The kSZ effect as a test of general radial inhomogeneity in LTB cosmology
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Volume
85
Publisher
Publisher URL
DOI
10.1103/PhysRevD.85.024002
Journal
Physical Review D: Particles, Fields, Gravitation and Cosmology
ISSN
1550-2368
Metadata
Show full item recordAbstract
The apparent accelerating expansion of the Universe, determined from observations of distant supernovae, and often taken to imply the existence of dark energy, may alternatively be explained by the effects of a giant underdense void if we relax the assumption of homogeneity on large scales. Recent studies have made use of the spherically symmetric, radially inhomogeneous Lemaître-Tolman-Bondi (LTB) models to derive strong constraints on this scenario, particularly from observations of the kinematic Sunyaev-Zel’dovich effect which is sensitive to large-scale inhomogeneity. However, most of these previous studies explicitly set the LTB “bang time” function to be constant, neglecting an important freedom of the general solutions. Here we examine these models in full generality by relaxing this assumption. We find that although the extra freedom allowed by varying the bang time is sufficient to account for some observables individually, it is not enough to simultaneously explain the supernovae observations, the small-angle CMB, the local Hubble rate, and the kinematic Sunyaev-Zel’dovich effect. This set of observables is strongly constraining, and effectively rules out simple LTB models as an explanation of dark energy.
Authors
CLIFTON, TA; BULL, P; FERREIRA, PGCollections
- Physics and Astronomy [1280]