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Cosmologies of Bianchi Type i with a Uniform Magnetic Field
Abstract
An analysis is presented of the effects of a uniform, primordial magnetic field upon spatially homogene- ous cosmological models with the anisotropic, Euclidean metric ds2 = d12 - A2(t)dx2 - B2(t)dy2 - W2(t)dz2. The stress-energy tensor consists of perfect-fluid matter with the equation of state PM = 7PM (0 «= y «= 1) and a uniform magnetic field of energy density PB Analytical solutions are obtained for four subcases, and all remaining cases are studied by numerical integration. Axisymmetric solutions (A = B) always emerge from point or pancake singularities, while non-axisymmetric solutions (A != B) always emerge from initial cigar or barrel singularities. The solutions are used in a cursory examination of the effects of a primordial magnetic field upon (a) the temperature isotropy of the observed 30 K cosmic microwave radiation, (b) the time when expansion anisotropies become small, and (c) primordial element formation
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Items 101–132 of 132
Anisotropic nonsingular quantum bounce as a seesaw and amplification mechanism for magnetic fields
Motaharfar, M., & Singh, P. (2024) · Physical review. D/Physical review. D. · doi:10.1103/physrevd.110.086020 · Cited by 3
“[87]) where ± denotes the expanding (contracting) branches when the mean scale factor reaches a max1 .”
BackgroundRelic vector field and CMB large scale anomalies
Chen, X., & Wang, Y. (2014) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2014/10/027 · Cited by 3
GRAVITOMAGNETIC INSTABILITIES IN ANISOTROPICALLY EXPANDING FLUIDS
Kleidis, K., Kuiroukidis, A., Papadopoulos, D., & Vlahos, L. (2008) · International Journal of Modern Physics A · doi:10.1142/s0217751x0804127x · Cited by 3
Liouville Type Dilatonic Potential in Locally Rotationally Symmetric Bianchi I Model
Banerjee, A., Ghosh, T., & Chakraborty, S. (2001) · General Relativity and Gravitation · doi:10.1023/a:1012010332625 · Cited by 3
Magnetohydrodynamics and Plasma Cosmology
Kleidis, K., Kuiroukidis, A., Papadopoulos, D., & Vlahos, L. (2007) · International Journal of Theoretical Physics · doi:10.1007/s10773-007-9346-x · Cited by 3
The Lepton Brusselator: Creation of structure in the early universe
Zimmermann, R. E. (1982) · General Relativity and Gravitation · doi:10.1007/bf00756287 · Cited by 2
“This has been dealt with in the works of Jacobs [9, 10 ] and more recently in those of Belinsky and Khalatnikov [2], Caderni [3], Caderni and Fabbri [4, 5], and Lorenz [12].”
ResultSymmetries of spacetimes embedded with an electromagnetic string fluid
Tsamparlis, M., Mitsopoulos, A., & Paliathanasis, A. (2018) · General Relativity and Gravitation · doi:10.1007/s10714-018-2488-8 · Cited by 2
“This excludes all analytical solutions found in [28].”
BackgroundA noncommutative Bianchi I model with radiation
Oliveira-Neto, G., & Abreu, T. M. (2024) · International Journal of Modern Physics D · doi:10.1142/s0218271824500329 · Cited by 2
“We may mention the following few examples of those models [6, 7, 8, 9, 10, 11, 12, 13, 14, 15, 16, 17, 18, 19, 20, 21, 22].”
BackgroundInfluentialIsotropization of the magnetic universe in Horndeski theory with G 3(X,ϕ) and G 5(X)
Muharlyamov, R. K., Pankratyeva, T. N., & Bashir, S. O. A. (2024) · Chinese Physics C · doi:10.1088/1674-1137/ad65de · Cited by 2
Limits on Cosmological Magnetic Fields and Other Anisotropic Stresses
Barrow, J. D. (1998) · Springer eBooks · doi:10.1007/978-94-011-5046-0_7 · Cited by 2
FOUR- AND HIGHER-DIMENSIONAL MODELS WITH DILATON–ELECTROMAGNETIC FIELDS
CHAKRABORTY, N. C., & Chakraborty, S. (2001) · International Journal of Modern Physics D · doi:10.1142/s0218271801001001 · Cited by 2
Influence of electromagnetic fields on the evolution of initially homogeneous and isotropic universe
Алексеев, Г. А. (2013) · Proceedings of the Steklov Institute of Mathematics · doi:10.1134/s0081543813040111 · Cited by 2
Bianchi Type V magnetized string dust cosmological models with Petrov-type degenerate
Bali, R., & Pareek, U. K. (2009) · Pramana · doi:10.1007/s12043-009-0071-2 · Cited by 2
Anisotropic matter in cosmology: locally rotationally symmetric Bianchi I and VII o models
Sloan, D. (2016) · Classical and Quantum Gravity · doi:10.1088/0264-9381/33/10/105011 · Cited by 2
“In this case, the Maxwell tensor Fi j is zero apart from = = F F B 2 y z z y , hence the stress-energy tensor is diagonal with entries B B B B , , , 2 2 2 2 ( ) and so = w 1 1 and = w 1 2 [21].”
