BEGIN:VCALENDAR VERSION:2.0 PRODID:-//CERN//INDICO//EN BEGIN:VEVENT SUMMARY:GRID DTSTART;VALUE=DATE-TIME:20040804T120000Z DTEND;VALUE=DATE-TIME:20040804T124500Z DTSTAMP;VALUE=DATE-TIME:20130520T064441Z UID:indico-event-a043086@cern.ch DESCRIPTION:The part of Dr Grey:\nThis talk will introduce the concept of computing Grid\, explain why CERN needs Grid technology\, and provide a br ief overview of the main Grid projects. This talk serves as a background i ntroduction to the following presentation by Markus Schulz concerning the LHC Computing Grid project.\n\n\n\n\n\n\n\n\n\nThe part of Dr Schulz:\nA s hort introduction of computing grid is given. Centered around the problems that a Grid has to solve examples are given how these problems have been solved in the LCG2 production service. Some of the most common commands ar e shown to illustrate how the grid is used from an endusers perspective.\n \n\n\nOrganiser(s): HR-RFA\n\nhttp://indico.cern.ch/conferenceDisplay.py?c onfId=a043086 LOCATION:CERN Main Auditorium URL:http://indico.cern.ch/conferenceDisplay.py?confId=a043086 END:VEVENT BEGIN:VEVENT SUMMARY:ROOT DTSTART;VALUE=DATE-TIME:20050720T081500Z DTEND;VALUE=DATE-TIME:20050720T090000Z DTSTAMP;VALUE=DATE-TIME:20130520T064441Z UID:indico-event-a054049@cern.ch DESCRIPTION:The talk will be a short introduction to the ROOT data analysi s and visualization system\, including a demonstration.Organiser(s): HR-RF ANote:The ROOT web site is available at http://root.cern.ch . Students are strongly encouraged to download the binary files from this web site. The full documentation is also available from this location.\n\nhttp://indico. cern.ch/conferenceDisplay.py?confId=a054049 LOCATION:CERN Main Auditorium URL:http://indico.cern.ch/conferenceDisplay.py?confId=a054049 END:VEVENT BEGIN:VEVENT SUMMARY:Super-conducting magnet technology for particle accelerators and d etectors DTSTART;VALUE=DATE-TIME:20050720T091500Z DTEND;VALUE=DATE-TIME:20050720T100000Z DTSTAMP;VALUE=DATE-TIME:20130520T064441Z UID:indico-event-a054050@cern.ch DESCRIPTION:Superconducting Magnets are today an essential equipment for H EP research. The high magnetic fields attainable by using the current dens ities in the coils of 50-500 A/mm2 allow increasing the bending strength f or charged particles\, enabling to reach higher energy and luminosity of c ircular collider and to have better momentum resolution in particle detect ors. The talk will review the basic properties of superconductivity\, and its fascinating phenomenology\, and will show how it can be used in partic le terms for conductors. Then a review of the main characteristics of the LHC superconducting magnets (both for the accelerator and detectors) will be given. A perspective of future developments for new more powerful accel erators based on very high field magnets will be eventually presented.Orga niser(s): HR-RFANote:Basic academic knowledge of physics and of accelerato rs.\n\nhttp://indico.cern.ch/conferenceDisplay.py?confId=a054050 LOCATION:CERN Main Auditorium URL:http://indico.cern.ch/conferenceDisplay.py?confId=a054050 END:VEVENT BEGIN:VEVENT SUMMARY:The CLIC Concept and Technology for an e+e- Collider at the Energy Frontier DTSTART;VALUE=DATE-TIME:20050727T091500Z DTEND;VALUE=DATE-TIME:20050727T100000Z DTSTAMP;VALUE=DATE-TIME:20130520T064441Z UID:indico-event-a054066@cern.ch DESCRIPTION:After a brief description of a novel CLIC scheme to extend Lin ear Colliders into the Multi-TeV colliding beam energy range\, the main ch allenges and the very promising results already achieved will be presented . The presentation will mainly focus on the Test Facility (CTF3) presently under construction at CERN within a broad collaboration to address the ma in key issues and demonstrate the feasibility of the CLIC technology befor e 2010.Organiser(s): HR-RFA\n\nhttp://indico.cern.ch/conferenceDisplay.py? confId=a054066 LOCATION:CERN Main Auditorium URL:http://indico.cern.ch/conferenceDisplay.py?confId=a054066 END:VEVENT BEGIN:VEVENT SUMMARY:The Higgs Saga at LEP DTSTART;VALUE=DATE-TIME:20050801T071500Z DTEND;VALUE=DATE-TIME:20050801T080000Z DTSTAMP;VALUE=DATE-TIME:20130520T064441Z UID:indico-event-a054073@cern.ch DESCRIPTION:The Higgs Boson plays a crucial role in the Standard Model\, a nd this lecture is about the search for the Higgs at LEP\, especially in t he last year of LEP running\, at the highest e+e- collision energies. The experimental signature for Higgs decays has to be picked out from all the other Standard Model processes. The debate on whether to extend the LEP ru nning after a hint of Higgs events was seen gave a nail biting finish to t he LEP programme.Organiser(s): HR-RFANote: The lecture will be much easier to understand for students who have followed courses on the Standard Mode l and on experimental techniques. However\, I will give a reminder of the existing constraints on the Higgs mass\, and will explain the main product ion and decay channels\, the experimental techniques used to pick out Higg s decays (especially b tagging) and the statistical methods used to assess the significance of the event sample selected.\n\nhttp://indico.cern.ch/c onferenceDisplay.py?confId=a054073 LOCATION:CERN Main Auditorium URL:http://indico.cern.ch/conferenceDisplay.py?confId=a054073 END:VEVENT BEGIN:VEVENT SUMMARY:Gravitation Waves DTSTART;VALUE=DATE-TIME:20050804T091500Z DTEND;VALUE=DATE-TIME:20050804T100000Z DTSTAMP;VALUE=DATE-TIME:20130520T064441Z UID:indico-event-a054085@cern.ch DESCRIPTION:We will present a brief introduction to the physics of gravita tional waves and their properties. We will review potential astrophysical sources of gravitational waves\, and the physics and astrophysics that can be learned from their study. We will survey the techniques and technologi es for detecting gravitational waves for the first time\, including bar de tectors and broadband interferometers\, and give a brief status report on the international search effort\, with special emphasis on the LIGO detect ors and search results.Organiser(s): HR-RFANote: The talk will be in the f orm of a university physics colloquium\, accessible to second-year undergr aduate physics students.