Built on

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2010

Spatial and temporal tuning in void models for acceleration

Foreman, Simon, Moss, Adam, Zibin, James P. et al.

Understand

There has been considerable interest in recent years in cosmological models in which we inhabit a very large, underdense void as an alternative to dark energy.

A longstanding objection to this proposal is that observations limit our position to be very close to the void centre.
By selecting from a family of void profiles that fit supernova luminosity data, we carefully determine how far from the centre we could be.
To do so, we use the observed dipole component of the cosmic microwave background, as well as an additional stochastic peculiar velocity arising from primordial perturbations.

Built on

G. Lemaître, Ann. Soc. Sci. Bruxelles 53
1933
Earlier work this paper cites.
R. C. Tolman, Proc. Nat. Acad. Sci. 20
1934
Earlier work this paper cites.
C. Pryke et al. (QUaD), Astrophys. J. 692 , 1247 (2009), arXiv: 0805.1944 [astro-ph]
Original
1944
Earlier work this paper cites.
H. Bondi, Mon. Not. Roy. Astron. Soc. 107
1947
Earlier work this paper cites.
J. V. Arnau, M. J. Fullana, L. Monreal, and D. Saez, Astrophys. J. 402 , 359 (1993)
1993
Earlier work this paper cites.
J. W. Moffat and D. C. Tatarski, Astrophys. J. 453 , 17 (1995), arXiv: astro-ph/9407036
1995
Earlier work this paper cites.
K.-i. Nakao et al., Astrophys. J. 453 , 541 (1995), arXiv: astro-ph/9502054
1995
Earlier work this paper cites.
K. Tomita, Astrophys. J. 461 , 507 (1996)
1996
Earlier work this paper cites.
N. P. Humphreys, R. Maartens, and D. R. Matravers, Astrophys. J. 477 , 47 (1997), arXiv: astro-ph/9602033
1997
Earlier work this paper cites.
C. Baccigalupi, L. Amendola, and F. Occhionero, Mon. Not. Roy. Astron. Soc. 288
1997
Earlier work this paper cites.
C. M. Grinstead and J. L. Snell, Introduction to Probability (American Mathematical Society, Providence, 1998), 2nd ed
1998
Earlier work this paper cites.
A. Lewis, A. Challinor, and A. Lasenby, Astrophys. J. 538 , 473 (2000), arXiv: astro-ph/9911177
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.
S. Carroll, in KITP: Colloquium Series (2002), arXiv: astro-ph/0107571
2002
Earlier work this paper cites.
D. Scott, Can. J. Phys. 84 , 419 (2006), arXiv: astro-ph/0510731
2006
Earlier work this paper cites.
H. Alnes and M. Amarzguioui, Phys. Rev. D 74 , 103520 (2006), arXiv: astro-ph/0607334
2006
Earlier work this paper cites.
W. C. Jones et al., Astrophys. J. 647 , 823 (2006), arXiv: astro-ph/0507494
2006
Earlier work this paper cites.