Null strings in Bianchi I models: dynamical anisotropy damping and consequences
Kuiroukidis, A., Kleidis, K., & Papadopoulos, D. (1999) · Classical and Quantum Gravity · doi:10.1088/0264-9381/16/8/314 · Cited by 2
An inhomogeneous magnetohydrostatic universe
Prakash, S., & Roy, S. R. (1980) · Journal of Physics A Mathematical and General · doi:10.1088/0305-4470/13/12/027 · Cited by 2
Spektrum und Anisotropiegrad der 3 °K‐Strahlung bei anisotroper kosmologischer Expansion
Dautcourt, G. (1970) · Astronomische Nachrichten · doi:10.1002/asna.19702920305 · Cited by 2
General Review of Cosmological Theories
HOYLE, F. (1972) · Symposium - International Astronomical Union · doi:10.1017/s0074180900006033 · Cited by 2
Muharlyamov, R. K., Pankratyeva, T. N., & Bashir, S. O. A. (2025) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2025/05/018 · Cited by 1
Bianchi Type-IX Universe with Magnetized Anisotropic Dark Energy
Ghate, H. R., & Sontakke, A. S. (2015) · Cited by 1
Cosmic anisotropic doomsday in Bianchi type I universes
Cataldo, M., Cid, A., Labraña, P., & Mella, P. (2016) · Journal of Mathematical Physics · doi:10.1063/1.4967954 · Cited by 1
A note on the magnetic perfect fluid Bianchi type-VIo solutions
Lorenz-Petzold, D. (1985) · Astrophysics and Space Science · doi:10.1007/bf00653796 · Cited by 1
Some Problems of the Dynamics of Waves in Relativistic Cosmology
Sibgatullin, N. R. (1991) · Springer eBooks · doi:10.1007/978-3-642-83527-8_6 · Cited by 1
Excitation of MHD waves in magnetized anisotropic cosmologies
Kuiroukidis, A., Kleidis, K., Papadopoulos, D., & Vlahos, L. (2007) · Springer Link (Chiba Institute of Technology) · doi:10.1051/0004-6361:20077109/pdf · Cited by 1
Maxwell's equations in spatially homogeneous cosmological models
Portugal, R. (1995) · Astrophysics and Space Science · doi:10.1007/bf00627541
Evans, C. R., & Fennelly, A. J. (1985) · Astrophysics and Space Science · doi:10.1007/bf00651011
Shikin, I. S. (1987) · General Relativity and Gravitation · doi:10.1007/bf00759576
Spatially homogeneous and anisotropic expanding universe
Johri, V. B., Goswami, G. K., & Singh, I. J. (1978) · Acta Physica Academiae Scientiarum Hungaricae · doi:10.1007/bf03158157
Early Universe evolution in presence of magnetic fields
Gaspar, I. D., Martínez, A. P., Piccinelli, G., & Sussman, R. A. (2015) · Astronomische Nachrichten · doi:10.1002/asna.201512219
Kleidis, K., Kuiroukidis, A., & Papadopoulos, D. (2023) · Astronomy · doi:10.3390/astronomy2020008
Izzah, R. F., Nasiroh, C., Yasir, M., Akbar, F. T., & Gunara, B. E. (2026) · Chinese Journal of Physics · doi:10.1016/j.cjph.2026.03.007
Bianchi-I cosmology with radiation in asymptotically safe gravity
Chen, C.-M., Fan, T.-K., Mandal, R., & Ohta, N. (2026) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2026/09/044 · Cited by 1
“A considerable body of work has explored BI cosmologies from various perspectives [34, 45–57].”
Metadata
- Authors
- Jacobs, K. C.
- Corresponding author
- Jacobs, Kenneth C.
- Venue
- The Astrophysical Journal
- Publisher
- American Astronomical Society
- Published
- 1969-02
- Volume
- 155
- Pages
- 379
- ISSN
- 0004-637X (ISSN-L)
- 1538-4357
- OpenAlex
- W2007557354
- Semantic Scholar
- 6b7a231a2a46dfd7fcdeb11b493d2de63c222054
- Cited by
- 133
- References
- 0
- Citations by year
- 2026: 2 · 2025: 1 · 2024: 6 · 2023: 3 · 2021: 2 · 2020: 1 · 2019: 2 · 2018: 2 · 2017: 4 · 2016: 7 · 2015: 3 · 2014: 4 · 2013: 1 · 2012: 1
- FWCI
- 3.65
- Type
- journal article
- Language
- en
- Open access
- closed
- Locations
- The Astrophysical Journal (publishedVersion)
- Topics
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Cosmology and Gravitation Theories
- Physical Sciences › Mathematics › Geometry and Topology › Advanced Differential Geometry Research
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Galaxies: Formation, Evolution, Phenomena
- Keywords
- Bianchi type I cosmology, primordial magnetic fields, anisotropic cosmology, perfect fluid, axisymmetric solutions, singularity formation, big bang nucleosynthesis
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