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NA61/Shine

Skip to main content. History of the Collaboration. Hotels in the area. The NA61/SHINE detector allows for precise measurements of properties of particles, produced in collisions of hadrons and atomic nuclei. The experiment is located in the North Area of CERN and the particles are accelerated by SPS. Central collision of two beryllium nuclei ' photographed' by our detector. We perform precise measurements needed in studies of neutrino and cosmic-ray properties. Lorem ipsum dolor sit amet, consectetur ad...

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NA61/Shine | shine.web.cern.ch Reviews

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Skip to main content. History of the Collaboration. Hotels in the area. The NA61/SHINE detector allows for precise measurements of properties of particles, produced in collisions of hadrons and atomic nuclei. The experiment is located in the North Area of CERN and the particles are accelerated by SPS. Central collision of two beryllium nuclei ' photographed' by our detector. We perform precise measurements needed in studies of neutrino and cosmic-ray properties. Lorem ipsum dolor sit amet, consectetur ad...

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1 cern accelerating science

2 directory

3 about us

4 collaboration structure

5 institutions

6 author list

7 physics

8 strong interactions

9 neutrinos

10 cosmic rays

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NA61/Shine | shine.web.cern.ch Reviews

https://shine.web.cern.ch

Skip to main content. History of the Collaboration. Hotels in the area. The NA61/SHINE detector allows for precise measurements of properties of particles, produced in collisions of hadrons and atomic nuclei. The experiment is located in the North Area of CERN and the particles are accelerated by SPS. Central collision of two beryllium nuclei ' photographed' by our detector. We perform precise measurements needed in studies of neutrino and cosmic-ray properties. Lorem ipsum dolor sit amet, consectetur ad...

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shine.web.cern.ch

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Time of flight | NA61/Shine

http://shine.web.cern.ch/content/time-flight

Skip to main content. History of the Collaboration. Hotels in the area. Two walls, ToF-L(eft) and ToF-R(ight), of 4.4 m. Ported to Drupal by Drupalizing. A Project of More than (just) Themes. Designed by Zsolt Kacso.

2

Physics | NA61/Shine

http://shine.web.cern.ch/content/physics

Skip to main content. History of the Collaboration. Hotels in the area. The NA61/SHINE team uses beams of hadrons and nuclei from the Super Proton Synchrotron (SPS) to measure production of hadrons in three different types of collisions:. Nucleus-nucleus, proton-proton and proton-nucleus collisions are used. By NA61/SHINE to investigate properties of the transition between. The quark-gluon plasma and hadron gas by collision energy scans. Within the programme on strong interactions. Designed by Zsolt Kacso.

3

Data acquisition | NA61/Shine

http://shine.web.cern.ch/content/data-acquisition

Skip to main content. History of the Collaboration. Hotels in the area. The readout electronics consists of three main subsystems: the part responsible for reading out the TPC Front-End Electronics, the part for reading out the FASTBUS based ToF system, and the part for reading out the CAMAC based beam detectors. Further reading with more details:. Nuclear Instruments and Methods in Physics Research. Https:/ twiki.cern.ch/twiki/bin/viewauth/NA61/WebHome#DAQ. Ported to Drupal by Drupalizing.

4

Strong Interactions | NA61/Shine

http://shine.web.cern.ch/content/strong-interactions

Skip to main content. History of the Collaboration. Hotels in the area. NA61/SHINE is the successor experiment of NA49 which studied the energy dependence of hadron production in Pb Pb interactions. Within this programme, the threshold for the quark-gluon plasma creation -. The onset of deconfinement. On the transition line between two phases of strongly interacting matter: quark-gluon plasma and hadron gas. A strong maximum of the ratio of K. A change of a slope of negatively charged hadrons multiplicit...

5

Author List | NA61/Shine

http://shine.web.cern.ch/content/author-list

Skip to main content. History of the Collaboration. Hotels in the area. Ported to Drupal by Drupalizing. A Project of More than (just) Themes. Designed by Zsolt Kacso.

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be-dep-op-sps.web.cern.ch

SPS Facilities | <SPS Operation Website...> <big>BE-OP-SPS Operations</big>

http://be-dep-op-sps.web.cern.ch/content/sps-facilities

Skip to main content. Think like a proton always positive since 1976. Old SPS OP Site.

guydoyen.fr

2015 février @ Guy DOYEN

http://guydoyen.fr/2015/02

Pour rendre la richesse du Web mondial accessible aux francophones. Un gigantesque trou noir supermassif défie les théories concernant l’évolution des trous noirs. Posté le 28th février 2015. Ce trou noir supermassif, 12 milliards de fois plus massif que notre Soleil, a été découvert en 2013 par des astronomes utilisant le télescope Lijiang situé à Yunnan (Chine). Il pose un défi aux théories actuelles concernant l’évolution des trous noirs car il est à la fois très jeune et extrêmement massif. On pense ...

www-hep.colorado.edu

University of Colorado Experimental High Energy Physics

http://www-hep.colorado.edu/experimental

University of Colorado Experimental High Energy Physics. CU A to Z. University of Colorado High Energy Experimental Physics. The University of Colorado. High energy experimental physics group has eight faculty members: John Cumalat. And Uriel Nauenberg (emeritus). The group is currently involved in several experiments:. Six faculty members are currently working on CMS. The group is currently working on several physics topics including searches for supersymmetry ( Ford. In addition, Stenson. NA61/SHINE is...

advance.colorado.edu

University of Colorado Experimental High Energy Physics

https://advance.colorado.edu/experimental

University of Colorado Experimental High Energy Physics. CU A to Z. University of Colorado High Energy Experimental Physics. The University of Colorado. High energy experimental physics group has eight faculty members: John Cumalat. And Uriel Nauenberg (emeritus). The group is currently involved in several experiments:. Six faculty members are currently working on CMS. The group is currently working on several physics topics including searches for supersymmetry ( Ford. In addition, Stenson. NA61/SHINE is...

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shine.web.cern.ch

NA61/Shine

Skip to main content. History of the Collaboration. Hotels in the area. The NA61/SHINE detector allows for precise measurements of properties of particles, produced in collisions of hadrons and atomic nuclei. The experiment is located in the North Area of CERN and the particles are accelerated by SPS. Central collision of two beryllium nuclei ' photographed' by our detector. We perform precise measurements needed in studies of neutrino and cosmic-ray properties. Lorem ipsum dolor sit amet, consectetur ad...

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University of St Andrews. Celebrating the International Year of Light in St Andrews with Science, Art and Music. Open Night at the Observatory. Tuesday March 17, 2015. Alastair Hodson and Rémy Köth demonstrating our pulsar keyboard during Science Discovery Day (credit: Carolin Villforth). It is now a bit more than a week ago that we celebrated an Open Night at the University Observatory. The St Andrews Brass Quintet performing ‘Auriga’ by composer Eddie McGuire (credit: Carolin Villforth). Your feedback ...

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