\n\nhttp://indico.cern.ch/conferenceDisplay.py?con fId=a054085 LOCATION:CERN Main Auditorium URL:http://indico.cern.ch/conferenceDisplay.py?confId=a054085 END:VEVENT BEGIN:VEVENT SUMMARY:The GRID DTSTART;VALUE=DATE-TIME:20050809T091500Z DTEND;VALUE=DATE-TIME:20050809T100000Z DTSTAMP;VALUE=DATE-TIME:20130520T064441Z UID:indico-event-a054094@cern.ch DESCRIPTION:The LHC has chosen Grid technology for the storage and analysi s of the data from the LHC. This lecture will introduce the Grid computing model that CERN and its partners worldwide are implementing in the LHC Co mputing Grid project (LCG). The lecture will also describe how this techno logy is already being applied to support Grid computing in other scientifi c domains through the Enabling Grids for E-sciencE project (EGEE)\, and ho w industry is getting involved through the CERN openlab partnership.Organi ser(s): HR-RFANote: Students are invited to browse the GridCafe website (w ww.gridcafe.org) for a general introduction to Grid technology.\n\nhttp:// indico.cern.ch/conferenceDisplay.py?confId=a054094 LOCATION:CERN Main Auditorium URL:http://indico.cern.ch/conferenceDisplay.py?confId=a054094 END:VEVENT BEGIN:VEVENT SUMMARY:The ILC Story DTSTART;VALUE=DATE-TIME:20050811T091500Z DTEND;VALUE=DATE-TIME:20050811T100000Z DTSTAMP;VALUE=DATE-TIME:20130520T064441Z UID:indico-event-a054095@cern.ch DESCRIPTION:The talk will discuss some of the key technological challenges of the ILC. I will also discuss the political\, socialogical and financia l aspects of such a global project.Organiser(s): HR-RFAMore information: h ttp://blueox.uoregon.edu/~lc/wwstudy/\n\nhttp://indico.cern.ch/conferenceD isplay.py?confId=a054095 LOCATION:CERN Main Auditorium URL:http://indico.cern.ch/conferenceDisplay.py?confId=a054095 END:VEVENT BEGIN:VEVENT SUMMARY:String Theory: Has Einstein's dream come true? DTSTART;VALUE=DATE-TIME:20050812T081500Z DTEND;VALUE=DATE-TIME:20050812T090000Z DTSTAMP;VALUE=DATE-TIME:20130520T064441Z UID:indico-event-a054096@cern.ch DESCRIPTION:After having outlined the difficulties that Einstein and other s have encountered in trying to unify our understanding of macroscopic/cla ssical and microscopic /quantum physics\, I will explain in simple terms h ow the latest particle theory revolution\, string theory\, may finally off er a surprisingly simple realization of these long-standing dreams. Einste in thought that his difficulties stemmed from a clash between the classica l and the quantum. Yet\, paradoxically\, superstrings appear to realize hi s dream thanks to -and not against- quantum mechanics.Organiser(s): HR-RFA Note: Some knowledge of quantum mechanics and special relativity is needed . Having followed previous courses of the school should provide a sufficie nt background.\n\nhttp://indico.cern.ch/conferenceDisplay.py?confId=a05409 6 LOCATION:CERN Main Auditorium URL:http://indico.cern.ch/conferenceDisplay.py?confId=a054096 END:VEVENT BEGIN:VEVENT SUMMARY:Superconducting magnet technology for particle accelerators and de tectors DTSTART;VALUE=DATE-TIME:20060714T081500Z DTEND;VALUE=DATE-TIME:20060714T090000Z DTSTAMP;VALUE=DATE-TIME:20130520T064441Z UID:indico-event-a062848@cern.ch DESCRIPTION:This lecture is an introduction to superconducting magnets for particle accelerators and detectors\, the aim being to explain the vocabu lary and describe the basic technology of modern superconducting magnets\, and to explore the limits of the technology. It will include the followin g:\n- Why we need superconducting magnets\n- Properties of superconductors \, critical field\, critical temperature\n- Why accelerators need fine fil aments and cables\; conductor manufacture\n- Temperature rise and temperat ure margin: the quench process\, training \n- Quench protection schemes. P rotection in the case of the LHC. \n- Magnets for detectors \n- The challe nges of state-of-the-art magnets for High Energy PhysicsPrerequisite Knowl edge:\nOnly a knowledge of basic physics is required References Books:\n- M. Tinkham\, Superconductivity\, Gordon & Breach \n- M. Wilson\, Supercond ucting Magnets\, Clarendon Press Oxford Talk: M. Wilson\, Pulsed Supercond ucting Magnets\, Academic Training\, CERN 2006\nOrganiser(s): HR-RFA\n\nht tp://indico.cern.ch/conferenceDisplay.py?confId=a062848 LOCATION:CERN Main Auditorium URL:http://indico.cern.ch/conferenceDisplay.py?confId=a062848 END:VEVENT BEGIN:VEVENT SUMMARY:Seminar on LHC upgrade DTSTART;VALUE=DATE-TIME:20060719T091500Z DTEND;VALUE=DATE-TIME:20060719T100000Z DTSTAMP;VALUE=DATE-TIME:20130520T064441Z UID:indico-event-a062750@cern.ch DESCRIPTION:This seminar will discuss the future program at the LHC. After the present program will be completed\, when about 300 fb-1 is collected by the experiments\, a simple continuation of the operation of the machine becomes less exciting. Studies are already made for upgrading the LHC\, b eyond its presently expected performance. Two scenarios are will be discus sed: - Upgrading the luminosity by a factor 10\, ie. 10^35 cm-2s-1 - Upgra ding the total energy to 28 TeV\, ie 14 TeV per beam This seminar will dis cuss a possible path for such upgrades and particularly the additional inc rease in physics reach that can be gained with such upgrades. It turns out that for essentially all scenarios of new physics\, the upgrade of the LH C will bring something new.Note: prerequisite knowledge:\nPhysics lectures in the summer student programmeOrganiser(s): HR-RFA\n\nhttp://indico.cern .ch/conferenceDisplay.py?confId=a062750 LOCATION:CERN Main Auditorium URL:http://indico.cern.ch/conferenceDisplay.py?confId=a062750 END:VEVENT BEGIN:VEVENT SUMMARY:ROOT DTSTART;VALUE=DATE-TIME:20060731T081500Z DTEND;VALUE=DATE-TIME:20060731T090000Z DTSTAMP;VALUE=DATE-TIME:20130520T064441Z UID:indico-event-a062741@cern.ch DESCRIPTION:The talk will describe the main ROOT features and review the c urrent developmentsOrganiser(s): HR-RFANote: The ROOT web site is availabl e at http://root.cern.ch. Students are strongly encouraged to download the binary files from this web site. The full documentation is also available from this location.