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DOI:10.18429/JACoW-COOL2015-TUPF01
Title Cooling for a High Luminosity 100 TeV Proton Antiproton Collider
Authors
  • S.J. Oliveros, J.G. Acosta, L.M. Cremaldi, D.J. Summers
    UMiss, University, Mississippi, USA
Abstract A 10³⁴ luminosity 100 TeV proton-antiproton collider is explored. The cross section for many high mass states is 10x higher in p-pbar than p-p collisions. Antiquarks for production can come directly from an antiproton rather than indirectly from gluon splitting. The higher cross sections reduce the synchrotron radiation in superconducting magnets and the vacuum system, because lower beam currents can produce the same rare event rates. Events are also more central, allowing a shorter detector with less space between quadrupole triplets and a smaller beta twiss for higher luminosity. To keep up with the antiproton burn rate, a Fermilab-like antiproton source would be adapted to disperse the beam into 12 different momentum channels, using electrostatic septa, to increase antiproton momentum capture 12x. At Fermilab, antiprotons were stochastically cooled in one debuncher and one accumulator ring. Because the stochastic cooling time scales as the number of particles, 12 independent cooling systems would be used, each one with one debuncher/momentum equalizer ring and two accumulator rings. One electron cooling ring would follow the stochastic cooling rings. Finally antiprotons in the collider ring would be recycled during runs without leaving the collider ring, by joining them to new bunches with snap bunch coalescence and longitudinal synchrotron damping.
Paper download TUPF01.PDF [0.479 MB / 4 pages]
Conference COOL2015, Newport News, VA, USA
Series International Workshop on Beam Cooling and Related Topics (10th)
Proceedings Link to full COOL2015 Proccedings
Session Poster Session II
Date 29-Sep-15   16:50–18:00
Main Classification Stochastic Cooling
Keywords antiproton, collider, luminosity, proton, quadrupole
Publisher JACoW, Geneva, Switzerland
Editors Evelyn (Jefferson Lab) Akers ()
ISBN 978-3-95450-174-8
Published November 2016
Copyright
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