Cosmological Magnetic Field Generation by the Weibel Instability
By R. Schlickeiser, P. K. Shukla. 2003
218 citations recorded by the source corpus.
Subfields: Astronomy and Astrophysics
View Paper: https://www.semanticscholar.org/paper/a1496956fc0d1b07f3f9304d54ec6a52a31c2b0c
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Citations in the corpus
- Titans of the early Universe: The Prato statement on the origin of the first supermassive black holes (2018, background): “Possible sources of magnetic fields in the early Universe are battery processes (Biermann 1950), the Weibel instability (Lazar et al. 2009; Medvedev et al. 2004), or thermal plasma fluctuations (Schlickeiser & Shukla 2003).”
- The Astrophysics of Ultrahigh-Energy Cosmic Rays (2011, background): “…1 µG, as it was produced out of the weakly magnetized void; thus shock acceleration can occur only if the magnetic field upstream can be strongly amplified (M. Lemoine and E. Zweibel, private comm., and see tentative amplification mechanisms by Schlickeiser & Shukla 2003; Zweibel & Everett 2010).”
- WEIBEL, TWO-STREAM, FILAMENTATION, OBLIQUE, BELL, BUNEMAN...WHICH ONE GROWS FASTER? (2009, background): “Filamentation, or Weibel, instabilities could also be responsible for the birth of cosmological magnetic fields (Schlickeiser & Shukla 2003; Schlickeiser 2005; Lazar 2008; Lazar et al. 2009) as unstable particle streams through the intergalactic medium can magnetize an initially un-magnetized…”
- Magnetic Fields in the Large-Scale Structure of the Universe (2011, background): “3 can operate and produce magnetic fields up to the level of εB ∼ 10−3εsh (Schlickeiser and Shukla 2003; Medvedev et al. 2006).”
- Evolution of magnetic fields in galaxies and future observational tests with the Square Kilometre Array (2008, background): “…for generating magnetic seed fields are kinetic plasma instabilities, the so-called Weibel instability (Weibel 1959) in cosmological shocks (Schlickeiser & Shukla 2003; Medvedev et al. 2004) or cosmological perturbations (proposed by Takahashi et al. 2006) that may produce field strengths…”
- THE GENERATION OF STRONG MAGNETIC FIELDS DURING THE FORMATION OF THE FIRST STARS (2010, background): “These studies have ignored the possible role of magnetic fields primarily, because the initial field strengths obtained from either cosmological processes like inflation and phase transition [6, 7] or astrophysical processes like the Biermann battery [8] or the Weibel instability [9, 10] are highly ”
- Cosmological Magnetic Fields: Their Generation, Evolution and Observation (2013, background): “Possible mechanisms for the generation of magnetic fields during the gravitational collapse are the Weibel instability (Schlickeiser and Shukla 2003; Medvedev et al 2006) or battery effects (Subramanian et al 1994; Kulsrud et al 1997; Gnedin et al 2000).”
- Small-scale dynamo action during the formation of the first stars and galaxies - I. The ideal MHD limit (2010, background): “Additional seed fields may be created via the Weibel instability in shocks (Schlickeiser & Shukla 2003; Medvedev et al. 2004; Lazar et al. 2009).”