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13 - Cosmic magnetic fields and our ultimate origins

Published online by Cambridge University Press:  22 September 2016

Philipp P. Kronberg
Affiliation:
University of Toronto
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Publisher: Cambridge University Press
Print publication year: 2016

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References

Biermann, L. 1950, Über den Ursprung der Magnetfelder auf Sternen und im interstellaren Raum (mit einem Anhang von A. Schlüter), Zeitschrift für Naturforschung, 5a, 65Google Scholar
Binétruy, P., Bohe, A., Caprini, C., & Dufaux, J.-F. 2012, Cosmological Backgrounds of Gravitational Waves and eLISA/NGO: Phase Transitions, Cosmic Strings and Other Sources, J. Cosmol. Astropart. Phys., 06, 027CrossRefGoogle Scholar
Bond, J. R. & Efstathiou, G. 1984, Cosmic Background Radiation Anisotropies in Universes Dominated by Nonbaryonic Dark Matter, Astrophys. J., 285, L45CrossRefGoogle Scholar
Dyer, C. C. & Shaver, E. G. 1992, On the Rotation of Polarization by a Gravitational Lens, Astrophys. J., 390, L5CrossRefGoogle Scholar
Hanson, D. et al. 2013, Detection of B-Mode Polarization in the Cosmic Microwave Background with Data from the South Pole Telescope, Phys. Rev. Lett., 111, 141301CrossRefGoogle ScholarPubMed
Hu, W., Scott, D., Sugiyama, N., & White, M. 1995, Effect of Physical Assumptions on the Calculation of Microwave Background Anisotropies, Phys. Rev. D., 52, 5498CrossRefGoogle ScholarPubMed
Hu, W. & Okamoto, T. 2002, Mass Reconstruction with Cosmic Microwave Background Polarization, Astrophys. J., 574, 566CrossRefGoogle Scholar
Hu, W. & White, M. 1997, A CMB Polarization Primer, New Astron., 2, 323CrossRefGoogle Scholar
Ichiki, K., Takahashi, K., Ohno, H., Hanayama, H., & Sugiyama, N. 2006, Cosmological Magnetic Field: A Fossil of Density Perturbations in the Early Universe, Science, 311, 827CrossRefGoogle ScholarPubMed
Kahniashvili, T., Brandenburg, A., Campanelli, A., Ratra, B., & Tevadze, A. G. 2012, Evolution of Inflation-Generated Magnetic Field through Phase Transitions, Phys. Rev. D., 86, 103005CrossRefGoogle Scholar
Kahniashvili, T., Tevadze, A. G., Brandenburg, A., & Neronov, A. 2013, Evolution of Primordial Magnetic Fields from Phase Transitions, Phys. Rev. D., 87, 083007CrossRefGoogle Scholar
Kamionkowski, M., Kosowsky, A., & Stebbins, A. 1997, Statistics of Cosmic Microwave Background Polarization, Phys. Rev. D., 55, 7368CrossRefGoogle Scholar
Knox, L. & Song, Y. 2002, Limit on the Detectability of the Energy Scale of Inflation, Phys. Rev. Lett., 89, 011303CrossRefGoogle ScholarPubMed
Kosowsky, A. & Loeb, A. 1996, Faraday Rotation of Microwave Background Polarization by a Primordial Magnetic Field, Astrophys. J., 469, 1CrossRefGoogle Scholar
Kovac, J. M., Leitch, E. M., Pryke, C., Carlstrom, J. E., Halverson, N. W., & Holzapfel, W. L. 2002, Detection of Polarization in the Cosmic Microwave Background Using DASI, Nature, 420, 772CrossRefGoogle ScholarPubMed
Mason, B., Pearson, T. J., Readhead, A. C. S., Shepherd, M. C., Sievers, J., Udomprasert, P. S., Cartwright, J. K., Farmer, A. J., Padin, S., Myers, S. T., et al. 2003, The Anisotropy of the Microwave Background to l = 3500: Deep Field Observations with the Cosmic Background Imager, Astrophys. J., 591, 540CrossRefGoogle Scholar
Polnarev, A. G. 1985, Polarization and Anisotropy Induced in the Microwave Background by Cosmological Gravitational Waves, Sov. Astron., 29, 607Google Scholar
Ratra, B. 1992a, Cosmological “Seed” Magnetic Field from Inflation, Astrophys. J. Lett., 391, L1CrossRefGoogle Scholar
Ratra, B. 1992b, Inflation in an Exponential-Potential Scalar Field Model, Phys. Rev. D., 45, 1913CrossRefGoogle Scholar
Ratra, B. & Peebles, P. J. E. 1988, Cosmological Consequences of a Rolling Homogeneous Scalar Field, Phys. Rev. D., 37, 3406CrossRefGoogle ScholarPubMed
Rees, M. J. 1968, Polarization and Spectrum of the Primeval Radiation in an Anisotropic Universe, Astrophys. J., 153, L1CrossRefGoogle Scholar
Seljak, U. & Zaldarriaga, M. 1997, Signature of Gravity Waves in the Polarization of the Microwave Background, Phys. Rev. Lett., 78, 2054CrossRefGoogle Scholar
Turner, M. S. & Widrow, L. M. 1988, Inflation-Produced, Large-Scale Magnetic Fields, Phys. Rev. D., 37, 2743CrossRefGoogle ScholarPubMed
Vachaspati, T. 1991, Magnetic Fields From Cosmological Phase Transitions, Phys. Lett., 265, 258CrossRefGoogle Scholar
Vachaspati, T. 2003, The Bubbling Universe, Int. J. Mod. Phys. D., 12, 1783CrossRefGoogle Scholar
Wang, S. 2010, New Primordial Magnetic Field Limit from the Latest LIGO S5 data, Phys. Rev. D., 81, 023002CrossRefGoogle Scholar
Widrow, L. M., Ryu, D., Schleicher, D. R. G., Subrahmanian, K., Tsagas, C. G., & Treumann, R. A. 2012, The First Magnetic Fields, Space Sci. Rev., 166, 37CrossRefGoogle Scholar

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