James Blunt special visit music 2017 2017 James Blunt at CERN (Antimatter Factory) Paola Catapano Noemi Caraban Gonzalez Michael Struik, CERN; Maximilien Brice, CERN; Daniel Barna, Photo-from-above (external footage). Paola Catapano AD Antimatter Factory BASE antiproton Antiproton Decelerator Stefan Ulmer 2017 2017 BASE is one of the experiments at CERN's Antimatter Factory. The video fotage starts with an aerial (drone) view of the Antimatter Factory building seen from outside (00'01''); the flight continues inside over the experimental area with an overview of the Alfa and ASACUSA experiments (00'13''); finally the drone flies over the BASE experiment (00'19''), where spokesperson Stefan Ulmer can be seen (00'25'') inserting a Nitrogen level metre inside BASE's cryostat. This probe is used to measure the level of Nitrogen in the vessel. BASE uses liquid Nitrogen and liquid Heliumto keep its penning trap cold, which is necessary to prevent its anti-protons to annihilate. CERN Video Productions Noemi Caraban antihydrogen Antiproton Decelerator antimatter; Antiproton Decelerator Antimatter Factory AEGIS 2017 2017 During technical stop 2017 the AEgIS experiment was open for upgrades and maintenance. We had the opportunity to take some 360 images from inside and see where antiprotons are ¨trapped¨ and anti-Hydrogen produced. 14.12.16 2016 2016 The ALPHA experiment at CERN’s antimatter factory reports first ever optical spectroscopy of a pure anti atom. ALPHA optical spectroscopy anti-atom 2016 2016 The ALPHA experiment at CERN’s antimatter factory reports first ever optical spectroscopy of a pure anti atom alpha hangst antimatter 2016 2016 Long interview of the spokesperon Jeffrey Hangs and some footages of ALPHA decelerator ELENA ring antiproton 2016 2016 ELENA is a compact ring for cooling and further deceleration of 5.3 MeV antiprotons delivered by the CERN Antiproton Decelerator. The AD physics program is focused on trapping antiprotons in Penning traps where antihydrogen is formed after recombination with positrons. The ultimate physics goal is to perform spectroscopy on antihydrogen atoms at rest and to investigate the effect of the gravitational force on matter and antimatter. In today’s set-up, most (99.9%) of the antiprotons produced are lost due to the use ofdegrader foils needed to decelerate them from the AD ejection energy down to around 5 keV; an energy suitable for trapping. By using a ring equipped with beam cooling, high deceleration efficiency and an important increase in phase-space density can be obtained, resulting in an increased number of trapped antiprotons. For the ATRAP and ALPHA experiments, improvements of up to 2 orders of magnitude can be expected. The same holds for the AEGIS experiment which is currently b Antimatter ASACUSA 2016 2016 CERN Audiovisual Production Service Jacques Fichet, Paola Catapano Julien Ordan, Arzur Catel Paola Catapano ASACUSA COLLABORATION Antimatter Antiprotonc Helium ASACUSA CPT 2016 2016 Latest precision measurement of the mass of the proton and the anti proton though the production of antiprotonic helium by the ASACUSA experiment at CERN's antimatter factory, with a beam from the Antiproton Decelerator Antripoton decelerator Antimatter Factory AD 2016 2016 A unique machine – the Antiproton Decelerator (AD) Live from CERN production antimatter AD 2000 2000 Discover the Antiproton Decelerator (or AD, CERN's new "antimatter factory") and find out how physicists are trying to make antimatter, and why. Noemi Caraban decelerator ELENA AD antimatter 2016 2016 Footage taken during the preparation of the ELENA decelerator. With a circumference of about 30 m, ELENA can be located in the AD hall where assembly and commissioning would not disturb the current AD operation. decelerator ELENA AD antimatter 2016 2016 ELENA stock Footage Antihydrogen Antimatter PET LHCb CP violation ALPHA CPT 2016 2016 This video is a teaser-introduction to the Antimatter Matters exhibtion at the Royal Society's Summer Science exhibition July 4-10 2016. The exhibition is jointly organised and hosted by UK members of the ALPHA and LHCb collaborations. antimatter neutral charge hangst vnr video news release alpha 2016 2016 Antimatter continues to intrigue physicists due to its apparent absence in the observable universe. Current theory requires that matter and antimatter should have appeared in equal quantities after the Big