\n\nhttp://indico.cern.ch/conferenceDisplay.py?confId= a062741 LOCATION:CERN Main Auditorium URL:http://indico.cern.ch/conferenceDisplay.py?confId=a062741 END:VEVENT BEGIN:VEVENT SUMMARY:"Double Simplex" - Visualizing elementary particles and their inte ractions DTSTART;VALUE=DATE-TIME:20060804T120000Z DTEND;VALUE=DATE-TIME:20060804T130000Z DTSTAMP;VALUE=DATE-TIME:20130520T064441Z UID:indico-event-a062836@cern.ch DESCRIPTION:The double simplex is a new way to envision the particles and interactions through a three-dimensional construction intended to serve as an invitation to narrative and a spur to curiosity. My goal is to represe nt what we know is true\, what we hope might be true\, and what we don't k now. Constructing the double simplex expresses the spirit of play\, of suc cessive approximations\, that animates the way scientists work. Organiser( s): HR-RFA\nNote: Prerequisites: preceding lectures in the CERN Summer Stu dents program. A short write-up is\, "The Double Simplex\," http://arxiv.o rg/abs/hep-ph/0509037Similar slides at http://www.hep.caltech.edu/seminars /monday/talks/2006/winter/Quigg.mov\n\nhttp://indico.cern.ch/conferenceDis play.py?confId=a062836 LOCATION:CERN Main Auditorium URL:http://indico.cern.ch/conferenceDisplay.py?confId=a062836 END:VEVENT BEGIN:VEVENT SUMMARY:The GRID DTSTART;VALUE=DATE-TIME:20060807T091500Z DTEND;VALUE=DATE-TIME:20060807T100000Z DTSTAMP;VALUE=DATE-TIME:20130520T064441Z UID:indico-event-a062808@cern.ch DESCRIPTION:The Grid infrastructure is a key part of the computing environ ment for the simulation\, processing and analysis of the data of the LHC e xperiments. These experiments depend on the availability of a worldwide Gr id infrastructure in several aspects of their computing model. The Grid mi ddleware will hide much of the complexity of this environment to the user\ , organizing all the resources in a coherent virtual computer center. The general description of the elements of the Grid\, their interconnections a nd their use by the experiments will be exposed in this talk. The computat ional and storage capability of the Grid is attracting other research comm unities beyond the high energy physics. Examples of these applications wil l be also exposed during the presentation. Organiser(s): HR-RFA\nNote:Prer equisite Knowledge:Not required.\nReferences:http://www.glite.org www.cern .ch/lcghttps://edms.cern.ch/file/722398//glite-3-UserGuide.pdf\n\nhttp://i ndico.cern.ch/conferenceDisplay.py?confId=a062808 LOCATION:CERN Main Auditorium URL:http://indico.cern.ch/conferenceDisplay.py?confId=a062808 END:VEVENT BEGIN:VEVENT SUMMARY:Future Linear Colliders DTSTART;VALUE=DATE-TIME:20060810T091500Z DTEND;VALUE=DATE-TIME:20060810T100000Z DTSTAMP;VALUE=DATE-TIME:20130520T064441Z UID:indico-event-a062746@cern.ch DESCRIPTION:After a brief introduction to Linear Colliders and the experie nce with the only Linear Colliders operated so far\, the SLC at SLAC\, the two schemes presently envisaged for future Linear Colliders as well as th eir planned perfomances\, their challenges and key issues are presented\, namely: - The International Linear Collider (ILC) based on Super-Conductin g RF technology for a Linear Collider with colliding beams in the TeV ener gy range - The Compact Linear Collider (CLIC) based on a novel Two Beam Ac celeration concept to extend Linear Colliders into the Multi-TeV colliding beam energy range. The present status and the planned R&D to develop thes e two technologies\, address the key issues\, demonstrate their feasibilit y and prepare their industrialisation will be presentedOrganiser(s): HR-RF A\n\nhttp://indico.cern.ch/conferenceDisplay.py?confId=a062746 LOCATION:CERN Main Auditorium URL:http://indico.cern.ch/conferenceDisplay.py?confId=a062746 END:VEVENT BEGIN:VEVENT SUMMARY:Gravitation Waves DTSTART;VALUE=DATE-TIME:20060810T081500Z DTEND;VALUE=DATE-TIME:20060810T090000Z DTSTAMP;VALUE=DATE-TIME:20130520T064441Z UID:indico-event-a062856@cern.ch DESCRIPTION:We will present a brief introduction to the physics of gravita tional waves and their properties. We will review potential astrophysical sources of gravitational waves\, and the physics and astrophysics that can be learned from their study. We will survey the techniques and technologi es for detecting gravitational waves for the first time\, including bar de tectors and broadband interferometers\, and give a brief status report on the international search effort.Organiser(s): HR-RFANote: The talk will be in the form of a university physics colloquium\, accessible to second yea r undergraduate physics students.\n\nhttp://indico.cern.ch/conferenceDispl ay.py?confId=a062856 LOCATION:CERN Main Auditorium URL:http://indico.cern.ch/conferenceDisplay.py?confId=a062856 END:VEVENT BEGIN:VEVENT SUMMARY:Closing Lecture: "From the very large to the very small and back" DTSTART;VALUE=DATE-TIME:20060811T091500Z DTEND;VALUE=DATE-TIME:20060811T100000Z DTSTAMP;VALUE=DATE-TIME:20130520T064441Z UID:indico-event-a062751@cern.ch DESCRIPTION:I shall review the main items of what I think you should have learned about particle physics and cosmology during your stay at CERN as S ummer Students.Organiser(s): HR-RFA\n\nhttp://indico.cern.ch/conferenceDis play.py?confId=a062751 LOCATION:CERN Main Auditorium URL:http://indico.cern.ch/conferenceDisplay.py?confId=a062751 END:VEVENT BEGIN:VEVENT SUMMARY:Introduction to the Root System DTSTART;VALUE=DATE-TIME:20070710T091500Z DTEND;VALUE=DATE-TIME:20070710T100000Z DTSTAMP;VALUE=DATE-TIME:20130520T064441Z UID:indico-event-a07140@cern.ch DESCRIPTION:An introduction to the ROOT system will be given. ROOT is used by most experiments to store\, query and visualize event data. In the sec ond part of the talk a demo will illustrate the main facets of the system. \n\nPrerequisite Knowledge and References: see \nhttp://root.cern.ch (ROO T web site)\nhttp://root.cern.ch/root/doc/RootDoc.html (Users Guide)\nbasi c knowledge of C++ required\n\nhttp://indico.cern.ch/conferenceDisplay.py? confId=a07140 LOCATION:CERN Main Auditorium URL:http://indico.cern.ch/conferenceDisplay.py?confId=a07140 END:VEVENT BEGIN:VEVENT SUMMARY:Introduction to the ROOT system- Root Demo Session DTSTART;VALUE=DATE-TIME:20070710T100000Z DTEND;VALUE=DATE-TIME:20070710T104500Z DTSTAMP;VALUE=DATE-TIME:20130520T064441Z UID:indico-event-a07141@cern.ch DESCRIPTION:An introduction to the ROOT system will be given. ROOT is used by most experiments to store\, query and visualize event data. In the sec ond part of the talk a demo will illustrate the main facets of the system. \n\nPrerequisite Knowledge and References: see \nhttp://root.cern.ch (ROO T web site)\nhttp://root.cern.ch/root/doc/RootDoc.html (Users Guide)\nbasi c knowledge of C++ required\n\nhttp://indico.cern.ch/conferenceDisplay.py? confId=a07141 LOCATION:CERN Main Auditorium URL:http://indico.cern.ch/conferenceDisplay.py?confId=a07141 END:VEVENT BEGIN:VEVENT SUMMARY:Astroparticle physics (1/3) DTSTART;VALUE=DATE-TIME:20070716T081500Z DTEND;VALUE=DATE-TIME:20070716T090000Z DTSTAMP;VALUE=DATE-TIME:20130520T064441Z UID:indico-event-17096@cern.ch DESCRIPTION:The lectures cover recent topics in astroparticle physics. Aft er a general introduction to the field\, the first lecture will explain th e origin of the elements in the universe (Big Bang Nucleosynthesis) and wi ll present the studies of the cosmic microwave background and of its aniso tropies. The next lecture will cover the ongoing experiments dedicated to the study of dark matter (direct detection or microlensing experiments) a nd dark energy (in particular the experiments searching for supernovae). The last lecture will be devoted to high energy astrophysics\, large scale cosmic ray detectors and high energy neutrino detectors.\n\nPrerequisite knowledge: Basic knowledge of physics and astrophysics\n\nhttp://indico.ce rn.ch/conferenceDisplay.py?confId=17096 LOCATION:CERN Main Auditorium URL:http://indico.cern.ch/conferenceDisplay.py?confId=17096 END:VEVENT BEGIN:VEVENT SUMMARY:Astroparticle physics (2/3) DTSTART;VALUE=DATE-TIME:20070716T091500Z DTEND;VALUE=DATE-TIME:20070716T100000Z DTSTAMP;VALUE=DATE-TIME:20130520T064441Z UID:indico-event-17097@cern.ch DESCRIPTION:The lectures cover recent topics in astroparticle physics. Aft er a general introduction to the field\, the first lecture will explain th e origin of the elements in the universe (Big Bang Nucleosynthesis) and wi ll present the studies of the cosmic microwave background and of its aniso tropies. The next lecture will cover the ongoing experiments dedicated to the study of dark matter (direct detection or microlensing experiments) a nd dark energy (in particular the experiments searching for supernovae). The last lecture will be devoted to high energy astrophysics\, large scale cosmic ray detectors and high energy neutrino detectors.\n\nPrerequisite knowledge: Basic knowledge of physics and astrophysics\n\nhttp://indico.ce rn.ch/conferenceDisplay.py?confId=17097 LOCATION:CERN Main Auditorium URL:http://indico.cern.ch/conferenceDisplay.py?confId=17097 END:VEVENT BEGIN:VEVENT SUMMARY:Astroparticle physics (3/3) DTSTART;VALUE=DATE-TIME:20070717T071500Z DTEND;VALUE=DATE-TIME:20070717T080000Z DTSTAMP;VALUE=DATE-TIME:20130520T064441Z UID:indico-event-17098@cern.ch DESCRIPTION:The lectures cover recent topics in astroparticle physics. Aft er a general introduction to the field\, the first lecture will explain th e origin of the elements in the universe (Big Bang Nucleosynthesis) and wi ll present the studies of the cosmic microwave background and of its aniso tropies. The next lecture will cover the ongoing experiments dedicated to the study of dark matter (direct detection or microlensing experiments) a nd dark energy (in particular the experiments searching for supernovae). The last lecture will be devoted to high energy astrophysics\, large scale cosmic ray detectors and high energy neutrino detectors.\n\nPrerequisite knowledge: Basic knowledge of physics and astrophysics\n\nhttp://indico.ce rn.ch/conferenceDisplay.py?confId=17098 LOCATION:CERN Main Auditorium URL:http://indico.cern.ch/conferenceDisplay.py?confId=17098 END:VEVENT BEGIN:VEVENT SUMMARY:Introduction to Medical Physics DTSTART;VALUE=DATE-TIME:20070718T091500Z DTEND;VALUE=DATE-TIME:20070718T100000Z DTSTAMP;VALUE=DATE-TIME:20130520T064441Z UID:indico-event-a07158@cern.ch DESCRIPTION:The lecture will first briefly review physical discoveries and tools developed for physics which later found applications in medicine\, and then it will illustrate the most relevant of these applications: magne tic resonance imaging\, computerized tomography\, single photon emission c omputerized tomography\, positron emission tomography\, conventional and a dvanced radiation therapy\n\nhttp://indico.cern.ch/conferenceDisplay.py?co nfId=a07158 LOCATION:CERN Main Auditorium URL:http://indico.cern.ch/conferenceDisplay.py?confId=a07158 END:VEVENT BEGIN:VEVENT SUMMARY:The ISOLDE Facility: Radioactive beams at CERN DTSTART;VALUE=DATE-TIME:20070725T121500Z DTEND;VALUE=DATE-TIME:20070725T130000Z DTSTAMP;VALUE=DATE-TIME:20130520T064441Z UID:indico-event-17147@cern.ch DESCRIPTION:The Isope Separation On-Line (ISOL) technique evolved from che mical techniques used to separate radioactive isotopes off-line from irrad iated "targets". The ISOL targets of today\, used at e.g. ISOLDE\, can be of many different types and in different phases but the isotopes are alway s delivered at very low energies making the technique ideal for study of g round state properties and collections for other applications such as soli d state physics and medical physics. The possibility of accelerating these low energy beams for nuclear structure studies\, and in the long term fut ure for neutrino physics\, is now being explored at first generation radio active beam facilities. The upgrade towards HIE-ISOLDE aim to consolidate ISOLDE's position as a world leading radioactive nuclear beam facility and it will be a pre-cursor to a future all European ISOL facility\, EURISOL\ , with order of magnitudes higher radioactive beam intensities and energie s.