TY - JOUR

T1 - Anisotropy and inhomogeneity of the universe from ΔT/T

AU - Maartens, Roy

AU - Ellis, George F R

AU - Stoeger, William R.

PY - 1996/5/1

Y1 - 1996/5/1

N2 - A recent paper (Martinez-Gonzalez & Sanz 1995) showed that if the universe is homogeneous but anisotropic, then the small quadrupole anisotropy in the cosmic microwave background radiation (CBR) implies that the spacetime anisotropy is very small. We point out that more general results may be established, assuming the weaker condition that all fundamental observers measure the CBR to be almost isotropic, instead of assuming that the universe is exactly homogeneous. Assuming this weak Copernican principle (which is partially testable), we have proved that if small anisotropies are observed in the CBR, then the observable universe is almost Friedmann-Robertson-Walker. Furthermore, the quadrupole and octopole place direct and explicit limits on the degree of anisotropy and inhomogeneity, as measured by the shear, vorticity, Weyl tensor and density gradients. (We follow the standard assumption that the CBR dipole is purely Doppler and may be removed by a velocity boost.) In the presence of inhomogeneity, it is only possible to set a much weaker limit on the shear than that given by Martinez-Gonzalez & Sanz.

AB - A recent paper (Martinez-Gonzalez & Sanz 1995) showed that if the universe is homogeneous but anisotropic, then the small quadrupole anisotropy in the cosmic microwave background radiation (CBR) implies that the spacetime anisotropy is very small. We point out that more general results may be established, assuming the weaker condition that all fundamental observers measure the CBR to be almost isotropic, instead of assuming that the universe is exactly homogeneous. Assuming this weak Copernican principle (which is partially testable), we have proved that if small anisotropies are observed in the CBR, then the observable universe is almost Friedmann-Robertson-Walker. Furthermore, the quadrupole and octopole place direct and explicit limits on the degree of anisotropy and inhomogeneity, as measured by the shear, vorticity, Weyl tensor and density gradients. (We follow the standard assumption that the CBR dipole is purely Doppler and may be removed by a velocity boost.) In the presence of inhomogeneity, it is only possible to set a much weaker limit on the shear than that given by Martinez-Gonzalez & Sanz.

KW - Cosmology: theory

KW - Cosmology:cosmic microwave background

UR - http://www.scopus.com/inward/record.url?scp=0346482626&partnerID=8YFLogxK

M3 - Article

AN - SCOPUS:0346482626

VL - 309

JO - Astronomy and Astrophysics

JF - Astronomy and Astrophysics

SN - 0004-6361

IS - 1

ER -