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9 - Baryon acoustic oscillations

Published online by Cambridge University Press:  05 July 2014

Bruce Bassett
Affiliation:
University of Cape Town
Renée Hlozek
Affiliation:
University of Oxford
Pilar Ruiz-Lapuente
Affiliation:
Universitat de Barcelona
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Summary

Introduction

Whilst often phrased in terms of discovering the nature of dark energy, cosmology in the twenty-first century might also aptly be described as ‘the distance revolution’. With new knowledge of the extragalactic distance ladder we are, for the first time, beginning to accurately probe the expansion history of the cosmos beyond the local universe, at redshifts z > 0.1. While standard candles - most notably Type Ia supernovae (SN Ia) - kicked off the distance revolution, it is clear that standard rulers, and the baryon acoustic oscillations (BAO) in particular, will play an important role in the coming revolution.

Here we review the theoretical, observational and statistical aspects of the BAO as standard rulers and examine the impact BAO will have on our understanding of dark energy, the distance and expansion ladder.

9.1.1 A brief history of standard rulers and the BAO

Let us start by putting the BAO in context. The idea of a standard ruler is one familiar from everyday life. We judge the distance of an object of known length (such as a person) by its angular size. The further away it is, the smaller it appears. The same idea applies in cosmology, with one major complication: space can be curved. This is similar to trying to judge the distance of our known object through a smooth lens of unknown curvature. Now when it appears small, we are no longer sure it is because it is far away.

Type
Chapter
Information
Dark Energy
Observational and Theoretical Approaches
, pp. 246 - 278
Publisher: Cambridge University Press
Print publication year: 2010

