Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/2399
 Title: B-L cosmic strings and baryogenesis Authors: Bhattacharjee, PSahu, NYajnik, U.A Keywords: Cosmic Strings;Baryon Asymmetry;Baryogenesis Issue Date: Oct-2004 Publisher: American Physical Society Citation: Physical Review D, Vol. 70, pp. 083534 Abstract: Cosmic strings arising from breaking of the $U(1)_{B-L}$ gauge symmetry that occurs in a wide variety of unified models can carry zero modes of heavy Majorana neutrinos. Decaying and/or repeatedly self-interacting closed loops of these $B-L$'' cosmic strings can be a non-thermal source of heavy right-handed Majorana neutrinos whose decay can contribute to the observed baryon asymmetry of the Universe (BAU) via the leptogenesis route. The $B-L$ cosmic strings are expected in GUT models such as SO(10), where they can be formed at an intermediate stage of symmetry breaking well below the GUT scale $\sim 10^{16}$ GeV; such light strings are not excluded by the CMB anisotropy data and may well exist. We estimate the contribution of $B-L$ cosmic string loops to the baryon-to-photon ratio of the Universe in the light of current knowledge on neutrino masses and mixings implied by atmospheric and solar neutrino measurements. We find that $B-L$ cosmic string loops can contribute significantly to the BAU for $U(1)_{B-L}$ symmetry breaking scale $\eta_{B-L}\gsim 1.7\times 10^{11}\gev$. At the same time, in order for the contribution of decaying $B-L$ cosmic string loops not to exceed the observed baryon-to-photon ratio inferred from the recent WMAP results, the lightest heavy right-handed Majorana neutrino mass $M_1$ must satisfy the constraint $M_1 \leq 2.4 \times 10^{12}(\eta_{B-L}/10^{13}\gev)^{1/2}\gev$. This may have interesting implications for the associated Yukawa couplings in the heavy neutrino sector and consequently for the light neutrino masses generated through see-saw mechanism. URI: http://hdl.handle.net/2248/2399 ???metadata.dc.relation.uri???: http://prola.aps.org/abstract/PRD/v70/i8/e083534http://arxiv.org/abs/hep-ph/0406054 Appears in Collections: IIAP Publications

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