnvo 2012: Christophe Grojean (CERN): Electroweak symmetry breaking and physics beyond the standard model Summary: It is often said that the Higgs boson is at the origin of the masses of all elementary particles. Actually, these masses are only controlled by the order parameter that measures the breaking of electroweak symmetry while the Higgs boson is only one possible, admittedly very appealing and simple, UV completion describing this symmetry breaking. In these lectures, I shall describe why new physics beyond the degrees of freedom already observed must exist and why most people believe that a single Higgs boson is unlikely to be the only particle populating the TeV scale. I shall argue that it might not even exist or that it might take a different form that the one predicted by the Standard Model. Recommended literature: Introductory material: - R. Barbieri "Ten lectures on the electroweak interactions" http://arXiv.org/abs/arXiv:0706.0684 - C. Grojean "New theories for the Fermi scale" http://arXiv.org/abs/arXiv:0910.4976 - S. Rychkov "EWSB Theory on the Eve of Higgs Boson Exclusion/Discovery" http://arXiv.org/abs/arXiv:1109.1180 - J. Lykken "Beyond the Standard Model" 2 http://arxiv.org/abs/1005.1676 as part of http://arxiv.org/abs/1012.4643 More technical material: - R. Contino "The Higgs as a Composite Nambu-Goldstone Boson" http://arXiv.org/abs/arXiv:1005.4269 - C. Grojean "New approaches to electroweak symmetry breaking" Phys.Usp. 50 (2007) 135 - T. Plehn "Lectures on LHC Physics" http://arxiv.org/abs/0910.4182 - M. Bustamante, L. Cieri, John Ellis "Beyond the Standard Model for Montaneros" http://arxiv.org/abs/0911.4409 as part of http://arxiv.org/abs/1010.5976 Elisabetta Pallante (RUG): Effective field theories In modern field theoretical language, a field theory can a priori be thought as an effective field theory, meaning that it provides a good description of a class of phenomena for a certain range of energies, distances or number of dimensions. In these lectures we first review basic concepts of renormalization on which the construction of any effective field theory is based: this includes dimensional analysis, criteria for renormalizability and Wilson’s approach to the renormalization group. We then consider three applications relevant for today’s high energy physics: the case of strong interactions at strong coupling, the case of electroweak interactions from high to low energy, and the case of theories with extra dimensions (compactification, Kaluza-Klein modes). There is a vast literature on effective field theories and applications. A selection is provided below. An 1. 2. 3. 4. 5. introduction to the general concepts can be found in various textbooks: S. Weinberg, The Quantum Theory of Fields, Volume I, Chapter 12 and Volume II M. Srednicki, Quantum Field Theory, Chapter 29 Peskin & Schroeder, Introduction to Quantum Field Theory, Chapter 8 J. Collins, Renormalization, Cambridge Monographs on Mathematical Physics K. Costello, Renormalization and Effective Field Theory, AMS 2011 A selection of lectures and reviews on applications of EFT: 1. A. Pich, Effective Field Theory, arXiv:hep-ph/9806303v1 (Les Houches 1997) 2. D.B. Kaplan, Five lectures on Effective Field Theory, arXiv:nucl-th/0510023v1 3. H. Georgi, Effective Field Theory, at http://www.people.fas.harvard.edu/~hgeorgi/review.pdf 4. E. Pallante, The Many Uses of Chiral Effective Theories, arXiv:0803.2347v1 [hep-ph] 5. M.J. Duff, Kaluza-Klein Theory in Perspective, arXiv:hep-th/9410046v1 6. T. Gherghetta, TASI Lectures on a Holographic View of Beyond the Standard Model Physics, arXiv:1008.2570v1 [hep-ph] Some original articles: 1. S. Weinberg, Phenomenological Lagrangians, Physica A 96 (1979) 327-340. 2. J. Gasser, H. Leutwyler, Chiral Perturbation Theory: Expansions in the Mass of the Strange Quark, Nucl. Phys. B250 (1985) 465. 3. J. Gasser, H. Leutwyler, Chiral Perturbation Theory to One Loop, Annals Phys. 158 (1984) 142. 