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References

Abdalla, F. B., and Rawlings, S. (2005). Mon. Not. R. Astron. Soc. 360, 27.CrossRef
Abdalla, F., Blake, C., and Rawlings, S. (2009). [arXiv:0905.4311].
Albrecht, A., and Bernstein, G. (2006). [astro-ph/0608269].
Alcock, C., and Paczynski, B. (1979). Nature (London) 281, 358.CrossRef
Allen, S. W., Schmidt, R. W., and Fabian, A. C. (2002). Mon. Not. R. Astron. Soc. 334, L11.CrossRef
Annis, J., Bridle, S., Castander, F. J., et al. (2005). [astro-ph/0510195].
Bashinsky, S., and Bertschinger, E. (2002). Phys. Rev. D 65, 123008.CrossRef
Bassett, B. A., and Kunz, M. (2004). Phys. Rev. D 69 101305.CrossRef
Bassett, B. A., Nichol, B., and Eisenstein, D. J. (2005). Astron. Geophys. 46, 26.CrossRef
Bassett, B. A., Fantaye, Y. T., Hlozek, R. A., and Kotze, J. (2008). Code available at www.cosmology.org.za.
Blake, C., and Bridle, S. (2005). Mon. Not. R. Astron. Soc. 363, 1329.CrossRef
Blake, C., and Glazebrook, K. (2003). Astrophys. J. 594, 665.CrossRef
Blake, C. A., Abdalla, F. B., Bridle, S. L., and Rawlings, S. (2004). New Astron. Rev 48, 1063.CrossRef
Blake, C., Parkinson, D., Bassett, B. A.et al. (2006). Mon. Not. R. Astron. Soc. 365, 255.CrossRef
Blake, C., Collister, A., Bridle, S., and Lahav, O. (2007).Mon. Not. R. Astron. Soc. 374, 1527.CrossRef
Blake, C., Jurek, R. J., Brough, S., et al. (2009). Mon. Not. R. Astron. Soc. 395, 240.CrossRef
Broadhurst, T., and Jaffe, A. (2000). In Clustering at High Redshift,A., Mazure, O. Le, Fèvre, and V. Le, Brun, Eds., Astron. Soc. Pacif. Conf. Ser.200, 241.Google Scholar
Broadhurst, T. J., Ellis, R. S., Koo, D. C., and Szalay, A. S. (1990). Nature (London) 343, 726.CrossRef
Buchalter, A., Helfand, D. J., Becker, R. H., and White, R. L. (1998). Astrophys. J. 494, 503.CrossRef
Cai, Y.-C., Angulo, R. E., Baugh, C. M., et al. (2008). [arXiv:0810.2300].
Carilli, C., and Rawlings, S. (2004). [astro-ph/0409274].
Chang, T.-C., Pen, U.-L., Peterson, J. B., and McDonald, P. (2008). Phys. Rev. Lett. 100, 091303.
Chevallier, M., and Polarski, D. (2001). Int. J. Mod. Phys. D 10, 213.CrossRef
Cimatti, A., Robberto, M., Baugh, C., et al. (2009). Exp. Astron. 23, 39.CrossRef
Clarkson, C., Cortés, M., and Bassett, B. (2007). JCAP 8, 11.CrossRef
Clarkson, C., Bassett, B., and Lu, T. H. C. (2008). Phys. Rev. Lett. 101, 011301.CrossRef
Cole, S., Percival, W. J., Peacock, J. A., et al. (2005). Mon. Not. R. Astron. Soc. 362, 505.CrossRef
Coles, P. (1993). Mon. Not. R. Astron. Soc. 262, 1065.CrossRef
Collister, A., Lahav, O., Blake, C., et al. (2007). Mon. Not. R. Astron. Soc. 375, 68.CrossRef
Cooray, A., Hu, W., Huterer, D., and Joffre, M. (2001). Astrophys. J. 557, L7.CrossRef
Cresswell, J. G., and Percival, W.J. (2008). [arXiv:0808.1101].
Crocce, M., and Scoccimarro, R. (2006a). Phys. Rev. D 73, 063519.
Crocce, M., and Scoccimarro, R. (2006b). Phys. Rev. D 73, 063520.
Crocce, M., and Scoccimarro, R. (2008). Phys. Rev. D 77, 023533.CrossRef
Daly, R. A. (1994). Astrophys. J. 426, 38.CrossRef
Daly, R. A., and Guerra, E. J. (2002). Astron. J. 124, 1831.CrossRef
Daly, R. A., Mory, M. P., O'Dea, C. P., et al. (2007). [arXiv:0710.5112].
Deng, Z., Xia, X., and Fang, L.-Z. (1994). Astrophys. J. 431, 506.CrossRef
Eisenstein, D.J. (1997). [astro-ph/9709054].
Eisenstein, D. (2003). [astro-ph/0301623]
Eisenstein, D., and White, M. (2004). Phys. Rev. D 70, 103523.CrossRef
Eisenstein, D. J., Hu, W., Silk, J., and Szalay, A. S. (1998). Astrophys. J. 494, L1.CrossRef
Eisenstein, D. J., Hu, W., and Tegmark, M. (1998). Astrophys. J. 504, L57.CrossRef
Eisenstein, D. J., Zehavi, I., Hogg, D. W., et al. (2005). Astrophys. J. 633, 560.CrossRef
Eisenstein, D. J., Seo, H.-J., and White, M. (2007). Astrophys. J. 664, 660.CrossRef
Eisenstein, D. J., Seo, H.-J., Sirko, E., and Spergel, D. N. (2007). Astrophys. J. 664, 675.CrossRef
Fry, J.N. (1996). Astrophys. J. 461, L65.CrossRef
Gaztanaga, E., Cabre, A., and Hui, L. (2008). [arXiv:0807.3551].