\n\nPrerequisite knowledge and references: None\n\nhttp://indico.cern.ch /conferenceDisplay.py?confId=17147 LOCATION:CERN Main Amphtitheatre URL:http://indico.cern.ch/conferenceDisplay.py?confId=17147 END:VEVENT BEGIN:VEVENT SUMMARY:Visit of The ISOLDE Facility DTSTART;VALUE=DATE-TIME:20070727T120000Z DTEND;VALUE=DATE-TIME:20070727T140000Z DTSTAMP;VALUE=DATE-TIME:20130520T064441Z UID:indico-event-17148@cern.ch DESCRIPTION:The Isope Separation On-Line (ISOL) technique evolved from che mical techniques used to separate radioactive isotopes off-line from irrad iated "targets". The ISOL targets of today\, used at e.g. ISOLDE\, can be of many different types and in different phases but the isotopes are alway s delivered at very low energies making the technique ideal for study of g round state properties and collections for other applications such as soli d state physics and medical physics. The possibility of accelerating these low energy beams for nuclear structure studies\, and in the long term fut ure for neutrino physics\, is now being explored at first generation radio active beam facilities. The upgrade towards HIE-ISOLDE aim to consolidate ISOLDE's position as a world leading radioactive nuclear beam facility and it will be a pre-cursor to a future all European ISOL facility\, EURISOL\ , with order of magnitudes higher radioactive beam intensities and energie s.\n\nPrerequisite knowledge and references: None\n\nhttp://indico.cern.ch /conferenceDisplay.py?confId=17148 LOCATION:CERN Meeting point in front of building 170 URL:http://indico.cern.ch/conferenceDisplay.py?confId=17148 END:VEVENT BEGIN:VEVENT SUMMARY:Superconducting Magnets DTSTART;VALUE=DATE-TIME:20070730T081500Z DTEND;VALUE=DATE-TIME:20070730T090000Z DTSTAMP;VALUE=DATE-TIME:20130520T064441Z UID:indico-event-a07179@cern.ch DESCRIPTION:http://indico.cern.ch/conferenceDisplay.py?confId=a07179 LOCATION:CERN Main Auditorium URL:http://indico.cern.ch/conferenceDisplay.py?confId=a07179 END:VEVENT BEGIN:VEVENT SUMMARY:The GRID DTSTART;VALUE=DATE-TIME:20070806T091500Z DTEND;VALUE=DATE-TIME:20070806T100000Z DTSTAMP;VALUE=DATE-TIME:20130520T064441Z UID:indico-event-a07194@cern.ch DESCRIPTION:Grid infrastructure is a key part of the computing environment for the simulation\, processing and analysis of the data of the LHC exper iments. These experiments depend on the availability of a worldwide Grid i nfrastructure in several aspects of their computing model. The Grid middle ware will hide much of the complexity of this environment to the user\, or ganizing all the resources in a coherent virtual computer center. The gene ral description of the elements of the Grid\, their interconnections and t heir use by the experiments will be exposed in this talk. The computationa l and storage capability of the Grid is attracting other research communit ies beyond the high energy physics. Examples of these applications will be also exposed during the presentation.\n\nNo prerequisite knowledge requir ed.\n\nhttp://indico.cern.ch/conferenceDisplay.py?confId=a07194 LOCATION:CERN Main Auditorium URL:http://indico.cern.ch/conferenceDisplay.py?confId=a07194 END:VEVENT BEGIN:VEVENT SUMMARY:The LHC upgrade DTSTART;VALUE=DATE-TIME:20070808T081500Z DTEND;VALUE=DATE-TIME:20070808T090000Z DTSTAMP;VALUE=DATE-TIME:20130520T064441Z UID:indico-event-a07202@cern.ch DESCRIPTION:This seminar will discuss the future program at the LHC. After the present program will be completed\, when about 300 fb-1 is collected by the experiments\, a simple continuation of the operation of the machine becomes less exciting. Studies are already made for upgrading the LHC\, b eyond its presently expected performance. Two scenarios are will be discus sed: - Upgrading the luminosity by a factor 10\, ie. 10^35 cm-2s-1 - Upgra ding the total energy to 28 TeV\, ie 14 TeV per beam This seminar will dis cuss a possible path for such upgrades and particularly the additional inc rease in physics reach that can be gained with such upgrades. It turns out that for essentially all scenarios of new physics\, the upgrade of the LH C will bring something new.\n\nPrerequisite knowledge: Physics lectures in the summer student programme\n\nhttp://indico.cern.ch/conferenceDisplay.p y?confId=a07202 LOCATION:CERN Main Auditorium URL:http://indico.cern.ch/conferenceDisplay.py?confId=a07202 END:VEVENT BEGIN:VEVENT SUMMARY:Future Linear Colliders DTSTART;VALUE=DATE-TIME:20070809T091500Z DTEND;VALUE=DATE-TIME:20070809T100000Z DTSTAMP;VALUE=DATE-TIME:20130520T064441Z UID:indico-event-a07203@cern.ch DESCRIPTION:Future Linear Colliders can open the way to new exciting physi cs.\nAfter a brief introduction to Linear Colliders\, the physics motivati on and history\, the two schemes presently envisaged for future Linear Col liders are presented:\n- The International Linear Collider (ILC) based on Super-Conducting RF technology with colliding beams in the TeV energy rang e \n- The Compact Linear Collider (CLIC) based on a novel Two Beam Acceler ation concept to extend Linear Colliders into the Multi-TeV colliding beam energy range.\nTheir planned performances\, challenges and key issues\, t he present status and the planned R&D to develop these two technologies wi ll be shown.\n\nNo prerequisite knowledge required.\n\nhttp://indico.cern. ch/conferenceDisplay.py?confId=a07203 LOCATION:CERN Main Auditorium URL:http://indico.cern.ch/conferenceDisplay.py?confId=a07203 END:VEVENT BEGIN:VEVENT SUMMARY:Particle Physics Circa 2010 DTSTART;VALUE=DATE-TIME:20070810T091500Z DTEND;VALUE=DATE-TIME:20070810T100000Z DTSTAMP;VALUE=DATE-TIME:20130520T064441Z UID:indico-event-a07204@cern.ch DESCRIPTION:We will survey the landscape of ideas for physics beyond the S tandard Model that have been developed in the last quarter century. These are now undergoing significant re-evaluation in view of the cosmological c onstant problem\, and the apparent presence of an enormous number of groun d states in string theory. We will also discuss experimental tests of thes e ideas at the Large Hadron Collider.