1996
DOI: 10.1017/s0373463300013400
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Whither Astro?

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Cited by 13 publications
(30 citation statements)
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“…In order to avoid the important drawbacks of Eckart's theory, we shall use transport equations derived from the Israel-Stewart approach [9][10][11]. However, since these equations are going to be evaluated immediately after the system leaves the perfect fluid (or the quasi-perfect fluid) regime, then the truncated version of the theory leads to the same result as the full theory, and therefore the former will be used here.…”
Section: Transport Equationsmentioning
confidence: 99%
“…In order to avoid the important drawbacks of Eckart's theory, we shall use transport equations derived from the Israel-Stewart approach [9][10][11]. However, since these equations are going to be evaluated immediately after the system leaves the perfect fluid (or the quasi-perfect fluid) regime, then the truncated version of the theory leads to the same result as the full theory, and therefore the former will be used here.…”
Section: Transport Equationsmentioning
confidence: 99%
“…If this observational evidence is correct, then the implications for cosmology are remarkable. Attempts to explain this phenomenon include "quintesssence" [2], the cosmological constant [3], a domain wall dominated universe [4] and non-perturbative vacuum contributions to the effective action of a massive scalar field [5]. In general it would appear that the cosmological fluid is dominated in the present universe by an exotic energy density, which has a negative pressure and which did not play an important role in the early universe.…”
Section: Introductionmentioning
confidence: 99%
“…The origin of these cosmical magnetic fields has been explained mainly by dynamo theory [3], which is one of the most active research areas across multiple subdisciplines of physics. In particular, generation of an electromotive force (EMF) along a mean field by turbulence, or the well-known α effect [4], is an essential process in amplifying large-scale magnetic fields [5]. Experimentally, the α effect has been observed in toroidal laboratory plasmas [6].Recently, there has been growing awareness that a topological constraint on the observed magnetic field, the conservation of magnetic helicity, may play an important role in solar flare evolution [7].…”
mentioning
confidence: 99%