Bang, but the Stan- dard Model offers no quantitative explanation for the apparent disappearance of half of the universe. It has recently become possible to study trapped atoms1–4 of antihydrogen to search for possible, as yet unobserved, differences in the physical behaviour of matter and antimatter. alpha hangst antimatter neutral charge 2016 2016 Antimatter continues to intrigue physicists due to its apparent absence in the observable universe. Current theory requires that matter and antimatter should have appeared in equal quantities after the Big Bang, but the Stan- dard Model offers no quantitative explanation for the apparent disappearance of half of the universe. It has recently become possible to study trapped atoms1–4 of antihydrogen to search for possible, as yet unobserved, differences in the physical behaviour of matter and antimatter. Season2 Run 2 Run2 gopro and photo images Barbara Storaci 2015 2015 Follow Italian @LHCbexperiment physicist Barbara Storaci from the University of Zürich, Switzerland, as she shares her thoughts about the new physics frontiers opening up now that the LHC has collisions at the higher energy of #13TeV. Each week a new video will be uploaded to https://www.youtube.com/playlist?list... allowing you to follow physicists from @ATLASexperiment @ALICEexperiment @CMSexperiment or @LHCbExperiment as they search the new frontiers in physics. Read more about these new frontiers in physics: http://cern.ch/go/x8VH FameLab Science communication Lillian Smestad antimatter Famelab 2015 CERN 2015 2015 Final talk by CERN Winner Lillian Smestad, Norwegian Research Council and CERN, at the Famleab 2015 competition, on the subjet of "The Unfamiliar Twin of Matter". Interview Patrick Koppenburg run 2 promo video Interview Mike Flowerdew audio Gopro Patrick Koppenburng and photo images 2015 2015 Follow Swiss @LHCbExperiment physicist @PKoppenburg from Nikhef National institute for subatomic physics in the Netherlands, as he shares his thoughts about the new physics frontiers opening up when the LHC begins collisions at the higher energy of #13TeV. Each week a new video will be uploaded to https://www.youtube.com/playlist?list... allowing you to follow physicists from @ATLASexperiment @ALICEexperiment @CMSexperiment or @LHCbExperiment as the search the new frontiers in physics. Read more about these new frontiers in physics: http://cern.ch/go/x8VH run 2 promo video run2 Mika Vesterinen Social Media MASTER OLD 12.02.15 antimatter LHC season 2 Mika Vesterinen Social Media Interview LHC run2 LHCb gopro and photo images 13 TeV 2015 2015 LHC physicists at CERN shares his thoughts about the new physics frontiers opening up when the LHC restarts at higher energy. 13 TeV Antimatter Beauty particle Beauty Quark LHC LHCb New physics Patrick Koppenburg Run 2 Season 2 2015 2015 LHCb physicists Patrick Koppenburg shares his thoughts about the new physics frontiers opening up when the LHC restarts at higher energy. Noemi Caraban Christoph Madsen Paola Catapano Corinne Pralavorio 13 TeV Antimatter Antimatter Mystery LHC LHCb Mater Antimatter Asymmetry Mika Vesterinen New physics Run 2 Season 2 2015 2015 LHCb physicist Mika Vesterinen shares his thoughts about the new physics frontiers opening up when the LHC restarts at higher energy. Atlas cern angels&demons Cern experiment atlas 2013 2013 CERN Video Productions CERN Video Productions 2012 Alpha2 Antimatter Bulletin Danish Carlsberg Foundation Interview Jeffrey Hangst Laser Magnet News Oxford Instruments 2012 2012 While many experiments are methodically planning for intense works over the long shutdown, there is one experiment that is already working at full steam: ALPHA-2. Its final components arrived last month and will completely replace the previous ALPHA set-up. Unlike its predecessor, this next generation experiment has been specifically designed to measure the properties of antimatter. CERN Video Productions CERN Video Productions 2012 Alpha2 Antimatter Bulletin Danish Carlsberg Foundation Laser Magnet News Oxford Instruments 2012 2012 Alors qu’un grand nombre d’expériences se préparent à un rythme de travail soutenu pendant la longue période d’arrêt, il en est une dont l’activité est déjà intense : ALPHA-2. Les derniers éléments, qui sont arrivés le mois dernier, vont permettre de remplacer complètement le dispositif expérimental ALPHA. À la différence de celle qui l’a précédée, cette