THE MAGNETIZED UNIVERSE
By M. Giovannini. 2003
321 citations recorded by the source corpus.
Cosmology, high-energy physics and astrophysics are today converging to the study of large scale magnetic fields. While the experimental evidence for the existence of large scale magnetization in galaxies, clusters and super-clusters is rather compelling, the origin of the phenomenon remains puzzling especially in light of the most recent observations. The purpose of the present review is to describe the physical motivations and the open theoretical problems related to the existence of large scale magnetic fields.
Subfields: Astronomy and Astrophysics, Electrical and Electronic Engineering, Instrumentation
View Paper: https://www.semanticscholar.org/paper/f6150536b1bee2a650898db20a8476d385745d0d
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Citations in the corpus
- Planck 2015 results: XIX. Constraints on primordial magnetic fields (2015, unknown): “We can identify three different classes of initial conditions for magneticallyinduced perturbations; compensated (Giovannini 2004a; Finelli et al. 2008), passive (Lewis 2004; Shaw & Lewis 2010), and inflationary (Bonvin et al. 2013).”
- Astrophysical magnetic fields and nonlinear dynamo theory (2004, background): “A number of ways of 23 breaking conformal invariance and generating magnetic fields have been explored [19,179,180,189,190].”
- Effects of rotation on the evolution of primordial stars (2008, background): “Moreover, this dynamo needs a pre-existing magnetic-field seed, and it is not yet clear whether magnetic fields were present in the early Universe or not (see Giovannini 2004, for a detailed discussion on this subject).”