4. J. Scherk, J.H. Schwarz, How to get Masses from Extra Dimensions, Nucl. Phys. B 153 (1979) 61. Handout Problem Session EFT Jan-Pieter van der Schaar (UvA): Quantum field theory in the early universe In these lectures, that include 3 problem sessions, I will address the implications of quantum field theory in cosmological spacetimes, with an emphasis on inflationary cosmology. To begin I will introduce and analyze quantum fields on De Sitter space, followed by a treaty on (slow-roll) inflation and the mechanism responsible for the generation of density fluctuations. After having introduced inflation and its properties I will outline problems with cosmological inflation from the point of view of effective field theory. This includes the UV sensitivity of models of inflation, but also the IR issues that arise when considering the "eternal inflation" limit. Finally, in the context of eternal inflation and the multiverse hypothesis I will discuss the idea of bubble nucleation in a false inflationary vacuum, reviewing the 3 Coleman-De Luccia instanton calculation. I will end with an overview and remaining challenges for future research. Literature: Mix of (parts of) textbooks, papers and lecture notes. Erik Verlinde (UvA):Emergent gravity: from strings and black holes to dark energy and dark matter The aim of these lectures is to explain the general principles behind the emergence of gravity, and show how these ideas can be relevant for the understanding of dark matter and dark energy. I begin a review of D-brane dynamics and basic aspects of open closed string duality. Next I will explain the role of Matrix quantum mechanics in string theory and M-theory. A second ingredient is black hole thermodynamics, which will also be briefly reviewed. The microscopic description of black holes in string theory is then used to motivate a general scenario for the emergence of gravity. The possible applications to cosmology, with new insights into the nature of dark matter and dark energy is described in the last lectures. In the first lecture we begin with a review of Polchinski's D-brane paper" Dirichlet Branes and Ramond-Ramond charges" http://arxiv.org/pdf/hep-th/9510017.pdf Additional reading material will be provided during the course. Evening speakers: Karla de Bruin (Netherlands Forensic Institute): Physics in forensic science In this talk, I will first give an overview of the work that is done at the NFI in general, and then more specific on bloodstain pattern analysis. Currently, at crime scenes the flight path of a blood drop is assumed to be a straight line. This neglection of gravity and air resistance may lead to an error of 45 cm in height estimation. In order to find a better model of the flight path we used high speed imaging to study the blood drop's flight. For unambigous assignment of the trajectory to a bloodstain, four parameters have to beknown: volume, impact velocity impact angle and impact position. In cooepration with the soft matter group at the UvA, methods are developed to estimate these three parameters from the bloodstain at a crime scene. By means of these methods murder and self-defence may be distinguished. David Norris (Donders Institute for Brain Cognition and Behaviour, RU Nijmegen): The imaging of position, velocity and displacement with magnetic resonance imaging: from the motion of sea water to tracking the fibres of the living brain. The phenomenon of nuclear magnetic resonance has found widespread application in almost all branches of natural science. However, its most widespread use has undoubtedly been in bio-medical imaging. MRI systems are distinguished from spectrometers in requiring pulsed magnetic field gradients along three orthogonal axes. With these it is possible to spatially encode the MR signal, and also by using specialised techniques to encode also the temporal derivatives of position as well as displacement. In this talk I shall give a brief historical overview as to how ideas on imaging stationary and moving spins have developed, and illustrate these with examples from latter day practice in imaging, angiography and diffusion. To conclude I will give a few examples as to how diffusion weighted imaging is helping us better understand the relationship between structure and function in the brain. 