\n\nPrerequisite knowledge: \nStandar d Model and beyond.\nCheng and Lee\, or Quigg\, or Ross\, or Weinberg\, or other books on the Standard Model and beyond.\nWeinberg's third volume\, on supersymmetry\, is helpful - especially the chapter on the supersymmetr ic standard model.\n\nhttp://indico.cern.ch/conferenceDisplay.py?confId=a0 7204 LOCATION:CERN Main Auditorium URL:http://indico.cern.ch/conferenceDisplay.py?confId=a07204 END:VEVENT BEGIN:VEVENT SUMMARY:Introduction to the ROOT System DTSTART;VALUE=DATE-TIME:20080708T091500Z DTEND;VALUE=DATE-TIME:20080708T100000Z DTSTAMP;VALUE=DATE-TIME:20130520T064441Z UID:indico-event-34816@cern.ch DESCRIPTION:Introduction to the ROOT data handling system. ROOT is used in some for or another by all LHC experiments and will be used by all for fi nal data analysis. The introduction gives an overview of the system.\n\nPr erequisite knowledge: C++\n\nhttp://indico.cern.ch/conferenceDisplay.py?co nfId=34816 LOCATION:CERN Main Auditorium URL:http://indico.cern.ch/conferenceDisplay.py?confId=34816 END:VEVENT BEGIN:VEVENT SUMMARY:Introduction to the ROOT System - Root Demo Session DTSTART;VALUE=DATE-TIME:20080708T100000Z DTEND;VALUE=DATE-TIME:20080708T103000Z DTSTAMP;VALUE=DATE-TIME:20130520T064441Z UID:indico-event-34817@cern.ch DESCRIPTION:http://indico.cern.ch/conferenceDisplay.py?confId=34817 LOCATION:CERN Main Auditorium URL:http://indico.cern.ch/conferenceDisplay.py?confId=34817 END:VEVENT BEGIN:VEVENT SUMMARY:Superconducting Magnets DTSTART;VALUE=DATE-TIME:20080716T091500Z DTEND;VALUE=DATE-TIME:20080716T100000Z DTSTAMP;VALUE=DATE-TIME:20130520T064441Z UID:indico-event-34818@cern.ch DESCRIPTION:Starting from the beam requirements for accelerator magnets\, we will outline the main issues and the physical limitations for producing strong and pure magnetic fields with superconductors. The seminar will ma inly focus on the magnets for the accelerator\, and give some hints on the magnets for the experiments.\n\nPrerequisite knowledge: Basic knowledge o f Maxwell equations\, and linear optics for particle accelerators (FODO ce ll\, beta functions).\n\nhttp://indico.cern.ch/conferenceDisplay.py?confId =34818 LOCATION:CERN Main Auditorium URL:http://indico.cern.ch/conferenceDisplay.py?confId=34818 END:VEVENT BEGIN:VEVENT SUMMARY:The ISOLDE Facility: Radioactive beams at CERN DTSTART;VALUE=DATE-TIME:20080724T120000Z DTEND;VALUE=DATE-TIME:20080724T124500Z DTSTAMP;VALUE=DATE-TIME:20130520T064441Z UID:indico-event-34903@cern.ch DESCRIPTION:ISOLDE is the longest running CERN experiment\, starting in 19 67 and going through regular metamorphoses ever since. The facility produc es intense and pure beams of up to 1000 different isotopes by irradiating targets with 1.4 GeV protons\, the different techniques for separating and manipulating the isotopes (e.g. in ion traps) will be explained. The isot opes are used in many experiments within nuclear physics\, astrophysics\, solid state physics\, life science and fundamental physics.\nSome of the e xperimental techniques used will be introduced\; more focus will be put on what physics questions can be answered by using radioactive beams. A brie f overview is given of the present and future European developments in thi s rapidly evolving field.\n\nPrerequisite knowledge: none\n\nhttp://indico .cern.ch/conferenceDisplay.py?confId=34903 LOCATION:CERN Main Auditorium URL:http://indico.cern.ch/conferenceDisplay.py?confId=34903 END:VEVENT BEGIN:VEVENT SUMMARY:Introduction to Medical Physics DTSTART;VALUE=DATE-TIME:20080801T091500Z DTEND;VALUE=DATE-TIME:20080801T100000Z DTSTAMP;VALUE=DATE-TIME:20130520T064441Z UID:indico-event-34840@cern.ch DESCRIPTION:The lecture will first briefly review physical discoveries and tools developed for physics which later found applications in medicine\, and then it will illustrate the most relevant of these applications: magne tic resonance imaging\, computerized tomography\, single photon emission c omputerized tomography\, positron emission tomography\, and conventional a nd advanced radiation therapy.\n\nPrerequisite knowledge: none\n\nhttp://i ndico.cern.ch/conferenceDisplay.py?confId=34840 LOCATION:CERN Main Auditorium URL:http://indico.cern.ch/conferenceDisplay.py?confId=34840 END:VEVENT BEGIN:VEVENT SUMMARY:Future Linear Colliders DTSTART;VALUE=DATE-TIME:20080804T071500Z DTEND;VALUE=DATE-TIME:20080804T080000Z DTSTAMP;VALUE=DATE-TIME:20130520T064441Z UID:indico-event-34843@cern.ch DESCRIPTION:Future Linear Colliders can open the way to new exciting physi cs.\nAfter a brief introduction to Linear Colliders\, the physics motivati on and history\, the two schemes presently envisaged for future Linear Col liders are presented:\n- The International Linear Collider (ILC) based on Super-Conducting RF technology with colliding beams in the TeV energy rang e\n- The Compact Linear Collider (CLIC) based on a novel Two Beam Accelera tion concept to extend Linear Colliders into the Multi-TeV colliding beam energy range.\nTheir planned performances\, challenges and key issues\, th e present status and the planned R&D to develop these two technologies wil l be shown.