BAND-POWER RECONSTRUCTION OF PRIMORDIAL PERTURBATION SPECTRUM FROM CMB ANISOTROPY

DOI10.1142/S0217732308027862zbMath1149.85313OpenAlexW2154967468MaRDI QIDQ3525356

Ryo Nagata, Jun'ichi Yokoyama

Publication date: 12 September 2008

Published in: Modern Physics Letters A (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1142/s0217732308027862

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Approximation procedures, weak fields in general relativity and gravitational theory (83C25) Radiative transfer in astronomy and astrophysics (85A25) Astrophysical cosmology (85A40)

Related Items (5)

Non-gaussianities for primordial black hole formation ⋮ Solving peak theory in the presence of local non-gaussianities ⋮ Galileon inflation evades the no-go for PBH formation in the single-field framework ⋮ Multi-field inflation with large scalar fluctuations: non-Gaussianity and perturbativity ⋮ Primordial non-Gaussianity from G-inflation

Cites Work

• Constraining Cosmological Parameters by the Cosmic Inversion Method
• Inflationary universe: A possible solution to the horizon and flatness problems

This page was built for publication: BAND-POWER RECONSTRUCTION OF PRIMORDIAL PERTURBATION SPECTRUM FROM CMB ANISOTROPY