expérience a été spécialement conçue pour mesurer les propriétés de l’antimatière. CERN video productions CERN video productions Alpha2 Antimatter Bulletin Danish Carlsberg Foundation Laser Magnet News Oxford Instruments 2012 2012 CERN video productions CERN video productions Alpha Antimatter Magnet Oxford 2012 2012 CERN video productions CERN video productions ALPHA2 CERN anti-hydrogen antimatter news 2012 2012 CERN video productions CERN video productions nature anti-hydrogen antimatter VNR ALPHA vnr 2012 2012 CERN video productions CERN video productions Welcome to the ALPHA experiment nature anti-hydrogen antimatter hangst measure quantum ALPHA hydrogen animation 2012 2012 CERN Visual Media Office Paola Catapano Antimatter Backgrounder CMS Compositeness Dark matter Extra dimension Higgs Joe Incandela LHC Spokesperson Supersymmetry W prime Z prime 2011 2011 Interview to Joe Incandela, CMS spokesperson elect, long version CERN Visual Media Office Paola Catapano Antimatter Backgrounder Jerome Friedman LHC 2011 2011 Jerome Friedman explains what is the matter antimatter asymmetry and how LHCb is studying it. CERN video productions CERN video productions Antimatter Antiproton ASACUSA Bulletin CERN News Decelerator Electron Masaki Hori Mass Matter Planck Proton Subtitles 2011 2011 CERN video productions CERN video productions Antimatter Antiproton ASACUSA Bulletin CERN News Decelerator Electron Masaki Hori Mass Matter Planck Proton 2011 2011 CERN video productions CERN video productions DOPESHEET_ASACUSA.pdf LASER ASACUSA Experiment Antimatter vnr Anti-protonic atom Video News Release Masaki Hori VNR 2011 2011 ASACUSA, the Japanese-European ASACUSA experiment at CERN. CERN video productions CERN video productions AD anti-proton anti-electron antimatter bulletin anti-protons Bulletin 2011 2011 CERN Video Productions Antihydrogen CERN News Jeffrey Hangst ALPHA Experiment Antimatter 2011 2011 CERN Video Productions Antihydrogen Universe Jeffrey Hangst Antimatter Matter vnr Video News Release ALPHA Experiment VNR 2011 2011 CERN Video Productions CERN Video Productions endeavour black matter launch CERN space antimatter astronauts ISS NASA astroparticle shuttle AMS physics detector 2011 2011 CERN Video Productions antimatière May 16th, 2011 launch dark matter antimatter NASA AMS matière noire 2011 2011 CERN Video Productions CERN Video Productions Roberto Battiston Endeavour Maurice Bourquin CERN universe STS-134 antimatter cosmic rays April 29th, 2011 Alpha Magnetic Spectrometer dark matter Live NASA VNR Video News Release ISS AMS Martin Pohl Rolf Heuer 2011 2011 antimatière dark matter antimatter NASA AMS Samuel Ting matière noire 2011 2011 CERN Video Productions antimatière dark matter antimatter NASA AMS Samuel Ting matière noire 2011 2011 CERN Video Productions Roberto Battiston Endeavour Maurice Bourquin CERN universe STS-134 antimatter cosmic rays Alpha Magnetic Spectrometer black matter NASA vnr Video News Release ISS AMS Martin Pohl Rolf Heuer VNR 2011 2011 The AMS particle detector will take off on 29 April 2011 at 21.47 CEST onboard the very last mission of the space Shuttle Endeavour. AMS, the Alpha Magnetic Spectrometer, will then be installed on the International Space Station from where it will explore the Universe for a period of over 10 years. AMS will address some of the most exciting mysteries of modern physics, looking for antimatter and dark matter in space, phenomena that have remained elusive up to now. CERN Video Productions antimatière dark matter antimatter April 29th, 2011 NASA AMS matière noire 2011 2011 CERN Video Productions antimatière dark matter antimatter NASA AMS Martin Pohl matière noire 2011 2011 CERN Video Productions antimatière dark matter antimatter NASA AMS Martin Pohl matière noire 2011 2011 CERN Video Productions antimatière dark matter antimatter Sylvie Rosier-Lees NASA matière noire AMS 2011 2011 CERN Video Productions antimatière Maurice Bourquin dark matter antimatter NASA AMS matière noire 2011 2011 CERN Video Productions antimatière AMS dark matter antimatter NASA Rolf Heuer matière noire 2011 2011 CERN Video Productions antimatière dark matter antimatter Roberto Battiston NASA AMS matière noire 2011 2011 Visual Media Office Josiane Uwantege Silvano de Gennaro shears LHCb dirac antimatter 2010 2010 The LHCb experiment, on the quest for the Beauty particle. CERN Video Productions CERN Video Productions CERN