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Physical Review D

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Effects of voids on the reconstruction of the equation of state of dark energy

Arnaud de Lavallaz^* and Malcolm Fairbairn^†

Department of Physics, King’s College London, Strand, London, WC2R 2LS, United Kingdom

^*arnaud.de_lavallaz@kcl.ac.uk
^†malcolm.fairbairn@kcl.ac.uk

Phys. Rev. D 84, 083005 – Published 11 October, 2011

DOI: https://doi.org/10.1103/PhysRevD.84.083005

Abstract

We quantify the effects of the voids known to exist in the Universe upon the reconstruction of the dark energy equation of state $w$ . We show that the effect can start to be comparable with some of the other errors taken into account when analyzing supernova data, depending strongly upon the low redshift cutoff used in the sample. For the supernova data alone, the error induced in the reconstruction of $w$ is much larger than the percent level. When the Baryonic Acoustic Oscillations and the Cosmic Microwave Background data are included in the fit, the effect of the voids upon the determination of $w$ is much lessened but is not much smaller than some of the other errors taken into consideration when performing such fits. We also look at the effect of voids upon the estimation of the equation of state when we allow $w$ to vary over time and show that even when supernova, Cosmic Microwave Background, and Baryonic Acoustic Oscillations data are used to constrain the equation of state, the best fit points in parameter space can change at the 10% level due to the presence of voids, and error-bars increase significantly.

Article Text

References (33)

R. Amanullah et al., Astrophys. J. 716, 712 (2010).
E. Komatsu et al., Astrophys. J. Suppl. Ser. 192, 18 (2011).
A. Labatie et al., arXiv:1009.1232.
W. L. Freedman et al., Astrophys. J. 553, 47 (2001).
K. A. Olive, arXiv:astro-ph/0301505.
F. Hoyle and M. S. Vogeley, Astrophys. J. 607, 751 (2004).
D. C. Pan et al., arXiv:1103.4156.
M. Boylan-Kolchin et al., Mon. Not. R. Astron. Soc. 398, 1150 (2009).
R. Van de Weygaert and E. Platen, arXiv:0912.2997.
R. A. Vanderveld, E. E. Flanagan, and I. Wasserman, Phys. Rev. D 78, 083511 (2008).
V. Marra, E. W. Kolb, S. Matarrese, and A. Riotto, Phys. Rev. D 76, 123004 (2007).
A. E. Romano and P. Chen, arXiv:1104.0730.
A. E. Romano, M. Sasaki, and A. A. Starobinsky, arXiv:1006.4735.
B. Sinclair, T. M.Davis, and T. Haugbolle, Astrophys. J. 718, 1445 (2010).
K. Bolejko, PMC Phys. A 2, 1 (2008).
H. Alnes and M. Amarzguioui, Phys. Rev. D 75, 023506 (2007).
S. Alexander et al., J. Cosmol. Astropart. Phys. 09 (2009) 25.
M. Blomqvist and E. Moertsell, J. Cosmol. Astropart. Phys. 5 (2010) 006.
E. W. Kolb and C. R. Callum, arXiv:0911.3852v1.
J. W. Moffat and D. C. Tatarski, Phys. Rev. D 45, 3512 (1992).
J. W. Moffat and D. C. Tatarski, Astrophys. J. 453, 17 (1995).
K. Tomita, Astrophys. J. 529, 38 (2000).
K. Tomita, Prog. Theor. Phys. 106, 929 (2001).
P. Hunt and S. Sarkar, Mon. Not. R. Astron. Soc. 401, 547 (2010).
S. Nadathur and S. Sarkar, Phys. Rev. D 83, 063506 (2011).
R. Biswas, E. Alizadeh, and B. D. Wandelt, Phys. Rev. D 82, 023002 (2010).
J. Lee and D. Park, Astrophys. J. Lett. 696, L10 (2009).
V. Kostov, J. Cosmol. Astropart. Phys. 04 (2010) 001.
W. Valkenburg, J. Cosmol. Astropart. Phys. 06 (2009) 010.
http://www.supernova.lbl.gov/Union.
D. J. Eisenstein et al., Astrophys. J. 633, 560 (2005).
M. Chevallier and D. Polarski, Int. J. Mod. Phys. D 10, 213 (2001).
E. V. Linder, Phys. Rev. Lett. 90, 091301 (2003).