Skip to main content
Log in

Radiation-matter interaction in the space translation method

  • Published:
Il Nuovo Cimento D

Summary

The space translation (ST) method frequently used to treat the radiation-matter interaction in the high-intensity domain is reconsidered. Limitations of the usual ST working program are pointed out together with the related difficulties in the evaluation of transition amplitudes. The theory of potential scattering in the presence of a strong radiation field within the ST method is considered as well, and a recent approximate treatment discussed.

Riassunto

Il metodo della «space translation» (ST) usato frequentemente nell'interazione radiazione-materia in regimi di alta intensità è riconsiderato. Alcune limitazioni del programma di lavoro della ST nel calcolo delle ampiezze di transizione sono messe in evidenza. Viene anche considerata la teoria della diffusione da potenziale nell'ambito del metodo della ST e viene discusso un recente trattamento approssimato.

Резюме

Заново рассмтривается метод трансляции пространства, часто используемый для изучения взаимодействия излучения с веществом в области высоких интенсивностей. Отмечаются ограничения обычного метода трансляции пространства, а также трудности, возникающие при вычислении амплитуд переходов. Исследуется теория потенциального рассеяния в присутствии сильного поля излучения в рамках метода трансляции иространства, а также обсуждаются недавние приближенные рассмотрения.

This is a preview of subscription content, log in via an institution to check access.

Access this article

Price excludes VAT (USA)
Tax calculation will be finalised during checkout.

Instant access to the full article PDF.

Similar content being viewed by others

References

  1. H. A. Kramers:Rapport et Discussions, Solvay Congress (Stoop, Brussels, 1948).

    Google Scholar 

  2. W. C. Henneberger:Phys. Rev. Lett.,21, 838 (1968).

    Article  ADS  Google Scholar 

  3. G. Ferrante andC. Leone:Phys. Rev. A,26, 3101 (1982) and references quoted therein.

    Article  ADS  Google Scholar 

  4. K. H. Yang:Ann. Phys. (N. Y.),101, 62 (1976);Y. Aharonov andC. K. Au:Phys. Rev. A,20, 1553 (1979);Y. Aharonov andC. K. Au:Phys. Lett. A,86, 269 (1981).

    Article  ADS  Google Scholar 

  5. S. K. Vermani andB. L. Beers:Phys. Rev. A,12, 715 (1975);C. K. Choi, W. C. Henneberger, S. N. Mian andF. C. Sanders:Phys. Rev. A,12, 2635 (1975).

    Article  ADS  Google Scholar 

  6. D. H. Kobe:J. Phys. A,17, 141 (1984).

    Article  ADS  Google Scholar 

  7. G. Ferrante andC. Leone:Nuovo Cimento B,48, 35 (1978).

    Google Scholar 

  8. M. Gavrila andJ. Z. Kaminski:Phys. Rev. Lett.,52, 613 (1984).

    Article  ADS  Google Scholar 

  9. M. J. Offerhaus, J. Z. Kaminski andM. Gavrila:Phys. Lett. A,112, 151 (1985).

    Article  ADS  Google Scholar 

  10. M. Mohan:Phys. Lett. A,50, 283 (1974).

    Article  ADS  Google Scholar 

  11. C. J. Joachain:Quantum Collision Theory (Elsevier Science Publisher, Amsterdam, 1975).

    Google Scholar 

Download references

Author information

Authors and Affiliations

Authors

Rights and permissions

Reprints and permissions

About this article

Cite this article

Messina, G., Cavaliere, P. & Ferrante, G. Radiation-matter interaction in the space translation method. Il Nuovo Cimento D 10, 901–914 (1988). https://doi.org/10.1007/BF02450193

Download citation

  • Received:

  • Issue Date:

  • DOI: https://doi.org/10.1007/BF02450193

PACS 32.80.kf

Navigation