Imprints of a primordial magnetic field upon the cosmic microwave background anisotropy and polarization
We review the imprints that a primordial magnetic field may have left upon the cosmic microwave background (CMB) anisotropy and polarization through Faraday rotation around the time of decoupling. Differential Faraday rotation reduces the degree of linear polarization acquired through anisotropic Th...
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| Formato: | Capítulo de libro |
| Lenguaje: | Inglés |
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Kluwer Academic/Plenum Publishers
1997
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| Acceso en línea: | Registro en Scopus DOI Handle Registro en la Biblioteca Digital |
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| 001 | PAPER-3153 | ||
| 003 | AR-BaUEN | ||
| 005 | 20250505094908.0 | ||
| 008 | 190411s1997 xx ||||fo|||| 00| 0 eng|d | ||
| 024 | 7 | |2 scopus |a 2-s2.0-0031485304 | |
| 040 | |a Scopus |b spa |c AR-BaUEN |d AR-BaUEN | ||
| 100 | 1 | |a Harari, Diego Darío | |
| 245 | 1 | 0 | |a Imprints of a primordial magnetic field upon the cosmic microwave background anisotropy and polarization |
| 260 | |b Kluwer Academic/Plenum Publishers |c 1997 | ||
| 270 | 1 | 0 | |m Harari, D.D.; Departamento de Física, Universidad de Buenos Aires, Ciudad Universitaria-Pab. 1, 1428 Buenos Aires, Argentina; email: harari@df.uba.ar |
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| 506 | |2 openaire |e Política editorial | ||
| 520 | 3 | |a We review the imprints that a primordial magnetic field may have left upon the cosmic microwave background (CMB) anisotropy and polarization through Faraday rotation around the time of decoupling. Differential Faraday rotation reduces the degree of linear polarization acquired through anisotropic Thomson scattering. Depolarization reduces the damping due to photon diffusion, which results in an increase of the anisotropy on small angular scales. The effect is significant at frequencies around and below 10 GHz · √B0/10-9 G where B0 is the present strength of the primordial magnetic field. |l eng | |
| 536 | |a Detalles de la financiación: Emory Eye Center | ||
| 536 | |a Detalles de la financiación: on this project. Most of the work reviewed here was done in collaboration with Matias Zaldarriaga and Justin Hayward. This work was partially supported by an EEC, DG-XII Grant No. CT94-0004, and by CONICET and Universidad de Buenos Aires. | ||
| 593 | |a Departamento de Física, Universidad de Buenos Aires, Ciudad Universitaria-Pab. 1, 1428 Buenos Aires, Argentina | ||
| 773 | 0 | |d Kluwer Academic/Plenum Publishers, 1997 |g v. 36 |h pp. 2513-2523 |k n. 11 |p Int. J. Theor. Phys. |x 00207748 |w (AR-BaUEN)CENRE-5330 |t International Journal of Theoretical Physics | |
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| 856 | 4 | 0 | |u https://doi.org/10.1007/BF02768940 |y DOI |
| 856 | 4 | 0 | |u https://hdl.handle.net/20.500.12110/paper_00207748_v36_n11_p2513_Harari |y Handle |
| 856 | 4 | 0 | |u https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_00207748_v36_n11_p2513_Harari |y Registro en la Biblioteca Digital |
| 961 | |a paper_00207748_v36_n11_p2513_Harari |b paper |c PE | ||
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| 963 | |a VARI | ||
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