DAFNE Operating Experience With Crab Waist Collisions

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DAFNE OPERATING EXPERIENCE WITH CRAB WAIST COLLISIONS

DAΦNE OPERATING EXPERIENCE WITH CRAB WAIST COLLISIONS M. Zobov, INFN Laboratori Nazionali di Frascati, Frascati, Italy for DAΦNE Collaboration Team[1] Abstract The Φ-factory DAΦNE was upgraded in the second half of 2007 in order to implement a recently proposed scheme of crab waist collisions aimed at substantial luminosity increase.

THE SUPERB-FACTORY ACCELERATOR PROJECT

the newly proposed crab waist method. A Conceptual Design Report has been published in April this year. A review of the design principles and of the project status will be given. INTRODUCTION A Super B-Factory like SuperB , an asymmetric energy e+ e-collider with a luminosity of the order 1036 cm-2 s-1,

th ICFA Advanced Beam Dynamics Workshop on High Luminosity e

The KEKB status is described focusing on the beam operation with crab crossing. This report deals mainly with the beam dynamics issues with crab crossing. There is a large discrepancy between the beam-beam simulation and the experiment at the high bunch currents. We discuss causes of this discrepancy in detail.

Experience with DANE Upgrade Including Crab Waist

EXPERIENCE WITH DA!NE UPGRADE INCLUDING CRAB WAIST C. Milardi for the DA!NE Commissioning Team*, LNF-INFN, Frascati, Italy. Abstract In 2007 DA!NE was upgraded to operate in a regime

Status of the SuperB project

The effect of the Crab Waist sextupoles of the beam profiles are displayed in fig. 3. The tune space, which was previously heavily populated by beam killing resonances, offers now very large resonance-free zones (see [3], p. 54). The crab waist scheme was very successfully demonstrated on the DAFNE storage ring in 2008-2009 [4].

SIMULATION OF CRAB WAIST COLLISIONS IN DAΦNE WITH KLOE-2

which is a double ring electron-positron collider operating at the c.m. energy of the Φ-resonance (1.02 GeV) [1]. The implementation of the Crab Waist collision scheme (CW) has led to the achievement of the record peak luminosity L=4.5×1032 cm-2s-1 while working for the SIDDHARTA experiment [2]. This success has led to a