James Blunt at CERN
James Blunt at CERN (Antimatter Factory)
eng
James Blunt;
special;
visit;
music;
;
2017
Imported from Invenio.
Paola Catapano
Noemi Caraban Gonzalez
Michael Struik, CERN;
Maximilien Brice, CERN;
Daniel Barna, Photo-from-above (external footage).
Paola Catapano
The BASE experiment at CERN's Antimatter Factory
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.
eng
AD;
Antimatter;
Factory;
BASE;
antiproton;
Antiproton Decelerator;
Stefan Ulmer;
2017
Imported from Invenio.
CERN Video Productions
Noemi Caraban
AEgIS
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.
eng
antihydrogen;
Antiproton Decelerator;
antimatter; Antiproton Decelerator;
Antimatter Factory;
AEGIS;
2017
Imported from Invenio.
ALPHA first ever optical spectroscopy of a pure anti atom (without text)
The ALPHA experiment at CERN’s antimatter factory reports first ever optical spectroscopy of a pure anti atom.
eng
14.12.16;
2016
Imported from Invenio.
ALPHA first ever optical spectroscopy of a pure anti atom
The ALPHA experiment at CERN’s antimatter factory reports first ever optical spectroscopy of a pure anti atom
eng
ALPHA;
optical spectroscopy;
anti-atom;
2016
Imported from Invenio.
Long interview of Jeffrey Hangs + footage ALPHA
Long interview of the spokesperon Jeffrey Hangs and some footages of ALPHA
eng
alpha;
hangst;
antimatter;
2016
Imported from Invenio.
ELENA
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
eng
decelerator;
ELENA;
ring;
antiproton;
2016
Imported from Invenio.
ASACUSA VNR
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
eng
Antimatter;
Antiprotonc Helium;
ASACUSA;
CPT;
2016
Imported from Invenio.
AD
A unique machine – the Antiproton Decelerator (AD)
eng
Antripoton decelerator;
Antimatter Factory;
AD;
2016
Imported from Invenio.
Live from CERN production
The Antimatter Factory: Live Webcast November 18th and 21st, 2000
Discover the Antiproton Decelerator (or AD, CERN's new "antimatter factory") and find out how physicists are trying to make antimatter, and why.
eng
antimatter;
AD;
2000
http://cds.cern.ch/record/885012/files/AntMatFactory.gif;
http://cds.cern.ch/record/885012/files/AntMatFactory.gif?subformat=icon;
MP4;
http://cern.ch/digital-memory/media-archive/video/open/mp4/CM-A00000370-024.mp4;
Imported from Invenio.
Noemi Caraban
ELENA decelerator
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.
eng
decelerator;
ELENA;
AD;
antimatter;
2016
Imported from Invenio.
ELENA stock Footage
ELENA stock Footage
eng
decelerator;
ELENA;
AD;
antimatter;
2016
Imported from Invenio.
Antimatter Matters
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.
eng
Antihydrogen;
Antimatter;
PET;
LHCb;
CP violation;
ALPHA;
CPT;
2016
Imported from Invenio.
Video News Release ALPHA experiment
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.
eng
antimatter;
neutral charge;
hangst;
vnr;
video news release;
alpha;
2016
http://cds.cern.ch/record/2121327/files/dopesheetJEFF HANGST_ALPHA_Aroll.pdf;
http://cds.cern.ch/record/2121327/files/dopesheetJEFF HANGST_ALPHA_Aroll.jpg?subformat=icon-700;
http://cds.cern.ch/record/2121327/files/dopesheetJEFF HANGST_ALPHA_Aroll.pdf?subformat=pdfa;
http://cds.cern.ch/record/2121327/files/dopesheetJEFF HANGST_ALPHA_Aroll.jpg?subformat=icon-180;
http://cds.cern.ch/record/2121327/files/dopesheetJEFF HANGST_ALPHA_Aroll.gif?subformat=icon;
http://cds.cern.ch/record/2121327/files/DOPESHEET_Hangst_Broll.pdf;
http://cds.cern.ch/record/2121327/files/DOPESHEET_Hangst_Broll.pdf?subformat=pdfa;
http://cds.cern.ch/record/2121327/files/DOPESHEET_Hangst_Broll.jpg?subformat=icon-180;
http://cds.cern.ch/record/2121327/files/DOPESHEET_Hangst_Broll.gif?subformat=icon;
Imported from Invenio.
