• Open Access

Direct Observation of Incoherent Cherenkov Diffraction Radiation in the Visible Range

R. Kieffer, L. Bartnik, M. Bergamaschi, V. V. Bleko, M. Billing, L. Bobb, J. Conway, M. Forster, P. Karataev, A. S. Konkov, R. O. Jones, T. Lefevre, J. S. Markova, S. Mazzoni, Y. Padilla Fuentes, A. P. Potylitsyn, J. Shanks, and S. Wang
Phys. Rev. Lett. 121, 054802 – Published 1 August 2018

Abstract

We report on the observation of incoherent Cherenkov radiation emitted by a 5.3 GeV positron beam circulating in the Cornell electron-positron storage ring as the beam passes in the close vicinity of the surface of a fused silica radiator (i.e., at a distance larger than 0.8 mm). The shape of the radiator was designed in order to send the Cherenkov photons towards the detector, consisting of a compact optical system equipped with an intensified camera. The optical system allows both the measurements of 2D images and angular distribution including polarization study. The corresponding light intensity has been measured as a function of the distance between the beam and the surface of the radiator and has shown a good agreement with theoretical predictions. For highly relativistic particles, a large amount of incoherent radiation is produced in a wide spectral range. A light yield of 0.8×103 photon per particle per turn has been measured at a wavelength of 600±10nm in a 2 cm long radiator and for an impact parameter of 1 mm. This will find applications in accelerators as noninvasive beam diagnostics for both leptons and hadrons.

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  • Received 3 April 2018

DOI:https://doi.org/10.1103/PhysRevLett.121.054802

Published by the American Physical Society under the terms of the Creative Commons Attribution 4.0 International license. Further distribution of this work must maintain attribution to the author(s) and the published article’s title, journal citation, and DOI.

Published by the American Physical Society

Physics Subject Headings (PhySH)

  1. Research Areas
Accelerators & BeamsParticles & Fields

Authors & Affiliations

R. Kieffer1,*, L. Bartnik3, M. Bergamaschi1, V. V. Bleko2, M. Billing3, L. Bobb4, J. Conway3, M. Forster3, P. Karataev5, A. S. Konkov2, R. O. Jones1, T. Lefevre1, J. S. Markova2, S. Mazzoni1, Y. Padilla Fuentes3, A. P. Potylitsyn2, J. Shanks3, and S. Wang3

  • 1CERN, CH-1211 Geneva 23, Switzerland
  • 2Tomsk Polytechnic University, Lenina avenue 30, Tomsk 634050, Russian Federation
  • 3Cornell University, Ithaca, New York 14850, USA
  • 4Diamond Light Source, Oxfordshire OX11 0DE, United Kingdom
  • 5Royal Holloway, University of London, Egham, Surrey TW20 0EX, United Kingdom

  • *robert.kieffer@cern.ch

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Issue

Vol. 121, Iss. 5 — 3 August 2018

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