Eliminating spectral distinguishability in ultrafast spontaneous parametric down-conversion
Source: Phys. Rev. A 80, 043815 (2009); doi:10.1103/PhysRevA.80.043815
Published 14 October 2009
KEYWORDS and PACS
RELATED DATABASES
To view database links for this article,
you need to log in.
you need to log in.
To view database links for this article,
you need to log in.
you need to log in.
PUBLICATION DATA
Generation of polarization-entangled photon pairs with a precise timing through down-conversion of femtosecond pulses is often faced with a degraded polarization entanglement quality. In a previous experiment, we have shown that this degradation is induced by spectral distinguishability between the two decay paths, in accordance with theoretical predictions. Here, we present an experimental study of the spectral compensation scheme proposed and first implemented by Kim and Grice [J. Mod. Opt. 49, 2309 (2002)]. By measuring the joint spectral properties of the polarization correlations of the photon pairs, we show that the spectral distinguishability between the down-converted components is eliminated. This scheme results in a polarization visibility of 97.9±0.5% without any spectral filtering.
©2009 The American Physical Society
| History: | Received 23 May 2009; published 14 October 2009 |
| Permalink: |
http://link.aps.org/abstract/PRA/v80/e043815 |
REFERENCES (36)
For access to fully linked references, you need to log in.
For access to fully linked references, you need to Log in.
- D. C. Burnham and D. L. Weinberg,
Phys. Rev. Lett. 25, 84 (1970) . - P. G. Kwiat, K. Mattle, H. Weinfurter, A. Zeilinger, A. V. Sergienko, and Y. Shih, Phys. Rev. Lett. 75, 4337 (1995).
- P. G. Kwiat, E. Waks, A. G. White, I. Appelbaum, and P. H. Eberhard, Phys. Rev. A 60, R773 (1999).
- T. Jennewein, C. Simon, G. Weihs, H. Weinfurter, and A. Zeilinger, Phys. Rev. Lett. 84, 4729 (2000).
- M. Eibl, S. Gaertner, M. Bourennane, C. Kurtsiefer, M. Żukowski, and H. Weinfurter, Phys. Rev. Lett. 90, 200403 (2003).
- A. M. Goebel, C. Wagenknecht, Q. Zhang, Y.-A. Chen, K. Chen, J. Schmiedmayer, and J.-W. Pan, Phys. Rev. Lett. 101, 080403 (2008).
- T. E. Keller and M. H. Rubin, Phys. Rev. A 56, 1534 (1997).
- W. P. Grice and I. A. Walmsley, Phys. Rev. A 56, 1627 (1997).
- W. P. Grice, R. Erdmann, I. A. Walmsley, and D. Branning, Phys. Rev. A 57, R2289 (1998).
- M. Atatüre, A. V. Sergienko, B. M. Jost, B. E. A. Saleh, and M. C. Teich, Phys. Rev. Lett. 83, 1323 (1999).
- H. S. Poh, C. Y. Lum, I. Marcikic, A. Lamas-Linares, and C. Kurtsiefer, Phys. Rev. A 75, 043816 (2007).
- M. Avenhaus, M. V. Chekhova, L. A. Krivitsky, G. Leuchs, and C. Silberhorn, Phys. Rev. A 79, 043836 (2009).
- R. Erdmann, D. Branning, W. P. Grice, and I. A. Walmsley, Phys. Rev. A 62, 053810 (2000).
- J. F. Hodelin, G. Khoury, and D. Bouwmeester, Phys. Rev. A 74, 013802 (2006).
- D. Branning, W. P. Grice, R. Erdmann, and I. A. Walmsley, Phys. Rev. Lett. 83, 955 (1999).
- W. Wasilewski, C. Radzewicz, R. Frankowski, and K. Banaszek, Phys. Rev. A 78, 033831 (2008).
- T. B. Pittman, D. V. Strekalov, A. Migdall, M. H. Rubin, A. V. Sergienko, and Y. H. Shih, Phys. Rev. Lett. 77, 1917 (1996).
- C. K. Hong, Z. Y. Ou, and L. Mandel, Phys. Rev. Lett. 59, 2044 (1987).
- C. Kurtsiefer, M. Oberparleiter, and H. Weinfurter, Phys. Rev. A 64, 023802 (2001).
- I. Marcikic, H. de Riedmatten, W. Tittel, V. Scarani, H. Zbinden, and N. Gisin, Phys. Rev. A 66, 062308 (2002).
- P. Walther, M. Aspelmeyer, K. J. Resch, and A. Zeilinger, Phys. Rev. Lett. 95, 020403 (2005).
- B. P. Lanyon, T. J. Weinhold, N. K. Langford, M. Barbieri, D. F. V. James, A. Gilchrist, and A. G. White, Phys. Rev. Lett. 99, 250505 (2007).
ADVERTISEMENT