\n\nPrerequisite knowledge: Common sense and a little bit of ph ysics\n\nhttp://indico.cern.ch/conferenceDisplay.py?confId=34843 LOCATION:CERN Main Auditorium URL:http://indico.cern.ch/conferenceDisplay.py?confId=34843 END:VEVENT BEGIN:VEVENT SUMMARY:Installation\, Commissioning and startup of the ATLAS experiment DTSTART;VALUE=DATE-TIME:20080804T081500Z DTEND;VALUE=DATE-TIME:20080804T090000Z DTSTAMP;VALUE=DATE-TIME:20130520T064441Z UID:indico-event-34844@cern.ch DESCRIPTION:http://indico.cern.ch/conferenceDisplay.py?confId=34844 LOCATION:CERN Main Auditorium URL:http://indico.cern.ch/conferenceDisplay.py?confId=34844 END:VEVENT BEGIN:VEVENT SUMMARY:The GRID DTSTART;VALUE=DATE-TIME:20080804T091500Z DTEND;VALUE=DATE-TIME:20080804T100000Z DTSTAMP;VALUE=DATE-TIME:20130520T064441Z UID:indico-event-34846@cern.ch DESCRIPTION:http://indico.cern.ch/conferenceDisplay.py?confId=34846 LOCATION:CERN Main Auditorium URL:http://indico.cern.ch/conferenceDisplay.py?confId=34846 END:VEVENT BEGIN:VEVENT SUMMARY:Installation\, Commisssioning and startup of the CMS experiment DTSTART;VALUE=DATE-TIME:20080805T071500Z DTEND;VALUE=DATE-TIME:20080805T080000Z DTSTAMP;VALUE=DATE-TIME:20130520T064441Z UID:indico-event-34847@cern.ch DESCRIPTION:Will outline the construction phases of CMS\, followed by spec ific strategy used by CMS to commission the experiment concurrently with t he installation in the cavern. All along examples of the performance of th e detector obtained mainly from cosmic ray data will be shown. At the end some example of early physics result aimed for the 2008 LHC run will be sh own.\n\nPrerequisite knowledge: Some knowledge of basic particle detectors will make it easier to follow the talk.\n\nhttp://indico.cern.ch/conferen ceDisplay.py?confId=34847 LOCATION:CERN Main Auditorium URL:http://indico.cern.ch/conferenceDisplay.py?confId=34847 END:VEVENT BEGIN:VEVENT SUMMARY:Commissioning and startup of the LHC accelerator DTSTART;VALUE=DATE-TIME:20080806T091500Z DTEND;VALUE=DATE-TIME:20080806T100000Z DTSTAMP;VALUE=DATE-TIME:20130520T064441Z UID:indico-event-34848@cern.ch DESCRIPTION:http://indico.cern.ch/conferenceDisplay.py?confId=34848 LOCATION:CERN Main Auditorium URL:http://indico.cern.ch/conferenceDisplay.py?confId=34848 END:VEVENT BEGIN:VEVENT SUMMARY:Closing Lecture - Particle Physics: The LHC and Beyond DTSTART;VALUE=DATE-TIME:20080808T091500Z DTEND;VALUE=DATE-TIME:20080808T100000Z DTSTAMP;VALUE=DATE-TIME:20130520T064441Z UID:indico-event-34860@cern.ch DESCRIPTION:http://indico.cern.ch/conferenceDisplay.py?confId=34860 LOCATION:CERN Main Auditorium URL:http://indico.cern.ch/conferenceDisplay.py?confId=34860 END:VEVENT BEGIN:VEVENT SUMMARY:Installation\, Commissioning and Startup of Atlas & CMS Experiment s DTSTART;VALUE=DATE-TIME:20090702T091500Z DTEND;VALUE=DATE-TIME:20090702T100000Z DTSTAMP;VALUE=DATE-TIME:20130520T064441Z UID:indico-event-57492@cern.ch DESCRIPTION:http://indico.cern.ch/conferenceDisplay.py?confId=57492 LOCATION:CERN Main Auditorium URL:http://indico.cern.ch/conferenceDisplay.py?confId=57492 END:VEVENT BEGIN:VEVENT SUMMARY:Future Colliders DTSTART;VALUE=DATE-TIME:20090717T091500Z DTEND;VALUE=DATE-TIME:20090717T100000Z DTSTAMP;VALUE=DATE-TIME:20130520T064441Z UID:indico-event-57330@cern.ch DESCRIPTION:http://indico.cern.ch/conferenceDisplay.py?confId=57330 LOCATION:CERN Main Auditorium URL:http://indico.cern.ch/conferenceDisplay.py?confId=57330 END:VEVENT BEGIN:VEVENT SUMMARY:Superconducting Magnets DTSTART;VALUE=DATE-TIME:20090724T081500Z DTEND;VALUE=DATE-TIME:20090724T090000Z DTSTAMP;VALUE=DATE-TIME:20130520T064441Z UID:indico-event-57533@cern.ch DESCRIPTION:http://indico.cern.ch/conferenceDisplay.py?confId=57533 LOCATION:CERN Main Auditorium URL:http://indico.cern.ch/conferenceDisplay.py?confId=57533 END:VEVENT BEGIN:VEVENT SUMMARY:Future Linear Colliders DTSTART;VALUE=DATE-TIME:20090729T071500Z DTEND;VALUE=DATE-TIME:20090729T080000Z DTSTAMP;VALUE=DATE-TIME:20130520T064441Z UID:indico-event-57575@cern.ch DESCRIPTION:http://indico.cern.ch/conferenceDisplay.py?confId=57575 LOCATION:CERN Main Auditorium URL:http://indico.cern.ch/conferenceDisplay.py?confId=57575 END:VEVENT BEGIN:VEVENT SUMMARY:Introduction to Medical Physics DTSTART;VALUE=DATE-TIME:20090803T091500Z DTEND;VALUE=DATE-TIME:20090803T100000Z DTSTAMP;VALUE=DATE-TIME:20130520T064441Z UID:indico-event-57576@cern.ch DESCRIPTION:http://indico.cern.ch/conferenceDisplay.py?confId=57576 LOCATION:CERN Main Auditorium URL:http://indico.cern.ch/conferenceDisplay.py?confId=57576 END:VEVENT BEGIN:VEVENT SUMMARY:The future of energy and climate DTSTART;VALUE=DATE-TIME:20090805T140000Z DTEND;VALUE=DATE-TIME:20090805T150000Z DTSTAMP;VALUE=DATE-TIME:20130520T064441Z UID:indico-event-64732@cern.ch DESCRIPTION:The talk will review some of the basic facts about the history and present status of the use of energy and its climatic consequences. I t is clear that the world will have to change its way of energy production \, the sooner the better. Because of the difficulty of storing electric e nergy\, by far the best energy source for the future is thermal solar from the deserts\, with overnight thermal storage. I will give some descripti on of the present status of the technologies involved and end up with a pi lot project for Europe and North Africa.\n\nhttp://indico.cern.ch/conferen ceDisplay.py?confId=64732 LOCATION:CERN Main Auditorium URL:http://indico.cern.ch/conferenceDisplay.py?confId=64732 END:VEVENT BEGIN:VEVENT SUMMARY:Closing Lecture DTSTART;VALUE=DATE-TIME:20090807T091500Z DTEND;VALUE=DATE-TIME:20090807T100000Z DTSTAMP;VALUE=DATE-TIME:20130520T064441Z UID:indico-event-57587@cern.ch DESCRIPTION:http://indico.cern.ch/conferenceDisplay.py?confId=57587 LOCATION:CERN Main Auditorium URL:http://indico.cern.ch/conferenceDisplay.py?confId=57587 END:VEVENT BEGIN:VEVENT SUMMARY:Superconducting Magnets DTSTART;VALUE=DATE-TIME:20100708T071500Z DTEND;VALUE=DATE-TIME:20100708T080000Z DTSTAMP;VALUE=DATE-TIME:20130520T064441Z UID:indico-event-91698@cern.ch DESCRIPTION:http://indico.cern.ch/conferenceDisplay.py?confId=91698 LOCATION:CERN Globe 1st Floor URL:http://indico.cern.ch/conferenceDisplay.py?confId=91698 END:VEVENT BEGIN:VEVENT SUMMARY: "What is a Jet?" DTSTART;VALUE=DATE-TIME:20100709T071500Z DTEND;VALUE=DATE-TIME:20100709T080000Z DTSTAMP;VALUE=DATE-TIME:20130520T064441Z UID:indico-event-93183@cern.ch DESCRIPTION:http://indico.cern.ch/conferenceDisplay.py?confId=93183 LOCATION:CERN Globe 1st Floor URL:http://indico.cern.ch/conferenceDisplay.py?confId=93183 END:VEVENT BEGIN:VEVENT SUMMARY:Future Colliders : Physics Motivations DTSTART;VALUE=DATE-TIME:20100729T071500Z DTEND;VALUE=DATE-TIME:20100729T080000Z DTSTAMP;VALUE=DATE-TIME:20130520T064441Z UID:indico-event-91703@cern.ch DESCRIPTION:http://indico.cern.ch/conferenceDisplay.py?confId=91703 LOCATION:CERN Globe 1st Floor