Fluctuations in the CMB Induced by Cosmic Strings: Methods and Formalism
classification
🌌 astro-ph
keywords
methodscosmicfluctuationsaccuracyangularboltzmanncodecompute
read the original abstract
We present methods to compute maps of CMB fluctuations from high resolution cosmic string networks using a full Boltzmann code, on both large and small angular scales. The accuracy and efficency of these methods are discussed.
This paper has not been read by Pith yet.
discussion (0)
Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.