Beamstrahlung on the Septum Blade Karsten Büßer 01.04.2003 ECFA/DESY Workshop Amsterdam The Extraction Line Problem Beamstrahlung Incoming Beam Outgoing Beam 01.04.2003 Karsten Büßer - Beamstrahlung on the Septum Blade ECFA/DESY.
Download ReportTranscript Beamstrahlung on the Septum Blade Karsten Büßer 01.04.2003 ECFA/DESY Workshop Amsterdam The Extraction Line Problem Beamstrahlung Incoming Beam Outgoing Beam 01.04.2003 Karsten Büßer - Beamstrahlung on the Septum Blade ECFA/DESY.
Beamstrahlung on the Septum Blade Karsten Büßer 01.04.2003 ECFA/DESY Workshop Amsterdam The Extraction Line Problem Beamstrahlung Incoming Beam Outgoing Beam 01.04.2003 Karsten Büßer - Beamstrahlung on the Septum Blade ECFA/DESY Workshop Amsterdam 2 Beamstrahlung Distributions N. Walker (Prague): Realistic Beam Effect of 10 σ offset Expectation: Power on septum blade can reach several kW 01.04.2003 Karsten Büßer - Beamstrahlung on the Septum Blade ECFA/DESY Workshop Amsterdam 3 Questions Formation of a working group to revisit the design of the extraction line. First Meeting on December 3rd 2002 identified the following questions: • Septum magnet design • Failure modes • What power can the thin blade cope with ? • Reliability of electro-static separators • IR is a highly charged environment • Power loss from the charged particle extraction ? • Is a (small or large) crossing angle a solution ? • 800 GeV upgrade How much energy is really deposited in the septum blade ? 01.04.2003 Karsten Büßer - Beamstrahlung on the Septum Blade ECFA/DESY Workshop Amsterdam 4 Disclaimer All I am going to present is right out of the press and is therefore to be considered VERY PRELIMINARY 01.04.2003 Karsten Büßer - Beamstrahlung on the Septum Blade ECFA/DESY Workshop Amsterdam 5 Simulating the Extraction Line Part of the extraction line included in BRAHMS: Shadow: • Distance from IP: 45m • 2m long • 5mm thick • 7mm vertical distance from nominal beam (~156 µrad) • Copper Septum Blade: • Distance from IP: 47m • 16m long • 5mm thick • ~7mm vertical distance from nominal beam • Copper 01.04.2003 Karsten Büßer - Beamstrahlung on the Septum Blade ECFA/DESY Workshop Amsterdam 6 Realistic Beams Simulation of the complete machine done by Glen White. Using: • LINAC: PLACET (D. Schulte) • BDS: MERLIN (N. Walker) • Beam-beam: GUINEA-PIG (D. Schulte) Takes into account: • Simulation of feedback loop • Orbit injection errors into LINAC • Wakefield effects in LINAC • Vibration of quads in BDS • Energy spread of e- due to undulator • Resolutions of BPMs • Jitter on kicker signals Beams and backgrounds are available through database at hepwww.ph.qmul.ac.uk/lcdata 01.04.2003 Karsten Büßer - Beamstrahlung on the Septum Blade ECFA/DESY Workshop Amsterdam 7 Nominal Beam • Total average Beamstrahlung power: ~360 kW • Integrated power in septum blade area: ~60 W 01.04.2003 Karsten Büßer - Beamstrahlung on the Septum Blade ECFA/DESY Workshop Amsterdam 8 Realistic Beam • Feedback system brings beams into stable collisions after ~100 BX • Total average Beamstrahlung power: ~500 kW (TDR 360 kW !) • Integrated power in septum blade area: ~35 kW 01.04.2003 Karsten Büßer - Beamstrahlung on the Septum Blade ECFA/DESY Workshop Amsterdam 9 Colliding with the Septum 5 GeV Photon 01.04.2003 Karsten Büßer - Beamstrahlung on the Septum Blade ECFA/DESY Workshop Amsterdam 10 Nominal Beam • Shadow: Average deposited power: ~40 W • Septum blade: Average deposited power: ~0.3 W 01.04.2003 Karsten Büßer - Beamstrahlung on the Septum Blade ECFA/DESY Workshop Amsterdam 11 Realistic Beam • Shadow: Average deposited power: ~15 kW • Septum blade: Average deposited power: ~80 W 01.04.2003 Karsten Büßer - Beamstrahlung on the Septum Blade ECFA/DESY Workshop Amsterdam 12 Conclusion • Under realistic beam conditions, 30-40 kW of Beamstrahlung are emitted under vertical angles larger than 0.155 mrad. • Roughly half of the emitted energy is deposited in the septum shadow. • Septum blade receives on average 80W. → Information from Efremov: 15 kW has to be cooled away from septum blade due to normal operation. → Septum will probably undergo no mechanical damage. → 40 kW of Beamstrahlung will irradiate the septum environment. To be done • Check backgrounds for the detector. → Backscattering → Pairs, neutrons with realistic beam • Check charged particle extraction losses. 01.04.2003 Karsten Büßer - Beamstrahlung on the Septum Blade ECFA/DESY Workshop Amsterdam 13