Built on

L. Verde, T. Treu and A. G. Riess, “Tensions between the Early and the Late Universe,” Nature Astron. 3
Original
1907
Earlier work this paper cites.
E. Hubble, “A relation between distance and radial velocity among extra-galactic nebulae,” PNAS USA 15 (1929) 168–173
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J. M. Stewart and G. F. R. Ellis, “Solutions of Einstein’s equations for a fluid which exhibit local rotational symmetry,” J. Math. Phys. 9
1968
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G. F. R. Ellis and M. A. H. MacCallum, “A Class of homogeneous cosmological models,” Commun. Math. Phys. 12
1969
Earlier work this paper cites.
A. R. King and G. F. R. Ellis, “Tilted homogeneous cosmological models,” Commun. Math. Phys. 31
1973
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R. M. Wald, “Asymptotic behavior of homogeneous cosmological models in the presence of a positive cosmological constant,” Phys. Rev. D 28
1983
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Similar

G. F. R. Ellis and H. van Elst, “Cosmological models: Cargese lectures 1998,” NATO Sci. Ser. C 541
1999
Cited alongside, same era.
M. Goliath and G. F. R. Ellis, “Homogeneous cosmologies with cosmological constant,” Phys. Rev. D 60
1999
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Closest in time.
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2022

A Tilt Instability in the Cosmological Principle

Krishnan, Chethan, Mondol, Ranjini, Sheikh-Jabbari, M. M.

Understand

We show that the Friedmann-Lema\^{i}tre-Robertson-Walker (FLRW) framework has an instability towards the growth of fluid flow anisotropies, even if the Universe is accelerating.

This flow (tilt) instability in the matter sector is invisible to Cosmic No-Hair Theorem-like arguments, which typically only flag shear anisotropies in the metric.
We illustrate our claims in the setting of ``dipole cosmology'', the maximally Copernican generalization of FLRW that can accommodate a flow.
Simple models are sufficient to show that the cosmic flow need not track the shear, even in the presence of a positive cosmological constant.

Built on

L. Verde, T. Treu and A. G. Riess, “Tensions between the Early and the Late Universe,” Nature Astron. 3
Original
1907
Earlier work this paper cites.
E. Hubble, “A relation between distance and radial velocity among extra-galactic nebulae,” PNAS USA 15 (1929) 168–173
1929
Earlier work this paper cites.
J. M. Stewart and G. F. R. Ellis, “Solutions of Einstein’s equations for a fluid which exhibit local rotational symmetry,” J. Math. Phys. 9
1968
Earlier work this paper cites.
G. F. R. Ellis and M. A. H. MacCallum, “A Class of homogeneous cosmological models,” Commun. Math. Phys. 12
1969
Earlier work this paper cites.
A. R. King and G. F. R. Ellis, “Tilted homogeneous cosmological models,” Commun. Math. Phys. 31
1973
Earlier work this paper cites.
R. M. Wald, “Asymptotic behavior of homogeneous cosmological models in the presence of a positive cosmological constant,” Phys. Rev. D 28
1983
Earlier work this paper cites.

Similar

G. F. R. Ellis and H. van Elst, “Cosmological models: Cargese lectures 1998,” NATO Sci. Ser. C 541
1999
Cited alongside, same era.
M. Goliath and G. F. R. Ellis, “Homogeneous cosmologies with cosmological constant,” Phys. Rev. D 60
1999
Cited alongside, same era.
A. A. Coley, S. Hervik and W. C. Lim, “Fluid observers and tilting cosmology,” Class. Quant. Grav. 23
2006
Cited alongside, same era.
S. Weinberg, “Gravitation and Cosmology: Principles and Applications of the General Theory of Relativity,” John Wiley and Sons, 1972; “Cosmology,” Oxford University press, 2008
2008
Cited alongside, same era.
E. Di Valentino, L. A. Anchordoqui, O. Akarsu, Y. Ali-Haimoud, L. Amendola, N. Arendse, M. Asgari, M. Ballardini, S. Basilakos and E. Battistelli, et al
Original
2008
Cited alongside, same era.