CERN Accelerating science

002207371 001__ 2207371
002207371 003__ SzGeCERN
002207371 005__ 20220810144848.0
002207371 0247_ $$2DOI$$9JACoW$$a10.18429/JACoW-IPAC2016-TUPMW018
002207371 0248_ $$aoai:inspirehep.net:1469930$$pcerncds:CERN:FULLTEXT$$pcerncds:FULLTEXT$$pcerncds:CERN$$qINSPIRE:HEP$$qForCDS
002207371 035__ $$9http://inspirehep.net/oai2d$$aoai:inspirehep.net:1469930$$d2016-08-11T09:22:25Z$$h2016-08-12T04:00:08Z$$mmarcxml
002207371 035__ $$9Inspire$$a1469930
002207371 041__ $$aeng
002207371 088__ $$aCERN-ACC-2016-254
002207371 100__ $$aMartin, [email protected]$$uCERN
002207371 245__ $$aRadiation Load Optimization in the Final Focus System of FCC-hh
002207371 260__ $$c2016
002207371 300__ $$a4 p
002207371 520__ $$9JACoW$$aWith a center-of-mass energy of up to 100 TeV, FCC-hh will produce highly energetic collision debris at the Interaction Point (IP). Protecting the final focus quadrupoles from this radiation is challenging, since the required amount of shielding placed inside the magnets will reduce the free aperture, thereby limiting the β^{*} reach and luminosity. Hence, radiation mitigation strategies that make best use of the available aperture are required. In this paper, we study the possibility to split the first quadrupole Q1 into two quadrupoles with individual apertures, in order to distribute the radiation load more evenly and reduce the peak dose.
002207371 540__ $$3publication$$aCC-BY-3.0$$uhttp://creativecommons.org/licenses/by/3.0/
002207371 542__ $$3publication$$dThe Author(s)$$g2016
002207371 65017 $$2SzGeCERN$$aAccelerators and Storage Rings
002207371 6531_ $$2JACoW$$ashielding
002207371 6531_ $$2JACoW$$aradiation
002207371 6531_ $$2JACoW$$aquadrupole
002207371 6531_ $$2JACoW$$aluminosity
002207371 6531_ $$2JACoW$$aoptics
002207371 690C_ $$aCERN
002207371 700__ $$aBesana, Maria Ilaria$$iINSPIRE-00211473$$jJACoW-00085451$$uCERN
002207371 700__ $$aCerutti, Francesco$$iINSPIRE-00344024$$jJACoW-00032797$$uCERN
002207371 700__ $$aTomás, Rogelio$$iINSPIRE-00286070$$jJACoW-00003672$$uCERN
002207371 710__ $$5ATS
002207371 710__ $$5BE
002207371 773__ $$cTUPMW018$$qIPAC2016$$wC16-05-08$$y2016
002207371 8564_ $$81237913$$s1628769$$uhttp://cds.cern.ch/record/2207371/files/tupmw018.pdf$$yPublished version from JACoW
002207371 960__ $$a13
002207371 962__ $$b2111498$$kTUPMW018$$nbusan20160508
002207371 980__ $$aARTICLE
002207371 980__ $$aConferencePaper
002207371 999C6 $$a0-0-0-1-0-0-1$$t2016-06-16 20:20:23$$vInvenio/1.1.2.1260-aa76f refextract/1.5.44$$vcontent.pdf;1