Project Overview Overview The Project(s) Goal Building Issues VERY VERY VERY Preliminary Planning

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Slide 2 Project Overview Slide 3 Overview The Project(s) Goal Building Issues VERY VERY VERY Preliminary Planning Slide 4 The Project(s) Originally one Project (started pushing for it in 1999) Split into three Sub-Projects The Cosm School Students Lab Microcosm Gardens UA1 Central Detector Display Slide 5 Situation Cosm is located in building 143 Slide 6 Project 1 Slide 7 Goal Present modern physics education in this direction is part of the CERN mandate. The School Students Lab will provide a hands-on lab area for visiting (school) students display and present modern physics to a more general public extend the educational programme Slide 8 Cosm currently the complete building is used as exhibition space most platforms are made of concrete Slide 9 Cosm School Students Lab General Idea Slide 10 Cosm School Students Lab General Idea contd Slide 11 What is a school students lab? In the recent past, many schools have faced the problem that out of financial reasons, only a very limited number of experiments could be acquired and performed in school. This lead to a wave of school students labs, where these experiments and even more modern ones are made available and can be performed together with the personnel there. Slide 12 Prototype School Students Lab Activity standard school student lab activity is planned for 2.5 hrs standard ingredients: general and safety introduction 2 experiment blocks 50 mins 5 intro 40 experiment 5 discussion break of 15 mins between final discussion done in 3 experiments 3 groups 3 participants/group Slide 13 Safety Considerations Experiments Voltages nearly all experiments are made for schools according to the prevailing standards CRT vacuum glass tube Gasses LN2 dry ice propane Radioactive Material Rutherford source in apparatus Cloud Chamber different sources , , Natural Radiation different sources , , different materials Slide 14 Project 2 Slide 15 Microcosm Gardens Slide 16 Project 3 Slide 17 UA1 Central Detector Display Slide 18 VERY VERY VERY Preliminary Planning Now Collecting Issues Fall 2012 Clean up area in 143 Store UA1 Central Detector in 185 End 2012 Build partitioning wall Winter 2012 Install services Spring 2013 Install lab systems Slide 19 Slide 20 X-Ray Experiments X-Ray spectra Material analysis Radiography MediPix radiation-tested by RP Slide 21 Experiment High T C Superconductor Record the voltage drop across a superconductor with varying temperature. Measurement by dipping a probe with superconductor and platinum resistor into a bath of liquid nitrogen. Handling of nitrogen by presenter. Handling of probe by students. Slide 22 Experiment Self-built Cloud Chamber Visualize charged tracks. dry ice for cooling IPA (C 3 H 8 O) for vapors see http://teachers/document/cloud-final.pdf Slide 23 Experiment Photoelectric Effect Measure the kinetic energy of the electrons as a function of the frequency of the light. Determine Plancks constant h. Measurement using a mercury lamp, filters, and an op-amp. Hot mercury lamp. Slide 24 Experiment Rutherford Experiment To record the direct counting rate N d of particles scattered by a gold foil as function of the angle . To determine the corrected counting rates N with respect to the scattering distribution in space. To validate the Rutherfords scattering formula Measurement of count rate. within plastic vessel emitter handled rarely by technical staff plastic vessel evacuated (to min 50 Pa) Slide 25 Experiment Radiation Look at different materials and their radioactivity. school experiment sources different materials, e.g. sands, watches, dust-bags Measurement of count rate. sources and other materials handled by presenter and participants Slide 26 Experiment Electron Diffraction Determination of wavelength of the electrons Verification of the de Broglies equation Determination of lattice plane spacings of graphite Measurement through ob- servation of ring radius. high voltage Slide 27 Study of the deflection of electrons in a magnetic field into a circular orbit. Determination of the magnetic field B as a function of the acceleration potential U of the electrons at a constant radius r. Determination of the specific charge of the electron. Measurement through ob- servation of beam radius. nothing specific Slide 28 Experiment Franck-Hertz To record a Franck-Hertz curve for neon. To measure the discontinuous energy emission of free electrons for inelastic collision. To interpret the measurement results as representing discrete energy absorption by neon atoms. To observe the Ne-spectral lines resulting from the electron-collision excitation of neon atoms. To identify the luminance phenomenon as layers with a high probability of excitation. nothing specific