2011 (Brazil): Rosenfeld and Sorella: http://www.sbfisica.org.br/~evjaspc/xvi/index.php?option=com_content&view=article&id= 9&Itemid=12 Gustavo Burdman (USP-São Paulo): generation New strong interactions at the TeV scale: the next Jan de Boer (Amsterdam): Topics in AdS-CFT 4 Bernard de Wit (Utrecht): Lessons learned from BPS black holes Francis Halzen (Wisconsin): Astroparticles and cosmology Eric Laenen (Nikhef/Amsterdam/Utrecht): All-order aspects of QCD Lecture contents: 1. Partons, factorization and evolution a) Factorization theorem, DGLAP evolution b) Stochastic evolution: parton showers, event generation 2. Infrared and collinear divergences in QCD a) Eikonal approximation b) Power counting c) Ward identities, factorization 3. Resummation a) All-order matrix elements and phase space b) Examples of resummed cross sections: Drell-Yan, Higgs, event shapes 4. Some new developments a) Soft-collinear effective theory b) Soft anomalous dimensions c) Webs: diagrams and path integrals Background literature: - G. Sterman, Introduction to Quantum Field Theory, CUP, Ch. 12, 13 & 14 - Ellis, Stirling, Webber; QCD and Collider Physics, CUP, Chapter 5 - E. Laenen, Pramana 63 - Lecture notes at school George Matsas (IFT/UNESP): Chris Quigg (FERMILAB): Low energy quantum effects in gravity Potential discoveries at the LHC Peter van Nieuwenhuizen (Stony Brook): Renormalization and unitarity of gauge theories Lecture contents: 1. BRST symmetry of gauge theories 2. Renormalization of unbroken gauge theories a) BRST Ward identities (Gamma-Gamma equations) for proper graphs b) Divergences allowed by BRST symmetry c) Divergences allowed by power counting d) Renormalization of unbroken gauge theories 3. Renormalization of spontaneously broken gauge theories a) SU(2) Goldstone model b) Spontaneously broken SU(2) Higgs model c) Renormalizability of the SU(2) Higgs model 4. Unitarity from the cutting rules a) Unitarity for spin 0 and 1/2 (the largest time equation) b) BRST Ward identities for connected graphs c) Analysis of divergences d) Unitarity of the renormalized theory Background literature: - G.'t Hooft and M. Veltman, Diagrammar - M. Veltman, Diagrammatica, CUP. Edward Witten (IAS - Princeton): A new look at the path integral of quantum mechanics Opening seminar by E. Witten: String theory and the universe 2010: W. Beenakker (RU): Introduction to SUSY phenomenology This course provides an introduction to the basic aspects of supersymmetric (SUSY) phenomenology. It covers the general structure of the minimal SUSY extension of the Standard Model, the issue of soft SUSY breaking and the translation of the SUSY parameter spectrum from the high-energy scale where the theory is formulated down to the energy scales of present-day experiments. In the last part of the course the experimental implications of this "low-energy" parameter spectrum will be discussed. 5 Reading suggestions: before the course starts the participants are recommended to refresh their Standard Model knowledge. At a later stage, some useful reviews for further reading are hep-ph/9709356 and hep-ph/0505105. R. Britto (Saclay): Scattering amplitudes in gauge theories Reading list: Witten: Perturbative gauge theory as a string theory in twistor space, hep-th/0312171 Sections 1-3 Dixon: Calculating scattering amplitudes efficiently, hep-ph/9601359 Bern, Dixon, Kosower: On-shell methods in perturbative QCD, arXiv:0704.2798 B. Craps (VUB Brussels): Holography and cosmology The course will focus on holography (in particular the AdS/CFT correspondence) and applications to cosmology (in particular the study of cosmological singularities). First, the importance of UV complete models for the study of the very early universe will be stressed, and the study of the big bang singularity motivated. Then, the basic ingredients of the AdS/CFT correspondence will be introduced: (super)gravity in anti-de Sitter (AdS) space (including a preview of "AdS cosmology"), the N=4 superYang-Mills conformal field theory, and D-branes, which provide the link between the two. Next, the AdS/CFT correspondence