Cargando…
Early Commissioning of the Luminosity Dither Feedback for SuperKEKB
SuperKEKB is an electron-positron collider, which aims to achieve a peak luminosity of 8×10³⁵ cm⁻² s^{−1} using what is known as the "nano-beam" scheme. This paper reports on the commissioning and performance of a luminosity dither feedback. The system, based on one previously used at SLAC...
Autores principales: | , , , , , , , , , , , , , , , |
---|---|
Lenguaje: | eng |
Publicado: |
JACoW
2019
|
Materias: | |
Acceso en línea: | https://dx.doi.org/10.18429/JACoW-IBIC2018-TUPC13 http://cds.cern.ch/record/2716027 |
_version_ | 1780965496206655488 |
---|---|
author | Masuzawa, Mika Bambade, Philip Brown, David Di Carlo, Salvatore El Khechen, Dima Fisher, Alan Funakoshi, Yoshihiro Jehanno, Didier Kawamoto, Takashi Nakamura, Shu Oki, Toshiyuki Pang, Chengguo Sullivan, Michael Tobiyama, Makoto Uehara, Sadaharu Wienands, Ulrich |
author_facet | Masuzawa, Mika Bambade, Philip Brown, David Di Carlo, Salvatore El Khechen, Dima Fisher, Alan Funakoshi, Yoshihiro Jehanno, Didier Kawamoto, Takashi Nakamura, Shu Oki, Toshiyuki Pang, Chengguo Sullivan, Michael Tobiyama, Makoto Uehara, Sadaharu Wienands, Ulrich |
author_sort | Masuzawa, Mika |
collection | CERN |
description | SuperKEKB is an electron-positron collider, which aims to achieve a peak luminosity of 8×10³⁵ cm⁻² s^{−1} using what is known as the "nano-beam" scheme. This paper reports on the commissioning and performance of a luminosity dither feedback. The system, based on one previously used at SLAC for PEP-II, is employed for collision orbit feedback in the horizontal plane. Twelve air-core Helmholtz coils drive the positron beam sinusoidally at a frequency near 80 Hz, forming a closed bump at the interaction point. A lock-in amplifier detects the amplitude and phase of the corresponding frequency component of the luminosity signal. When the beams are aligned for peak luminosity, the magnitude of the luminosity component at the dithering frequency becomes zero. The magnitude grows as the beams are offset, and the phase shifts by 180 degrees when the direction of the necessary correction reverses. The hardware and algorithm were tested during SuperKEKB Phase II run. The electron beam orbit was successfully adjusted to minimize the amplitude of the dither frequency component of the luminosity signal, and the optimal condition was maintained by continuously adjusting the electron beam orbit. |
id | oai-inspirehep.net-1736105 |
institution | Organización Europea para la Investigación Nuclear |
language | eng |
publishDate | 2019 |
publisher | JACoW |
record_format | invenio |
spelling | oai-inspirehep.net-17361052020-05-03T21:20:54Zdoi:10.18429/JACoW-IBIC2018-TUPC13http://cds.cern.ch/record/2716027engMasuzawa, MikaBambade, PhilipBrown, DavidDi Carlo, SalvatoreEl Khechen, DimaFisher, AlanFunakoshi, YoshihiroJehanno, DidierKawamoto, TakashiNakamura, ShuOki, ToshiyukiPang, ChengguoSullivan, MichaelTobiyama, MakotoUehara, SadaharuWienands, UlrichEarly Commissioning of the Luminosity Dither Feedback for SuperKEKBAccelerators and Storage RingsSuperKEKB is an electron-positron collider, which aims to achieve a peak luminosity of 8×10³⁵ cm⁻² s^{−1} using what is known as the "nano-beam" scheme. This paper reports on the commissioning and performance of a luminosity dither feedback. The system, based on one previously used at SLAC for PEP-II, is employed for collision orbit feedback in the horizontal plane. Twelve air-core