ALPHA experiment : limit on the charge of antihydrogen atom
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.
eng
alpha;
hangst;
antimatter;
neutral charge;
2016
Imported from Invenio.
Understand antimatter better #13TeV
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
ita
Season2;
Run 2;
Run2;
gopro and photo images;
Barbara Storaci;
2015
Imported from Invenio.
Famelab 2015 CERN Winner Lillian Smestad
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".
eng
FameLab;
Science communication;
Lillian Smestad;
antimatter;
Famelab 2015 CERN;
2015
Imported from Invenio.
More beauty quarks to understand antimatter better Follow LHCb physicist Patrick Koppenburg
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
fre
Interview Patrick Koppenburg;
run 2 promo video;
Interview Mike Flowerdew;
audio;
Gopro Patrick Koppenburng and photo images;
2015
Imported from Invenio.
Where has all the antimatter gone? Interview with Mika Vesterinen
LHC physicists at CERN shares his thoughts about the new physics frontiers opening up when the LHC restarts at higher energy.
eng
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
Imported from Invenio.
More beauty quarks to understand antimatter better - Interview with Patrick Koppenburg
LHCb physicists Patrick Koppenburg shares his thoughts about the new physics frontiers opening up when the LHC restarts at higher energy.
eng
13 TeV;
Antimatter;
Beauty particle;
Beauty Quark;
LHC;
LHCb;
New physics;
Patrick Koppenburg;
Run 2;
Season 2;
2015
Imported from Invenio.
Noemi Caraban
Christoph Madsen
Paola Catapano
Corinne Pralavorio
Where has all the antimatter gone? Interview with Mika Vesterinen
LHCb physicist Mika Vesterinen shares his thoughts about the new physics frontiers opening up when the LHC restarts at higher energy.
eng
13 TeV;
Antimatter;
Antimatter Mystery;
LHC;
LHCb;
Mater Antimatter Asymmetry;
Mika Vesterinen;
New physics;
Run 2;
Season 2;
2015
Imported from Invenio.
ATLAS-antimatter-angels&demons
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.
eng
2012;
Alpha2;
Antimatter;
Bulletin;
Danish Carlsberg Foundation;
Interview;
Jeffrey Hangst;
Laser;
Magnet;
News;
Oxford Instruments;
2012
Imported from Invenio.
CERN Video Productions
CERN Video Productions
ALPHA spokesperson Jeffrey Hangst gives a tour of the new ALPHA-2 french subtitles
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.
eng-fre
2012;
Alpha2;
Antimatter;
Bulletin;
Danish Carlsberg Foundation;
Laser;
Magnet;
News;
Oxford Instruments;
2012
Imported from Invenio.
CERN video productions
CERN video productions
ALPHA spokesperson Jeffrey Hangst gives a tour of the new ALPHA-2 set-up
Interview to Joe Incandela, CMS spokesperson elect, long version
eng
Antimatter;
Backgrounder;
CMS;
Compositeness;
Dark matter;
Extra dimension;
Higgs;
Joe Incandela;
LHC;
Spokesperson;
Supersymmetry;
W prime;
Z prime;
2011
Imported from Invenio.
CERN Visual Media Office
Paola Catapano
Jerome Friedman on the matter antimatter asymmetry
Jerome Friedman explains what is the matter antimatter asymmetry and how LHCb is studying it.
eng
Antimatter;
Backgrounder;
Jerome Friedman;
LHC;
2011
Imported from Invenio.
CERN video productions
CERN video productions
CERN News ASACUSA Experiment
ASACUSA, the Japanese-European ASACUSA experiment at CERN.
eng
LASER;
ASACUSA Experiment;
Antimatter;
vnr;
Anti-protonic atom;
Video News Release;
Masaki Hori;
VNR;
2011
http://cds.cern.ch/record/1367850/files/DOPESHEET_ASACUSA.pdf;
http://cds.cern.ch/record/1367850/files/DOPESHEET_ASACUSA.gif?subformat=icon;
Imported from Invenio.
CERN video productions
CERN video productions
Histoire de l'AD
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.
eng
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
Imported from Invenio.
CERN Video Productions
CERN - AMS teaser
The LHCb experiment, on the quest for the Beauty particle.
eng
shears;
LHCb;
dirac;
antimatter;
2010
Imported from Invenio.