Glazebrook, K., Baldry, I., Moos, W., Kruk, J., and McCandliss, S. (2005a). New Astron. Rev. 49, 374.CrossRef
Glazebrook, K., Eisenstein, D., Dey, A., Nichol, B., and The WFMOS Feasibility Study Dark Energy Team (2005b). [astro-ph/0507457].
Gurvits, L. I. (1994). Astrophys. J. 425, 442.CrossRef
Hamilton, A. J. S. (1998). In The Evolving Universe,D., Hamilton, Ed., Astrophys. Space Sci. Libr. 231, 185.Google Scholar
Hill, G. J., Gebhardt, K., Komatsu, E., and MacQueen, P. J. (2004). In The New Cosmology: Conference on Strings and Cosmology,R. E., Allen, D. V., Nanopoulos, and C. C., Pope, Eds., Amer. Inst. Phys. Conf. Ser. 743, 224.Google Scholar
Hill, G. J., Gebhardt, K., Komatsu, E., et al. (2008). [arXiv:0806.0183].
Hlozek, R., Cortés, M., Clarkson, C., and Bassett, B. (2008). Gen. Relat. Grav. 40, 285.CrossRef
Hui, L., and Parfrey, K. P. (2007). [arXiv:0712.1162].
Jackson, J. C., and Dodgson, M. (1997). Mon. Not. R. Astron. Soc. 285, 806.CrossRef
Kaiser, N. (1987). Mon. Not. R. Astron. Soc. 227, 1.CrossRef
Kellermann, K. I. (1993). Nature (London) 361, 134.CrossRef
Komatsu, E., Dunkley, J., Nolta, M. R., et al. (2008). [arXiv:0803.0547].
Linder, E.V. (2003). Phys. Rev. Lett. 90, 091301.CrossRef
Mantz, A., Allen, S. W., Ebeling, H., and Rapetti, D. (2008). Mon. Not. R. Astron. Soc. 387, 1179.CrossRef
McDonald, P., and Eisenstein, D.J. (2007). Phys.Rev. D 76, 063009.CrossRef
Meiksin, A., White, M. and Peacock, J. A. (1999). Mon. Not. R. Astron. Soc. 304, 851.CrossRef
Miller, C. J., Nichol, R. C. and Chen, X. (2002). Astrophys. J. 579, 483.CrossRef
Padmanabhan, N., Schlegel, D. J., Seljak, U.et al. (2007). Mon. Not. R. Astron. Soc. 378, 852.CrossRef
Parkinson, D., Blake, C., Kunz, M., et al. (2007). Mon. Not. R. Astron. Soc. 377, 185.CrossRef
Parkinson, D., Kunz, M., Liddle, A. R., et al. (2009). [arXiv:0905.3410].
Percival, W. J., and White, M. (2008). [arXiv:0808.0003].
Percival, W. J., Nichol, R. C., Eisenstein, D. J., et al. (2007). Astrophys. J. 657, 51.CrossRef
Refregier, A., Douspis, M., and the DUNE collaboration (2008). [arXiv:0807.4036].
Robberto, M., Cimatti, A., and The Space Science Team (2007). Nuovo Cimento B 122, 1467.
Roukema, B. F., and Mamon, G. A. (2000). Astron. Astrophys. 358, 395408.
Roukema, B. F., Mamon, G. A., and Bajtlik, S. (2002). Astron. Astrophys. 382, 397.CrossRef
Sánchez, A. G., and Cole, S. (2008). Mon. Not. R. Astron. Soc. 385, 830.CrossRef
Seo, H.-J., and Eisenstein, D. J. (2003). Astrophys. J. 598, 720.CrossRef
Seo, H.-J., and Eisenstein, D. J. (2007). Astrophys. J. 665, 14.CrossRef
Shanks, T., Fong, T., Boyle, B. J., and Peterson, B. A. (1987). Mon. Not. R. Astron. Soc. 227, 739.CrossRef
Smith, R. E., Scoccimarro, R., and Sheth, R. K. (2007). Phys. Rev. D 75, 063512.CrossRef
Smith, R. E., Scoccimarro, R. and Sheth, R.K. (2008). Phys.Rev. D 77, 043525.
Spergel, D. N., Bean, R., Doré, O., et al. (2007). Astrophys. J. Suppl. 170, 377.CrossRef
Tegmark, M., and Zaldarriaga, M. (2008). [arXiv:0805.4414].
Tegmark, M., Taylor, A. N., and Heavens, A.F. (1997). Astrophys. J. 480, 22.CrossRef
Tegmark, M., Eisenstein, D. J., Strauss, M. A., et al. (2006). Phys. Rev. D 74, 123507.CrossRef
Totsuji, H., and Kihara, T. (1969). Publ. Astron. Soc. Japan 21, 221.
Tyson, J. A. (2002). In Survey and Other Telescope Technologies and Discoveries,J., Tyson and S., Wolff, Eds., Proc. SPIE 4836, 10.Google Scholar
Wang, X., Chen, X., Zheng, Z., et al. (2008). [arXiv:0809.3002].
Weinberg, D.H. (1995). Bull. Amer. Astron. Soc. 27, 853.
Weinberg, S. (1972). Gravitation and Cosmology: Principles and Applications of the General Theory of Relativity,New York: Wiley.Google Scholar
Wyithe, S., Loeb, A., and Geil, P. (2007). [arXiv:0709.2955].
Yamamoto, K., Bassett, K., and Nishioka, H. (2005). Phys. Rev. Lett. 94, 051301.CrossRef
Zhan, H., Wang, L., Pinto, P., and Tyson, J. A. (2008). Astrophys J 675, L1.CrossRef
Zhang, P. (2008). [arXiv:0802.2416].

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