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Is the CMB cold spot a gate to extra dimensions?

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2008-10
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IOP Publishing Ltd
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One of the most striking features found in the cosmic microwave background data is the presence of an anomalous cold spot (CS) in the temperature maps made by the Wilkinson Microwave Anisotropy Probe (WMAP). This CS has been interpreted as the result of the presence of a collapsing texture, perhaps coming from some early universe grand unified theory (GUT) phase transition. In this work we propose an alternative explanation based on a completely different kind of texture which appears in a natural way in a broad class of brane-world models. This type of texture, known as a brane-skyrmion, can be understood as a hole in the brane which makes it possible to pass through them along the extra-dimensional space. The typical scales needed for the proposed brane-skyrmions to correctly describe the observed CS can be as low as the electroweak scale.
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©2008 IOP Publishing Ltd and SISSA. This work has been partially supported by the DGICYT (Spain) under projects FPA2004-02602, FPA2005-02327 and CAM/UCM 910309, by UCM-Santander PR34/07-15875 and by DOE grant DOE/DE-FG02-94ER40823.
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[1] Spergel D N et al, 2007 Astrophys. J. Suppl. 170 377. [2] Hinshaw et al, 2007 Astrophys. J. Suppl. 170 288. [3] Vielva P, Mart´ınez-González E, Barreiro R B, Sanz J L and Cayón L, 2004 Astrophys. J. Suppl. 609 22. [4] Cruz M, Martínez-Gonz´alez E, Vielva P and Cayón L, 2005 Mon. Not. R. Astron. Soc. 365 29. [5] Cruz M, Cay´on L, Martínez-González E, Vielva P and Jin J, 2007 Astrophys. J. 655 11 [SPIRES]. [6] Naselsky P D et al, 2007 arXiv:0712.1118 [astro-ph]. [7] Cruz M, Turok N, Vielva P, Martinez-Gonzalez E and Hobson M, 2007 Science 318 1612. [8] Turok N, 1989 Phys. Rev. Lett. 63 2625 [SPIRES] Turok N, 1991 Phys. Scr. T 36 135. [9] Turok N and Spergel D, 1990 Phys. Rev. Lett. 64 2736 [SPIRES]. [10] Arkani-Hamed N, Dimopoulos S and Dvali G, 1998 Phys. Lett. B 429 263 [SPIRES] Antoniadis I et al, 1998 phys. Lett. B 436 257 [SPIRES]. [11] Dobado A and Maroto A L, 2001 Nucl. Phys. B 592 203 [SPIRES]. [12] Cembranos J A R, Dobado A and Maroto A L, 2003 Phys. Rev. Lett. 90 241301 [SPIRES]. Cembranos J A R, Dobado A and Maroto A L, 2003 Phys. Rev. D 68 103505 [SPIRES]. [13] Cembranos J A R, Dobado A and Maroto A L, 2002 Phys. Rev. D 65 026005 [SPIRES]. [14] Spergel D N et al, 1991 Phys. Rev. D 43 1038 [SPIRES]. [15] Giovannini M, 2005 Int. J. Mod. Phys. D 14 363 [SPIRES]. [16] Yao W M et al (Particle Data Group), 2006 J. Phys. G: Nucl. Part. Phys. 33 1 [SPIRES] Mirabelli E A, Perelstein M and Peskin M E, 1999 Phys. Rev. Lett. 82 2236 [SPIRES]. [17] Cembranos J A R, Dobado A and Maroto A L, 2004 Phys. Rev. D 70 096001 [SPIRES]. [18] Alcaraz J et al, 2003 Phys. Rev. D 67 075010 [SPIRES]. [19] Achard P et al (L3 Collaboration), 2004 Phys. Lett. B 597 145 [SPIRES].
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