Helmholtz coils drive the positron beam sinusoidally at a frequency near 80 Hz, forming a closed bump at the interaction point. A lock-in amplifier detects the amplitude and phase of the corresponding frequency component of the luminosity signal. When the beams are aligned for peak luminosity, the magnitude of the luminosity component at the dithering frequency becomes zero. The magnitude grows as the beams are offset, and the phase shifts by 180 degrees when the direction of the necessary correction reverses. The hardware and algorithm were tested during SuperKEKB Phase II run. The electron beam orbit was successfully adjusted to minimize the amplitude of the dither frequency component of the luminosity signal, and the optimal condition was maintained by continuously adjusting the electron beam orbit.SuperKEKB is an electron–positron double ring collider that aims to achieve a peak luminosity of 8 x 10$^{35}$ cm$^{-2}$ s$^{-1}$ by using what is known as the “nano-beam” scheme. A luminosity dither system is employed for collision orbit feedback in the horizontal plane. This paper reports the dither hardware and algorithm tests during the SuperKEKB Phase II luminosity run.JACoWoai:inspirehep.net:17361052019 |
spellingShingle | Accelerators and Storage Rings Masuzawa, Mika Bambade, Philip Brown, David Di Carlo, Salvatore El Khechen, Dima Fisher, Alan Funakoshi, Yoshihiro Jehanno, Didier Kawamoto, Takashi Nakamura, Shu Oki, Toshiyuki Pang, Chengguo Sullivan, Michael Tobiyama, Makoto Uehara, Sadaharu Wienands, Ulrich Early Commissioning of the Luminosity Dither Feedback for SuperKEKB |
title | Early Commissioning of the Luminosity Dither Feedback for SuperKEKB |
title_full | Early Commissioning of the Luminosity Dither Feedback for SuperKEKB |
title_fullStr | Early Commissioning of the Luminosity Dither Feedback for SuperKEKB |
title_full_unstemmed | Early Commissioning of the Luminosity Dither Feedback for SuperKEKB |
title_short | Early Commissioning of the Luminosity Dither Feedback for SuperKEKB |
title_sort | early commissioning of the luminosity dither feedback for superkekb |
topic | Accelerators and Storage Rings |
url | https://dx.doi.org/10.18429/JACoW-IBIC2018-TUPC13 http://cds.cern.ch/record/2716027 |
work_keys_str_mv | AT masuzawamika earlycommissioningoftheluminosityditherfeedbackforsuperkekb AT bambadephilip earlycommissioningoftheluminosityditherfeedbackforsuperkekb AT browndavid earlycommissioningoftheluminosityditherfeedbackforsuperkekb AT dicarlosalvatore earlycommissioningoftheluminosityditherfeedbackforsuperkekb AT elkhechendima earlycommissioningoftheluminosityditherfeedbackforsuperkekb AT fisheralan earlycommissioningoftheluminosityditherfeedbackforsuperkekb AT funakoshiyoshihiro earlycommissioningoftheluminosityditherfeedbackforsuperkekb AT jehannodidier earlycommissioningoftheluminosityditherfeedbackforsuperkekb AT kawamototakashi earlycommissioningoftheluminosityditherfeedbackforsuperkekb AT nakamurashu earlycommissioningoftheluminosityditherfeedbackforsuperkekb AT okitoshiyuki earlycommissioningoftheluminosityditherfeedbackforsuperkekb AT pangchengguo earlycommissioningoftheluminosityditherfeedbackforsuperkekb AT sullivanmichael earlycommissioningoftheluminosityditherfeedbackforsuperkekb AT tobiyamamakoto earlycommissioningoftheluminosityditherfeedbackforsuperkekb AT ueharasadaharu earlycommissioningoftheluminosityditherfeedbackforsuperkekb AT wienandsulrich earlycommissioningoftheluminosityditherfeedbackforsuperkekb |