Bulletin Issue: 48/2010 & 49/2010, Mon 29 Nov 2010 antimatière universe Jeffrey Hangst antimatter big bang matter atom ALPHA hydrogen 2010 2010 ALPHA Collaboration Chris Robbins, Grallator antihydrogen ALPHA animation antimatter matter 2010 2010 ALPHA collaboration Chris Robbins, Grallator antihydrogen ALPHA antimatter matter 2010 2010 CERN Video Productions CERN Video Productions About ALPHA -Antihydrogen Laser PHysics Apparatus Matter CERN Universe Antimatter Antihydrogen Experiment vnr Video News Release ALPHA VNR 2010 2010 - What is antimatter ? - What are you doing with the ALPHA experiment ? What's new about it ? - What is the purpose of research with antimatter ? - How many people work on ALPHA ? What is the budget ? - Can you describe the apparatus here at CERN ? - How do you know you have made antihydrogen ? CERN Video productions Silvano de Gennaro Bulletin Issue: 36/2010 & 37/2010, Mon 06 Sep 2010 ams cern nasa space ting shuttle iss space 2010 2010 The Alpha Magnetic Spectrometer leaves CERN to embark on a USAF plane, on its journey to Cape Canaveral, and then Space. It will be installed on the International Space Station next year, where it will look for antimatter in Space. CERN Video Productions CERN Video Productions ISS prof. Ting Station spatiale internationale Alpha Magnetic Spectrometer NASA ESA Kennedy Space Center AMS 2010 2010 2010 Geneva, 18 August 2010. The Alpha Magnetic Spectrometer (AMS), an experiment that will search for antimatter and dark matter in space, leaves CERN next Tuesday on the next leg of its journey to the International Space Station. The AMS detector is being transported from CERN to Geneva International Airport in preparation for its planned departure from Switzerland on 26 August, when it will be flown to the Kennedy Space Center in Florida on board a US Air Force Galaxy transport aircraft. LHCb OUTREACH Josiane Uwantege Andrey Goloutvin Beauty particules control room symmetry lhcfirstphysics antimatter Big Bang matter LHCb physicists animations interview collider detector physics 2010 2010 2010 CERN Video Productions CERN Video Productions CERN Press Release - AMS experiment embarks on first leg of mission into space International Space Station departure space shuttle NASA interview AMS Samuel Ting 2010 2010 2010 Geneva, 12 February 2010. The Alpha Magnetic Spectrometer (AMS) left CERN1 this morning on the first leg of its journey to the International Space Station (ISS). A special convoy carrying the experiment is due to arrive at the European Space Agency's research and technology centre, ESTEC, at Noordwijk in the Netherlands in six days time. Once there, the detector will undergo testing of its ability to survive a shuttle lift-off and to operate in space. Twenty members of the AMS collaboration will accompany the detector on its journey. Construction of the AMS detector components was carried out by an international team with significant contributions from CERN Member States France, Germany, Italy, Portugal Spain and Switzerland, as well as China, China (Taipei) and the USA. Assembly was carried out at CERN with help from the Laboratory’s engineering services. From 4 February until Tuesday morning, the detector was put through its paces using a test beam from the Super Proton Synchrotron accelerator. This was the first of a series of tests on the fully assembled detector and it gave excellent results, demonstrating AMS’s ability to work as a coherent whole once it reaches space. A beam of primary protons from the SPS was used to check the detector’s momentum resolution, and it qualified the spectrometer’s ability to measure particle curvature and momentum. AMS’s ability to distinguish electrons from protons was also tested. This is very important for the measurement of cosmic rays, 90% of which are protons and constitute a natural background for other signals that AMS scientists are interested in. AMS will be looking for an abundance of positrons and electrons from space, one of the possible markers for dark matter. AMS being prepared for transport Once at ESTEC, AMS will be placed in ESA’s thermo vacuum room that simulates space vacuum to test the detector’s capacity of exchanging heat and thus maintain its thermal balance, which is essential for the functioning of the detector’s electronics and especially of its unique superconducting magnet, which is the first of its kind to be launched into