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E. Gaztanaga, A. Cabre, and L. Hui (2008a), arXiv: 0807.3551 [astro-ph]; E. Gaztanaga, R. Miquel, and E. Sanchez (2008b), arXiv: 0808.1921 [astro-ph]
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2006
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Original
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2008
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The details of our treatment of the ISW effect, reionization, and polarization do not affect our conclusions, and will be reported elsewhere Moss et al. 2008
2008
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2008

Can we avoid dark energy?

Zibin, J. P., Moss, A., Scott, D.

Understand

The idea that we live near the centre of a large, nonlinear void has attracted attention recently as an alternative to dark energy or modified gravity.

We show that an appropriate void profile can fit both the latest cosmic microwave background and supernova data.
However, this requires either a fine-tuned primordial spectrum or a Hubble rate so low as to rule these models out.
We also show that measurements of the radial baryon acoustic scale can provide very strong constraints.

Built on

E. Gaztanaga, A. Cabre, and L. Hui (2008a), arXiv: 0807.3551 [astro-ph]; E. Gaztanaga, R. Miquel, and E. Sanchez (2008b), arXiv: 0808.1921 [astro-ph]
Original
1921
Earlier work this paper cites.
C. Pryke et al. (QUaD) (2008), arXiv: 0805.1944 [astro-ph]
Original
1944
Earlier work this paper cites.
G. Lemaître, Ann. Soc. Sci. Bruxelles 53
1947
Earlier work this paper cites.
J. Silk, Astron. Astrophys. 59
1977
Earlier work this paper cites.
D. J. Eisenstein and W. Hu, Astrophys. J. 496 , 605 (1998), arXiv: astro-ph/9709112
1998
Earlier work this paper cites.
J. C. Mather et al., Astrophys. J. 512 , 511 (1999), arXiv: astro-ph/9810373
1999
Earlier work this paper cites.
M.-N. Celerier, Astron. Astrophys. 353
2000
Earlier work this paper cites.
A. Lewis, A. Challinor, and A. Lasenby, Astrophys. J. 538 , 473 (2000), arXiv: astro-ph/9911177 ; information on camb
2000
Earlier work this paper cites.
A. Lewis and S. Bridle, Phys. Rev. D66 , 103511 (2002), arXiv: astro-ph/0205436
2002
Earlier work this paper cites.
H.-J. Seo and D. J. Eisenstein, Astrophys. J. 598 , 720 (2003), arXiv: astro-ph/0307460
2003
Earlier work this paper cites.
A. C. S. Readhead et al., Astrophys. J. 609 , 498 (2004), arXiv: astro-ph/0402359
2004
Earlier work this paper cites.
D. Scott, Can. J. Phys. 84 , 419 (2006), arXiv: astro-ph/0510731
2006
Earlier work this paper cites.

Similar

H. Alnes and M. Amarzguioui, Phys. Rev. D74 , 103520 (2006), arXiv: astro-ph/0607334
2006
Cited alongside, same era.
W. C. Jones et al., Astrophys. J. 647 , 823 (2006), arXiv: astro-ph/0507494
2006
Cited alongside, same era.
W. J. Percival et al., Mon. Not. Roy. Astron. Soc. 381 , 1053 (2007), arXiv: 0705.3323 [astro-ph]
Original
2007
Cited alongside, same era.
S. Alexander, T. Biswas, A. Notari, and D. Vaid (2007), arXiv: 0712.0370 [astro-ph]
Original
2007
Cited alongside, same era.
J. P. Zibin, A. Moss, and D. Scott, Phys. Rev. D76 , 123010 (2007), arXiv: 0706.4482 [astro-ph]
Original
2007
Cited alongside, same era.

Then

J. Garcia-Bellido and T. Haugboelle, JCAP 0804 , 003 (2008a), arXiv: 0802.1523 [astro-ph]; K. Bolejko and J. S. B. Wyithe (2008), arXiv: 0807.2891 [astro-ph]
Original
2008
Closest in time.
P. Hunt and S. Sarkar (2008), arXiv: 0807.4508 [astro-ph]
Original
2008
Closest in time.
J. P. Zibin, Phys. Rev. D78 , 043504 (2008), arXiv: 0804.1787 [astro-ph]
Original
2008
Closest in time.
A. Moss, J. P. Zibin, and D. Scott (2008), in preparation
2008
Closest in time.
The details of our treatment of the ISW effect, reionization, and polarization do not affect our conclusions, and will be reported elsewhere Moss et al. 2008
2008
Closest in time.

Beyond the bibliography

alphaXiv searches the wider corpus for related work and actual follow-ups.

Open on alphaXiv

alphaXiv is searching for related work…

N. Jackson, Living Rev. Rel. 10

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D. J. H. Chung and A. E. Romano, Phys. Rev. D74 , 103507 (2006), arXiv: astro-ph/0608403 ; C.-M. Yoo, T. Kai, and K.-i. Nakao (2008), arXiv: 0807.0932 [astro-ph]

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2008

Cited alongside, same era.

Note that the Union dataset assumes a standard Λ \Lambda background (e.g., in the treatment of outliers), although we do not expect this to significantly affect our results

Cited in the paper.

C. L. Reichardt et al. (2008), arXiv: 0801.1491 [astro-ph]

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2008

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C. Clarkson, B. Bassett, and T. H.-C. Lu, Phys. Rev. Lett. 101 , 011301 (2008), arXiv: 0712.3457 [astro-ph]

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J. Goodman, Phys. Rev. D52 , 1821 (1995), arXiv: astro-ph/9506068 ; R. R. Caldwell and A. Stebbins, Phys. Rev. Lett. 100 , 191302 (2008), arXiv: 0711.3459 [astro-ph]

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2008