will be formulated, including a discussion of the AdS/CFT dictionary and the UV/IR correspondence. The remaining lectures will introduce concepts and techniques useful for the study of AdS cosmologies (but also more generally). These include propagators, scalar fields in AdS, boundary conditions in AdS and (multi-trace) deformations of CFTs, Coleman-De Luccia instantons, and self-adjoint extensions. The exercises will illustrate many concepts in the lectures, in particular D-brane actions, boundary conditions and propagators for scalar fields in AdS, and multitrace deformations. The aim will be to compute the quantum effective potential for spherical D-branes in AdS with boundary conditions corresponding to multi-trace deformations. Required reading before the course: A basic discussion of big bang cosmology and slow-roll inflation. If you know what slow-roll parameters are, you probably know enough for this course; otherwise, it is recommended that you read for instance the first 18 pages of Liddle's lectures http://arxiv.org/abs/astro-ph/9901124. Recommended reading before the course: It is recommended that you read pages 1-20 of Maldacena's TASI 2003 lectures on AdS/CFT, hep-th/0309246. Parts of this material will be discussed in the course, but it will be helpful to have been exposed to it before. Depending on your background, some parts will be easier to read/digest than others, but most likely everyone will get something out of it. If you would like a more elaborate pedagogical introduction to large N field theories, lecture 8 in Coleman's book "Aspects of symmetry", Cambridge University Press (1985) is highly recommended. A basic discussion of big bang cosmology and slow-roll inflation. If you know what slow-roll parameters are, you probably know enough for this course; otherwise, it is recommended that you read for instance pages 2-14 of Marieke Postma's lecture notes from last year's school, http://www.nikhef.nl/~mpostma/inflation.pdf, or the first 18 pages of Liddle's lectures http://arxiv.org/abs/astro-ph/9901124. Other references: *For more details on the ingredients and formulation of the AdS/CFT correspondence, a good starting point is the review by Aharony, Gubser, Maldacena, Ooguri & Oz, hepth/9905111. Look here if you find anything in Maldacena's TASI 2003 lectures too compact. *For AdS cosmologies, see Hertog & Horowitz, hep-th/0406134. *The lecture on D-brane actions will be based on the presentation in Craps, hepth/0004198, pages 80-86. *Useful references on propagators in AdS include Dullemond & Van Beveren, J. Math. Phys. 26 (8), 1985; Allen & Jacobson, CMP 103, 669 (1986); and Burgess & Lutken, PLB 153 (3) 137 (1985). *For more on self-adjoint extensions, see for instance Carreau, Farhi, Gutmann & Mende, Annals Phys.204:186-207, 1990. *The exercises will in part be based on some of the computations behind Bernamonti & Craps, arXiv: 0907.0889. Y. Levin (UL): Supermassive black holes I will discuss black holes from a point of view of an astrophysicist. In particular, 6 I will present observational phenomenology and outline outstanding issues in theoretical astrophysics of supermassive black holes. B. Schellekens (Nikhef/RU): The emperor's last clothes? Once upon a time string theorists believed that they were going to derive the Standard Model uniquely. This turned out to be a fairy tale. I will discuss why the expectations were wrong, and will discuss the current status of string theory in the light of realistic expectations. The anthropic principle, deeply hated by many physicists, plays an inevitable and scientifically justifiable role in this context. Based on Rept. Prog. Phys. 71: 072201, 2008 (e-Print: arXiv: 0807.3249) S. Vandoren (UU): Non-perturbative effects in classical and quantum field theory In these lectures, we discuss instantons in (super) Yang-Mills theory in four dimensions and in quantum mechanics. First the basics are derived from scratch: the regular and singular one-instanton solutions for Yang-Mills theories with gauge groups SU(2) and SU(N), their bosonic and fermionic zero modes, the path integral instanton