Anisotropies in the cosmic microwave background: Theoretical foundations
From MaRDI portal
Publication:1381698
DOI10.1007/BF02768937zbMath0897.58062arXivastro-ph/9610234MaRDI QIDQ1381698
Publication date: 19 October 1998
Published in: International Journal of Theoretical Physics (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/astro-ph/9610234
Related Items (14)
Dynamics of minimally coupled dark energy in spherical halos of dark matter ⋮ Unified approach to secondary effects on the CMB B-mode polarization ⋮ The CMB bispectrum from bouncing cosmologies ⋮ What do we know and what can we learn about the topology of the universe? ⋮ Theoretical Cosmology ⋮ The Hawking energy in a perturbed Friedmann-Lemaître universe ⋮ Observables in theories with a varying fine structure constant ⋮ Probing eos and correspondences to the agegraphic dark energy through a new \(f(R)\) model of gravity ⋮ Kinetic evolution and correlation of fluctuations in an expanding quark gluon plasma ⋮ Kinematical implications of a new \(f(R)\) theory of gravity: the redshift ⋮ On nonlinear functionals of random spherical eigenfunctions ⋮ Lemaître model and cosmic mass ⋮ Multiple testing of local maxima for detection of peaks on the (celestial) sphere ⋮ Some Mathematical Aspects in the Expanding Universe
Cites Work
This page was built for publication: Anisotropies in the cosmic microwave background: Theoretical foundations
