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Recent studies have indicated that an anisotropic cosmic expansion may exist. In this paper, we use three datasets of type Ia supernovae (SNe Ia) to probe the isotropy of cosmic acceleration. For the Union2.1 dataset, the direction and magnitude of the dipole are $(l=309.3^{circ} {}^{+ 15.5^{circ}}_{-15.7^{circ}} , b = -8.9^{circ} {}^{ + 11.2^{circ}}_{-9.8^{circ}} ), A=(1.46 pm 0.56) times 10^{-3}$. For the Constitution dataset, the results are $(l=67.0^{circ}{}^{+ 66.5^{circ}}_{-66.2^{circ}}, b=-0.6^{circ}{}^{+ 25.2^{circ}}_{-26.3^{circ}}), A=(4.4 pm 5.0) times 10^{-4}$. For the JLA dataset, no significant dipolar deviation is found. We also explore the effects of anisotropic distributions of coordinates and redshifts on the results using Monte-Carlo simulations. We find that the anisotropic distribution of coordinates can cause dipole directions and make dipole magnitude larger. Anisotropic distribution of redshifts is found to have no significant effect on dipole fitting results.
Despite its fundamental importance in cosmology, there have been very few straight-forward tests of the cosmological principle. Such tests are especially timely because of the hemispherical asymmetry in the cosmic microwave background recently observ
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We present a new signature by which to one could potentially discriminate between a spectrum of gravitational radiation generated by a self-ordering scalar field vs that of inflation, specifically a comparison of the magnitude of a flat spectrum at f
The isotropy of the late Universe is an assumption greatly used in astronomy. However, many studies have recently reported deviations from isotropy with a definitive conclusion yet to be made. New, independent methods to robustly test the cosmic isot
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