measure, and supersymmetric Yang-Mills theories in Euclidean space. Then we discuss applications: the theta-angle of QCD, the solution of the U(1) problem, the way Higgs fields solve the large-instanton problem, and tunneling and phase transitions in quantum mechanics and in nonabelian gauge theories. If time permits, we also discuss instantons in gravity and string theory. References: arXiv: 0802.1862; hep-th/0004186 2009: E. Bergshoeff (RUG): Introduction to supersymmetry This course provides an introduction into the basics of supersymmetry. It starts with supersymmetric quantum mechanics and it ends with the supersymmetric Wess-Zumino model. This course is self-contained. For an in-depth discussion of the supersymmetry literature see the blog website: http://fliptomato.wordpress.com/2008/03/20/supersymmetry-literature-for-theperplexed/ J.-S. Caux (UvA): Transmutation and fractionalization, or when 1 plus 1 isn't simply 2 Many-body systems can sometimes display one of the most surprising quirks of nature, whereby the constituent fundamental particles can be superseded by collective excitations of an altogether different nature. These excitations carry very specific signatures of nonperturbative effects, and are actively studied both from the experimental and theoretical side. Important examples occur in quasi-1D magnetic systems, in which inelastic neutron scattering allows the characterization of fractionalized spinons, and also in systems of cold atoms in optical lattices, which offer a brand new way of realizing tunable toy models of quantum condensed matter. On the theory side, many methods having close connections with high-energy physics can be used to gain important insights and provide quantitative phenomenology. This talk, aimed at non-condensed matter physicists, will highlight some of the recent developments in this area. M. Postma (Nikhef): Inflationary cosmology These lectures give an introduction to cosmic inflation. In the first part I'll review big bang cosmology, and outline the motivations for inflation. The second part is devoted to the theory of cosmological perturbations generated during inflation, which are thought to be the origin of all structure in the universe. Finally, in the third part, I'll discuss some inflation models motivated by particle physics. This course is self-contained. Some useful reviews of inflation are: hep-ph/9807278, hep-ph/0210162, arXiv: 0708.2865. V. Rychkov (SNS, Pisa): Beyond the standard model at the LHC Does the Higgs boson exist? Is the world supersymmetric above a TeV? Are new strong interactions responsible for the electroweak symmetry breaking? Such and related questions will receive a definite answer at the Large Hadron Collider. In these lectures we will discuss the three main scenarios for the LHC physics beyond the Standard Models, concentrating on their characteristic features and experimental signals. These are Supersymmetry, Higgs as a pseudo-Goldstone boson, and Higgsless models. Prerequisites and indications for literature: 7 0) The Standard Model basics. Do you know the mass of the top quark? How the Z boson decays? If not, please refresh your memory by looking up all Standard Model particles, their masses and main decay channels at the Particle Data Group http://pdg.lbl.gov/ "Summary Tables" -> Gauge and Higgs bosons, Leptons, and Quarks. 1) Electroweak phenomenology. Look at Particle Data Group http://pdg.lbl.gov/ "Reviews, Tables, Plots" -> Standard Model and related topics -> the Electroweak model, Cabibbo-Kobayashi-Maskawa matrix Alternatively, study R. Barbieri "10 lectures on electroweak interactions", http://arxiv.org/abs/0706.0684v1 (go to v1 to access the file) 2) Collider physics. hep-ph/0508097 is a good review of the basics. K. Schalm (UL): Strings and strongly coupled gauge theory G. 