M. Jaroszynski et B. Paczynski, THE COSMIC MICROWAVE BACKGROUND DIPOLE CANNOT BE THE RESULT OF THE COSMOLOGICAL ENTROPY GRADIENT, The Astrophysical journal, 448(2), 1995, pp. 488-493
A conventional explanation of the dipole anisotropy of the cosmic micr
owave background radiation is in terms of the Doppler effect: our Gala
xy is moving with respect to the cosmic microwave background frame wit
h similar to 600 km s(-1). However, as the deep redshift surveys fail
to reveal a convergence of the large-scale flow to zero at distances a
s large as d similar to H-1 15,000 km s(-1) (Lauer and Postman 1994),
the uniqueness of the conventional interpretation has to be investigat
ed. A possible alternative might be a cosmological entropy gradient, a
s suggested by Paczynski and Piran (1990). We find that contrary to th
at suggestion a quadrupole anisotropy is generically of the same order
of magnitude as the dipole anisotropy (or larger) not only for adiaba
tic but also for isocurvature initial perturbations. Hence, the observ
ed dipole cannot be explained with a very large scale perturbation whi
ch was initially isocurvature.