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The Largest Accelerators and Colliders of Their Time
The Study Group for a GeV-scale Proton Synchrotron was launched in 1952 at CERN. Initially, an up-scaled version of the 3 GeV Cosmotron was considered but soon a new design based on the newly discovered alternating-gradient principle and promising a proton energy of 30 GeV was adopted by the CERN Co...
Autores principales: | , , , , , , , , , |
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Lenguaje: | eng |
Publicado: |
Springer
2020
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Materias: | |
Acceso en línea: | https://dx.doi.org/10.1007/978-3-030-34245-6_10 http://cds.cern.ch/record/2743159 |
_version_ | 1780968586370613248 |
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author | Hübner, K Ivanov, S Steerenberg, R Roser, T Seeman, J Oide, K Mess, Karl Hubert Schmüser, Peter Bailey, R Wenninger, J |
author_facet | Hübner, K Ivanov, S Steerenberg, R Roser, T Seeman, J Oide, K Mess, Karl Hubert Schmüser, Peter Bailey, R Wenninger, J |
author_sort | Hübner, K |
collection | CERN |
description | The Study Group for a GeV-scale Proton Synchrotron was launched in 1952 at CERN. Initially, an up-scaled version of the 3 GeV Cosmotron was considered but soon a new design based on the newly discovered alternating-gradient principle and promising a proton energy of 30 GeV was adopted by the CERN Council in the same year. In order to limit cost the energy was subsequently limited to 25 GeV and the project led by J.B. Adams was approved in 1953. The final parameters were fixed in 1954 and construction started in 1955. The CPS [1] became operational towards the end of 1959 reaching an energy of 28 GeV [2, 3]. It has turned out to be an extremely versatile facility [4] (Table 10.1). |
id | oai-inspirehep.net-1802484 |
institution | Organización Europea para la Investigación Nuclear |
language | eng |
publishDate | 2020 |
publisher | Springer |
record_format | invenio |
spelling | oai-inspirehep.net-18024842020-11-06T15:59:36Zdoi:10.1007/978-3-030-34245-6_10http://cds.cern.ch/record/2743159engHübner, KIvanov, SSteerenberg, RRoser, TSeeman, JOide, KMess, Karl HubertSchmüser, PeterBailey, RWenninger, JThe Largest Accelerators and Colliders of Their TimeAccelerators and Storage RingsThe Study Group for a GeV-scale Proton Synchrotron was launched in 1952 at CERN. Initially, an up-scaled version of the 3 GeV Cosmotron was considered but soon a new design based on the newly discovered alternating-gradient principle and promising a proton energy of 30 GeV was adopted by the CERN Council in the same year. In order to limit cost the energy was subsequently limited to 25 GeV and the project led by J.B. Adams was approved in 1953. The final parameters were fixed in 1954 and construction started in 1955. The CPS [1] became operational towards the end of 1959 reaching an energy of 28 GeV [2, 3]. It has turned out to be an extremely versatile facility [4] (Table 10.1).Springeroai:inspirehep.net:18024842020 |
spellingShingle | Accelerators and Storage Rings Hübner, K Ivanov, S Steerenberg, R Roser, T Seeman, J Oide, K Mess, Karl Hubert Schmüser, Peter Bailey, R Wenninger, J The Largest Accelerators and Colliders of Their Time |
title | The Largest Accelerators and Colliders of Their Time |
title_full | The Largest Accelerators and Colliders of Their Time |
title_fullStr | The Largest Accelerators and Colliders of Their Time |
title_full_unstemmed | The Largest Accelerators and Colliders of Their Time |
title_short | The Largest Accelerators and Colliders of Their Time |
title_sort | largest accelerators and colliders of their time |
topic | Accelerators and Storage Rings |
url | https://dx.doi.org/10.1007/978-3-030-34245-6_10 http://cds.cern.ch/record/2743159 |
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