Cherenkov Radiation at Speeds Below the Light Threshold: Phonon-Assisted Phase Matching

Author:

Stevens T. E.12,Wahlstrand J. K.1,Kuhl J.2,Merlin R.1

Affiliation:

1. The Harrison M. Randall Laboratory of Physics, University of Michigan, Ann Arbor, MI 48109–1120, USA.

2. Max-Planck-Institut für Festkörperforschung, D-70569 Stuttgart, Germany.

Abstract

Charged particles traveling through matter at speeds larger than the phase velocity of light in the medium emit Cherenkov radiation. Calculations reveal that a given angle of the radiation conical wavefront is associated with two velocities, one above and one below a certain speed threshold. Emission at subluminal but not superluminal speeds is predicted and verified experimentally for relativistic dipoles generated with an optical method based on subpicosecond pulses moving in a nonlinear medium. The dipolar Cherenkov field, in the range of infrared-active phonons, is identical to that of phonon polaritons produced by impulsive laser excitation.

Publisher

American Association for the Advancement of Science (AAAS)

Subject

Multidisciplinary

Reference40 articles.

1. V. P. Zrelov Cherenkov Radiation in High-Energy Physics (Israel Program for Scientific Translations Jerusalem 1970).

2. Ypsilantis T., Seguinot J., Nucl. Instrum. Methods A 433, 1 (1999).

3. and references therein.

4. Cherenkov P. A., Dokl. Akad. Nauk SSSR 2, 451 (1934).

5. Vavilov S., Dokl. Akad. Nauk SSSR 2, 457 (1934).

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