skip to main content
OSTI.GOV title logo U.S. Department of Energy
Office of Scientific and Technical Information

Title: Corrections to the apparent value of the cosmological constant due to local inhomogeneities

Journal Article · · Journal of Cosmology and Astroparticle Physics
;  [1]
  1. Department of Physics, National Taiwan University, Taipei 10617, Taiwan, R.O.C. (China)

Supernovae observations strongly support the presence of a cosmological constant, but its value, which we will call apparent, is normally determined assuming that the Universe can be accurately described by a homogeneous model. Even in the presence of a cosmological constant we cannot exclude nevertheless the presence of a small local inhomogeneity which could affect the apparent value of the cosmological constant. Neglecting the presence of the inhomogeneity can in fact introduce a systematic misinterpretation of cosmological data, leading to the distinction between an apparent and true value of the cosmological constant. We establish the theoretical framework to calculate the corrections to the apparent value of the cosmological constant by modeling the local inhomogeneity with a ΛLTB solution. Our assumption to be at the center of a spherically symmetric inhomogeneous matter distribution correspond to effectively calculate the monopole contribution of the large scale inhomogeneities surrounding us, which we expect to be the dominant one, because of other observations supporting a high level of isotropy of the Universe around us. By performing a local Taylor expansion we analyze the number of independent degrees of freedom which determine the local shape of the inhomogeneity, and consider the issue of central smoothness, showing how the same correction can correspond to different inhomogeneity profiles. Contrary to previous attempts to fit data using large void models our approach is quite general. The correction to the apparent value of the cosmological constant is in fact present for local inhomogeneities of any size, and should always be taken appropriately into account both theoretically and observationally.

OSTI ID:
22280227
Journal Information:
Journal of Cosmology and Astroparticle Physics, Vol. 2011, Issue 10; Other Information: Country of input: International Atomic Energy Agency (IAEA); ISSN 1475-7516
Country of Publication:
United States
Language:
English

Similar Records

Inverse construction of the ΛLTB model from a distance-redshift relation
Journal Article · Sat Oct 01 00:00:00 EDT 2016 · Journal of Cosmology and Astroparticle Physics · OSTI ID:22280227

Redshift and structure formation in a spatially flat inhomogeneous universe
Journal Article · Fri May 15 00:00:00 EDT 1992 · Physical Review, D (Particles Fields); (United States) · OSTI ID:22280227

Limits to verification in cosmology
Conference · Tue Jan 01 00:00:00 EST 1980 · Ann. N.Y. Acad. Sci.; (United States) · OSTI ID:22280227