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Lett. , J. Abdallah et al, Euro. Phys. Jour. , M. Acciarri et al, Phys. Lett. , G. Abbiendi et al, Euro. Phys. Jour. C26 “2003“ 479 ALEPH, DELPHI, L3 and OPAL Collaborations & the LEP Working Group for Higgs “ oson Searches, Phys. Lett. B565 “2003“ 61 28. F. Abe et al, Phys. Rev. D50 “1994“ 2966“ Phys. Rev. 73 “1994“ 225 29. S. Abachi et al, Phys. Rev. 74 “1995“ 2632 30. Erich W. “ arnes, “Top “ uark Physics”, Plenary talk at the 34th Intern. Conf. on High Energy Physics, Philadelphia, PA, 29 July to 5 August, 2008 Accelerator Physics and Technological Challenges of the LHC Oliver Br¨ uning, Vinod Chohana and Swapan Chattopadhyayb a CERN, Geneva, Switzerland b Cockcroft Institute, Daresbury, Cheshire, United Kingdom The LHC at CERN has completed its construction in summer 2008.

Most important innovations and strategies which essentially helped in achieving a high throughput included the introduction of a template based tests approach, web-based tools for tests management, magnet training rules and criteria for 24-hour operator decision taking and empowerment, general and cryogenic priorities handling by the shift crew, thermal cycle criteria and so forth. For the final, smooth operation of the facility with 12 benches, it was necessary to ensure a minimum staff strength of 24 at any time, comprising at least 15 experienced staff; however, the staff strength had to be appropriately adjusted according to the expected departures, arrivals and experience as and when required.

Furthermore, the webbased network backbone of CERN and computer facilities have been widely used for developing the supporting tools. Most important innovations and strategies which essentially helped in achieving a high throughput included the introduction of a template based tests approach, web-based tools for tests management, magnet training rules and criteria for 24-hour operator decision taking and empowerment, general and cryogenic priorities handling by the shift crew, thermal cycle criteria and so forth.

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Absurdity of the calculation of the intensity of gravitational radiation in the general theory of relativity


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