CERN Video Productions
CERN Video Productions
Antimatter atoms produced and trapped at CERN: ALPHA experiment
CERN Bulletin Issue: 48/2010 & 49/2010, Mon 29 Nov 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 ?
eng
Matter;
CERN;
Universe;
Antimatter;
Antihydrogen;
Experiment;
vnr;
Video News Release;
ALPHA;
VNR;
2010
Imported from Invenio.
CERN Video productions
Silvano de Gennaro
CERN News - Aug 2010: AMS, from CERN to Space!
Bulletin Issue: 36/2010 & 37/2010, Mon 06 Sep 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.
eng
ams cern nasa space ting shuttle iss space;
2010
Imported from Invenio.
CERN Video Productions
CERN Video Productions
AMS experiment takes off for Kennedy Space Center August 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.
eng
ISS;
prof. Ting;
Station spatiale internationale;
Alpha Magnetic Spectrometer;
NASA;
ESA;
Kennedy Space Center;
AMS;
2010;
2010
Imported from Invenio.
LHCb OUTREACH
Josiane Uwantege
LHCb Experiment - Footage
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.
eng
International Space Station;
departure;
space shuttle;
NASA;
interview;
AMS;
Samuel Ting;
2010;
2010
Imported from Invenio.
CERN Video Productions
Interview with Andrei Golutvin, LHCb Spokesperson
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?
eng
2009;
Andrei Golutvin;
Interview;
LHC;
LHCb;
LHCFirstPhysics;
Restart;
2009
Imported from Invenio.
CERN
Peut-on voler de l'antimatiere Can antimatter be stolen? (french subtitles)
Avec <b>Rolf Landua</b>
eng
antimatter;
2009
Imported from Invenio.
Cern Audiovisual Service
Why does CERN study antimatter?- French subtitles
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?
eng-fre
globe;
exposition;
2009
Imported from Invenio.
CERN Multimedia Productions
Silvano de Gennaro
"Why does CERN study antimatter?" - with Michael Doser
Angels and Demons: the science behind the story
Physicist Michael Doser replies to questions related to the movie "Angels & Demons"
eng
Michael Doser;
Angels & Demons;
Antimatter;
2009
Imported from Invenio.
CERN Multimedia Productions
Silvano de Gennaro
Paola Catapano
Silvano de Gennaro; Josiane Uwantege
Josiane Uwantege
"Can Antimatter be stolen?"- with Rolf Landua
Angels and Demons: the science behind the story
Physicist Rolf Landua replies to questions related to the movie "Angels & Demons"
eng
Angels & Demons;
Rolf Landua;
Antimatter;
2009
Imported from Invenio.
CERN Multimedia Productions
Silvano de Gennaro
Paola Catapano
Silvano de Gennaro; Josiane Uwantege
Josiane Uwantege
"Do we make antimatter at CERN?"- with Rolf Landua
Angels and Demons: the science behind the story
Physicist Rolf Landua replies to questions related to the movie "Angels & Demons"
eng
Angels & Demons;
Rolf Landua;
Antimatter;
2009
Imported from Invenio.
CERN Audiovisual Service
CERN Audiovisual Unit
Video News Release Athena and Atrap experiments at the AD
<!--HTML-->Interview with <b>Tom Ypsilantis and Mario Macri</b>.
eng
AD;
webcast;
antimatiere;
webcast;
antimatiere;
antimatter;
AD;
2000
Imported from Invenio.
"A passion for precision" : colloquium given by Theodor Hänsch, who shared the 2005 Nobel Prize in Physics for his contributions to the development of laser-based precision spectroscopy.
The Nobel Prize in Physics 2005
<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.
eng
Nobel laureate;
Theodor Hänsch;
2006
http://cds.cern.ch/record/964279/files/icon-cern-movie-2006-01.gif;
http://cds.cern.ch/record/964279/files/icon-cern-movie-2006-01.gif?subformat=icon;
Imported from Invenio.
Live from CERN production
Antimatter : Mirror of the Universe: Live Webcast May 10th, 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.
eng
antimatter;
AD;
2000
http://cds.cern.ch/record/886084/files/AntMirrUniverse.gif;
http://cds.cern.ch/record/886084/files/AntMirrUniverse.gif?subformat=icon;
MP4;
http://cern.ch/digital-memory/media-archive/video/open/mp4/ac_S1V1_CM-A00000373-038.mp4;
Imported from Invenio.