't Hooft (UU): The CKM matrix: a question of flavor The latest Nobel Prizes were for three elementary particle physicists of Japanese origin, Y. Nambu, M. Kobayashi and T. Maskawa. The first stood at the basis of the development of the Englert-Brout-Higgs theory for spontaneous symmetry breakdown in particle physics. The last two made an essential step by casting the coupling between the Higgs field and the quarks in the form of a matrix. This matrix not only describes the masses and the weak interaction parameters of the quarks, thus defining their "flavor" properties, but also allows for one effect that is not symmetric under CP, the combination of a parity inversion and the replacement particle-antiparticle. This gave an elegant explanation of CP violation in the weak interactions, provided that the matrix was at least three dimensional. It turned out to be the first hint for the existence of a third generation of quarks and leptons. Careful analysis of the relation between this matrix and experimental data is used to investigate whether the Standard Model of the Subatomic Particles, as it is known today, needs to be extended. 2008: A. Achúcarro (UL): Cosmology with strings attached R. Harlander: Higgs physics at higher orders Different methods for the evaluation of higher order corrections in Quantum Field Theory are introduced. Beginning with standard techniques for 1-loop integrals, we move on to exact approaches to the multi-loop case. In particular, this involves the Integration-by-Parts method and its modern implementations. On the other hand, we explain approximation techniques like asymptotic expansions. All these methods are discussed in the background of applications to high energy particle colliders, in particular to Higgs physics at the Large Hadron Collider and a future Linear Collider. * Feynman Integral Calculus, V.A. Smirnov, Springer 2006 * Integration by Parts: The Algorithm to Calculate Beta Functions in 4 Loops, K. Chetyrkin, F. Tkachov, Nucl. Phys. B192:159-204, 1981 * Asymptotic Expansions: Methods and Applications, R. Harlander, Acta Phys. Polon. B30:3443-3462, 1999 (hep-ph/9910496) D. Litim: Functional renormalisation group and applications The course provides a pedagogical introduction into modern functional renormalisation group methods for quantum field theory. Applications cover the physics of phase transitions and critical phenomena, finite temperature field theory, gauge theories, and quantum gravity. * Introduction to Quantum Field Theory, Peskin/Schroeder, Chapter 12: The Renormalisation Group. See also Daniel's website: http://www.pact.cpes.sussex.ac.uk/~dl79/winterschool08.html H. Stoof (UU): About ultracold fermi gases and neutron stars M. Taylor (UvA): Black objects in string theory This course will give an introduction to recent progress in string theory on understanding the properties of black holes. In particular, we will see that string theory can explain microscopically the entropy of black holes, and that it gives suggestions for the resolution of the black hole information loss paradox. * The first part of the course will focus on black holes in general relativity. A 8 useful reference would be chapter 7 of Sean Carroll's lecture notes, available as the preprint gr-qc/9712019, or the black hole chapters of his textbook Spacetime and Geometry: an Introduction to General Relativity. * For the second part of the course, the first part of chapter 12 of Elias Kiritsis' book String Theory in a Nutshell would be useful. Note however that necessary background material in string theory will be covered by the course. R. Timmermans (RUG/KVI): Precision tests of the standard model 2007 (Brazil): R. Forty (CERN): Physics challenges of the LHC G. 't Hooft (UU): Feynman rules and unitarity * The Conceptual Basis of Quantum Field Theory, (2007 version) G. 