space. “This is a very important milestone for AMS, as it’s the first time that it is going to be tested in vacuum. After the test, AMS may come back to CERN for a final check and then it’s off to the Kennedy Space Center for launch,” said the experiment’s Nobel-prize winning spokesman, Professor Sam Ting. “The contribution of CERN has been crucial. Without the work of CERN’s accelerator, magnet and vacuum groups we wouldn’t be at this stage here today.” AMS will leave ESTEC towards the end of May aboard a special US Air Force flight to the Kennedy Space Center in Florida. Lift-off aboard the space shuttle Discovery is scheduled for July. Once docked to the ISS, AMS will examine fundamental issues about matter and the origin and structure of the Universe directly from space. Its main scientific target is the search for dark matter and antimatter in a programme that is complementary to that of the Large Hadron Collider. AMS data from space will be transmitted from the ISS to Houston, USA, and on to CERN, where the detector control centre will be located, and a number of regional physics analysis centres set up by the collaborating institutes. CERN Video Productions 2009 Andrei Golutvin Interview LHC LHCb LHCFirstPhysics Restart 2009 2009 Questions : 1. How does it feel to be the Spokesperson of a large worldwide collaboration as LHCb at the very moment when the LHC is going to produce the first data? 2. Is your detector ready for the data taking? 3. Did you take advantage of the long shut down? 4. What was the LHCb detector designed for and why is it different from the other ones? 5. What can you expect to find at 3.5 TeV and later at 7 per beam? 6. Is Andrei Sakarov's theory on matter and antimatter asymetry a guiding line for you? 7. What is going to happen in the LHCb control room on collision day? CERN stolen Antimatter 2009 2009 CERN Audio Visual Service antimatter 2009 2009 Avec <b>Rolf Landua</b> Cern Audiovisual Service Antimatter 2009 2009 CERN audiovisual service CERN audiovisual service globe exposition 2009 2009 Angels & Demons – the science behind the story. A race against the clock to prevent antimatter stolen from CERN from blowing up the Vatican: following a tried and tested Hollywood formula, the 'ticking-bomb' thriller, Angles & Demons can hardly fail to entertain. But how does the science stand up to scrutiny? CERN Multimedia Productions Silvano de Gennaro Angels and Demons: the science behind the story Michael Doser Angels & Demons Antimatter 2009 2009 Physicist Michael Doser replies to questions related to the movie "Angels & Demons" CERN Multimedia Productions Silvano de Gennaro Paola Catapano Silvano de Gennaro; Josiane Uwantege Josiane Uwantege Angels and Demons: the science behind the story Angels & Demons Rolf Landua Antimatter 2009 2009 Physicist Rolf Landua replies to questions related to the movie "Angels & Demons" CERN Multimedia Productions Silvano de Gennaro Paola Catapano Silvano de Gennaro; Josiane Uwantege Josiane Uwantege Angels and Demons: the science behind the story Angels & Demons Rolf Landua Antimatter 2009 2009 Physicist Rolf Landua replies to questions related to the movie "Angels & Demons" CERN Audiovisual Service CERN Audiovisual Unit CERN Antimatter Factory AD antihydrogen antimatter experiment news Atrap Antiproton Decelerator Athena 2004 2004 Multimedia Productions Silvano Michele de Gennaro antimatiere antimatiere Antimatter AD 2000 2000 Silvano Michele de Gennaro AD webcast antimatiere webcast antimatiere antimatter AD 2000 2000 <!--HTML-->Interview with <b>Tom Ypsilantis and Mario Macri</b>. The Nobel Prize in Physics 2005 Nobel laureate Theodor Hänsch 2006 2006 <HTML>Currently, Hänsch is also working with the ATRAP Collaboration at CERN, which is studying hydrogen and antihydrogen atoms. If it were possible to measure precisely up to 14 or 15 digits, then it might be possible to see whether matter and antimatter are the same or if they differ in some unexpected way. This could explain why there is more matter than antimatter in the universe. To explore these questions, researchers have to look where no-one has ever looked before, and for that reason, Hänsch has a passion for precision. Live from CERN production antimatter AD 2000 2000 Find out from CERN physicists Alvaro de Rújula, Rolf Landua and Tommy Eriksson the theoretical, experimental and technical aspects of CERN's new antimatter adventure.