URL:http://indico.cern.ch/conferenceDisplay.py?confId=91703 END:VEVENT BEGIN:VEVENT SUMMARY:Future Linear Colliders : Accelerator Physics DTSTART;VALUE=DATE-TIME:20100802T081500Z DTEND;VALUE=DATE-TIME:20100802T090000Z DTSTAMP;VALUE=DATE-TIME:20130520T064441Z UID:indico-event-91701@cern.ch DESCRIPTION:http://indico.cern.ch/conferenceDisplay.py?confId=91701 LOCATION:CERN Globe 1st Floor URL:http://indico.cern.ch/conferenceDisplay.py?confId=91701 END:VEVENT BEGIN:VEVENT SUMMARY:LHC/Grid Computing DTSTART;VALUE=DATE-TIME:20110721T091500Z DTEND;VALUE=DATE-TIME:20110721T100000Z DTSTAMP;VALUE=DATE-TIME:20130520T064441Z UID:indico-event-134624@cern.ch DESCRIPTION:http://indico.cern.ch/conferenceDisplay.py?confId=134624 LOCATION:CERN Main Auditorium URL:http://indico.cern.ch/conferenceDisplay.py?confId=134624 END:VEVENT BEGIN:VEVENT SUMMARY:Superconducting Magnets DTSTART;VALUE=DATE-TIME:20110722T091500Z DTEND;VALUE=DATE-TIME:20110722T100000Z DTSTAMP;VALUE=DATE-TIME:20130520T064441Z UID:indico-event-134625@cern.ch DESCRIPTION:http://indico.cern.ch/conferenceDisplay.py?confId=134625 LOCATION:CERN Main Auditorium URL:http://indico.cern.ch/conferenceDisplay.py?confId=134625 END:VEVENT BEGIN:VEVENT SUMMARY:What is String Theory? (Theoretical Physics) DTSTART;VALUE=DATE-TIME:20110729T091500Z DTEND;VALUE=DATE-TIME:20110729T100000Z DTSTAMP;VALUE=DATE-TIME:20130520T064441Z UID:indico-event-135042@cern.ch DESCRIPTION:http://indico.cern.ch/conferenceDisplay.py?confId=135042 LOCATION:CERN Main Auditorium URL:http://indico.cern.ch/conferenceDisplay.py?confId=135042 END:VEVENT BEGIN:VEVENT SUMMARY:Particle Accelerators in Cancer Therapy DTSTART;VALUE=DATE-TIME:20110805T091500Z DTEND;VALUE=DATE-TIME:20110805T100000Z DTSTAMP;VALUE=DATE-TIME:20130520T064441Z UID:indico-event-135089@cern.ch DESCRIPTION:http://indico.cern.ch/conferenceDisplay.py?confId=135089 LOCATION:CERN Main Auditorium URL:http://indico.cern.ch/conferenceDisplay.py?confId=135089 END:VEVENT BEGIN:VEVENT SUMMARY:Future Colliders and Physics DTSTART;VALUE=DATE-TIME:20110809T091500Z DTEND;VALUE=DATE-TIME:20110809T100000Z DTSTAMP;VALUE=DATE-TIME:20130520T064441Z UID:indico-event-135176@cern.ch DESCRIPTION:http://indico.cern.ch/conferenceDisplay.py?confId=135176 LOCATION:CERN Main Auditorium URL:http://indico.cern.ch/conferenceDisplay.py?confId=135176 END:VEVENT BEGIN:VEVENT SUMMARY:Introduction to Root DTSTART;VALUE=DATE-TIME:20120709T091500Z DTEND;VALUE=DATE-TIME:20120709T100000Z DTSTAMP;VALUE=DATE-TIME:20130520T064441Z UID:indico-event-190186@cern.ch DESCRIPTION:http://indico.cern.ch/conferenceDisplay.py?confId=190186 LOCATION:CERN Main Auditorium URL:http://indico.cern.ch/conferenceDisplay.py?confId=190186 END:VEVENT BEGIN:VEVENT SUMMARY:Detector simulation DTSTART;VALUE=DATE-TIME:20120724T071500Z DTEND;VALUE=DATE-TIME:20120724T080000Z DTSTAMP;VALUE=DATE-TIME:20130520T064441Z UID:indico-event-190218@cern.ch DESCRIPTION:http://indico.cern.ch/conferenceDisplay.py?confId=190218 LOCATION:CERN Main Auditorium URL:http://indico.cern.ch/conferenceDisplay.py?confId=190218 END:VEVENT BEGIN:VEVENT SUMMARY:Nuclear Physics DTSTART;VALUE=DATE-TIME:20120724T091500Z DTEND;VALUE=DATE-TIME:20120724T100000Z DTSTAMP;VALUE=DATE-TIME:20130520T064441Z UID:indico-event-190220@cern.ch DESCRIPTION:http://indico.cern.ch/conferenceDisplay.py?confId=190220 LOCATION:CERN Main Auditorium URL:http://indico.cern.ch/conferenceDisplay.py?confId=190220 END:VEVENT BEGIN:VEVENT SUMMARY:String Physics DTSTART;VALUE=DATE-TIME:20120801T091500Z DTEND;VALUE=DATE-TIME:20120801T100000Z DTSTAMP;VALUE=DATE-TIME:20130520T064441Z UID:indico-event-190221@cern.ch DESCRIPTION:http://indico.cern.ch/conferenceDisplay.py?confId=190221 LOCATION:CERN Main Auditorium URL:http://indico.cern.ch/conferenceDisplay.py?confId=190221 END:VEVENT BEGIN:VEVENT SUMMARY:Physics at future colliders DTSTART;VALUE=DATE-TIME:20120802T081500Z DTEND;VALUE=DATE-TIME:20120802T090000Z DTSTAMP;VALUE=DATE-TIME:20130520T064441Z UID:indico-event-190222@cern.ch DESCRIPTION:http://indico.cern.ch/conferenceDisplay.py?confId=190222 LOCATION:CERN Main Auditorium URL:http://indico.cern.ch/conferenceDisplay.py?confId=190222 END:VEVENT BEGIN:VEVENT SUMMARY:Closing Lecture DTSTART;VALUE=DATE-TIME:20120810T081500Z DTEND;VALUE=DATE-TIME:20120810T090000Z DTSTAMP;VALUE=DATE-TIME:20130520T064441Z UID:indico-event-190321@cern.ch DESCRIPTION:http://indico.cern.ch/conferenceDisplay.py?confId=190321 LOCATION:CERN Main Auditorium URL:http://indico.cern.ch/conferenceDisplay.py?confId=190321 END:VEVENT BEGIN:VEVENT SUMMARY:Physics at future colliders (1/1) DTSTART;VALUE=DATE-TIME:20130724T071500Z DTEND;VALUE=DATE-TIME:20130724T080000Z DTSTAMP;VALUE=DATE-TIME:20130520T064441Z UID:indico-event-243745@cern.ch DESCRIPTION:http://indico.cern.ch/conferenceDisplay.py?confId=243745 LOCATION:CERN Main Auditorium URL:http://indico.cern.ch/conferenceDisplay.py?confId=243745 END:VEVENT BEGIN:VEVENT SUMMARY:Detector Simulation (1/1) DTSTART;VALUE=DATE-TIME:20130807T071500Z DTEND;VALUE=DATE-TIME:20130807T080000Z DTSTAMP;VALUE=DATE-TIME:20130520T064441Z UID:indico-event-243726@cern.ch DESCRIPTION:Simulation of particle interaction in a detector.\n\nhttp://in dico.cern.ch/conferenceDisplay.py?confId=243726 LOCATION:CERN Main Auditorium URL:http://indico.cern.ch/conferenceDisplay.py?confId=243726 END:VEVENT BEGIN:VEVENT SUMMARY:String Theory DTSTART;VALUE=DATE-TIME:20130808T071500Z DTEND;VALUE=DATE-TIME:20130808T080000Z DTSTAMP;VALUE=DATE-TIME:20130520T064441Z UID:indico-event-243791@cern.ch DESCRIPTION:What is String Theory ?\n\nhttp://indico.cern.ch/conferenceDis play.py?confId=243791 LOCATION:CERN Main Auditorium URL:http://indico.cern.ch/conferenceDisplay.py?confId=243791 END:VEVENT BEGIN:VEVENT SUMMARY:Closing Lecture DTSTART;VALUE=DATE-TIME:20130809T081500Z DTEND;VALUE=DATE-TIME:20130809T090000Z DTSTAMP;VALUE=DATE-TIME:20130520T064441Z UID:indico-event-243814@cern.ch DESCRIPTION:http://indico.cern.ch/conferenceDisplay.py?confId=243814 LOCATION:CERN Main Auditorium URL:http://indico.cern.ch/conferenceDisplay.py?confId=243814 END:VEVENT END:VCALENDAR