't Hooft, http://www1.phys.uu.nl/drstp/Postgr.courses/THEP/2007Brazil/conceptual%20basis.pdf Y. Nomura (UC Berkeley): Beyond the standard model H. Ooguri (Caltech): Topological string theory T. Plehn (Munich): Collider phenomenology K. Skenderis (UvA): Introduction to AdS-CFT * Large N Field Theories, String Theory and Gravity, O. Aharony, S.S. Gubser, J. Maldacena, H. Ooguri, Y. Oz (hep-th/9905111), http://arxiv.org/abs/hep-th/9905111 * Supersymmetric Gauge Theories and the AdS/CFT Correspondence, Eric D'Hoker, Daniel Z. Freedman (hep-th/0201253), http://arxiv.org/abs/hep-th/0201253 * Lecture Notes on Holographic Renormalization, Kostas Skenderis (hep-th/0209067), http://arxiv.org/abs/hep-th/0209067 * AdS/CFT Correspondence and Geometry, Ioannis Papadimitriou and Kostas Skenderis (hep-th/0404176), http://arxiv.org/abs/hep-th/0404176 J. Smit (UvA/UU): Finite-temperature field theory * Finite-temperature field theory, principles and applications, Joseph I. Kapusta and Charles Gale, Cambridge Monographs on Mathematical Physics, second edition 2006, Cambridge University Press (ISBN-13: 978-0521820820, ISBN-10: 0521820820) * Thermal field theory, Michel Le Bellac, Cambridge Monographs on Mathematical Physics, 1996, paperback edition 2000, Cambridge University Press (ISBN-13: 9780521654777, ISBN-10: 0521654777) * An Introduction to Real- and Imaginary-Time Thermal Field Theory, Ch.G. van Weert S. Sorella (UERJ): Issues on the quantization of Yang-Mills theories J. Takahashi (UNICAMP/São Paulo): Relativistic heavy ions: probing the big bang at the LHC B. de Wit (UU): Introduction to AdS-CFT * Supersymmetric Black Holes, B. de Wit (hep-th/0511261), http://arxiv.org/abs/hepth/0511261 * Black Hole Entropy Functions and Attractor Equations, G.L. Cardoso, B. de Wit and S. Mahapatra (hep-th/0612225), http://arxiv.org/abs/hep-th/0612225 * Black Hole Partition Functions and Duality, G.L. Cardoso, B. de Wit, J. Käppeli and T. Mohaupt (hep-th/0601108), http://arxiv.org/abs/hep-th/0601108 2006: G. Arutyunov (UU): Introduction to AdS/CFT * Large N Field Theories, String Theory and Gravity, O. Aharony, S.S. Gubser, Maldacena, H. Ooguri and Y. Oz, Phys. Rept. 323 (2000) 183 (hep-th/9905111) J.M. D. Boer (VUA): QCD 9 K. Jungmann (KVI, RUG): Precision tests of the standard model * Physics with Low-Energy Muons at a Neutrino Factory Complex, J. Aysto et al. (hep-ph/0109217) * Fundamental Symmetries and Interactions, K. Jungmann, Nucl. Phys. A751 (2005), pp. 87-106 and (nucl-ex/0502012) * Electric Dipole Moments of Charged Particles, P.G.H. Sandars, Contemp. Phys. 42, 97 (2001) * Searches for Permanent Electric Dipole Moments - Some Recent Developments, K. Jungmann (physics/0501154) p. B. Schellekens (Nikhef/UvA): Beyond the standard model * http://idisk.mac.com/aschellekens-Public/BSM.pdf J.-W. van Holten (Nikhef,/UvA): Black holes, compact stars and gravitational waves * Gravitational Waves and Black Holes, Fortschr. Phys. 45 (1997) p. 439 * General Relativity, R.M. Wald, University of Chicago Press (1984) * Gravitation Freeman, Ch. Misner, K. Thorne and J.A. Wheeler, (San Francisco, 1973) * Gravitation and Cosmology, S. Weinberg, J. Wiley (New York, 1972) B. de Wit (UU): Black hole entropy 2005: S. Bais (UvA): To be or not to be: Monopoles in gauge theories G. 't Hooft (UU): Topics in advanced quantum field theory * http://www.phys.uu.nl/~thooft/ T. Prokopec (UU): Inflation, baryogenesis and the CMB spectrum E. Verlinde (UvA): String theory and black holes S. Weinzierl (Max Planck Insitute Munich): Higher-order perturbation theory 2004: S. Bentvelsen (RU): Extra dimensions and black hole production at LHC R. Dijkgraaf (UvA): Supersymmetric gauge theories, strings and matrix models * Supersymmetry and Supergravity, J. Wess and J. Bagger, (ISBN 0691085560, Princeton University Press, 1992) * Lectures on supersymmetric gauge theories and electric-magnetic duality, K. Intriligator and N. Seiberg, Nucl. Phys. Proc. Suppl. 45BC (1996) 1-28, (hep-th/9509066) * An Introduction to Random Matrices, B. Eynard, http://wwwspht.cea.fr/articles/t01/014/publi.ps.gz K. Gaemers (UvA): Neutrino physics * Neutrino Physics, E. Kh. Akhmedov (hep-ph/0001264) * Neutrino Physics (2nd edition), Klaus Winter, Cambridge Monograph (ISBN 0 521 65003 8) * http://www.nu.to.infn.it/ M. Henneaux (ULB, Brussel): BRST-antifield approach to gauge theories: a primer * The Quantum Theory of Fields, vol II, S. Weinberg, chapters 15, 16, 17, 22 * Quantization of Gauge Systems, M. Henneaux and C. Teitelboim, chapters 3, 17, 18 * Physics Reports, G. Barnich, F. Brandt and M. Henneaux, vol. 338: 439-569, 2000 R. Kleiss (RU) /W. 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